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The Future of RHIC: An eRHIC Physics Overview Brian Page Brookhaven National Laboratory RHIC & AGS Users’ Meeting

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The Future of RHIC: An eRHIC Physics Overview

Brian Page

Brookhaven National Laboratory

RHIC & AGS Users’ Meeting

Pressing Questions in QCD • How are the sea quarks and gluons, and their spins, distributed in space and

momentum inside the nucleon? • How are these quark and gluon distributions correlated with overall nucleon

properties, such as spin direction? • What is the role of the orbital motion of sea quarks and gluons in building the nucleon

spin?

• Where does the saturation of gluon densities set in?

• Is there a simple boundary that separates this region from that of more dilute quark-gluon matter?

• If so, how do the distributions of quarks and gluons change as one crosses the boundary?

• Does this saturation produce matter of universal properties in the nucleon and all nuclei viewed at nearly the speed of light?

• How does the nuclear environment affect the distribution of quarks and gluons

and their interactions in nuclei? • How does the transverse spatial distribution of gluons compare to that in the nucleon? • How does nuclear matter respond to a fast moving color charge passing through it? • Is this response different for light and heavy quarks? 2 RHIC & AGS Users Meeting - 2015

Pressing Questions in QCD • How are the sea quarks and gluons, and their spins, distributed in space and

momentum inside the nucleon? • How are these quark and gluon distributions correlated with overall nucleon

properties, such as spin direction? • What is the role of the orbital motion of sea quarks and gluons in building the nucleon

spin?

• Where does the saturation of gluon densities set in?

• Is there a simple boundary that separates this region from that of more dilute quark-gluon matter?

• If so, how do the distributions of quarks and gluons change as one crosses the boundary?

• Does this saturation produce matter of universal properties in the nucleon and all nuclei viewed at nearly the speed of light?

• How does the nuclear environment affect the distribution of quarks and gluons

and their interactions in nuclei? • How does the transverse spatial distribution of gluons compare to that in the nucleon? • How does nuclear matter respond to a fast moving color charge passing through it? • Is this response different for light and heavy quarks? 3 RHIC & AGS Users Meeting - 2015

Hera

Jlab, Compass

& HERMES

RHIC

eRHIC: Polarized ep Collider

Colliders: Large kinematic coverage

DIS: Kinematic precision

Polarization: Spin observables

eRHIC!

4 RHIC & AGS Users Meeting - 2015

5

RHIC

NSRL LINAC

Booster

AGS

STAR

PHENIX

Jet/C-Polarimeters

RF

CeC

EBIS

eRHIC

eRHIC Detector

eRHIC Detector

e-

p

polarized leptons 15 & 21.2 GeV and lower Ee >1.6 GeV

Light ions (d,Si,Cu) Heavy ions (Au,Pb,U) 10-100 GeV/u

70% Polarized protons 25-250 GeV

Electron accelerator

to be build

RHIC Existing = $2B

goal: 80% e- polarization

Polarized light ions He3 17-166 GeV/u

From RHIC to eRHIC

RHIC & AGS Users Meeting - 2015

Detector II

Detector I

Energy Recovery Linac,

1.32 GeVCoherent

Electron CoolerPolarized

Electron Source

electrons

hadrons

From AGS

Beam Dump

100 meters

FFAG Recirculating Electron Rings ERL Cryomodules

1.3-5.3 GeV

6.6-21.2 GeV

6

eRHIC: Energy recovery linac + fixed-field alternating-gradient ring design Record luminosity (>1033/cm-2s-1) 100 – 1000 x HERA

When completed, eRHIC will be the most advanced and energy efficient accelerator in the world

eRHIC Design

RHIC & AGS Users Meeting - 2015

Azimuthal asymmetries in DIS

Adds their transverse momentum dependence

Inclusive and semi-inclusive DIS

Longitudinal motion of spinning quarks and gluons

ma

chin

e &

de

tect

or

req

uir

em

en

ts

All need √sep > 50 GeV to access x < 10-3 where sea quarks and gluons dominate

7

• multi-dimensional binning x, Q2, z, pT (or t), Θ • to reach pT > 1 GeV • to reach |t| > 1 GeV2

L ≃ 10 fb-1

L ≃ 10 - 100 fb-1

Exclusive processes

Adds their transverse position

What is Needed

RHIC & AGS Users Meeting - 2015

Longitudinal Spin Structure

8 RHIC & AGS Users Meeting - 2015

• Integral of ∆g(x) in range 0.05 < x < 1.0 increases from roughly 0.05 to 0.20−0.07

+0.06 . First indication of non-zero gluon polarization!

