35
SIDIS/A1n Andrew Puckett University of Connecticut SBS Summer 2017 Collaboration Meeting July 13, 2017

Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

  • Upload
    others

  • View
    2

  • Download
    0

Embed Size (px)

Citation preview

Page 1: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

SIDIS/A1nAndrew Puckett

University of ConnecticutSBS Summer 2017 Collaboration Meeting

July 13, 2017

Page 2: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Semi-Inclusive Deep Inelastic Scattering

• Detecting the leading (high-energy) hadrons in DIS collisions; i.e., the single inclusive hadron electroproduction N(e,e’h)X process provides sensitivity to additional aspects of the nucleon’s partonicstructure not accessible in inclusive DIS, including:

• quark flavor• quark transverse momentum• quark transverse spin

• Goal of SIDIS studies is (spin-correlated) 3D imaging of nucleon’s quark structure in momentum space.• Transverse Momentum Dependent (TMD) PDF formalism: Bacchetta et al. JHEP 02 (2007) 093, Boer and Mulders, PRD 57, 5780 (1998), etc, etc...

7/13/17 2SBS Collaboration 2017

Page 3: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Transverse target spin effects in SIDIS

Transverse target spin-dependent cross section for SIDIS

• Collins effect—chiral-odd quark transversity DF; chiral-odd Collins FF• Sivers effect—access to quark OAM and QCD FSI mechanism• “Transversal helicity” g1T—real part of S wave-P wave interference (Sivers = imaginary part) (requires polarized beam)• “Pretzelosity” or Mulders-Tangerman function—interference of wavefunction components differing by 2 units of OAM

AUT

(⇤,⇤S

) =1

PT

d⇥(⇤,⇤S

)� d⇥(⇤,⇤S

+ �)

d⇥(⇤,⇤S

) + d⇥(⇤,⇤S

+ �)

= ACollins

UT

sin(⇤+ ⇤S

) +

ASivers

UT

sin(⇤� ⇤S

) +

APretz

UT

sin(3⇤� ⇤S

)

ACollins

UT

/ �q ⌦H?1

ASivers

UT

/ f?1T ⌦D1

APretz

UT

/ h?1T ⌦H?

1

D1 = unpolarized

fragmentation function

H?1 = Collins

fragmentation function

ALT (�,�S) =

1

PePT

Y+

(�,�S)� Y�(�,�S)

Y+

(�,�S) + Y�(�,�S)

⇠ Acos(���S)

LT cos(�� �S)

⇠ g1T ⌦D

1

7/13/17 3SBS Collaboration 2017

Page 4: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Transversity and Collins Functions: Existing Knowledge

7/13/17 SBS Collaboration 2017 4

Anselmino et al., Phys. Rev. D 92, 114023 (2015) arXiv:1510.05389v1: latest extractions of valence u and d quark transversities and favored/unfavored Collins FFs

• SIDIS data from HERMES on proton target, COMPASS on proton and deuteron targets• Data on azimuthal asymmetries in e+/e- annihilation to pion pairs from BELLE and BaBar

collaborations—very recent, high statistical precision• First look at combined z and pT dependencies of Collins FFs.• Note—d quark transversity is poorly constrained—proton data dominated by u quarks, limited

sensitivity to d from COMPASS deuteron and JLab Hall A 3He data.

Page 5: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Sivers effect—Existing knowledge

7/13/17 SBS Collaboration 2017 5

Anselmino et al., Phys.Rev. D86 (2012) 014028, arXiv:1204.1239v1

• Fits to most recent HERMES and COMPASS SIDIS Sivers data with TMD/DGLAP evolution

• As in the case of Collins/Transversity, d-quark Siversis poorly constrained by existing data• Proton data dominated by u-quarks• Limited precision/sensitivity to d quark from

COMPASS deuteron/JLab Hall A 3He data

Page 6: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

E12-09-018: Transverse Target SSA in 3He(e,e’h)X

High-luminosity Polarized 3He Target (1.2 × 1037 cm-2 s-1)

Electron Arm: BigBiteSpectrometer @30 deg.

JLab E12-09-018 in Hall A: Approved for

64 beam-days, A-

rating by PAC38 (2011)

Hadron Arm: Super BigBiteSpectrometer @14 deg.

