In Medium Nucleon Structure Function, SRC, and the …orchen/Talks/PR11-107_EMC_SRC_pac38_V1… ·...
Transcript of In Medium Nucleon Structure Function, SRC, and the …orchen/Talks/PR11-107_EMC_SRC_pac38_V1… ·...
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In Medium Nucleon Structure Function, SRC, and the EMC Effect
Spokepersons: O. Hen (TAU), L. B. Weinstein (ODU), S. A. Wood (JLab), S. Gilad (MIT)
Proposal PR12-11-107
PAC 38 Aug. 2011
Collaboration:Experimental groups from : ANL, CNU, FIU, HU, JLab, KSU, MIT, NRCN, ODU, TAU, U. of Glasgow, U. of Ljubljana, UTFSM, UVaTheoretical support: Accardi, Ciofi Degli Atti, Cosyn, Frankfurt, Kaptari, Melnitchouk, Mezzetti, Miller, Ryckebusch, Sargsian, Strikman
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The European Muon Collaboration (EMC) effect DIS cross section per nucleon in nuclei ≠ DIS off a free nucleon
Can not be explained only by simple Fermi motion and binding effects
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DIS scale: several tens of GeV
Nucleons
Nucleon in nuclei are bound by ~MeV
Naive expectation :
DIS off a bound nucleon = DIS off a free nucleon
(Except some small Fermi momentum correction)
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DIS scale: several tens of GeV
Nucleons
Nucleon in nuclei are bound by ~MeV
Naive expectation :
(Except some small Fermi momentum correction)
DIS off a deuteron = DIS off a free proton neutron pair
Naive expectation :
Deuteron: binding energy ~2 MeV
Nucleons
Average nucleons separation ~2 fm
DIS off a bound nucleon = DIS off a free nucleon
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DIS scale: several tens of GeV
Nucleons
Nucleon in nuclei are bound by ~MeV
Naive expectation :
(Except some small Fermi momentum correction)
Naive expectation :
Deuteron: binding energy ~2 MeV
Nucleons
Average nucleons separation ~2 fm
Question 1:
Is there an ‘EMC effect’ in Deuterium ?
σdDIS=σp
DIS+σnDIS?
DIS off a deuteron = DIS off a free proton neutron pair
DIS off a bound nucleon = DIS off a free nucleon
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Q2=−qμq
μ=q2−ω2
ω=E'−E
xB= Q2
2mω
xB gives the fraction of nucleon momentum carried by the struck parton
Deep InelasticScattering (DIS)
E E`
(ω,q)
nucleon
Final state Hadrons
W2
Incident lepton
scattered lepton
Nucleons
E E`
(ω,q)
nucleus
Incident lepton
scattered lepton
xB counts the minimum number of nucleons involved
xB>1 xB>2
2N-SRC 3N-SRC
Inclusive electron scattering A(e,e’)
xB>1 determines minimum pmiss
0≤xB≤1 0≤x B≤A
→sensitive to the high momentum tail of the nuclear wave function→scaling
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Q2=−qμq
μ=q2−ω2
ω=E'−E
xB= Q2
2mω
xB gives the fraction of nucleon momentum carried by the struck parton
Deep InelasticScattering (DIS)
E E`
(ω,q)
nucleon
Final state Hadrons
W2
Incident lepton
scattered lepton
Nucleons
E E`
(ω,q)
nucleus
Incident lepton
scattered lepton
xB counts the minimum number of nucleons involved
Inclusive electron scattering A(e,e’)
0≤xB≤1 0≤x B≤A
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Plateau shows same high-p distributions
K. Sh. Egiyan et al. PRL. 96, 082501 (2006)
1-2% probability for 3N-SRC
JLab CLAS A(e,e') Result
K. Sh. Egiyan et al. PRC 68, 014313 (2003)
20% probability for 2N-SRC in 12C
More A/d data:SLAC D. Day et al. PRL 59,427(1987) JLab. Hall C E02-019
4He/3He
12C/3He
56Fe/3He
Scaling
Scale factors give relative probabilities for SRC
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The probability for a nucleon to have p ≥ 300 MeV/c in medium nuclei is 20-25%
More than ~90% of all nucleons with p ≥ 300 MeV/c belong to 2N-SRC.