∆G: Where Are We Now?

• Uncertainty on integral over low x region is still sizable

• Uncertainty shrinks substantially from DSSV* to new DSSV fit

9

Phys. Rev. Lett. 113, 012001

RHIC & AGS Users Meeting - 2015

∆G: Where We Will Be Soon

• High statistics data sets from 2012 and 2013 are being analyzed

• 200 GeV longitudinal run recently concluded

• Expected effect of data sets taken after 2009 on uncertainty of ∆g running integral shown

Integral of ∆g(x,Q2) from xmin to 1 as a function of xmin

• 200 GeV: xmin > 10-2

• 500 GeV + Forward Rapidity: xmin > 10-3

10

arXiv:1501.01220

RHIC & AGS Users Meeting - 2015

∆G: Where We Are Going (eRHIC)

• Several observables are sensitive to ∆G in DIS but golden measurement at an eRHIC would be scaling violation of g1(x,Q2)

• Current DIS constraints on ∆G hampered by limited x & Q2 coverage

• eRHIC would greatly expand kinematic reach and precision of g1(x,Q2) measurements!

Current Data

11

arXiv:1206.6014

RHIC & AGS Users Meeting - 2015

eRHIC: Impact on ∆G

• eRHIC will have the ability to vastly reduce the uncertainty on ∆G, especially at low x where constraints from data are virtually non-existent

• The excellent statistical precision achievable with an eRHIC means control of systematics will be critical

• Above plot shows how the constraint on ∆G is affected by systematic uncertainty

12

arXiv:1212.1701

RHIC & AGS Users Meeting - 2015

0

0.2

0.4

0.6

0.8

1

10-6

10-5

10-4

10-3

10-2

10-1

1

DSSV 2014with 90% C.L. band

eRHIC data:

15 ´ 100 GeV

+ 15 ´ 250 GeV

+ 20 ´ 250 GeV

all bands 90% C.L.

ò d

x D

g(x

,Q2)

xm

in

1

xmin

Q2 = 10 GeV

2

0

0.2

0.4

0.6

10-6

10-5

10-4

10-3

10-2

10-1

1

DSSV 2014with 90% C.L. band

eRHIC data:

15 ´ 100 GeV

+ 15 ´ 250 GeV

+ 20 ´ 250 GeV

all bands 90% C.L.

ò d

x D

S(x

,Q2)

xm

in

1

xmin

Q2 = 10 GeV

2

-0.2

0

0.2

0.4

0.6

10-6

10-5

10-4

10-3

10-2

10-1

1

DSSV 2014

eRHIC data:

15 ´ 100 GeV

+ 15 ´ 250 GeV

+ 20 ´ 250 GeV

all bands 90% C.L.

1/2

- ò

dx [

1/2

DS

+ D

g]

xm

in

1

(x,Q

2)

xmin

Q2 = 10 GeV

2

Gluon Quarks orbital angular momentum

1/2 - - =

eRHIC: Solving the Spin Puzzle

• Above plot shows the running integral of ∆g(x,Q2) from xmin to 1 as a function of xmin

• Large reduction in uncertainty on ∆G from eRHIC can be seen

• eRHIC will also reduce the uncertainty on the quark contribution to the proton spin

• No assumptions about hyperon beta decay in eRHIC uncertainty

• Constraints on gluon and quark contributions will provide independent check of orbital angular momentum component of proton spin

