Upload
britton-ford
View
216
Download
0
Tags:
Embed Size (px)
Citation preview
University of Massachusetts AmherstChristine A. Aidala
April 12, 2008
Peering into Hadronic Matter:The Electron-Ion Collider
Winter Workshop on Nuclear Dynamics
C. Aidala, WWND, April 12, 2008 2
The EIC: Communities Coming Together
• At RHIC, heavy ions and nucleon spin structure already meet, but in some sense by “chance”– Genuinely different physics
– Communities come from different backgrounds
– Bound by an accelerator that has capabilities relevant to both
• The proposed EIC a facility where HI and nucleon structure communities truly come together, peering into various forms of hadronic matter to uncover the secrets the QCD Lagrangian doesn’t reveal . . .
C. Aidala, WWND, April 12, 2008 3
aaa
aQCD GGAqTqgqmiqL4
1)()(
QCD: Confounded Confinement!
– Salient features of QCD not evident from Lagrangian!• Asymptotic Freedom & Color Confinement
• Due largely to non-perturbative structure of QCD vacuum
– Gluons: mediator of the strong interactions• Determine essential features of strong interactions
• Dominate structure of QCD vacuum (fluctuations in gluon fields)
• Responsible for > 98% of the visible mass in universe(!)
QCD requires fundamental investigation
via experiment
C. Aidala, WWND, April 12, 2008 4
Goals & Key Questions• Explore the new QCD frontier: strong color
fields in nuclei– How do the gluons contribute to the structure of the
nucleus? – What are the properties of high-density gluon matter?– How do fast quarks or gluons interact as they traverse
nuclear matter?
• Precisely image the sea quarks and gluons in the nucleon
– How do the gluons and sea quarks contribute to the spin structure of the nucleon?
– What is the spatial distribution of the gluons and sea quarks in the nucleon?
– How do hadronic final states form in QCD?
How do we understand the visible matter in our universe in terms of the fundamental quarks
and gluons of QCD?
C. Aidala, WWND, April 12, 2008 5
Deep-Inelastic Scattering: A Tool of the Trade in Probing
the Partons within Nucleons/Nuclei
• Probe nucleon with an electron or muon beam• Interacts electromagnetically with (charged) quarks
and antiquarks• “Clean” process theoretically—quantum
electrodynamics well understood and easy to calculate!
C. Aidala, WWND, April 12, 2008 6
DIS Kinematic Variables
Deep Inelastic Scattering:
e
ee
E
EEy
'
Measure of momentum fraction of struck quark
Measure of inelasticity
“Perfect” Tomography
Measure of resolution power:~1/wavelength2
222 )( kkqQ
pq
Qx
2
2
Inclusive DIS: Measure only energy and scattering angle of outgoing eSemi-inclusive DIS: Measure outgoing e & some final-state hadrons
Exclusive DIS: Measure entire final state
“Bjorken x”
C. Aidala, WWND, April 12, 2008 7
Goals & Key Questions• Explore the new QCD frontier: strong color
fields in nuclei– How do the gluons contribute to the structure of the
nucleus? – What are the properties of high-density gluon matter?– How do fast quarks or gluons interact as they traverse
nuclear matter?
• Precisely image the sea quarks and gluons in the nucleon
– How do the gluons and sea quarks contribute to the spin structure of the nucleon?
– What is the spatial distribution of the gluons and sea quarks in the nucleon?
– How do hadronic final states form in QCD?
Investigate using the tools of deep-inelastic scattering
at high energies:An Electron-Ion Collider
C. Aidala, WWND, April 12, 2008 8
Goals & Key Questions• Explore the new QCD frontier: strong color
fields in nuclei– How do the gluons contribute to the structure of the
nucleus? – What are the properties of high-density gluon matter?– How do fast quarks or gluons interact as they traverse
nuclear matter?
• Precisely image the sea quarks and gluons in the nucleon
– How do the gluons and sea quarks contribute to the spin structure of the nucleon?
– What is the spatial distribution of the gluons and sea quarks in the nucleon?
– How do hadronic final states form in QCD?
