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Charm and the Virtual Photon at HERA and a Global Tracking Trigger for ZEUS Benjamin John West UCL University College London August 2001 Thesis submitted in fulfillment of the requirements for the degree of Doctor of Philosophy in Physics

Charm and the Virtual Photon at HERA and a Global Tracking ...€¦ · Charm and the Virtual Photon at HERA and a Global Tracking Trigger for ZEUS Benjamin John West UCL University

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  • Charm and th e V irtual P h oton

    at H E R A and a G lobal

    Tracking Trigger for ZEUS

    Benjamin John West

    U C L

    University College London

    August 2001

    Thesis subm itted in fulfillment of the requirem ents for

    the degree of D octor of Philosophy in Physics

  • ProQuest Number: U642447

    All rights reserved

    INFORMATION TO ALL USERS The quality of this reproduction is dependent upon the quality of the copy submitted.

    In the unlikely event that the author did not send a com plete manuscript and there are missing pages, th ese will be noted. Also, if material had to be removed,

    a note will indicate the deletion.

    uest.

    ProQuest U642447

    Published by ProQuest LLC(2015). Copyright of the Dissertation is held by the Author.

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  • A b stract

    Previous m easurem ents a t ZEUS have dem onstra ted suppression of photon s tructu re

    like effects due to bo th the v irtuality of the photon, and the presence of charm .

    In this thesis aspects of these two m easurem ents have been com bined in order to

    determ ine w hether these two suppressions are independent.

    The m easurem ent was m ade w ith the ZEUS detecto r a t HERA in the kinem atic

    region 0 < < 5 • 10^ GeV^ using dijet events containing a D* meson. Events

    having two or more je ts w ith large transverse energies were selected using the

    longitudinally invariant kr algorithm in the labo ra to ry frame. The dijet cross section

    was m easured as a function of the fractional m om entum of the photon partic ipa ting

    in the dijet production, , and of

    The ratio of low to high cross sections was found not to change significantly w ith

    Q^. This is in m arked con trast to previous m easurem ents which did not require a D*,

    dem onstrating for the first tim e th a t the observed suppressions of the low cross

    section due to non-zero photon v irtuality and due to charm are not independent.

    The ratio was also com pared to the predictions of leading-order pQCD. C alculations

    which included either a resolved v irtual photon in the D G LAP evolution scheme

    or used CCFM evolution gave a b e tte r description of the d a ta th an a D G LA P

    calculation w ith no photon structure .

    D uring the 2000-2001 shutdow n bo th the H ERA accelerator and ZEUS detector

    were upgraded. In order to take advantage of these im provem ents a new “global

    tracking trigger” , com bining inform ation from the C entral Tracking D etector and

    the newly installed Micro Vertex D etector a t th e Second Level Trigger, has been

    developed. T he algorithm is described and its perform ance evaluated. T he event

    z vertex resolution is two orders of m agnitude b e tte r th an th a t for the present

    algorithm . This will enable fu ture m easurem ents of the cross section ra tio to be

    m ade w ith much greater precision.

  • To my family and friends

    “W riting a book is an undertak ing far more horrific th a n I ’d ever imagined. Not

    only m ust the w riter come up w ith several tens of thousands of words, not all of

    them the same, bu t he or she m ust arrange them in an order th a t makes some sort

    of sense to the first tim e reader. I t ’s no use s ta rtin g your book ‘Linford Christie

    stepped into the horse-box bem used by th e wall of m ushroom s which stood grinning

    a t the back’ if you have no in tention of tak ing these ideas any further. To s ta rt

    a book w ith th is sentence, b u t then take your eye off the ball for a m om ent and

    end up w riting a tw enty-thousand word guide to Polish war m em orials, deserves the

    highest criticism . I t ’s a fau lt th a t took me m any m onths of practice to avoid.

    O thers have been less m eticulous. I ’m surely not the only one to have noticed th a t

    W ill H u tto n ’s otherw ise adm irably w ritten economics bestseller The State W e ’re In

    opens w ith the sentence ‘This book has been carefully graded so th a t you can begin

    w ith one or two elem entary dishes yet soon be able to set ou t a full T hai meal

    w ith all its unique flavours.’ Nor is there any earth ly explanation other th an sheer

    au thorial incom petence for a few stray lines in S tephen H aw king’s A Brief History

    of Time which, a t the end of a brilliant explanation of the sym biotic relationship

    between quan tum theory and relativity, seductively h in ting a t a unified theory of

    gravity, suddenly continue:

    Bevin let out a gasp of astonishm ent and playful pleasure a t the

    Professor’s rem arks. ‘Ooh boy,’ she yelped, like a cat. ‘Tell it to me one

    more tim e, ’cos I ’m on fire, particle m an!’ She rem em bered now their

    curiously in terrup ted lovemaking from the previous n ight and resolved

    to ham m er the door shut th is tim e.

    T he rem aining ninety pages revert to a discussion of partic le /w ave duality w ithin

    light emissions.

    Consistency is therefore a prerequisite for even the m ost vaguely com petent s tab

    a t a book.”

    A rm ando lannucci. Facts and Fancies^ 1997

  • Acknowledgments

    Over the last three years I have been fo rtunate enough to work w ith m any excellent

    people, w ithout whom th is thesis would not have been possible. For help w ith

    my analysis, I would like to thank Jon B utterw orth for his advice and m otivation

    throughout; M ark Hayes for teaching me the basics; Leonid G ladilin for his

    knowledge of all things heavy flavoured; Jo Cole for her advice on D*s in DIS;

    Alex Tapper for his extensive knowledge of DIS and generosity in sharing it; M att

    Light wood for his hard work reproducing my analysis; and R ichard H all-W ilton for

    continuing where I left off. For all his hard work on the G T T , bo th before and

    after I joined the effort, I owe a great deal to M ark S utton . The product of our

    collaboration is som ething I th ink we can bo th be proud of. I would also like to

    th an k Stew Boogert for m any random physics conversations which helped bo th my

    understanding and enthusiasm .

    Fortunately, there has been much more to my life th a n ju s t work during my PhD ,

    and for th a t I owe m any people thanks. In particu la r I would like to thank Alex

    Ferguson for being a good friend and housem ate; A nn W hittle for the tim e we had

    together; K ate Evans for listening and being a good friend; B eth Purse for staying

    close even when far away; Stew Boogert for being a good cook, host and m ate; Alex

    T apper for m any enjoyable hours in bars; Rod W alker for his citrus theory of life;

    E laine McLeod for enjoyable conversations, bo th home and abroad; R icardo Gonçalo

    for being a great neighbour and friend; Claire Gwenlan for the m any chats; and Jon

    B utterw orth for being m ore th a n ju s t a supervisor.

    Finally, I would like to th an k my parents for the ir unconditional support and

    encouragem ent th roughou t my life.

  • Contents

    I Charm and the virtual photon at HERA 19

    1 H ER A and the ZEUS detector 20

    1.1 The H ERA a c c e le r a to r ..................................................................................... 20

    1 .2 The ZEUS d e t e c to r ............................................................................................ 2 1

    1.3 The C entral Tracking D etector (CTD ) ..................................................... 22

    1.4 ZEUS c a lo r im e try ....................................................................................................... 23

    1.5 The lum inosity m onitor ..................................................................................24

    1.6 The ZEUS trigger system .............................................................................. 25

    2 QCD and ep Interactions 27

    2.1 P ro ton s truc tu re ....................................................................................................... 28

    2 .1 .1 T he naive quark parton m odel ............................................................... 30

    2.1.2 The QCD improved quark parton m o d e l ............................................31

    2.2 Evolution e q u a tio n s ....................................................................................................33

    2.2.1 BFK L e v o lu tio n ..............................................................................................34

    2.2.2 CCFM e v o l u t i o n .......................................................................................... 35

    2.3 Pho ton s t r u c t u r e ....................................................................................................... 36

    2.3.1 H ard p h o to p ro d u c t io n ............................................................................... 38

    2.3.2 Pho ton s truc tu re fu n c tio n s ........................................................................ 39

    2.4 V irtual photon s t r u c t u r e ......................................................................................... 41

    2.4.1 Experim ental r e v i e w ................................................................................... 42

    2.5 Heavy flavour p ro d u c tio n ......................................................................................... 43

    2.5.1 E xperim ental r e v i e w ................................................................................... 44

    3 K inem atic reconstruction 47

    3.1 R econstruction of y and .................................................................................. 47

    3.1.1 E lectron m e t h o d .......................................................................................... 47

    9

  • Acknowledgments

    Over the last th ree years I have been fo rtunate enough to work w ith m any excellent

    people, w ithou t whom this thesis would not have been possible. For help w ith

    my analysis, I would like to thank Jon B u tterw orth for his advice and m otivation

    throughout; M ark Hayes for teaching me th e basics; Leonid G ladilin for his

    knowledge of all things heavy flavoured; Jo Cole for her advice on D*s in DIS;

    Alex Tapper for his extensive knowledge of DIS and generosity in sharing it; M att

    Lightwood for his hard work reproducing my analysis; and R ichard H all-W ilton for

    continuing where I left off. For all his hard work on the G T T , bo th before and

    after I joined the effort, I owe a great deal to M ark Sutton . The product of our

    collaboration is som ething I th ink we can bo th be proud of. I would also like to

    thank Stew Boogert for m any random physics conversations which helped bo th my

    understanding and enthusiasm .

