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April 2004 Ivo van Vulpen 1 Moriond Calo r LSP LSB Ivo van Vulpen

April 2004Ivo van Vulpen 1 MoriondCalor LSPLSB Ivo van Vulpen

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Page 1: April 2004Ivo van Vulpen 1 MoriondCalor LSPLSB Ivo van Vulpen

April 2004 Ivo van Vulpen 1

MoriondCalor

LSPLSB

Ivo van Vulpen

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April 2004 Ivo van Vulpen 2

Introduction:

Moriond (Electroweak)

La Thuile

Calorimetry 2004

Perugia

Real ‘hardware’ conference.

Real ‘physics’ conference

Disclaimer:

Most of the sheets are taken directly from the talks given at Moriond.

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April 2004 Ivo van Vulpen 3

Small and very nice conference, but still: 90 talks !

EW results & precision measurements

Searches and SUSY

Dark matter

Large extra dimensions

Neutrinos

B-physics

Theory:

Experiment:

Discovery of new particles Discovery claim

What is happening

top quark mass, g-2, s in2(w)

Babar & Bell + frustrating sheet

Higgs at Tevatron

Penta-quarks

why and how can we seen it

TALK

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top quark

8 sheets

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Top quark production

(tt) 8 pb

gqq t

tWb

Wb

W->qq (2/3) and lv (1/3)

WWbb

production

Final states

bb qqqq

bb qqlv

bb lvlv Large QCD background

Di-lepton. small statistics

lepton + jets. Most sensitive

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Tevatron run 2: CDF

di-lepton

6 events (0.5 background)

Lepton + jets

22 events (6 background)

126/102 pb-

1

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Tevatron run 2: D0

“First we have something to say on our run 1 result.”

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New D0 analysis technique:

Tevatron run 1: D0

Use only 4 jet (clean) events (22 events instead of 77 previously) & all combinations

i i

ii

i ii m

nm

m1

of instead 1

1

m 2

2

Basically same as difference between:

Can it be so important ??

Compute event-by-event probabilityMatch measured 4-momenta to

expectations for signal (mtop = 170,175,180 etc) and background.

YES!!

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GeV (syst) 5.5(stat) 5.6173.3m top 91 events22 events

D0 l+jets (old)

GeV (syst) 3.9(stat) 3.6180.1m top (new)

As if you had 2.4 times more dataMtop moves up by 7

GeV !!!

Tevatron run 1: D0

Improvement in statistical error is roughly 1.5 (comparable to 2.4 times more data)

wow !!

SAME DATA

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New top quark mass averages

RUN2 (l+jets) GeV 6.2177.8m 4.55.0-top

GeV 4.3178.0m top

GeV 5.1174.3m top TEVATRON RUN1 (old)

RUN1 (new)Mtop moves up by +4.7 GeV

D0 lepton + jets

Influence on rest of EW physics results

Tevatron

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Another example: Influence new top mass on tan() exclusion region from LEP:

In MSSM benchmarks: mtop = 175 GeV

mh

LEP-excluded tan() region will shrink

mh-max benchmark scenario

FeynHiggs:

Computation of mh-max:

Loop corrections m4top

higher order corr. -> mh 3 GeV mtop 5 GeV -> mh 5

GeV

Maximum mh: in the MSSM 135 GeV

hZ

hA

Scenario mh mA Excluded tan()

Mh-max >91.0 >91.9 0.5 < tan() < 2.4

LEP

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Impact new top mass on the electroweak fit

Old (new): mh = 96 (117) GeV mh < 219 (251) GeV @ 95% CL

new

old

mh

)ln(2htM mm

W

Example: W mass. contributions from:

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April 2004 Ivo van Vulpen 13

Electroweak

g-2

4 sheets

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“Compare to SM prediction: there is a 1.4/2.7 sigma deviation”

Anomalous magnetic moment of the muon

g-2 collaboration final results

Depends on e+e- data or tau data

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Theoretical computation of a [ (g-2)/2] part (1)

(1) light by light scattering: theory!

Tedious work. Done by 1 guy basically.

Sign flip found in 2002 (PhD student from Marseille ??)

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(2) Hadronic vacuum polarization: experiment (2 ways to extract it)

Cannot be calculated

(1) CMD: e+e- results:

Claim 0.6% uncertainty, but new rad corr shifted cross section by 3%

Region < 1.8 GeV dominates

They were alone (check needed)

Now confirmed by KLOE (radiative events). Maybe BaBar and Cleo can do something as well

1

(2) Tau decay Gives different e+e- -> hadrons

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FINAL

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w2sin

Electroweak

4 sheets

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E = 48 GeV, Q2 = 0.03 GeV2

tree level: -3 •10-7

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Still the old NuTeV ‘discrepancy’

APV = -160 21 17

Significance of parity non-conservation is 6.3 sigma !!

Translate to sin2(w)

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clean events

neutrino–nucleus deep inelastic scattering

probe strange sea

hadronsnucleus

v and anti-v beam

Measure sin2 W through NC CC cross section ratio:

NuTeV:

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Extracting sin2(W) from DIS cross sections:

RwR 2sin2

1

More precise corrections:

(1) Z protons and N neutrons

(3) Fermi-motion and nucleair binding effects from target

(10 x experimental error)

(sin2(W)) = - 0.5 NuTeV (towards SM

value)

NuTeV shifts towards SM value (almost 1 sigma) !