C. Aidala, WWND, April 12, 2008 9
What Do We Know About Glue in Matter?
),(2
),(2
14
:DIS 22
22
2
4
2..
2
2
QxFy
QxFy
yxQdxdQ
dL
meeXep
Access the gluons in DIS via scaling violations:
dF2/dlnQ2 and linear DGLAP evolution in Q2
G(x,Q2)
Gluons dominate low-x wave function
)201( xG
)201( xS
vxu
vxd
!
C. Aidala, WWND, April 12, 2008 10
Other Handles on the Gluon
Gluon distribution G(x,Q2)– Shown here:
• Scaling violation in F2: F2/lnQ2
• FL ~ s G(x,Q2)
– Other Methods:• 2+1 jet rates (needs jet algorithm and modeling of
hadronization for inelastic hadron final states)
• inelastic vector meson production (e.g. J/)
• diffractive vector meson production ~ [G(x,Q2)]2
C. Aidala, WWND, April 12, 2008 11
Limitations of Linear Evolution in QCDEstablished models: • Linear DGLAP evolution
in Q2
• Linear BFKL evolution in x
Linear evolution in Q2 has a built-in high-energy “catastrophe”
• xG rapid rise for decreasing x and violation of unitary bound
must saturate– What’s the underlying
dynamics? Need new approach
C. Aidala, WWND, April 12, 2008 12
Non-Linear QCD - Saturation• Linear BFKL evolution in x
– Explosion of color field as x0??
• New: BK/JIMWLK based models
– introduce non-linear effects saturation
– characterized by a scale Qs(x,A)
– arises naturally in the Color Glass Condensate (CGC) framework
proton
N partons new partons emitted as energy increasescould be emitted off any of the N partons
proton
N partons any 2 partons can recombine into one
Regimes of QCD Wave Function
C. Aidala, WWND, April 12, 2008 13
Scattering of electrons off nuclei:
• Probes interact over distances L ~ (2mN x)-1
• For L > 2 RA ~ 2A1/3 probe cannot distinguish between nucleons in front or back of nucleus
• Probe interacts coherently with all nucleons
e+A: Studying Non-Linear Effects
Nuclear “Oomph” FactorPocket Formula: )(
1/320
2
x
AcQQ s
As
3.03.02
22 :dependence A
1~ : HERA
proton)for 1(
),(~
x
A ~ xG
xxG
R
QxxGQ A
A
sss
Enhancement of QS with A non-linear QCD regime reached at significantly lower energy in heavy nuclei than in proton
C. Aidala, WWND, April 12, 2008 14
Nuclear “Oomph” Factor
More sophisticated analyses Oomph exceeds that of pocket formula (e.g. Armesto et al., PRL 94:022002, Kowalski, Teaney, PRD 68:114005)
)(
)(
:Note
222
222
ssss
sss
QQQ
QQQ
C. Aidala, WWND, April 12, 2008 15
Universality & Geometric ScalingCrucial consequence of non-linear
evolution towards saturation:• Physics invariant along trajectories
parallel to saturation regime (lines of constant gluon occupancy)
• Scale with Q2/Q2s(x) instead of x and Q2
separately
Geometric Scaling• Consequence of saturation
x < 0.01
C. Aidala, WWND, April 12, 2008 16
Qs : A Scale that Binds Them All
Freund et al., hep-ph/0210139
Nuclear shadowing Geometric scaling
Is the wave function of hadrons and nuclei universal at low x?
proton x 5
nuclei
)(/ 22 xQQ S
C. Aidala, WWND, April 12, 2008 17
e+A Landscape and a New Electron-Ion Collider
• Well mapped in ℓ+p
• Not in ℓ+A!– Mostly small A– Low statistics
Much to be learned from an Electron-Ion Collider!