    Fortunately, there has been much more to my life th an ju s t work during my PhD ,

    and for th a t I owe m any people thanks. In particu la r I would like to thank Alex

    Ferguson for being a good friend and housem ate; Ann W hittle for the tim e we had

    together; K ate Evans for listening and being a good friend; B eth Purse for staying

    close even when far away; Stew Boogert for being a good cook, host and m ate; Alex

    T apper for m any enjoyable hours in bars; R od W alker for his citrus theory of life;

    E laine McLeod for enjoyable conversations, bo th hom e and abroad; R icardo G onçalo

    for being a g reat neighbour and friend; Glaire G wenlan for th e m any chats; and Jon

    B utterw orth for being m ore than ju s t a supervisor.

    Finally, I would like to th an k my parents for their unconditional support and

    encouragem ent th roughou t my life.

  • Contents

    I Charm and the virtual photon at HERA 19

    1 H ERA and the ZEUS detector 20

    1 .1 The HERA a c c e le r a to r ...............................................................................................20

    1 .2 The ZEUS d e t e c to r ......................................................................................................2 1

    1.3 The C entral Tracking D etector (CTD) ...............................................................22

    1.4 ZEUS c a lo r im e try ......................................................................................................... 23

    1.5 The lum inosity m onitor ...........................................................................................24

    1.6 The ZEUS trigger system ....................................................................................... 25

    2 QCD and ep Interactions 27

    2.1 P ro ton s truc tu re .......................................................................................................28

    2 .1 .1 The naive quark parton m o d e l ...................................................................30

    2.1.2 T he QCD im proved quark parton m o d e l ..............................................31

    2.2 Evolution e q u a t io n s ......................................................................................................33

    2.2.1 BFK L e v o lu tio n ..............................................................................................34

    2.2.2 CCFM e v o l u t i o n .......................................................................................... 35

    2.3 P ho ton s t r u c t u r e ......................................................................................................... 36

    2.3.1 H ard p h o to p ro d u c t io n ............................................................................... 38

    2.3.2 Photon s truc tu re fu n c tio n s ........................................................................ 39

    2.4 V irtual photon s t r u c t u r e .........................................................................................41

    2.4.1 Experim ental r e v i e w ...................................................................................42

    2.5 Heavy flavour p ro d u c tio n .........................................................................................43

    2.5.1 E xperim ental r e v i e w ...................................................................................44

    3 K inem atic reconstruction 47

    3.1 R econstruction of y and ....................................................................................47

    3.1.1 E lectron m e t h o d .......................................................................................... 47

    9

  • Contents

    3.1.2 Jacquet-B londel m e t h o d .............................................................................48

    3.2 Je t re c o n s tru c tio n ..........................................................................................................48

    3.2.1 Cone a lg o r i th m ...............................................................................................49

    3.2.2 C lustering a l g o r i t h m ....................................................................................50

    3.3 r e c o n s t r u c t io n .....................................................................................................51

    4 Event selection 53

    4.1 Definition of the cross s e c t io n s .................................................................................53

    4.2 Online event se lec tio n ...................................................................................................54

    4.2.1 F irst Level Trigger (FLT) ......................................................................... 54

    4.2.2 Second Level Trigger (SLT) ..................................................................... 55

    4.2.3 T hird Level Trigger ( T L T ) .........................................................................55

    4.2.4 Efficiency of the trigger c h a i n ............................................................. 56

    4.3 Offline event se lec tio n ...................................................................................................58

    4.3.1 C o r r e c t io n s .....................................................................................................58

    4.3.2 K inem atic s e le c t io n ....................................................................................... 59

    4.3.3 D* re c o n s tru c tio n ...........................................................................................60

    4.4 Background E s tim a tio n ............................................................................................... 61

    5 Event description and correction 63

    5.1 M onte Carlo s im u la tio n ............................................................................................... 63

    5.1.1 M onte C arlo s a m p le s ....................................................................................63

    5.2 Com parison of d a ta and M onte C a r l o ...................................................................64

    5.3 Acceptance correction ............................................................................................... 67

    5.4 S tudy of system atic uncertain ties on the r a t i o ............................................... 70

    5.4.1 U ncertain ties arising from calorim eter q u a n t i t ie s .............................. 70

    5.4.2 U ncertain ties arising from tracking quantities ..................................71

    5.4.3 U ncertain ties arising from the M onte Carlo description . . . . 72

    5.4.4 In itia l s ta te r a d ia t io n ....................................................................................73

    6 R esults and D iscussion 75

    6 .1 Com parison to LO pQ CD p re d ic tio n s ...................................................................75

    6 .2 Im plications for ...................................................................................................... 77

    6.3 Com parison to ra tio w ithou t a D* tag ...............................................................78

    6.4 Je t production in DIS and the Y p f r a m e ........................................................... 81

    10

  • Contents

    II A global tracking trigger for ZEUS 83

    7 The upgrades to H ERA and the ZEUS detector 84

    7.1 In tro d u c t io n ...................................................................................................................84

    7.2 H E R A ............................................................................................................................. 85

    7.3 Straw Tube Tracker ( S T T ) .......................................................................................8 6

    7.4 Micro Vertex D etector ( M V D ) ............................................................................... 87

    7.4.1 Barrel s e c t i o n ...................................................................................................8 8

    7.4.2 Forward s e c t io n ............................................................................................... 90

    8 The G TT algorithm 91

    8.1 E xisting C T D - S L T .....................................................................................................91

    8.1.1 Segment f in d in g ............................................................................................... 91

    8.1.2 Vector h it f in d in g ............................................................................................93

    8.1.3 Track f i n d i n g ...................................................................................................93

    8.1.4 Event vertex determ ination ...................................................................... 95

    8.2 M otivation for a G T T ..............................................................................................96

    8.2.1 Im provem ents to the C T D - S L T ............................................................... 96

    8.2.2 Heavy fiavour tagging a t the S L T ............................................................97

    8.3 T he G T T algorithm ................................................................................................. 97

    8.3.1 Segment f in d in g ............................................................................................... 98

    8.3.2 Axial track f i n d i n g ........................................................................................ 98

    8.3.3 z track f in d in g .................................................................................................100

    8.3.4 Event vertex determ ination .................................................................... 106

    8.4 Future w o r k .................................................................................................................107

    8.4.1 Second pass of z-track f in d i n g .................................................................108

    8.4.2 Dealing w ith non-ideal w a f e r s .................................................................108

    8.4.3 Secondary vertex f in d in g ........................................................................... 109

    9 Perform ance of the G TT 111

    9.1 MVD sim ulation ...................................................................................................... I l l

    9.2 Event s a m p l e ..............................................................................................................1 1 2

    9.3 Track r e s o lu t io n s ...................................................................................................... 116

    9.3.1 p t resolution .................................................................................................117

    9.3.2 (j) r e s o lu t io n .................................................................................................... 118

    11

  • Contents

    9.3.3 77 r e s o lu t io n .................................................................................................. 119

    9.3.4 ztrack r e s o lu t io n ........................................................................................... 119

    9.4 Track e ff ic ie n c y ........................................................................................................ 120

    9.5 Event v e r te x ................................................................................................................122

    9.6 L a t e n c y ...................................................................................................................... 123

    III Summary 125

    A M onte Carlo event generators 129

    A .l H E R W I G ...................................................................................................................130

    A.2 P Y T H IA ...................................................................................................................... 131

    A.3 A R O M A ...................................................................................................................... 131

    A.4 CASCADE .................................................................................................................131

    B D erivation of Errors 133

    B .l P u r i t y ..........................................................................................................................133

    B .2 Efficiency ...................................................................................................................134

    B.3 Correction f a c t o r .....................................................................................................134

    C M aths of the GTT algorithm 136

    C .l C onstrained r-cj) track f i t ...................................................................................... 136

    C .2 U nconstrained r-cf) track f i t ...................................................................................137

    C.3 Intersection of an axial track w ith a stereo wire in z - s ............................. 138

    R eferences 141

    12

  • List of Figures

    1.1 The HERA accelerator chain (left) and delivered lum inosity from1992-2000 (righ t)............................................................................................................20

    1 .2 Overview of the ZEUS detec to r.................................................................................21

    1.3 x-y view of the CTD showing the wire layout (left) and a C TD driftcell (righ t).........................................................................................................................2 2

    1.4 Cut-away view of an FCAL m odule........................................................................ 23

    1.5 The Lum inosity M onito r..............................................................................................24

    1.6 The ZEUS d a ta acquisition and trigger system .................................................. 25

    2 .1 K inem atics of a deep inelastic scattering event...................................................28

    2 .2 The NC and CC cross sections as a function of m easured a t HERA. 29

    2.3 vs. for fixed x. The fixed-target results from NMC, BCDMS,and E665 and the ZEUS NLO QCD fit are also show n.................................. 32

    2.4 Schem atic representation of the applicability of various evolutionequations across the {x, Q^) p lane .......................................................................... 34