• E12-09-018 in Hall A: transverse spin physics with high-luminosity polarized 3He. • 40 (20) days production at E = 11 (8.8) GeV—significant Q2 range at fixed x• Collins, Sivers, Pretzelosity, ALT for n(e,e’h)X, h = 𝝅+/𝝅-/𝝅0/K+/K-

• Re-use HERMES RICH detector for charged hadron PID • Reach high x (up to ~0.7) and high statistical FOM (~1,000X Hall A E06-010 @6 GeV)

7/13/17 SBS Collaboration 2017 6

Page 7: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

SBS+BB Projected Results: Collins and Sivers

7/13/17 SBS Collaboration 2017 7

• E12-09-018 will achieve statistical FOM for the neutron ~100X better than HERMES proton data and ~1000X better than existing neutron data from Hall A at 6 GeV a• Kaon and neutral pion data will aid flavor decomposition, and understanding of reaction-mechanism effects.

Projected AUTSivers precision vs. x Projected AUT

Collins precision vs. x

Page 8: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Summary of E12-09-018 Physics Impact• Pioneering HERMES+COMPASS experiments conclusively

demonstrated the existence of the Collins and Sivers effects in SIDIS.• SSAs in SIDIS are large, especially in the valence region• Experiment E12-09-018 will be the first SIDIS experiment in

the JLab 12 GeV era on a transversely polarized neutron (3He) target. • First precise measurements of Collins/Sivers effects in multi-

dimensional phase space.• Extend knowledge further into the valence region (where

asymmetries are large) to x ~ 0.7 at Q2 values between those of HERMES and COMPASS• Polarized neutronsà unrivaled d quark sensitivity• Large impact to global TMD extraction

7/13/17 SBS Collaboration 2017 8

Page 9: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

E12-06-122: A1n in the valence region using

BigBite in Hall A

7/13/17 SBS Collaboration 2017 9

Page 10: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Polarized DIS and Spin Structure Functions• Helicity asymmetries in the scattering of longitudinally polarized electrons on longitudinally and transversely (in the scattering plane) polarized nucleons provide access to spin structure functions g1, g2. • The longitudinal virtual photon asymmetry A1 is defined as the asymmetry between parallel and antiparallel virtual photoabsorption cross sections and is related to the spin structure function g1(x,Q2):

• In the naïve parton model, g1 is an incoherent sum over parton helicity distributions Δqi, equal to the difference in number density of quarks polarized parallel and antiparallel to the nucleon spin:

A1 =�1/2 � �3/2

�1/2 + �3/2

A1 ⇡ g1F1

, Q2 ! 1

g1F1

⇡P

i e2i (�qi +�q̄i)Pj e

2j (qj + q̄j)

7/13/17 SBS Collaboration 2017 10

Page 11: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Experimental Status of Δq

DSSV: PRD 80, 034030 (2009)

Blumlein and Bottcher, hep-ph/1005.3113• Recent Global Analyses:

• DSSV, includes SIDIS and pp data, asymmetric sea• BB, DIS data only

7/13/17 SBS Collaboration 2017 11

Page 12: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

7/13/17 SBS Collaboration 2017 12

Page 13: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

7/13/17 SBS Collaboration 2017 13

Page 14: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

A1n Requirements and Status• High-luminosity polarized 3He target• BigBite detector upgrades:• GRINCH• Replace MWDCs with GEMs• Upgraded BigBite Timing hodoscope

• BigBite configurations are largely identical between A1n and neutron SIDIS proposal• Status—A1n still approved but not scheduled. • Jeopardy process for proposals approved for more than 4

years but not scheduled will start in 2019 (according to draft policy presented by B. McKeown at recent Users’ Group Meeting).

7/13/17 SBS Collaboration 2017 14

Page 15: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

A1n Resubmission• Hall A BigBite + HRS proposal E12-06-122 with

8.8 and 6.6 GeV beam energy was submitted assuming it could run as an early/”commissioning experiment”, prior to the main SBS program, and (potentially) prior to establishment of reliable, 11 GeV CEBAF ops.• Given schedule realities and evolution of

BigBite/SBS apparatus, this no longer entirely makes sense• A1n resubmission in preparation—target

submission in 2018 • Hall A A1n faces jeopardy as soon as 2019.