Terra incognita: small-x, Q Qs
high-x, large Q2
C. Aidala, WWND, April 12, 2008 18
),(2
),(2
14 2
22
2
2
4
2
2
2
QxFy
QxFy
yxQdxdQ
dL
eXep
F2 : Sea Quarks Generated by Glue at Low x
F2 will be one of the first measurements at EIC
nDS, EKS, FGS:
pQCD-based models with different amounts of shadowing
Syst. studies of F2(A,x,Q2):• GA(x,Q2) with precision• distinguish among models
C. Aidala, WWND, April 12, 2008 19
FL at EIC: Measuring the Glue Directly
),( 2QxGF sL
),(2
),(2
14 2
22
2
2
4
2
2
2
QxFy
QxFy
yxQdxdQ
dL
eXep
Access by making measurements at fixed x, Q2 for different y
y= Q2/xs
Scan in !
GA(x,Q2) with great precision
s
C. Aidala, WWND, April 12, 2008 20
Connection to RHIC & LHC Physics
Matter at RHIC– Thermalizes fast ( ~ 0.6 fm/c)
– We don’t know why and how
– Initial conditions? G(x, Q2)
Role of saturation?– RHIC → forward region
– LHC → midrapidity
• bulk (low-pT matter) & semi-hard jets
Jet Quenching:– Need Reference: E-loss in cold matter
– No HERMES data for
• charm energy loss
• in LHC energy range
RHICLHC
EIC provides essential new input:• Precise handle on x, Q2
• Means to study exclusive effects
)(/)( xGxG DPb
C. Aidala, WWND, April 12, 2008 21
Goals & Key Questions• Explore the new QCD frontier: strong color
fields in nuclei– How do the gluons contribute to the structure of the
nucleus? – What are the properties of high-density gluon matter?– How do fast quarks or gluons interact as they traverse
nuclear matter?
• Precisely image the sea quarks and gluons in the nucleon
– How do the gluons and sea quarks contribute to the spin structure of the nucleon?
– What is the spatial distribution of the gluons and sea quarks in the nucleon?
– How do hadronic final states form in QCD?
C. Aidala, WWND, April 12, 2008 22
gS
S
xS > xg ???
A low Q2 puzzle …
50% of Momentum Carried by Gluons … But Still Gluon Puzzles
If sea quarks come from gluon splitting, how can the gluon and sea distributions diverge as they appear to at low Q2??
EIC luminosity 100x > HERA Precision measurements!
C. Aidala, WWND, April 12, 2008 23
Spin Structure of the NucleonQuark spin contribution to the proton spin:
“Spin Crisis”The rest from gluons and orbital angular momentum.
%30
qGLG 2
1
2
1
• Gluon spin contribution, G, still poorly constrained
• Only recent ideas on probing orbital angular momentum!
C. Aidala, WWND, April 12, 2008 24An EIC makes it possible!Region of existing g1p data
World Data on g1pWorld Data on F2
p
Not enough range in x, Q2 to access G via scaling violations
C. Aidala, WWND, April 12, 2008 25
L
R
Observed LargeSingle-Spin Asymmetry
Now confirmed at much higher energies at RHICFermilab E704:
p p X at 400 GeV
Must be due to spin-orbit effects in the proton itself and/or in the fragmentation
process
Spin-Orbit Effects and Transverse Spin
STAR
TkpS
Also access orbital angular momentum and spatial distribution of partons within nucleon via measurements of
Generalized Parton Distributions (GPD’s)- Exclusive measurements
- Possible due to high luminosities, large detector coverage
C. Aidala, WWND, April 12, 2008 26
EIC Status: White Papers 2007• The Electron Ion Collider
White Paper• The GPD/DVCS White
Paper• Position Paper: e+A Physics
at an Electron Ion Collider• The eRHIC machine:
Accelerator Position Paper• ELIC ZDR Draft