    2.5 Schem atic representation of the gluon ladder and quark box E ................... 35

    2.6 T he to ta l photon-proton cross section....................................................................37

    2.7 Exam ples of leading-order processes resulting in two jets; (a) QCD C om pton, (b) boson gluon fusion, (c) fiavour excitation from the proton, (d) gluon gluon fusion, (e) and (f) fiavour excitation fromthe pho to n ........................................................................................................................ 38

    2.8 The d istribu tion in dijet events for d a ta (black dots) com pared w ith HERW IG w ith and w ithou t M PI (solid line and do tted line),and PY TH IA w ith M PI (dashed line) M onte Carlo genera to rs ...................39

    2.9 Feynm an diagram for e j d iagram w ith a v irtual photon , 7 *, probingan on-shell photon, 7 (left). Sum m ary of current results on (right). 40

    2.10 Triple differential cross section a / dx^^dQi^ a s a function of

    ^obs different regions in and F ^ (le ft) . T he ra tio of cross sections R = cr(T°^^ < 0.75)/cr(T°^^ > 0.75) as a function of(righ t).................................................................................................................................42

    13

  • Figures

    2 .1 1 D ifferential cross sections for D* p roduction in DIS. T he open (shaded) band shows the result of an NLO QCD calculation using Peterson (R A PG A P extracted) fragm entation (left). as afunction of x and (righ t)...................................................................................... 45

    2.12 The differential cross section da/dri^* for photoproduction com pared to several NLO calculations (left). T he differential cross section da/dx^^ for dijets w ith an associated D* (right) com pared to LO (upper) and NLO (lower) predic tions..............................................................46

    3.1 y and resolutions using the electron and Jacquet Blondel m ethods. 49

    3.2 Je t Et and rj resolutions for GAL cell je ts using the KTGLUS algorithm . 51

    3.3 resolution in photoproduction and D IS........................................................ 52

    4.1 TLT Efficiency for d a ta (points) and M onte Carlo (bands).................... 57

    4.2 Box cut applied to the scattered electron .......................................................59

    4.3 H adron level in GeV for events passing all detector level cuts. . . 60

    4.4 Signals for the 1996-2000 d a ta , the line shows the resu lt of anunbinned fit to the signal and the h istogram the wrong charge background estim ate .............................................................................................. 61

    5.1 Com parison of d a ta (points) and PY T H IA M onte Carlo (histogram )^obs d istribu tions in P H P and DIS events..................................................... 65

    5.2 C om parison of d a ta (points) and M onte Carlo (histogram ) for event,je t and D* properties of the events entering the cross section m easurem ent............................................................................................................. 6 6

    5.3 Purity , efficiency and correction factor shown for th e unfolding procedure as a function of x^^ for each region............................................6 8

    5.4 Low and high cross sections for events w ith a D* as a functionof Q^. E rrors are sta tistica l only.............................................................................. 69

    5.5 R atio of low to high x^^ cross sections for events w ith a D* as a function of Q^. E rrors are s ta tis tica l only............................................................ 70

    5.6 System atic uncertain ties due to the kinem atic cuts as a function of 3:°^ . T he shaded band shows th e s ta tis tica l error on the central ra tio value.................................................................................................................................... 71

    5.7 System atic uncertain ties due to the D* as a function of . The shaded band shows the s ta tis tica l error on the central ra tio value. . . 72

    5.8 System atic U ncertainties due to the M onte Carlo as a function of. T he shaded band shows th e s ta tis tica l error on the central ra tio

    value.................................................................................................................................... 73

    6.1 R atio of low to high cross sections for events w ith a D* com pared to the LO pQ CD predictions of HERW IG using the S aS lD P D F (upper), and AROM A and CASCAD E (lower).................................................. 76

    14

  • Figures

    6 .2 Predicted ratio of low to high for events containing a D*, w ith7and w ithout D* cuts (left) for H E R W IG /SaS ID . M onte Carlo hadron level p t {D*) and ri[D*) d istribu tions predicted by H ER W IG /SaS ID for events passing all other hadron level cuts (r ig h t).................................. 79

    6.3 R atio of low to high events w ith a D* com pared to the7predictions of the SaS lD photon stru c tu re function for the ra tio w ithou t a D* tag. The upper edge of the band represents the expected ra tio for the full D* phase space.............................................................................. 80

    6.4 R atio of low to high for events containing a D* in the LAB and 7 *p fram es (left). Change in r]{D*) and 77-̂ *̂ when boosting to the Y p fram e (righ t).................................................................................................................... 82

    7.1 An exploded view of the Straw Tube Tracker......................................................8 6

    7.2 A cross section of an STT layer.................................................................................87

    7.3 A cross sectional view of the M V D .......................................................................... 87

    7.4 3D and 2D views of the barrel section of the M V D ...........................................8 8

    7.5 Top view of a ladder...................................................................................................... 8 8

    7.6 Side view of a m odule................................................................................................... 89

    7.7 Schem atic diagram of a half m odule........................................................................89

    7.8 P a rtia l cross section of a sensor w ith two readout s tr ip s .................................89

    7.9 3D and 2D views of the forward section of the M V D .......................................90

    8 .1 Axial segment ghost am biguity..................................................................................92

    8.2 P a tte rn recognition in a strip detecto r w ith two h its ........................................97

    8.3 Stereo segment ghost am biguity................................................................................ 98

    8.4 Schem atic diagram of the r-4> track finding..........................................................99

    8.5 T he (j) residuals of the closest M VD hits to ex trapo la ted track duringthe MVD r-cf) m atching stage.................................................................................. 100

    8 .6 Schem atic diagram of the z-s track finding........................................................ 101

    8.7 T he d istribu tion of %^/nseg for superlayer 9, 7, 5 and 3 tracks............... 102

    8 .8 The z-segm ent residuals of the segm ent end points w ith respect tothe ex trapo lated track position during the stereo segm ent finding.From the top: superlayer 5, 7 and 9 tracks; from left to right: th e ex trapo la ted positions in superlayer 2 , 4 and 6 . The dashed (solid) histogram shows th e residuals (w ithout) using the MVD wafer guide position ............................................................................................................................ 104

    8.9 T he z residuals of th e closest M VD h its to ex trapo la ted track duringthe MVD z m atching stage for superlayer 9 tracks........................................ 105

    8.10 Secondary vertex displacem ents and im pact param eters for D mesons(histogram ) and D mesons whose daughters have p > 0.3 GeV and|?7|

  • Figures

    9.1 Pt , t], Ztrack and m ultiplicity d istribu tions of the M onte Carlo used toevaluate th e G T T ........................................................................................................112

    9.2 Event displays showing the offline (upper) and G T T (lower) tracksfor the sam e MG event.............................................................................................. 114

    9.3 Event displays showing the offline (upper) and G T T (lower) tracksfor a busy MG event...................................................................................................115

    9.4 Pt , ÿ, rj, and Ztrack residuals for G T T track s .....................................................116

    9.5 Pt resolution as a function of p t , p, ztrack, and event m ultiplicity forG T T and offline tracks .............................................................................................. 117

    9.6 0 resolution as a function o fp ^ , P, Ztrack, and event m ultiplicity forG T T and offline tracks .............................................................................................. 118

    9.7 p resolution as a function of p, Ztrack, and event m ultiplicity for G T T and offline tracks .............................................................................................. 119

    9.8 Ztrack icsolution as a function of p t , p, Ztrack, and event m ultiplicityfor G T T and offline tracks....................................................................................... 120

    9.9 Track finding efficiency as a function of p t , p, Ztrack, and eventm ultiplicity for G T T and offline tracks............................................................... 121

    9.10 Track finding efficiency as a function of p t , p, ztrack, and eventm ultiplicity for axial G T T tracks and full G T T tracks w ith andw ithout a second pass................................................................................................ 1 2 1

    9.11 G T T and offline event Zytx resolution and efficiency..................................... 122

    9.12 The latency of the GTD only algorithm on d a ta after a GELT accept taken during the 2000 running period (left) and of the G TD +M V D algorithm on dijet M onte Garlo (righ t)............................................................... 124

    9.13 A real cosmic event reconstructed by the G T T using GTD and MVD inform ation in A ugust 2001................................................................................... 127

    9.14 G T T (GTD Only) event vertex d istribu tion for real d a ta after GELTand TLT accepts. The beam -gas con tribu tion can clearly be seen. . . 127

    16

  • List of Tables

    5.1 G enerated MC subsam ples.................................................................................. 64

    5.2 LO -D IR and LO-RES norm alisations for PY TH IA and HERW IG. . . 65

    9.1 Table showing p t , , p, and Ztrack resolutions for CTD-SLT, G T T ,and offline tracks...................................................................................................... 116

    9.2 Event Zytx resolution for GTD-SLT, G T T , and offline algorithm s. . . . 123

    17

  • Part I

    Charm and the virtual photon atHERA

    19

  • Chapter 1

    HERA and the ZEUS detector

    1.1 The H E R A accelerator

    H E RA

    W est Hall (HERA-B!

    OOBIS

    South Hall (ZEUS!

    HERA luminosity 1992 - 2000

    2000

    e•a

  • C hapter 1 1.2 The ZEUS detector

    are passed to the PETR A accelerator, where they are accelerated to 40 GeV and

    injected into the HERA proton machine. This process continues until HERA is

    filled w ith 210 bunches, which are then accelerated to the HERA operation proton

    energy^ using conventional radio frequency cavities. The proton beam is focused

    and guided by superconducting quadrupole and dipole magnets.