7/13/17 SBS Collaboration 2017 15

Page 16: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

A1n with SBS+BB @11 GeV, 250h, 50 uA, PbPT ~= 0.5, 10.5 atm 3He

7/13/17 SBS Collaboration 2017 16

Bjx0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8

)2>

(GeV

2<Q

0

2

4

6

8

10

12

14

Bjx0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8

DIS

cou

ntin

g ra

te (H

z)

2−10

1−10

1

10

210

310

410

Bjx0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8

n 1A

0.0

0.2

0.4

0.6

0.8

Bjx0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8

n 1 A

0.10−

0.08−

0.06−

0.04−

0.02−

0.00

0.02

0.04

0.06

0.08

0.10

• BigBite @35 deg• BigBite @30 deg• SBS @20 deg.

PRELIMINARY

Page 17: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Summary• SBS Transversity (E12-09-018), first submitted to

PAC34, fully approved by PAC38, has the most approved beam time of any SBS experiment• Original Hall A E06-010 produced a large number of

physics publications beyond the main physics goal and scope of the experiment. • Similarly large output could be expected from E12-09-

018. • A1n with BigBite @8.8 and 6.6 GeV, approved over 10

years ago, is sub-optimal in light of current realities• Resubmission in preparation for 11 GeV beam with

BigBite and SBS to reflect evolution of Hall A status and equipment

7/13/17 SBS Collaboration 2017 17

Page 18: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Backups

7/13/17 SBS Collaboration 2017 18

Page 19: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

General Expression for SIDIS Cross Section: Bacchetta et al., JHEP 02, 093 (2007)

d⇧

dxdydzd⌃hd⌃Sdp2T=

�2

xyQ2

y2

2(1� ⇤)

✓1 +

⇥2

2x

◆(FUU,T + ⇤FUU,L +

p2⇤(1 + ⇤) cos⌃hF

cos�h

UU + ⇤ cos(2⌃h)Fcos 2�h

UU +

⌅e

p2⇤(1� ⇤) sin⌃hF

sin�h

LU +

Sk

hp2⇤(1 + ⇤) sin⌃hF

sin�h

UL + ⇤ sin(2⌃h)Fsin 2�h

UL

i+

Sk⌅e

hp1� ⇤2FLL +

p2⇤(1� ⇤) cos⌃hF

cos�h

LL

i+

S?

"sin(⌃h � ⌃S)F

sin(�h��S)

UT +

⇤ sin(⌃h + ⌃S)Fsin(�h+�S)

UT +

⇤ sin(3⌃h � ⌃S)Fsin(3�h��S)

UT +

p2⇤(1 + ⇤)

⇣sin⌃SF

sin�S

UT + sin(2⌃h � ⌃S)Fsin(2�h��S)

UT

⌘#+

S?⌅e

"p1� ⇤2 cos(⌃h � ⌃S)F

cos(�h��S)

LT +

p2⇤(1� ⇤)

⇣cos⌃SF

cos�S

LT + cos(2⌃h � ⌃S)Fcos(2�h��S)

LT

⌘#)

• SIDIS structure functions F depend on x, Q2, z, pT• U, L, T subscripts indicate unpolarized, longitudinally and transversely polarized beam, target, respectively • S = nucleon spin• λ = lepton helicity• 18 structure functions up to twist-three• Eight terms survive at leading twist; the rest are twist-3 (M/Q suppressed)

� =2Mx

Q

⇥ =1� y � 1

4�2y2

1� y + 12y

2 + 14�

2y2

• Sivers• Collins• “Pretzelosity”

7/13/17 19SBS Collaboration 2017

Page 20: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Quark-parton Model Interpretation of SIDIS: Transverse Momentum Dependent PDFs (TMDs)

7/13/17 SBS Collaboration 2017 20

Quarkpolarization

Unpolarized(U)

LongitudinallyPolarized(L)

TransverselyPolarized(T)

Nucleon

Polarization

U

L

Th?1T =

h?1L =

h?1 =

g1T =f?1T =

f1 =

g1 =

h1 =

Page 21: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

SIDIS Structure Functions in Terms of TMDs

D1(z,Q2, p2?) = Unpolarized TMD FF

H?1 (z,Q2, p2?) = Collins TMD FF

• Only f1, g1, h1 survive integration over quark kT•All eight leading-twist TMDs are accessible in SIDIS with polarized beams/targets via azimuthal angular dependence of the SIDIS cross section• Physical observables are convolutions over two (unobserved) transverse momenta:

• Initial quark kT• Hadron pT relative to recoiling quark, generated during fragmentation

FUU,T ⇠ f1

⌦D1

F cos 2�h

UU ⇠ h?1

⌦H?1

F sin 2�h

UL ⇠ h?1L ⌦H?