Available at:• NSAC LRP2007 home page• Rutgers Town Meeting page• http://www.bnl.gov/eic
C. Aidala, WWND, April 12, 2008 27
The EIC Working Group17C. Aidala, 28E. Aschenauer, 10J. Annand, 1J. Arrington, 26R. Averbeck, 3M. Baker, 26K. Boyle, 28W. Brooks, 28A. Bruell, 19A. Caldwell, 28J.P. Chen, 2R. Choudhury, 10E. Christy, 8B. Cole, 4D. De Florian, 3R. Debbe, 26,24-1A. Deshpande*, 18K. Dow, 26A. Drees, 3J. Dunlop, 2D. Dutta, 7F. Ellinghaus, 28R. Ent, 18R. Fatemi, 18W. Franklin, 28D. Gaskell, 16G. Garvey, 12,24-1M. Grosse-Perdekamp, 1K. Hafidi, 18D. Hasell, 26T. Hemmick, 1R. Holt, 8E. Hughes, 22C. Hyde-Wright, 5G. Igo, 14K. Imai, 10D. Ireland, 26B. Jacak, 15P. Jacobs, 28M. Jones, 10R. Kaiser, 17D. Kawall, 11C. Keppel, 7E. Kinney, 18M. Kohl, 9H. Kowalski, 17K. Kumar, 2V. Kumar, 21G. Kyle, 13J. Lajoie, 16M. Leitch, 27A. Levy, 27J. Lichtenstadt, 10K. Livingstone, 20W. Lorenzon, 145. Matis, 12N. Makins, 6G. Mallot, 18M. Miller, 18R. Milner*, 2A. Mohanty, 3D. Morrison, 26Y. Ning, 15G. Odyniec, 13C. Ogilvie, 2L. Pant, 26V. Pantuyev, 21S. Pate, 26P. Paul, 12J.-C. Peng, 18R. Redwine, 1P. Reimer, 15H.-G. Ritter, 10G. Rosner, 25A. Sandacz, 7J. Seele, 12R. Seidl, 10B. Seitz, 2P. Shukla, 15E. Sichtermann, 18F. Simon, 3P. Sorensen, 3P. Steinberg, 24M. Stratmann, 22M. Strikman, 18B. Surrow, 18E. Tsentalovich, 11V. Tvaskis, 3T. Ullrich, 3R. Venugopalan, 3W. Vogelsang, 28C. Weiss, 15H. Wieman,15N. Xu,3Z. Xu, 8W. Zajc.
1Argonne National Laboratory, Argonne, IL; 2Bhabha Atomic Research Centre, Mumbai, India; 3Brookhaven National Laboratory, Upton, NY; 4University of Buenos Aires, Argentina; 5University of California, Los Angeles, CA; 6CERN, Geneva, Switzerland; 7University of Colorado, Boulder,CO; 8Columbia University, New York, NY; 9DESY, Hamburg, Germany; 10University of Glasgow, Scotland, United Kingdom; 11Hampton University, Hampton, VA; 12University of Illinois, Urbana-Champaign, IL; 13Iowa State University, Ames, IA; 14University of Kyoto, Japan; 15Lawrence Berkeley National Laboratory, Berkeley, CA; 16Los Alamos National Laboratory, Los Alamos, NM; 17University of Massachusetts, Amherst, MA; 18MIT, Cambridge, MA; 19Max Planck Institüt für Physik, Munich, Germany; 20University of Michigan Ann Arbor, MI; 21New Mexico State University, Las Cruces, NM; 22Old Dominion University, Norfolk, VA; 23Penn State University, PA; 24RIKEN, Wako, Japan; 24-1RIKEN-BNL Research Center, BNL, Upton, NY; 25Soltan Institute for Nuclear Studies, Warsaw, Poland; 26SUNY, Stony Brook, NY; 27Tel Aviv University, Israel; 28Thomas Jefferson National Accelerator Facility, Newport News, VA
~100 Scientists, 30 Institutions, 9 countries*Contact People
C. Aidala, WWND, April 12, 2008 28
Electron Ion Collider Concepts
• eRHIC (BNL): Add Energy Recovery Linac to RHIC
PHENIX
STAR
e-cooling (RHIC
II)
Four e-beam passes
Main ERL (2 GeV per pass)
Electron Cooling
Snake
Snake
IR
IReRHIC(Linac-Ring)
ELIC
• ELIC (JLAB): Add hadron beam facility to CEBAF
C. Aidala, WWND, April 12, 2008 29
Main detector: Top view
Hadronic calorimete
rAdditional detector:
Emphasize low-x, low-Q2
diffractive physics (Abt, Caldwell, Liu, Sutiak, hep-ex/0407053)
Main detector:
Emphasize high-luminosity,
full physics program(Pasukonis, Surrow,
physics/0608290)
Si tracking stations
EM calorimete
r
e
p/ADetector Design
Learn from experience at HERA!