    Lepton injection commences with LINACS’s I and II which accelerate lepton beam s

    to 220 and 450 MeV respectively. These are then transferred to the DESY II

    synchrotron and accelerated to 7.5 GeV before being injected into the PETR A II

    storage ring in bunches w ith 96 ns spacing. The beam is then accelerated to 14 GeV

    and injected into the HERA lepton machine. After it is filled with 210 bunches the

    beam is accelerated to the operating energy of 27.52 GeV, using bo th conventional

    and superconducting cavities.

    1.2 T he ZEUS detector

    OverView o f t h e Z E U S D E J E C I O R 2 0 0 0 ( I o p v i e w c u t

    - 1 0 m

    5m 0 -5mFigure 1.2; Overview of the ZEUS detector.

    The ZEUS detector, shown in Figure 1 .2 , is a general purpose m agnetic detector,

    w ith nearly herm etic calorim etric coverage. A detailed description of the ZEUS

    detector can be found elsewhere [1]. A brief outline of the com ponents which are

    most relevant for th is analysis is given below.

    1820 GeV from 1992-1997 and 920 GeV from 1998-2000.

    21

  • Chapter 1 1.3 The Central Tracking Detector (CTD)

    f ie ld w ire

    sh a p e r w ire

    — g u a rd w ire

    — g ro u n d w ire

    Figure 1.3; x-y view of the CTD showing the wire layout (left) and a CTD drift cell (riyht).

    1.3 The Central Tracking D etector (C T D )

    The CTD [2] is a cyliiiclrical drift chamber, which operates in a m agnetic field of

    1.43T, provided by a thin superconducting coil. The CTD consists 72 cylindrical

    drift cham ber layers, organised in 9 superlayers, covering the polar angle range 15°-

    164°. A superlayer contains between 32 and 96 drift cells, each com prising eight

    sense wires oriented in a plane a t 45° to the radial line from the cham ber axis. The

    drift field is a t a Lorentz angle of 45° to the radial axis so th a t the drift electrons

    follow radially transverse paths which is im portan t in left-right am biguity breaking.

    W ires in the odd numbered “axial” superlayers run parallel to the z axis^, whereas

    wires in the even numbered “stereo” superlayers are at a small stereo angle (~ ±5°),

    allowing both r-cf) and z coordinates to be accurately m easured. The nominal

    resolution for full length tracks in the CTD is 180 y m in r — ( f ) and % 2 mm in

    z. The first three axial layers are also instrum ented with a z-by-tim ing system

    which estim ates the position of a h it along a wire from the pulse arrival times at

    each end of the chamber. The resolution using this m ethod is ~ 4 cm and it is

    predom inantly used for trigger purposes.

    The transverse m om entum resolution for full length tracks is (j (p t ) / pt = 0.0058pr@

    0.0065 © 0.0014/pT, w ith p r in GeV [3].

    ^The ZEUS coordinate system is a right-handed Cartesian system, with the z axis pointing in the proton beam direction, referred to as “forward direction” , and the x axis pointing left towards the centre of HERA. The coordinate origin is at the nominal interaction point.

    22

  • Chapter 1 1.4 ZEUS calorimetry

    1.4 ZEUS calorim etry

    te n s io n s tra p ^ |

    The high-resolution iiranium -scintillator calorim eter (CAL) [4] consists of three

    parts: the forward (FCAL), the barrel (BCAL) and the rear (RCAL) calorimeters.

    Each part is subdivided transversely into towers and longitudinally into one

    electrom agnetic section (EMC) and either one (in RCAL) or two (in BCAL and

    ECAL) hadronic sections (HAC). The smallest subdivision of the calorim eter is

    called a cell. Each HAC cell is approxim ately 2 0 x 2 0 cm and each EMC cell is

    approxim ately 5x20 cm (in BCAL and FCAL) or 10x20 cm (in RCAL). The readout

    is performed by two photom ultipliers (coupled to the scintillator by wavelength

    shifters) per cell; the pair ensuring the measurement to be independent of the im pact

    point of the particles. A typical FCAL module w ith EM C and HAC divisions can

    be seen in Figure 1.4.

    The EMC is the inner section of the tower,

    with two hadronic sections (HACl and HAC2 )

    outside this. The a lternating layers of De-

    ])leted Uranium and scintillator can also be seen.

    The unequal res])onse, due to hadronic showers

    l)roducing fewer photons than electrom agnetic

    showers for a particle of the same energy, is com

    pensated by the uranium , which absorbs neu

    trons from the hadronic shower and em its pho

    tons which can then be detected by the photo

    m ultipliers. By choosing a suital)le thickness of

    uranium , the same num ber of photons are pro

    duced for hadronic and electrom agnetic showers

    of the same energy. This is im portan t in the re

    construction of je ts which are composed of both

    electrom agnetic and hadronic com ponents in an

    unknown proportion. The CAL energy resolu

    tions, as measured under test beam conditions,

    are a { E ) / E = 0 .18 \ /Ê for electrons and a { E ) / E = 0 .35 \Æ ’ for hadrons {E in GeV).

    Associated w ith the CAL are several subcom ponents, designed to improve the energy

    resolution or particle identification properties of the calorim eter, two of which are

    relevant to this analvsis.

    P A R T IC L E

    HAC low er

    Silicon d e te c to r

    sc in tilla to r p la te

    ZEUS FCAL MODULE

    Figure 1.4: Cut-away view of an FCAL module.

    23

  • Chapter 1 1.5 The luminosity monitor

    Presampler

    The Presam pler [5] is a th in segmented layer of scin tillator on the inner face of

    the calorim eter. This can be used to estim ate the am ount of showering, and hence

    energy loss, th a t a particle has undergone while passing through the dead m aterial

    before the CAL.

    SRTD

    The Small-angle Rear Tracking D etector (SRTD) [6 ], is designed to measure

    electrons scattered at small angles and improve the m easurem ent of their position

    and energy. The SRTD is located on the face of the RCAL, around the beam pipe,

    covering the polar angle region 162°-170°. This region is particularly im portan t

    because it is the region in which most DIS electrons are scattered. The SRTD

    consists of two layers of hnely segmented silicon strips, resulting in a tracking

    resolution of about 3mm, compared to 1cm in the calorim eter. The SRTD also

    provides a m easurem ent of the am ount of showering before the CAL wliich can be

    used to correct the energy obtained from the calorim eter.

    1.5 The lum inosity m onitor

    Luminosity Monitor

    BU

    # 0BU BU BU

    10 20

    lumi-e

    lumi-Y

    30 40 50 60 70 80 90 100 110(m )

    Figure 1.5: The Luminosity Monitor.

    Tlie lum inosity is m easured using the rate of B ethe-H eitler photons, ep -4- epy,

    where the 7 is em itted by the electron at a very low angle to the incident electron

    direction in negative z. The cross section for th is process is very high and can

    be calculated to w ithin 0.5%. The m easurem ent of the small angle electron and

    24

  • Chapter 1 1.6 The ZEUS trigger system

    Event Builder

    TLTProcessor

    TLTProcessor

    LocalSLT

    TLTProcessor

    LocalFLT

    GSLTDistribution

    GFLT

    GSLT

    ComponentProcessor

    ComponentProcessor

    ComponentProcessor

    ComponentProcessor

    Optical Link / Mass Storage

    Figure 1 .6 : The ZEUS data acquisition and trigger system.

    photon is performed by two se])arate detectors. The photon detector is situated

    close to the beam pipe between 104 and 107 m from the in teraction point, in the

    electron direction. The electron detector is situated 34 m from the interaction point.

    Both detectors are based on lead-scintilla tor sandwich calorim eters w ith an energy

    resolution of a { E ) / E = 0 .18 \Æ .

    1.6 The ZEUS trigger system

    The nominal bunch crossing ra te of the HERA accelerator is ~ 10 MHz which poses

    challenges for the D ata AcQuisition (DAQ) and trigger systems. The interaction

    ra te is dom inated by interactions between the proton beam and residual gas, “beam

    gas” , which contributes about lO-lOOkHz, whilst the rate w ritten to tape for ep

    interactions is between a few and 10 Hz.

    25

  • Chapter 1 1.6 The ZEUS trigger system

    To reduce the rate to less than ~ 1 0 Hz w hilst efficiently selecting ep events, ZEUS

    uses a th ree stage trigger system [7] shown in Figure 1.6.

    The ra te is initially reduced to ~ 1 kHz by the F irs t Level Trigger (FLT) which is

    a hardw are based trigger. Each com ponent used a t th e FLT has its own FLT and

    stores the d a ta in a pipeline aw aiting a decision. The decision is m ade w ith in ~ 2 /zs

    of the bunch crossing and passed onto the Global F irs t Level Trigger (GFLT) which

    then makes a final decision in 4.4 /is, passing the decision back to the com ponent

    readout.

    Events which pass the FLT proceed onto the Second Level Trigger (SLT). The SLT

    is a software based trigger run on a network of transpu ters, designed to reduce the

    ra te by approxim ately a factor of ten. Analogously to the FLT, each com ponent

    can have its own SLT, which passes decisions onto the G lobal Second Level Trigger

    (GSLT).