1

FLL ⇠ g1

⌦D1

Fsin(�h��S)

UT ⇠ f?1T ⌦D

1

Fsin(�h+�S)

UT ⇠ h1

⌦H?1

Fsin(3�h��S)

UT ⇠ h?1T ⌦H?

1

Fcos(�h��S)

LT ⇠ g1T ⌦D

1

7/13/17 21SBS Collaboration 2017

Page 22: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

High-luminosity Polarized 3He target development

7/13/17 SBS Collaboration 2017 22

• Significant recent progress by UVA group (Cates) in the development of high-luminosity polarized 3He targets for SBS SIDIS and GEN experiments based on convection-driven circulation of polarized gas

• Now published in Phys. Rev. C 91, 055205 (2015)• See also: Phys.Rev. C84 (2011) 065201 and

https://arxiv.org/abs/1706.02747• Acceptable spin relaxation times now demonstrated in prototype cells

with glass-to-metal seals

• Conceptual and engineering designs for GEn-II target underway

Page 23: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

3D and “4D” extraction of SIDIS SSAs with SBS

7/13/17 SBS Collaboration 2017 23

Increasing z è

çIn

crea

sing

pT

A

sin(�h��S)UT for n(e, e0⇡+

)X :

0.1 x 0.7,�x = 0.1

0.2 z 0.7,�z = 0.1

0 pT (GeV) 1.2,�pT = 0.2 GeV

Example result for 3D binning (x,z,pT)

• E = 11 GeV, 40 days

• “4D” with Q2 dependence from 20 days at 8.8 GeV:

E = 11 GeV

E = 8.8 GeV

E = 5.9 GeV (E06-010 Hall A)

Page 24: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

) h� −

S�

sin

(U

TA

x0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8

−0.2

−0.1

0

0.1

0.2

JLAB 12

X+� l��lN

= 4.63922 (GeV) s

(x)

(1)

1Tx

fN

ud

ud

ss

) (x

, k 1T

x f

ud

ud

ss

x (GeV)k

0

0.02

0.04

−0.02

0

0

0.01

0.02

0.03

−0.01

−0.005

0

0

0.0005

0.001

0 0.2 0.4 0.6 0.8

−0.005

0

0

0.05

0.1

0.15

−0.4

−0.2

0

0

0.5

1

−0.2

0

0

0.01

0.02

0 0.2 0.4 0.6 0.8 1 1.2 1.4−0.15−0.1−0.05

0

Example Impacts of SBS SIDIS Experiment

7/13/17 SBS Collaboration 2017 24

• 2011 impact study by A. Prokudin, global fit with E12-09-018 projected results, π+ Sivers moments at E = 11 GeV, ½ of projected statistics. • Left: >5X shrinking of n(e,e’ π+)X Sivers AUT band• Right: reducing the uncertainty in d quark Sivers in six-flavor extraction• E12-09-018 will provide π±/π0/K± at similar precision (Kaon errors 2-3X pion errors) for both E = 8.8 GeV and E = 11 GeV Collins/Sivers (and Pretzelosity)

Page 25: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Example Impacts of SBS SIDIS Experiment

7/13/17 SBS Collaboration 2017 25

• 2011 impact study by A. Prokudin, global fit with E12-09-018 projected results, π+ Sivers moments at E = 11 GeV, ½ of projected statistics. • Left: >5X shrinking of n(e,e’ π+)X Sivers AUT band• Right: reducing the uncertainty in d quark Sivers in six-flavor extraction• E12-09-018 will provide π±/π0/K± at similar precision (Kaon errors 2-3X pion errors) for both E = 8.8 GeV and E = 11 GeV Collins/Sivers (and Pretzelosity)

) h� −

S�

sin

(U

TA

x0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8

−0.2

−0.1

0

0.1

0.2

JLAB 12

X+� l��lN

= 4.63922 (GeV) s

(x)

(1)