C. Aidala, WWND, April 12, 2008 30
EIC Timeline & Status• NSAC Long Range Plan 2007
– Recommendation: $6M/year for 5 years for machine and detector R&D
• Goal for Next Long Range Plan 2012– High-level recommendation for construction
• EIC Roadmap (Technology Driven)– Finalize Detector Requirements from Physics 2008– Revised/Initial Cost Estimates for eRHIC/ELIC 2008– Investigate Potential Cost Reductions 2009– Establish process for EIC design decision 2010– Conceptual detector designs 2010– R&D to guide EIC design decision 2011– EIC design decision 2011– “MOU’s” with foreign countries? 2012
C. Aidala, WWND, April 12, 2008 31
Summary
• What is the role of gluons and gluon self-interactions in nucleons and nuclei?
– Explore non-linear QCD
– Existence of universal saturation regime?
• What is the internal spin, flavor, and space-time structure of the nucleon?
An Electron-Ion Collider would offer unprecedented opportunities to explore the next
QCD frontier
New collaborators and ideas welcome!
C. Aidala, WWND, April 12, 2008 32
C. Aidala, WWND, April 12, 2008 33
Extra Slides
C. Aidala, WWND, April 12, 2008 34
• Peak luminosity 2.6 x 1033 cm-2s-1 in electron-hadron collisions• Electron beam polarization not affected by energy• +- 5 meter “element-free” straight section for detectors• Ion beams up to U• Ability to take full advantage of electron cooling of the hadron
beams• Can run hadron-hadron collisions in RHIC simultaneously
PHENIX
STAR
e-cooling (RHIC II)
Four e-beam passes
Main ERL (2 GeV per pass)
eRHIC at BNL
Add energy-recovery linac to RHIC
24-250 GeV protons30-100 GeV/n ions
3-10 (20) GeV electrons
C. Aidala, WWND, April 12, 2008 35
Electron Cooling
Snake
Snake
3-9 GeV electrons
30-225 GeV protons30-100 GeV/n ions
IR
IR
Visionary green-field design:• Peak luminosity up to ~8 x 1034 cm-2s-1 through short ion bunches• “Figure-8” lepton and ion rings• +- 3m “element-free” straight sections• Ion beams up to Au• Superconducting RF ion linac concept for all ions• 12 GeV CEBAF accelerator serves as injector to electron ring
ELIC at JLab
Add hadron beam facility to CEBAF
C. Aidala, WWND, April 12, 2008 36
eRHIC vs. ELIC• eRHIC could potentially go up to higher electron
energy of 20 GeV, compared to 9 for ELIC.
• eRHIC can run hadron-hadron collisions simultaneously
• Successful R&D for ELIC could lead to luminosities ~10-50 times higher than eRHIC
• ELIC costs higher
• ELIC timeline longer
C. Aidala, WWND, April 12, 2008 37
LHeC: L = 1.1x1033 cm-
2s-1 Ecm = 1.4 TeV
EIC: L > 1x1033 cm-2s-1
Ecm = 20-100+ GeV
• Add 70-100 GeV electron ring to interact with LHC ion beam• Use LHC-B interaction region• High luminosity mainly due to large ’s (= E/m) of beams
• Variable energy range• Polarized and heavy ion beams• High luminosity in energy region of interest for nuclear scienceNuclear science goals:• Explore the new QCD frontier: strong color fields in nuclei• Precisely image the sea-quarks and gluons to determine the spin, flavor and spatial structure of the nucleon.