    Each com ponent then passes the filtered events to an event builder which fills the

    d a ta s tru c tu re for the T h ird Level Trigger (TLT). The TLT runs a crude version

    of the full reconstruction software and is able to make decisions concerning global

    event properties, je t properties and event kinem atics. The event ra te is now reduced

    to a m anageable ~ 1 Hz. The final stage is to transfer the events by an optical fibre

    link to storage for processing by the full ZEUS reconstruction software a t a la ter

    date.

    26

  • Chapter 2

    QCD and ep Interactions

    T he in teractions of quarks and gluons are described by Q uantum Chrom odynam ics

    (Q CD), a non-abelian gauge theory based on the SU(3) colour sym m etry group. The

    quarks, each in three colours, in teract by the exchange of electrically neu tra l vector

    bosons, gluons, which form a colour octet. The gluons are no t colour neu tra l and

    thus they themselves in teract strongly. A consequence of th is p roperty is asym ptotic

    freedom , which states th a t the in teraction streng th of two coloured objects decreases

    th e shorter the distance between them . The effective strong coupling constant

    then depends on the scale a t which the QCD process occurs. T he leading-order

    solution of the renorm alisation group equation gives

    = /3oln(QVA2) ’ (2.1)

    where denotes the scale a t which as is probed and A is a QCD cutoff param eter.

    T he param eter is related to the num ber of quark flavors in the theory, Nf, by

    ^ 0 = 11 — 0 ^ / - (2 -2 )

    Since the known num ber of flavors is six, /3o > 0, the coupling constan t becomes

    sm aller the larger the scale Q^. The p roperty of asym ptotic freedom has been proven

    rigorously and allows predictions for the properties of strong in teractions to be m ade

    in the p ertu rba tive QCD (pQ CD) regime, in which is sm all. One such exam ple

    is the production of jets^ in annihilation a t LEP in which ~ M |. A t lower

    scales as becomes large m aking pertu rba tive calculations unreliable and accurate

    ^The produced quarks and gluons cannot be observed directly due to the phenomena known as “colour confinement”. Instead a spray of hadrons, called a jet, emerges in the approximate direction of each parton.

    27

  • C hapter 2 2.1 Proton structure

    predictions cannot be made. For example, the d istribu tion of the “partons” bound

    in hadrons, cannot be calculated from first principles.

    QCD has been tested in dep th in the pertu rba tive regim e and describes the d a ta

    very well [8 ]. However, because the observables are based on hadrons ra th e r th an the

    partons to which pertu rba tive calculations apply the precision achieved in testing

    QCD is lower th an in the case of electroweak in teractions and a detailed experim ental

    knowledge of the struc tu re of hadrons is essential.

    2.1 P roton structure

    l { k )

    ^ V»(

  • C hapter 2 2.1 Proton structure

    10

    10

    10

    10

    10

    10

    10

    10

    * HI e^p NC 94-00 prelim.A H I e p NC□ ZEUS e^p NC 99-00 prelim, o ZEUS e p NC 98-99 prelim.

    -- SM e^p NC (CTEQ5D)— SM e p NC (CTEQ5D)

  • C hapter 2 2.1 Proton structure

    F2 is th e generalised stru c tu re function of 7 and exchange, F l is the longitudinal

    s tru c tu re function, and F 3 is the parity violating te rm arising from exchange.

    Since F 3 is small for « M | it is neglected in all fu rth er discussions here. A

    detailed derivation of all these term s is given, for exam ple, in [9].

    2.1.1 The naive quark parton model

    The form of the cross sections given above is com pletely general, all the physics

    detail is contained in the s truc tu re functions. A priori these m ight be expected

    to be com plicated functions of p and reflecting the com plexity of the inelastic

    scattering process. However, in 1969, Bjorken predicted th a t in the deep inelastic

    region^ the structu re functions should “scale” , i.e. becom e functions not of and

    1/ independently bu t only of the ir ratio Q'^/u. T his predicted scaling was confirmed

    by results from SLAC [1 0 ].

    Feynm an gave an in tu itive explanation of B jorken’s argum ents in his parton

    m odel [1 1 ], in which the p ro ton is assum ed to be com posed of point-like objects,

    called partons. The inelastic scattering of the lepton off th e p ro ton is then described

    as the elastic scattering of the lepton off a parto n within th e proton. The ep

    cross section is then given by the incoherent sum of the electron-parton scattering

    processes.

    If a parton of mass m , carrying a fraction, of the to ta l p ro ton m om entum is

    struck, conservation of four-m om entum implies ^

    t)^rn^ = {^p + q f = V - g

    T he Bjorken scaling variable, x, then has a simple in te rp re ta tio n as the fraction of

    the longitudinal pro ton m om entum , carried by th e p arton in the hard scatter.

    W ith in the parton m odel the s truc tu re functions are given by

    (2 .12)i

    f i W = (2.13)

    u 00 but f v finite.^This is in the infinite momentum frame of the proton, where the partons have no transverse

    momentum and the masses can be neglected.

    30

  • C hapter 2 2.1 Proton structure

    where are the parto n charges and fi{x) are the parto n density functions which

    can be in terpreted as th e probability of finding a p arton i w ith m om entum fraction

    X in the proton. F2 and Fi are connected by the C allan-G ross relation

    2 j;F iW (2.14)

    which is a direct consequence of the assum ption th a t partons are massless, sp in-1 / 2 ,

    non-in teracting particles and implies th a t Fl is zero.

    T hrough m easurem ents a t SLAC and in u N scattering [12], these partons were

    associated w ith the quarks of the Gell-M ann and Zweig and the m odel becam e the

    quark parton model (Q PM ).

    2.1.2 The QCD improved quark parton model

    If the proton consisted solely of charged quarks the sum of the ir m om enta would be

    equal to th a t of the p ro ton , i.e.

    1

    f dxf i {x)x = 1. (2.15)* 0

    However, experim entally th is value was found to be % 0.5 [13]. This im plies th a t

    there are also electrically neu tra l particles w ith in the p ro ton which carry ~ 50%

    of its m om entum . These particles are identified w ith gluons, the gauge bosons of

    QCD. D irect evidence for the existence of these gluons, was provided in 1979 via

    the observation of 3-jet events in e+e" annih ilation a t DESY [14].

    In th is QCD im proved Q PM , the assum ption th a t the transverse m om entum of the

    partons is zero, in the infinite m om entum frame, no longer holds. A quark can em it

    a gluon and acquire a large transverse m om entum kr w ith probability proportional

    to CKg dk ‘̂ /k^ a t large kx- This integral extends up to the kinem atic lim it, ^

    and gives rise to con tribu tions proportional to CKg log which break scaling. This

    was experim entally confirm ed by the observation of a logarithm ic dependence on

    of F2 ( x ,Q ‘̂ ) and was one of the first m ajor successes of p ertu rba tive QCD.

    Figure 2.3 shows th e la tes t m easurem ent of the x and dependence of F2 from

    ZEUS, clearly showing these scaling violations [15]. A t large values of x, where the

    valence quarks dom inate, F2 (and hence the quark density) can be seen to fall w ith

    increasing At low x, where the num ber of “sea” quarks and gluons is larger, F2

    is clearly seen to increase w ith Q^.

    31

  • Chapter 2 2.1 Proton structure

    ZEUS

    CJDO

    0

    x = 6 .3 E -0 5 x = 0 .0 0 0 1 0 2

    (= 0 .000161x = 0 .0 0 0 2 5 3

    x = 0 .0004 x = 0 .0005

    (= 0 .0 0 0 6 3 2 x = 0 .0 0 0 8

    .00102 .0013

    1.00161

    0.0021 .00253

    0 .0032

    x = 0 .005

    • ZEUS 96/97 A Fixed Target - NLO QCD Fit

    x = 0 .008

    x = 0 .0 1 3

    x = 0.021

    x = 0 .0 3 2

    l _ x = 0 .05

    x= 0 .0 8

    x = 0 .13

    *- i , > j i x = 0 .18

    x = 0 .25

    x = 0.4

    x = 0 .65

    1 0 1 0 ̂ 1 0 ̂ l o ' ' , l o C(GeV^)

    Figure 2.3: vs. for fixed x. The fixed-target results from NMC, BCDMS,and E665 and the ZEUS NLO QCD fit are also shown.

    32

  • Chapter 2 2.2 Evolution equations

    2.2 E volution equations

    The factorisation theorem of collinear (mass) singularities [16] sta tes th a t, in

    a general hard collision (i.e. a scattering process involving a large transferred

    m om entum )$> A^) of incoming hadrons, all long-distance (non-perturbative)

    effects can be factorised into universal (process-independent) parton densities thus

    leading to a pertu rbatively calculable dependence on the hard scattering scale

    called parton evolution. This dependence arises because a quark seen a t a scale

    Ql as carrying a fraction Xq of the proton m om entum can be resolved into more

    quarks and gluons, having x < xq, when the scale is increased.