1Tx

fP

ud

ud

ss

) (x

, k 1T

x f

ud

ud

ss

x (GeV)k

−0 04

−0.02

0

0

0.02

0.04

−0.005

0

0

0.01

0.02

0

0.0005

0.001

0 0.2 0.4 0.6 0.8

−0.005

0

−0.2

0

0

0.05

0.1

0.15

−0.3

−0.2

−0.1

0

0

0.5

1

0

0.01

0.02

0 0.2 0.4 0.6 0.8 1 1.2 1.4−0.15−0.1−0.05

0

Page 26: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

7/13/17 SBS Collaboration 2017 26

Page 27: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

SBS+BB Projected Precision in 2D (x,z) binning

7/13/17 SBS Collaboration 2017 27

• 2D Extraction: Sivers AUT in n(e,e’π+)X, 6 x bins 0.1<x<0.7, 5 z bins 0.2<z<0.7• Curves are phenomenological predictions from global analysis (Anselmino et al.) with central value and error band

Uncertainty in this x, z bin ~ 0.6%

Large neutron π+ asymmetry expected at high z, large uncertainty in global fit

Page 28: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

3D and “4D” extraction of SIDIS SSAs with SBS

7/13/17 SBS Collaboration 2017 28

Increasing z è

çIn

crea

sing

pT

A

sin(�h��S)UT for n(e, e0⇡+

)X :

0.1 x 0.7,�x = 0.1

0.2 z 0.7,�z = 0.1

0 pT (GeV) 1.2,�pT = 0.2 GeV

Example result for 3D binning (x,z,pT)

• E = 11 GeV, 40 days

• “4D” with Q2 dependence from 20 days at 8.8 GeV:

E = 11 GeV

E = 8.8 GeV

E = 5.9 GeV (E06-010 Hall A)

Page 29: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

SIDIS Kinematic Coverage in E12-09-018

7/13/17 SBS Collaboration 2017 29

• Wide, independent coverage of x, z, pT, ϕh ± ϕS in a single kinematic configuration.• At least four (preferably 8) target spin directions to achieve full ϕS coverage• Q2, x strongly correlated due to dimensions of BigBite magnet gap.• Data at E = 11, 8.8 GeV provide data for significantly different Q2 at same x• Systematics control à independent spectrometers, detectors in field-free regions,

straight-line tracking, simple, well-defined (but adequately large) acceptance, etc.

Page 30: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

(Some) Unique Challenges for SBS-SIDIS• Small raw asymmetries ó tight control of systematics => As

fast as possible change of spin orientation—with adiabatic rotation of target holding field expect T ~ 120 s?• Inclusive kinematics—low trigger thresholds ó high

accidental coincidence rates. Proposal estimate was ~20 kHz online coincidence trigger rate. • Addition of GRINCH to the trigger for BigBite would be extremely

helpful here, since ~90% of BigBite calorimeter-based triggers are photon-induced!

• GEM-based tracking with no real constraints on track search area (other than HCAL hadronic shower signal and SBS acceptance) due to inclusive kinematics (but 40X lower luminosity than GEP helps)

7/13/17 SBS Collaboration 2017 30

Page 31: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

SIDIS Kinematics—Notation and Definitions

7/13/17 SBS Collaboration 2017 31

Page 32: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

E12-09-018 Apparatus and Requirements• Target: High-luminosity polarized 3He; similar to GEN target, but

requires (almost) complete freedom in target polarization orientation. Required orientations include (at a minimum) horizontal and vertical polarization transverse to the beamline (and preferably ±45∘ as well), plus longitudinal polarization for calibrations/corrections.• Hadron arm: SBS at 14 deg. central angle, equipped with:

• HCAL for hadron trigger• Large-area GEM-based tracker• RICH for charged hadron PID

• Electron arm: BigBite at 30 deg. central angle equipped with:• Pre-shower and shower for electron trigger• Timing hodoscope• GEM-based tracker• GRINCH

• DAQ and trigger:• HCAL threshold low enough to be efficient for SIDIS charged hadrons p > 2-3

GeV• BigBite threshold low enough to be efficient for electrons p > 1 GeV

7/13/17 SBS Collaboration 2017 32

Page 33: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

Progess in gluon and sea polarization from RHIC-spin

DSSVà RHICspinprogramconstraintstogluonpolarization(arXiv:1404.4293v1)

7/13/17 SBS Collaboration 2017 33

Page 34: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

7/13/17 SBS Collaboration 2017 34

Page 35: Puckett A1n SIDIS 2017 · •Replace MWDCs with GEMs •Upgraded BigBiteTiming hodoscope •BigBiteconfigurations are largely identical between A1n and neutron SIDIS proposal •Status—A1n

7/13/17 SBS Collaboration 2017 35