High-Energy physics goals:• Parton dynamics at the TeV scale - physics beyond the
Standard Model - physics of high parton
densities (low x)
Important cross fertilization of ideas:• Significant European interest in an EIC• EIC collaborators on LHeC Science Advisory Committee
(with Research Directors of CERN, FNAL, DESY)
The EIC and the LHeC
C. Aidala, WWND, April 12, 2008 38
A Truly Universal Regime?
A.H. Mueller, hep-ph/0301109
Small x QCD evolution predicts:
• QS approaches universal behavior for all hadrons and nuclei
Not only functional form f(Qs) universal but even Qs becomes the same
?
• Radical View: – Nuclei and all hadrons have a component of their
wave function with the same behavior– This is a conjecture! Needs to be tested
C. Aidala, WWND, April 12, 2008 39
Nuclear Modification of Structure Functions
C. Aidala, WWND, April 12, 2008 40
Diffractive Structure Function F2D at EIC
- Distinguish between linear evolution and saturation models
- Insight into the nature of pomeron - Search for exotic objects (Odderon)
xIP = momentum fraction of the pomeron w.r.t the hadron
Curves: Kugeratski, Goncalves, Navarra, EPJ C46, 413
= x/xIP
d4 eh eXh
dxdQ2ddt
4 e.m.2
2Q41 y
y 2
2
F2
D y 2
2FL
D
C. Aidala, WWND, April 12, 2008 41
Connection to p+A Physics– e+A and p+A provide excellent
information on properties of gluons in the nuclear wave functions
– Both are complementary and offer the opportunity to perform stringent checks of factorization/universality
– Issue:
• p+A lacks the direct access to x, Q2
F. Schilling, hex-ex/0209001
Breakdown of factorization (e+p HERA versus p+p TeVatron) seen for diffractive final states.
C. Aidala, WWND, April 12, 2008 42
• Experimentally can be determined directly IF VARIABLE ENERGIES!• Highly sensitive to effects of gluon
+ 12-GeV data+ EIC alone
(includes systematic uncertainties)
Longitudinal Structure Function FL
C. Aidala, WWND, April 12, 2008 43
at small x
Superb sensitivity to g
at small x!
Gluon Contribution to the Proton Spin150 GeV x 7 GeV, 5 fb-1
C. Aidala, WWND, April 12, 2008 44
G Via Open Charm and Dijet Production
HERMES, COMPASS, SMC
C. Aidala, WWND, April 12, 2008 45
Projected data on g/g with an EIC, via + p D0 + X
K- + +
RHIC-Spin
Advantage: measurements directly at single Q2 ~ 10 GeV2 scale!
• Uncertainties in xg smaller than 0.01 • Measure 90% of G (@ Q2 = 10 GeV2)
g
/g
G Via Open Charm and Dijets at EIC
g
Dijets
C. Aidala, WWND, April 12, 2008 46
RHIC-Spin region
Spin-Flavor Decomposition of the Light Quark Sea
| p = + + + …>u
u
d
u
u
u
u
d
u
u
dd
dMany
models predict
u > 0, d < 0
Precisely Image the Sea Quark Polarization
C. Aidala, WWND, April 12, 2008 47gives transverse position of quark (parton) with longitud. mom. fraction x
Fourier transform in momentum transfer
x = 0.01 x = 0.40 x = 0.70
Wigner function: Probability to find a u(x) quark with a certain polarization at position r and with momentum k
Wu(x,k,r)
GPDu(x,,t) Hu, Eu, Hu, Eu
~~
p
m
BGPD
d2k
T
u(x)u, u
F1u(t)
F2u,GA
u,GPu
f1(x)g1, h1
PartonDistributions
Form Factors
d2k
T
dx
= 0, t = 0
Link to Orbital
Momentum
Towards a 3D spin-flavor landscape
Link to Orbital
Momentum
p
m
xTMD
d3 r
TMDu(x,kT) f1,g1,f1T ,g1T
h1, h1T ,h1L ,h1
C. Aidala, WWND, April 12, 2008 48
Detector Design
But: - low-field region around central tracker- better particle identification- forward-angle detectors- auxiliary detectors for exclusive events- auxiliary detectors for normalization
Main detector: Learn from ZEUS + H1
at HERA