2N-SRC dominated by np pairs
Three nucleon SRC are present in nuclei
PRL. 96, 082501 (2006)
PRL 162504(2006); Science 320, 1476 (2008)
1
2
3
1
4
2
3
4
~80% of kinetic energy of nucleon in nuclei is carried by nucleons in 2N-SRC.
1
2
More on 2N-SRC from inclusive and exclusive data
EV
A /
BN
LJL
ab /
HA
LL-A
CLA
S /
HA
LL-B
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Where is the EMC effect ?
High local nuclear matter density, large momentum, large off shell. large virtuality ( )
Largest attractive forceMean field
SRC
OR
ν=p2−m2
80% nucleons(20% kinetic energy)
20% nucleons(80% kinetic energy)
np
ppnn
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Where is the EMC effect ?
High local nuclear matter density, large momentum, large off shell. large virtuality ( )
Largest attractive forceMean field
SRC
OR
ν=p2−m2
80% nucleons(20% kinetic energy)
20% nucleons(80% kinetic energy)
np
ppnn
Question 2:
Is the EMC effect predominantly associated withhigh momentum nucleons?
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EMC
SRC Scaling factors XB ≥ 1.4
L. B. Weinstein et al. PRL. 106, 052301 (2011)
Slo
pes
0.3
5 <
xB <
0.7
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EMC
SRC Scaling factors XB ≥ 1.4
L. B. Weinstein et al. PRL. 106, 052301 (2011)
Slo
pes
0.35
< x
B <
0.7Possible explanation for EMC / SRC correlation
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SRC=0 free nucleons
a2N (Fe /d )ASRC
Question 1:
Is there an ‘EMC effect’ in Deuterium ?
σd
σp+σn
(x=0.6)= 0.975
0.079±0.06
σdDIS=σp
DIS+σnDIS
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SRC=0 free nucleons
a2N (Fe /d )ASRC
Question 1:
Is there an ‘EMC effect’ in Deuterium ?
σ p*
σ p
≈ σ n*
σ n
≈ 2.5%
5%≈ 50%0.5
σd
σp+σn
(x=0.6)= 0.975
0.079±0.06
σdDIS=σp
DIS+σnDIS
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SRC=0 free nucleons
σ d≠σ p+σn
a2N (Fe /d )ASRC
Question 1:
Is there an ‘EMC effect’ in Deuterium ?
σ p*
σ p
≈ σ n*
σ n
≈ 2.5%
5%≈ 50%0.5
σd
σp+σn
(x=0.6)= 0.975
0.079±0.06
EMC
Question 3:
Is there a large ‘EMC effect’ in tagged DIS off Deuterium ? Is the In-Medium structure function momentum dependent?
σdDIS=σp
DIS+σnDIS
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Question 4:
How does the nucleon structure function F2 depend
on the nucleon virtuality ?
Note: Other models predict no dependence on virtuality
PLC suppression
α s = (Es − psz) /ms
Rescalingmodel
Binding/off shell
Z. Phys. A359 (1997) 99
Phys. Lett. B 335, 11 (1994)
Phys. Lett. B 356, 157 (1995)
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Theory Report
We Agree :)
Now: can we do it ?