    One set of p arton evolution equations derived on the basis of the collinear

    factorisation theorem are the D okshitzer-G ribov-Lipatov-A ltarelli-Parisi (D G LA P)

    evolution equations [17]. The D GLAP equations describe the way the quark q and

    gluon g m om entum distribu tions in a hadron evolve w ith the scale of the in teraction

    Q '.

    dqi(x ,Q ‘̂ )dlogQ^

    dg{x ,Q ‘̂ )dlogQ^

    ^ f dy

    yX

    1

    ^ f dy2 % y V

    + givi Q )Pqg -X

    Y ^ g i { y , Q ^ ) Pgq ( - ) +9{y,Q^)Pgg ( - )

    (2,16)

    ,{2.17)

    where qi{x,Q^) is the quark density function, for each quark flavour i and g { x , Q ‘̂ )

    is the gluon density function. The “sp litting functions” Pjk represent the

    probability of a parton k of m om entum fraction y em itting a parton j of m om entum

    fraction x. This probability will depend on the num ber of splittings allowed in

    the approxim ation. Given a specific factorisation and renorm alisation scheme, the

    sp litting functions Pjk are obtained in QCD by p ertu rba tive expansion in CKg,

    y j \ y J 27t \ y

    The truncation after the first two term s in th e expansion defines the next-to-

    leading order (NLO) D G LA P evolution. This approach assumes th a t the dom inant

    contribution to the evolution comes from subsequent parton emissions which are

    strongly ordered in transverse m om enta the largest corresponding to the p arton

    in teracting w ith the probe.

    At small X, higher order contributions to the sp litting functions of the form

    (2.18)

    33

  • Chapter 2 2.2 Evolution equations

    High density region

    CCFM

    Unconventional DGLAP Modified BFKL

    DGLAP

    £ n

    Figure 2.4: Schematic representation of the applicability of various evolutionequations across the (x, Q^) plane.

    P (n) ~ —InX

    n —1X

    will be enhanced, spoiling the convergence of (2.18). T hus th e conventional

    D G LAP equations may be inadequate a t low x and m ust e ither be modified or an

    a lternative set of evolution equations used. Figure 2.4 shows th e expected regions of

    applicability of various alternatives across the (x, plane. T he BFK L and CCFM

    evolution equations, which are based on a generalisation of th e collinear factorisation

    theorem called kr factorisation [18] will now be discussed.

    2.2.1 BFKL evolution

    The B alitsky-Fadin-K uraev-L ipatov (BFKL) [19] evolution equation allows the

    resum m ation of term s w ith a leading (a^ In a;)" in the expansion of E quation (2.18),

    independent of In This involves considering the evolution of a gluon d istribu tion

    which is not in tegrated over /c^, since breaking the association to leading In

    implies th a t the gluon ladder need not be ordered in hr- T he unin tegrated gluon

    density is related to the m ore fam iliar gluon d istribu tion by

    2x g { x , Q ‘̂ ) = J ^ Q ( x , k T ) (2.19)

    34

  • Chapter 2 2.2 Evolution equations

    y,Q

    Figure 2.5: Schematic representation of the gluon ladder and quark box 5 .

    The BFK L equation then describes the ln (l/a :) evolution of the un in tegrated gluon

    density:

    dÇ{x, k f)(2 .20)

    d ln { l / x )

    This evolution corresponds roughly to cascades w ith emissions strongly ordered in

    X w ith no restric tion on h r -

    In order for the BFK L equation to make predictions, e.g. of F2 , the gluon ladder

    m ust be convoluted w ith the quark box (Figure 2.5) according to th e hr factorisation

    theorem :

    1

    F2{x ,Q^) = [ ~ [ (2 .2 1 )J y J i T̂ V

    2.2.2 CCFM evolution

    W hereas the conventional D G LA P equations deal w ith evolution and may

    be inadequate a t low x, the BFK L equation deals w ith 1 /x evolution and may

    be inadequate a t high The C iafaloni-C atani-F iorani-M archesini (CCFM ) [20]

    35

  • C hapter 2 2.3 Photon structure

    evolution equations a ttem p t to be applicable across the whole kinem atic plane by

    sum m ing more general classes of diagram s. They are based on the idea of coherent

    gluon rad ia tion , which leads to angular ordering of gluon emissions in the gluon

    ladder such th a t 6i > 9i-\ where 6i is the ith gluon makes to the original direction.

    O utside th is angular region there is destructive interference such th a t m ulti-gluon

    con tribu tions vanish to leading-order. A ngular ordering implies ordering in k r / E of

    the gluon ladder. Because of angular ordering, the unin tegrated gluon d istribu tion

    in CC FM depends on the m axim um allowed angle, in addition to the m om entum

    fraction x and the transverse m om entum of the propagator gluon. This ex tra scale

    can be taken to be the scale Q of the probe, leading to a scale dependent gluon

    density

    At sm all T, where A becomes independent of and ordering m k T / E does no t im ply

    ordering in the integral equation for A{x , k^, can be approxim ated by the B FK L equation. However, a t m oderate x, kr ordering is im plied and the D G LA P equation for the in tegrated gluon d istribu tion g[x^ Q^)is recovered. Cross sections

    can then be calculated according to the kr factorisation theorem by convoluting the un in teg rated gluon density w ith the off-shell boson gluon fusion m a trix elem ent, d,

    cr = y* dk^dXgA{xg, kT^Q) î'y*9* ^ (2.22)

    2.3 P h oton structure

    T he DIS cross section, given in E quation (2.9), is dom inated by the exchange of

    very low v irtuality photons. The lifetim e of these photons varies as ^E^jQ^ which

    a t very low virtualities can be long com pared to th e characteristic tim e of the hard

    subprocess. The electron beam can then be considered a source of approxim ately

    massless, collinear, photons and an ep collider effectively becomes a 7 p collider. The

    to ta l cross section, .y(p) which is the probability of finding a

    photon w ith energy E^ = yE^ inside th e electron. In the lim it -4- 0, the photons

    can only be transversely polarised, and to a good approxim ation

    (2.23)

    where the photon flux is Q^), is given by

    36

  • Chapter 2 2.3 Photon structure

    ^ 220DL98

    ALLM97

    PDG96180 -

    140

    200

    100

    170

    200 210 220

    100

    Figure 2.6: The total photon-pj'oton cross section.

    1 + (1 - v Y _ c ^ - y Q 2rnin (2.24)

    where = rjLjy'^/{l — y) is the kiiieniatic lower bound. This is known as theequivalent photon approxim ation (EPA). Neglecting the Q' ̂ dependence of the 7 p

    interaction and integrating over photon virtualities from the lower kinem atic lim it

    to some m axim um , , yields

    a 1 + (1 - _ 2 -̂ ~ 1 - Q2m in (2.25)

    ^ z/ \ Q L

    which is the W eizsacker-Williams approxim ation (WWA) [21].

    Figure 2.6 shows a/JJ measured a t HERA together w ith the results from low energy

    experim ents [21]. The shape strongly resembles th a t of rneson-nucleon scattering

    and can be described using the same models. Here, bo th photon and proton

    behave as objects with spatial extent. These types of events are term ed “soft”

    photoproduction. At larger m om entum transfers, high transverse m om entum je ts

    of hadrons are produced, and the meson-nucleon model of scattering is no longer

    able to explain the observed final state. It can however be explained in term s

    of parton-parton scattering, where the partons which collide to produce je ts of

    hadrons are considered to be point-like. These types of events are term ed “hard”

    photoproduction and will now be discussed in more detail.

    37

  • Chapter 2 2.3 Photon structure

    (a) (b) (c)

    (d) _ (e) , (f)

    Figure 2.7: Examples of leading-order processes resulting in two jets; (a) QCD Compton, (h) boson gluon fusion, (c) flavour excitation from the proton, (d) gluon gluon fusion, (e) and (f) ft,avour excitation from the photon.

    2.3.1 Hard photoproduction

    At leading-order, hard photoprodiiction processes, such as those in Figure 2.7, can

    he s])lit into two classes; “d irect” , where the photon takes part directly in the hard

    scatter (Figures 2.7(a)-(c)), and “resolved” , where a parton from the photon takes

    part in the hard scatter (Figures 2.7(d)-(f)) and the scatter can be viewed as having

    resolved the structu re of the photon.

    These two classes of events can be separated based on the knowledge of the fraction

    of the photon’s m om entum participating in the hard scatter, x^. For the LO QCD

    diagram s shown in Figure 2.7, energy and m om entum conservation yield

    E m p a r i o n s _ ^ p a r t o n 3partons T ^

    “ 2yE, '

    where yEf, is the initial photon energy. For direct events, this is one and for resolved

    events it is less than one. By summing over je ts instead of partons can be

    translated into an experim entally m easurable ciuantity, , and Equation (2.26)

    becomes:

    y.obs _ C ^ je ts T _________ 0 7 ^

    “ 2 ,/E , ’

    38

  • Chapter 2 2.3 Photon structure

    ZEUS 19942000

    > 1750

    1500

    1250

    1000

    750

    500

    resolved direct250

    Figure 2.8: The distribution in dijet events for data (black dots) compared with HERWIG with and without MPI (solid line and dotted line), and PYTHIA with MPI (dashed line) Monte Carlo generators.

    where the sum runs over the two highest transverse energy je ts and is the

    fraction of the pho ton ’s m om entum entering the d ijet system.

    The ability to separate direct and resolved events using 2;°̂ ̂ was dem onstrated

    in [22]. F igure 2.8 shows the the m easured d istribu tion together w ith the

    predictions of two LO M onte C arlo’s. D irect events (filled histogram ) are strongly

    peaked a t x̂ ^̂ > 0.75 and the resolved a t x°̂ ̂ < 0.75.