13

arXiv:1409.1633

RHIC & AGS Users Meeting - 2015

RHIC: Probing the Sea

• STAR W AL data from 2011 + 2012 included in preliminary DSSV analysis (DSSV++) and recent NNPDF analysis (NNPDFpol1.1)

• STAR W data shifts best fit values for first moments of ∆u̅(x,Q2) and ∆d̅(x,Q2) for x > 0.05

• ∆u̅ best fit value changes sign between DSSV+ and new DSSV++ and the node which existed in DSSV08 is absent in NNPDFpol1.1

14

arXiv:1304.0079

Nucl. Phys. B 887, 276 (2014) RHIC & AGS Users Meeting - 2015

eRHIC: Probing the Sea

• DIS largely 1-photon exchange, but can also proceed via charged current (CC) interaction mediated by W boson

• CC interactions in polarized DIS give access to quark / antiquark helicity distributions as well as unique structure functions

• Because W is virtual, can access lower values of Q2 to overlap with and provide cross check to SIDIS measurements

15

arXiv:1409.1633

RHIC & AGS Users Meeting - 2015

eRHIC: Quark / Anti-Quark Constraints

∆d̅ ∆u̅

∆d ∆u

• eRHIC with 5 GeV electrons colliding with 100 and 250 GeV protons greatly reduce uncertainty on u and d anti-quark helicity distributions

• See significant reduction in uncertainty on first moment of quark/anti-quark helicity distributions for x > 0.05 from 20 x 250 GeV electron on proton collisions

arXiv:1212.1701

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2D+1 picture in momentum space 2D+1 picture in coordinate space

17

Spin as vehicle to do tomography of the nucleon

• What is the dynamic structure of the proton and nuclei • 2D+1 picture in momentum and coordinate space • Visualize color interactions in QCD • Collective phenomena and correlations in fragmentation • New physics aspects due to confined motion

Quantum Tomography of the Nucleons

RHIC & AGS Users Meeting - 2015

TMDs

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TMDs

• Theoretically interesting multi-scale problem: Q2, pT

Observable: azimuthal modulations

of 6-fold differential SIDIS cross section

• TMD framework/factorization applicable for Q2 >> pT

• So far if at all only valence quark TMDs extracted from fixed target data

• Slew of different TMDs can be defined

• Very different evolution then collinear PDFs perturbative & non-perturbative contributions

Sivers function

• measures spin-orbit correlations • link to parton orbital motion (through models) • reveals non-trivial aspects of QCD color gauge invariance

Example

19 RHIC & AGS Users Meeting - 2015

TMDs: Before and After eRHIC

Current data on Sivers asymmetry is currently limited to low Q2 and relatively large x values

• Projected precision of Sivers asymmetries achievable at an eRHIC corresponding to an integrated luminosity of 10 fb-1

• Asymmetry is shown as a function of x

and Q2 for different z and PhT bins

• Estimation of the reduction in 2σ uncertainty of the Sivers function for the valence and sea up quarks for eRHIC data at √s = 45 GeV for a specific functional form of the Sivers asymmetry

20 RHIC & AGS Users Meeting - 2015

Accessing The Gluon Sivers Function

Measure a pair of D mesons

k⊥ = |k1T + k2T|

PT = (k1T - k2T) / 2 Statistically challenging

• Beam Energies: 20 GeV x 250 GeV • Q2: 1 – 10 GeV2, y: 0.01 – 0.95, z>0.25 • No cut on k⊥ and pt, but on k⊥/pt < 0.5 for “correlation limit”

• Statistical precision corresponds to roughly 8 months of running (50% efficiency) at L = 1034 cm2s-1

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• TMD inspired fit is not a good representation

• Need to account for different underlying sub-processes

• Neglects other dependences RHIC & AGS Users Meeting - 2015

Parameterizing Primordial kT

For the first time: very precise multidimensional data (x, Q2, pt, z) Remember: xF > 0 Fit:

4 different contributions to the pt of a hadron • kt: non-perturbative; very often

called “intrinsic” • kt

PS: from parton showers connection to soft factors in TMDs

• ptfrag: pt contribution from the

fragmentation • pt

hard : from hard QCD scattering

(QCDC, PGF, …)