Nuclear effects due to target corrections

(2) QCD radiative corrections

(sin2(W)) = - 0.5 NuTeV (towards SM

value)

new

new

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4 sheets

B-physics

Babar/Belle

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2 odd things

BABAR and Belle attacking the CKM matrix from all sides

CP violation in B0->+-

Belle B->Ks 3.5 deviation from SM

Do they agree on everything ??

Are there anomalies left ??

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Difference between J/Difference between J/KKss and and KKss

Bb

d

W

ss

sg

Kd

b

d

d

Wcc

s

0B /J

0K

NP contributions to B0 Ks penguin can result in

sin(2)J/Ks sin(2)Ks

B0 Ks penguin diagram

Babar : sin(2)J/Ks=0.730.06

: sin(2)Ks= 0.50.5

Belle : sin(2)Ks=-1.00.6

Jeroen van Hunen (NIKHEF)Belle B->Ks 3.5 deviation from SM

sin(2)

sin(2)

Old numbers

Diff !

asy

mm

etr

y

t decay time between tag-B and decay-B

SM exp

Measured

3.5

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CP violation in B0->+-

Fit asymmetry to: )sin()()cos()()( tmtStmtAtACP

No CP violation

Excluded at 5.2

time

time

SUMMARY (BABAR/Belle): doing well, some mysteries left.

For no B,B0 and B0 decays no CP –violation is observed (except Belle in B0->+-)

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Most frustrating slide in the conference !!

Quite a few talks on theoretical aspects of rare B decays as well.

D0

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Higgs

1 sheet

Tevatron running&

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Nothing new on the Higgs front & SUSY searches (updates from HERA, LEP, Tevatron)

Tevatron accelerator review:

4.4 fb-1 at FY 09 feasible

8.5 fb-1 at FY 09 very challenging

SM cross section

Excluded cross section

Tevatron operation

started bad, now ok

20042003

2002

Higgs cross section exclusion

Expected Higgs boson mass exclusion

Factor 50

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4 sheets

Penta-quarks

other new patricles

&

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New particle

‘New’ particles are discovered all the time:

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New particle

Could have seen it in Run1 I guess. Now studying decay properties. Seems like charmonium state.

charmonium

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K+n-invariant mass

Trying to understand the structure

Pentaquarks: + and --

Penta-quark

New particle

m+ 1542 5 1592 50

Exp. Theory (3+2)

m--

1862 5 1720 50

P-wave

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New particle

Penta-quark

A 3rd penta-quark ?? (NA49)

(1860)

Not confirmed by CDF

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5 sheets

Extra dimensions

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e.g. Randall-Sundrum Models

Apparently I was not the only one who was surprised !

prior reality

Many theory talks on this subject, a hot topic

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Tevatron (direct) and LEP (indirect)

Depend on size dimension(like harmonic oscillator

boundary conditions)

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11 sheets

Dark matter

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Dark matter/energy

Dark matter halo around galaxies

What is dark matter ??AxionWIMP (SUSY stable LSP, 1

0)

matter > baryon --> Non baryonic dark

mattertotal > matter --> Dark Energy

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Assume WIMP = SUSY stable LSPDetecting WIMPS (1)

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Detecting WIMPS (2)

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WIMPS

Sensitive underground detectors, but need large (mass * exposure time)

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WIMPS

DAMA & Edelweiss

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DAMA at Moriond

WIMPS

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DAMA at MoriondDAMA at CALOR

Talks from DAMA 95% the same:

They see something !!

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EDELWEISS-I (Frejus, inonization-heat measurement, small)

Plans: 10-6 pb (now), 10-8 (soon), 10-10 (10 years)

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Axions

8o, so shifts only at sunrise(set)

2005: Probe higher axion masses

Interact with magnetic field (B2L2) and produce X-rays (a-> )

L=10 m, B = 9T

100 times more a-> conversions

X ray telescope.

(fill magnet with helium)

can be produced in the sun.

LHC magnet than any other experiment

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Other underground experiments: proton decay

Explore lifetimes > 1035

yearsAmbitious:

100,000,000 kg liquid argon

74 sheets in 30 minutes

Rubbia

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7 sheet

Neutrinos

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Mass eigenstates are mixture of flavour eigenstates (a la CKM matrix)

massPMNSflavour U ||

Atmospheric

Solar (KAMLAND)Reactor (CHOOZ)

If 13 0 --> CP-violation

2-3 mixing

1-3 mixing

1-2 mixing

massCKMflavour qUq ||

Superkamiokande

(m23)2 = 2-3 eV2 23

= 45o

(m13)2 = ?? (m12)2 = 5-7 eV2

How do we probe the neutrino sector of the SM:

MNS = Maki-Nakagawa-Sakata

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Super Kamiokande

Is disappearance really caused by oscillations ??

3.5sigma disfavored

2 allowed regions are compatible

Do they really oscillate ??

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KARMEN excludes part of it

(confirmation needed): --> miniBOONE

Close to 4 Are there 3 families ??

Sterile neutrinos

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miniBOONE energy spectrum requires more precise cross section data

miniBOONE will cross-check LSND result

Depends on Tevatron programme

Use identical targets at HARP

Sensitivity nmu->ne

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What about the absolute mass scale and hierarchy ??We only know mass differences squared (m2)

n -> p + e- + v

m3

m2m

1 ?m3

m1

m2

Lepton number violation

Neutrinoless double beta decay

Klapdor-Kleingrothaus

hep-ph/0201231

Radon down factor 10

NEMO:

Page 60: April 2004Ivo van Vulpen 1 MoriondCalor LSPLSB Ivo van Vulpen

ciao

I will leave CERN on the 1st of June

NL

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