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Measurement technique
1. Spectator Tagging:d(e,e'N
s), DIS in coincidence with a
fast, backwards, recoil nucleon. Selects DIS off high momentum (high virtuality) nucleons
x'=Q2
2pμqμ
Goal: Measure DIS off high p nucleon
W ' 2=(qμ
+pdμ−ps
μ)
2
ν=p2−M p2
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Measurement technique
1. Spectator Tagging:d(e,e'N
s), DIS in coincidence with a
fast, backwards, recoil nucleon. Selects DIS off high momentum (high virtuality) nucleons
2. cross sections ratio Minimize experimental uncertainties
σDIS( xhigh' ,Q1
2 , p⃗s )
σDIS( xlow' ,Q2
2 , p⃗s )
xhigh'
≥0 . 45 0 . 25≥x low'
≥0. 35(No ‘EMC effect ‘ is expected)
x'=Q2
2pμqμ
Goal: Measure DIS off high p nucleon
W ' 2=(qμ
+pdμ−ps
μ)
2
ν=p2−M p2
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Measurement technique
1. Spectator Tagging:d(e,e'N
s), DIS in coincidence with a
fast, backwards, recoil nucleon. Selects DIS off high momentum (high virtuality) nucleons
ν=p2−M p2
2. cross sections ratio Minimize experimental and theoretical uncertainties
=F2
bound( x high
' ,Q12 , p⃗s )
F 2free
( xhigh ,Q12)
⋅σDISfree
( x low ,Q22)
σDISfree
( xhigh ,Q12)⋅RFSI
σDIS( xhigh' ,Q1
2 , p⃗s )
σDIS( xlow' ,Q2
2 , p⃗s )
xhigh'
≥0 . 45 0 . 25≥x low'
≥0. 35(No ‘EMC effect ‘ is expected)
x'=Q2
2pμqμ
RFSI is the FSI correction factor
Goal: Measure DIS off high p nucleon
W ' 2=(qμ
+pdμ−ps
μ)
2
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d(e,e'ps)
Obstacles (FSI)
Increase with W’
Decrease with Q2
Not sensitive to x’
* Collect data at very large recoil angles (small FSI) and at ~900 (large FSI)
* look at ratios of two different x’
* Use the low x’ large phase space to check / adjust the FSI calculations(Study the dependence of FSI on Q2, W' and θ
pq)
* Get a large involvement of theoretical colleges at all stages of proposal, measurement, analysis
θpq
>107o 72o<θpq
<107o
What do we know about FSI:
How are we going to minimize (correct for) FSI:
PdPd PdPd
p or n p or n
Small for θpq
>107oDEEPS, PRC 73, 035212 (2006)
PWIA PWIA
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Experimental setup - Hall-C
SHMS HMS
beam
LAD
e’e’
p/n GEM
10 cm LD2 target
LAD
SHMS
HMS
beam
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Large Acceptance Detector (LAD)
Use retired CLAS-6 TOF counters.132, 5-cm thick counters in 12 panels.1.5 sr, ~20% neutron detection efficiency
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GEM based Vertex cutDominated by Multiple Scattering
UVA group has experience and is interested in developing the GEMs for this experiment
Assuming a 0.5-1 cm vertex reconstruction resolutionImproves (e,e'p
s) S/BG by
a factor of 2-4
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Proton Detection
Momentum resolution (300-500MeV/c):
Use Energy loss and TOF to identify particles
and reject accidentals
∆pp
= ∆TOFTOF
= 0.250ns
(50 − 33)ns= 0.5 − 0.8%
Singles measured at 90o in Hall-A
Overestimates background at larger angles
Detailed signal to BG simulations
S/BG
Threshold
200 MeV/c
300 MeV/c
400 MeV/c
500 MeV/c
TOF [ns/meter]
E
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Neutron Detection
5 LAD layers
Veto charged particles using GEM and first layer
5 MeVee threshold reduces n and γ background
Done in Hall-A and B with scintillator detectors
Detailed, bin by bin, background simulation, based on Hall-C singles neutron measurements and simulations
1:200 S/BG ratio at high x' Cut on x' and W' Remove worst bins
Cut on θpq
>110o
1:20 S/BG ratio at high x' Subtract random background with mixed events
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Kinematics: xB Vs. x'
B
Moving to the Struck Nucleon Rest Framex'=
Q2
2pμqμ
x=Q2
2mω
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Kinematics
Recoil Nucleon
Scattered Electron
virtuality
Ps [G
eV/c]
x’B>0.5
Q2>2 W’>2
x’B<0.35
E’ [G
eV]
θe' [deg . ]
Q2>2 W’>2
θqp [deg . ]
Ps [
GeV
/c]
Ps [GeV/c]
X’B
x'=Q2
2pμqμ
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Beam Time Request
• Setup and Calibration: 6 days
• Production:– SHMS: low x’B HMS: high x’B 300 hours
– SHMS: high x’B HMS: low x’B 300 hours
– SHMS: high x’B HMS: high x’B 210 hours
Total Production Time: 34 days[Determined by the (e,e'p
s) statistics]
• Total Beam Time: 40 Days
• PAC approval will justify the effort of intact removal of LAD counters
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Expected Results
d(e,e’ps)
α s = (Es − psz) /ms
Systematic Uncertainties (4-7% total):– SHMS and HMS efficiency and acceptance (1-2%)
– LAD efficiency (3% protons, 5% neurons)
– Al walls subtraction (1%)
– FSI ratio (4%)
– Free nucleon structure function ratio (1% protons, 4% neutrons)
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Expected Results
d(e,e’ps)
Systematic Uncertainties (4-7% total):– SHMS and HMS efficiency and acceptance (1-2%)
– LAD efficiency (3% protons, 5% neurons)
– Al walls subtraction (1%)
– FSI ratio (4%)
– Free nucleon structure function ratio (1% protons, 4% neutrons)
α s = (Es − psz) /ms
d(e,e’ns)
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summery
A direct measurement of theA direct measurement of the
nucleon structure function in the nuclear mediumnucleon structure function in the nuclear medium
as a function of its virtuality / momentumas a function of its virtuality / momentum
Is it modified?