23

Fx

-1 -0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.8 1

>2 T

<p

0

0.2

0.4

0.6

0.8

1

1.2

1.4

0

0.2

0.4

0.6

0.8

1

1.2

1.4

15x100 ep2>1.0 GeV2Chgd. hadrons Q

= 1.3 GeV EIC det. acceptanceTk

= 0.88 GeV EIC det. acceptanceTk

= 0.44 GeV EIC det. acceptanceTk

15x100 ep2>1.0 GeV2Chgd. hadrons Q

• xF>0: “struck” parton hemisphere

• xF<0 “target remnant” hemisphere sensitive to intrinsic kt

• What else can be learned from xF<0 region?

Fx

-1 -0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.8 1

>2 T

<p

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

15x100 ep2>1.0 GeV2Chgd. hadrons Q

Full QCD on (std) EIC det. acceptance

pQCD, NO PS EIC det. acceptance

PS only EIC det. acceptance

No QCD EIC det. acceptance

15x100 ep2>1.0 GeV2Chgd. hadrons Q

Accessing Primordial kT

RHIC & AGS Users Meeting - 2015

Generalized Parton Distributions

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Proton form factors, transverse charge & current densities

Structure functions, quark longitudinal momentum & helicity distributions

X. Ji, D. Mueller, A. Radyushkin (1994-1997)

Correlated quark momentum and helicity distributions in transverse space - GPDs

the way to 3d imaging of the proton and the orbital angular momentum Lq & Lg

Constrained through exclusive reactions

Beyond Form Factors and PDFs

RHIC & AGS Users Meeting - 2015

GPDs: Kinematic Coverage

Fourier

Transform

• Kinematic coverage of existing DVCS data and eRHIC range

• H1 and ZEUS DVCS cross sections and projected eRHIC statistical precision

• Fourier transform gives impact parameter dependence

26 RHIC & AGS Users Meeting - 2015

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y

xp

xz

bT

x

bT decreasing as a function of x

Valence (high x) quarks at the center small bT

Sea (small x) quarks at the periphery high bT

GLUONS ???

eRHIC

Model of a Quark GPD

RHIC & AGS Users Meeting - 2015

DVCS Asymmetries

28 RHIC & AGS Users Meeting - 2015

• A global fit over all pseudo data was done, based on the GPDs-based model: [K. Kumerički, D Müller, K. Passek-Kumerički 2007]

• Known values q(x), g(x) are assumed for Hq, Hg (at x=0, t=0 forward limits Eq, Eg are unknown)

• Excellent reconstruction of Hsea, Esea

and good reconstruction of Hg (from dσ/dt)

2D+1 Structure of the Nucleon

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To improve imaging on gluons add J/ψ observables

cross section AUT …..

GPD Hg: J/Ψ

RHIC & AGS Users Meeting - 2015

Summary

31

• Adding a polarized electron beam to RHIC will combine the large kinematic reach of colliders, the precision of leptonic probes, and full polarization control to produce the ultimate laboratory for the exploration of QCD

• Precision measurements of the g1(x,Q2) structure function, along with SIDIS and charged current probes will pin down the helicity structure of the proton

• Access to TMDs and GPDs will give full 2D+1 structure of the proton in transverse momentum and impact parameter space and probe the orbital angular momentum component of the proton spin

• In addition to polarized e+p, a rich physics program utilizing heavy nuclei will be possible

RHIC & AGS Users Meeting - 2015

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PDF Family Tree

RHIC & AGS Users Meeting - 2015

Golden Probes and Requirements

All measurements need √sep > 50 GeV to reach x < 10-3 where sea quarks and gluons dominate

𝐿𝑑𝑡 = 10 fb-1

𝐿𝑑𝑡 = 10 fb-1 -

𝐿𝑑𝑡 = 100 fb-1

33 RHIC & AGS Users Meeting - 2015

Golden Measurements

34 RHIC & AGS Users Meeting - 2015