    Beyond leading-order th e separation between direct and resolved is am biguous; the

    processes in Figures 2.7(d) and (e), classed as the resolved production of two je ts a t

    LO could be considered as the direct production of th ree je ts a t NLO. The term s

    direct and resolved are then only defined a t leading-order, beyond th is they depend

    on the factorisation scale and can thus have no physical m eaning. T he definition

    of , however, is valid a t all orders and it rem ains a powerful too l to identify

    “photon struc tu re like” effects.

    2.3.2 Photon structure functions

    The struc tu re of the photon is measured directly in deep inelastic 0 7 sca ttering [23],

    shown in Figure 2.9, which is form ally analogous to deep inelastic ep scattering. The

    cross section for a probing photon, virtuality, = —q ,̂ scattering off a real ta rg e t

    39

  • Chapter 2 2.3 Photon structure

    %

    10 10 10 10Q- ((;eV-)

    Figure 2.9: Feynman diagram for ê y diagram with a virtual photon, j* , probing an on-shell photon, 7 (left). Summary of current results on jRj (right).

    photon w ith virtuality^ ^ 0 producing a final s ta te e X is given by,

    ^ [ ( 1 + (1 - VŸ) m - , Q^) - y ^ m - , Q ')] (2 .2 8 )

    As in ep scattering the s tru c tu re function can be w ritten in term s of the parton

    densities

    F i ( ï , = 2 ï y ] e]qj{x, Q^), (2.29)

    where the sum runs over all quark flavours, i, of charge and the factor of

    two accounts for quarks and anti-quarks. These p arton densities obey a set of

    inhom ogeneous evolution equations [24]:

    dqj{x,Q'^) . X 0 5̂(Q^) fdlogQ^ ^ ^ 2tt J y

    (2.30)

    d g (x ,Q ‘̂ ) as {Q ‘̂ ) f d^

    ydlogQ ' 27T+ Pgg 9{y,Q^) (2.31)

    '^This is the nomenclature used in two-photon interactions at LEP. Unfortunately, at HERA, denotes the virtuality of the probed photon and the scale of the probing interaction is ~ Thus, to go from LEP to HERA nomenclature, -> and Q ^ .

    40

  • Chapter 2 2.4 Virtual photon structure

    where

    a{x) = 3e^— \x ̂ + (1 — x)^] . (2.32)

    These are the s tandard D GLA P evolution equations, e.g. for th e pro ton , except for

    the so-called anom alous term , a(x), which comes from branchings 7 —)■ qq, and is

    unique to the photon evolution equations. The solution can be w ritten as th e sum

    of two term s [25],

    Q') = Q'; QD + Q'; Q l ) (2.33)

    where a = fqi{x,Q^) = qi{x,Q‘̂) and /g (x ,Q ^) = g{x,Q^). T he first term is a solution to the homogeneous equation w ith a non-pertu rbative inpu t at Q = Qo, and the second is a solution to the full inhom ogeneous equation w ith the boundary

    condition f]'^'^{x,Ql-,Ql) = 0. One possible physics in terp re ta tion is to let

    correspond to 7 -4- V fluctuations, where V = J /^ ; , . . . is a set of vector

    mesons, ( “vector meson dom inance” ), and let correspond to pertu rba tive

    J ^ qq fluctuations, q = u , d , s , c and b ( “anom alous” ). T he discrete spectrum

    of vector mesons can be combined w ith the continuous (in v irtua lity spectrum

    of qq fluctuations to give

    2

    /2(^,Q ") = E Q ' ; Q o ) + ^ E 24 [ ^ / a ' ” (x ,Q ';k^) (2.34)y I v i-K ̂ J kVo

    where each com ponent, and obeys a un it m om entum sum rule.

    There are currently a large num ber of photon p arton density param eterisa tions

    and usually involve some fits to data . W ith the large errors on additional

    assum ptions need to be made. These assum ptions differ in different m odels and

    involve the trea tm en t of heavy quarks, the choice of the scale Q l and the m ethods

    of deciding the form of the inpu t densities.

    2.4 V irtual p hoton structure

    The evolution equations (in Q^) of the PD F s of the v irtual photon can be exactly

    calculated in pertu rba tive QCD for th e restric ted range Q l Q^.

    41

  • Chapter 2 2.4 Virtual photon structure

    d^O / dx°®® d o ' d f g p ' fp jb /G e V ^ ;(E j)^ G tV ')= 49-85 ^ 85-150

    •ZEUS 96/97 y’p— SaS ID (HERWIG 5.9)— GRV LO (HERWIG 5.9)

    5

    §?

    §

    • 96/97 ZEUS Preliminary

    Figure 2.10: Triple differential cross section d^a/dx^^^dQ^dEj^ as a function of

    for different regions in and E^(left). The ratio of cross sections R = < 0.75)/cr(T°^ > 0.75) as a function of (right).

    Theoretically challenging, however, is the region ^ ^ Q o where evolution

    equations cannot be derived from pertu rba tive QCD.

    In [26] PD Fs th a t are valid for all 0 < were proposed and a generalised

    form of Equation (2.34) given:

    +

    V

    a em27T Y.Hj

    dE“p2 VA;2 + p 2 (2.35)

    Ql

    T his extension of real-photon P D Fs to those of the v irtual photon can be applied

    to any set of parton d istribu tions, provided th a t the VMD and anom alous p arts are

    available separately.

    2.4.1 Experimental review

    M easurem ents of the v irtua l photon struc tu re in tw o-photon in teractions require

    the detection of bo th scattered leptons a t non-zero scattering angles. This was first

    done by the PLU TO collaboration in 1984 [27] and, more recently, by L3 [28] and

    OPAL [29]. However, all these analyses suffer from low statistics. T he extensive

    42

  • Chapter 2 2.5 Heavy flavour production

    range, together w ith the large centre-of-mass energies, available a t HERA enable

    m ore detailed studies of the evolution of photon struc tu re [30-32].

    Two recent results from ZEUS are shown in Figure 2 .1 0 . T he m easured trip le

    differential dijet cross sections (Pa/dx^^^dQ‘̂ dE^ are shown as a function of in

    different bins of and E^. For each bin, the cross section in the low region

    falls faster w ith increasing th a n the cross section in the high region. For

    the bins w ith > Ej, the d a ta are well described by the HERW IG predictions

    including only LO direct processes. In the bins w ith < E^ LO direct processes

    alone are not enough to describe the data.

    The faster fall of the low region can be seen more clearly in the ra tio of

    cross sections R = < 0. 75) / a > 0.75). The ra tio of the d a ta falls

    w ith increasing Q'̂ . The HERW IG prediction, using the suppressed v irtual photon

    s truc tu re function SaSlD [25], also falls w ith increasing and describes the shape

    b u t no t the norm alisation of the ra tio (requiring a norm alisation factor of 1.3).

    2.5 H eavy flavour production

    The conventional QCD parton m odel is form ulated in the zero m ass parton lim it.

    T here are two basic m ethods of trea tin g charm in the evolution equations based on

    the factorisation equation [33]

    a^ ^ x{S ,Q ^ ) = Y^qi{x, i i^) (2.36)i

    where i is the sum over all flavours which can actively partic ipa te in the in teraction

    a t th e energy scale Q^. â is the cross section for th e hard scatter which

    is convoluted w ith the parton d istribu tion functions qi{x,fi^) where fi is the

    factorisation scale. C harm can then either be included in the sum as an active

    flavour above some threshold (variable flavour num ber (YEN)) or excluded from

    the in itia l s ta te and trea ted separately (fixed flavour num ber (F F N )). In principal,

    the two alternatives can be regarded as two different bu t equivalent schemes for

    organising the pertu rba tion series in pQCD. In practice, since the p e rtu rb a tio n series

    is te rm inated after one or two term s, the effectiveness of the two approaches can be

    quite different in different kinem atic regions. For a full review of the theoretical and

    experim ental s ta tu s of heavy flavour production see, for exam ple, [34] and references

    therein.

    43

  • Chapter 2 2.5 Heavy flavour production

    M a ss iv e F F N 3 sc h e m e

    In th is scheme, the num ber of active quark flavours is fixed, independent of Q^. Only

    light quarks (u, d, s) are included in the in itia l s ta te pro ton and photon and charm

    quarks are only produced dynam ically in the hard process. T he presence of th e two

    large scales^, (j? and m^, can spoil the convergence of the pertu rba tive series because

    the neglected term s of orders higher than contain log(//^/m ^) factors th a t can

    become large. Therefore the results of massive FFN 3 calculations are expected to

    be m ost accurate a t /i^ ~ and to become less reliable when ^ m^.