Can it explain the EMC effect?
How is it related to short range correlated nucleons?
This is not a EMC measurement. A further EMC measurement is proposed in LOI 11-104
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Thank You!Thank You!
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EMC-SRC correlationEMC-SRC correlation
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EMC slope
SRC scaling factor
Comparing the magnitude of the EMC effect and the SRC scaling factors
σ Fe
σ d
dREMC
dx
a2N (Fe /d )
Frankfurt, Strikman, Day, Sargsyan, Phys. Rev. C48 (1993) 2451. Q2=2.3 GeV/c2
Gomez et al., Phys. Rev. D49, 4348 (1983). Q2=2, 5, 10, 15 GeV/c2 (averaged)
SLAC data:
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Comparing the EMC and SRC strengths
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Virtuality dependent mediumVirtuality dependent mediummodification of the form factor ratiomodification of the form factor ratio
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Medium modification of form factor ratios
Medium modification of the proton's form factor ratio (G
e/G
m) observed
in polarization transfer measurements
The observed modification grows as a function of nucleon virtuality
PR11-107 will cover a much larger virtuality range of ~ 0.2-0.5 (GeV/c2)2
M. Paolone, et al., Phys. Rev. Lett. 105, 072001 (2010)
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Pion BackgroundPion Background(response to TAC report)(response to TAC report)
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Pion BackgroundCLAS EG2 data
Pi:Proton = 3:1
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Pi:Proton = 3:1
Pion BackgroundHall-A E07-006 (SRC) data, BigBite at 92o no magnetic field
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Pion BackgroundSimulations by Pavel Degtiarenko
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Pion Background
Backwards pion to proton ratio is ~1:5Pions are a problem only in they nuclear interact within the
LAD scintillator countersThe (pi,p) cross section drops for low energy pion
Backwards pions are not an issueBackwards pions are not an issue
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Neutron singles RatesNeutron singles Rates(response to TAC report)(response to TAC report)
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Neutron Singles Rates
Singles Measurementsat Hall-C
Hall-C singles neutronmeasurements are consistent
with the simulations (~106 Hz/sr for our luminosity)
Simulations by Pavel Degtiarenko
3X larger luminositythan PR11-107 E01-015 proposal, December (2000)
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Neutron Detection EfficiencyNeutron Detection Efficiency
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Neutron Detection Efficiency
5 MeVeeThreshold
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SHMS, HMS, and LADSHMS, HMS, and LADcalibration plancalibration plan
(response to TAC report)(response to TAC report)
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SHMS, HMS and LAD calibration plan
Final calibration run plan is dependent on the final LAD design and flexibility. From our experience with the exclusive SRC experiments (E01-015 and E07-006) we expect these measurements to include: Standard spectrometers calibrations.
Neutron detection efficiency measurement using kinematically complete d(e,e'pn) measurements with the electron and proton detected by the spectrometers and the neutron by LAD.
H(e,e’p) measurements with the electron being detected by the spectrometers and well defined (energy and angle) protons by LAD.
(Will be used for TOF, energy loss, threshold, and coincidence times measurements)
Al Dummy target to get the target cell window contribution.
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KinematicsKinematics
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Electron Kinematics
12 GeV needed for kinematicalrange and higher cross section
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LAD Phase Space Coverage
SHMSHMS
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
SHMSHMS
SHMSHMS
SHMSHMS
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
SHMSHMS
SHMSHMS
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
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Phase Space Coverage (W'>2, Q2>2, θpq
>110o)
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Analysis ExampleI – W' Dependence
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Analysis ExampleII – P
recoil Dependence
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Analysis ExampleIII – x'
B Dependence
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LAD DrawingsLAD Drawings
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LAD Drawings
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LAD Drawings
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LAD Drawings