    M a ss le s s V F N sc h e m e

    In this scheme, charm is trea ted as an additional active flavour w ith zero mass above

    some threshold, ~ In th is way, the large logarithm s in present a t high

    fl are au tom atically resum m ed. This m eans th a t besides charm produced in the

    hard process flavour excitation processes are also included. Therefore the results of

    massless V FN calculations are expected to be m ost accurate a t ^ m l and to

    become less reliable when

    2.5.1 Experimental review

    D e e p in e la s t ic s c a t te r in g

    Early studies of charm production in DIS [35] suggested th a t the p roduction of

    charm ed mesons in ep collisions is dom inated by the boson gluon fusion (BG F)

    mechanism, already shown in Figure 2.7(c). C alculations for th is process exist to

    NLO and the cross section depends directly on th e gluon density in the proton. If

    the gluon density from the inclusive m easurem ent of F2 are used in the calculation,

    the results can be com pared to the m easured charm cross section, giving a powerful

    cross check of pQ CD which states th a t the same, universal, gluon d istribu tion should

    contribute to bo th the inclusive structu re function F 2 , and the exclusive charm

    struc tu re function In addition, the presence of two large scales, namely, the

    v irtuality of the exchanged boson {Q^) and the square of the charm quark mass

    {ml), provides a testing ground for resum m ation techniques. F igure 2 .1 1 show the

    differential D* cross sections m easured a t ZEUS com pared to a massive FFN 3 NLO

    calculation [36] which uses the gluon density ex tracted from fits to F2 as input.

    The description of the Q^, x and W d istribu tions is very good, confirm ing the

    ^In DIS fjL is the photon virtuality, Q , in photoproduction it is p r -

    44

  • Chapter 2 2.5 Heavy flavour production

    ZEUS 1996-97

    SJ) 1b

    ZE U S 1 9 9 6 - 9 7

    log,„x

    P t ( D ') (GeV) 77(D-)

    W(GeV)

    I , = 0.00005(x 4*)

    . i- 0.00013(x 4’)

    J 0.00030(x 4')

    0.00050(x 4‘)

    0.00080(x 4*)

    0 .00120(x 4’)

    r^ '0.00200(x4")

    ^ 0.00400(x 4')

    0 .00800(x4’)

    ^ ZEUS NLO QCD0.02000(x4°)

    (GeV̂)Figure 2.11: Differential cross sections for D* production in DIS. The open (shaded) band shows the result of an NLO QCD calculation using Peterson (R A P G A P extracted) fragmentation (left). as a function of x and (right).

    universality of the gluon d istribu tion . However, in order to describe the p t {D *) and

    t]{D*) d istribu tions it was necessary to use a charm fragm entation ex tracted from

    the LO M onte Carlo R A PG A P. W ith th is fragm entation included the description

    is good enough to be used to ex trapo la te the m easurem ent into the full D* phase

    space and ex tract The m easured Fff ̂ is com pared to the value derived from the

    gluon d istribu tion extracted from NLO fits to F2 in Figure 2 .1 1 .

    Photoproduction

    NLO calculations for the pho toproduction of heavy quarks such as charm also exist,

    where the heavy quark m ass or the high transverse m om entum of the produced

    partons is used as the hard scale. Significant differences between calculation

    schemes can be expected since massless V FN calculations will include charm

    excitation processes and thus predict, for a given factorisation scale, a larger

    resolved com ponent in com parison w ith a massive FFN 3 calculation. Therefore, it

    is interesting to com pare the predictions of these models to d a ta and to investigate

    th e sensitivity of the experim ental results to the partonic content of the photon and

    specifically to the charm excitation contribution.

    Figure 2.12 shows the differential cross section da/dp^* for various ranges of pt

    m easured a t ZEUS com pared to bo th massive and massless calculations [37]. As

    expected as p r —̂ me the description of the d a ta by th e massless calculation

    degrades. However, the NLO predictions generally lie below the d a ta , particu larly

    45

  • Chapter 2 2.5 Heavy flavour production

    Z E U S 1 9 9 6 + 9 7 ZEUS 1996+97(a)p^D ->2G eV

    V • D -» {K n) \ Massive, e *

    Massive, )ip = 0.5 m ., aa

    I 10

    n

    (b) p^D- > 3 GeV

    (upper)

    S 5

    — Herwig: direct + resolved r/XJ Herwig: direct

    Herwig: resolved Herwig: resolved without

    (d) Pĵ D- > 6 GeV(c) Pĵ D- > 4 GeV • D -> (K n) ÏI, D D -» (Kirmi); f

    QT

    ■D

    (b)

    Massive NLO, parlon level, e- 0.02

    — p„ = 1.0 m , riij = 1.5 GeV

    - -- = 0.5 m^, = 1.2 GeV

    Figure 2.12: The differential cross section da/drj^* for photoproduction compared to several NLO calculations (left). The differential cross section da/dxf^^ for dijets with an associated D* (right) compared to LO (upper) and NLO (lower) predictions.

    in the forward region, in all the plots. Given the discrepancy between d a ta and

    NLO predictions in the inclusive D* m easurem ents it is im po rtan t to study the

    kinem atics of charm production in more detail. This was done in the sam e paper by

    m easuring the dijet cross section as a function of , also shown in Figure 2.12.

    A t LO the d a ta require a resolved contribution of 45%, th is com pares to 75% for

    th e cross section of Figure 2.8 which did not require the presence of a D*. The

    charm excitation contribution to the LO resolved process was 93% in the M onte

    Carlo. The prediction of a massive NLO calculation, lies significantly below the

    d a ta for < 0.75, however a massless calculation could be expected to give a

    b e tte r description.

    46

  • Chapter 3

    K inem atic reconstruction

    T he event and je t kinem atics m ust be reconstructed from m easured quantities. The

    m ethods used for the reconstruction of the event variables in th is thesis are now

    described.

    3 .1 R e c o n s t r u c t io n o f y a n d

    T here are m any ways of reconstructing the variables y and [38], two of which are

    used in th is thesis; the “electron” and “Jacquet-B londel” m ethods.

    3.1.1 Electron m ethod

    T h e electron m ethod is theoretically simple and relies only on the knowledge of

    th e energy of the scattered lepton, E' ̂ and the angle of the scatter, 6e- For a given

    in itia l lepton energy, Eg, th e variables, y and can be calculated from the scattered

    le p to n ’s energy E' ̂ and polar angle 6e as follows;

    He = ̂ (1 — cosOe) , (3.1)

    + (3.2)

    T h is assumes th a t there were no additional emissions from the lepton, i.e. th a t it

    en tered the hard scatter w ith the beam energy Eg and it left w ith the m easured

    energy E ' and as a result is sensitive to bo th initial- and final-state electroweak

    rad ia tiv e corrections (ISR and FSR).

    47

  • Chapter 3 3.2 Jet reconstruction

    3.1.2 Jacquet-Blondel method

    T he Jacquet-B londel m ethod [39] calculates the variables y and from the hadronic final s ta te and can thus be used when the scattered lepton is not measured. The hadronic final s ta te is defined as all particles except th e scattered lepton and sum m ing over these gives:

    (3.3)

    + (3.4)1 - yjB

    E xperim entally this sum is not over hadrons b u t calorim eter cells. If the scattered lepton is found in the calorim eter, then the cluster of cells associated w ith it are elim inated from the calculation. If the scattered lepton is m isidentified its energy deposit will enter into the above sum m ations. This results in high values of ?/jb , allowing events w ith an unidentified electron to be rejected.

    Since th is m ethod measures the energy transferred to the hadronic system , it is unaffected by FSR, however it will still be sensitive to ISR th rough Eg.

    R esolutions

    T he resolutions on y and using the two m ethods described above are shown in F igure 3.1. The resolution is significantly worse using th e Jacquet Blondel m ethod. This is a result of energy lost due to dead m ateria l and acceptance. As a result, Q jg is only used in high-Q^ events when there is no scattered electron, i.e. charged current DIS. Thus, when an electron is present in an event the electron m ethod has been used to reconstruct Q^. W hen there is no identified lepton, is restric ted to be below 1 GeV^ by means of an an ti-tag requirem ent (see Section

    4.3).

    T he y resolution is again b e tte r using the electron m ethod, and there is a system atic bias in the m easurem ent of yjB due to energy loss in dead m ateria l before the GAL. However, in order to be consistent a t different regions, yjB is used for the estim ate of y w hether or not an electron is found.

    3.2 Jet reconstruction

    There are two types of je t algorithm in com m on use; the “cone” and “cluster” algorithm s. In the analysis presented in th is thesis bo th types of algorithm are

    48

  • Chapter 3 3.2 Jet reconstruction

    1400800700600500400300200100

    1200

    1000

    800

    600

    400

    200

    - 0.3 - 0.25 0.250.3 0

    20001750150012501000750500250

    100045040035030025020015010050

    800

    600

    400

    200

    1 1 - 0.4 0 0.4 - 0.4 0.40

    Figure 3.1: y and resolutions using the electron and Jacquet Blondel methods.

    used. The EU CELL cone algorithm is used in the online trigger selection, described

    in Section 4.2, and the KTCLUS [40] algorithm is used in the offline selection,

    described in Section 4.3, and the cross section definition of Section 4.1.

    D etailed discussions of each of these can be found elsewhere [41], so only a brief

    description is included here.

    3.2.1 Cone algorithm

    The Snowmass Convention [42] for cone algorithm s defines th e transverse energy

    and the coordinates of a cone je t as;

    i

    (3,5)

    T i

    49

  • Chapter 3 3.2 Jet reconstruction

    where the sum runs over all hadron or calorim eter cells w ith in the cone defined by

    a given prescribed radius, i?, in 77 — ^ space.

    In EUCELL, the hadrons/cells are clustered using a grid in 77 — ^ space. The size of the cell