Quasi-elastic 3 He(e,e’p) experiment (E89-044) at Jefferson Lab :
description
Transcript of Quasi-elastic 3 He(e,e’p) experiment (E89-044) at Jefferson Lab :
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
1July, 7th, 2004
Quasi-elastic 3He(e,e’p) experiment (E89-044) at Jefferson Lab :
study of the 2-bbu parallel kinematics.
E. Penel - Nottaris
Expérience E89-044 de diffusion quasi-élastique sur l’3Heau Jefferson Laboratory :
analyse des sections efficaces 3He(e,e’p)den cinématique parallèle.
Hall A collaboration
2 other PhD students : F. Benmokhtar and M. Rvachev
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
2July, 7th, 2004
Electromagnetic probe
- interaction described by QED- electron is a point like particle- small coupling (Z1)- kinematical flexibility
(e,e’p) experiments study the nucleon inside the nucleus
- energy and momentum distribution of nucleon- electromagnetic properties of bound proton
3He nucleus- exact calculations for 3-body systems- ingredients of complex nuclei
NN and 3-body forcesShort range correlationsRelativistic effects
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
3July, 7th, 2004
Plane Wave Impulse Approximation- absorbed by the detected nucleon- independent particles model for the nucleus- particles described by plane waves.
misspp )p,S(E
dΩ
σd
dE'dΩdΩ
σdmissmiss
e'
ep2
p'e'
5
ep : electron-(off shell) proton elastic cross section
Born Approximation : one photon exchange
S(Emiss, pmiss) : spectral function
of 3He
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
4July, 7th, 2004
• 2-body-break-up : 3He(e,ep)d
Emiss = 5.5 MeV
• 3-body-break-up : 3He(e,ep)pn
Emiss 7.7 MeV
Emiss = Mp + Mrecoil – M3He
Missing energy :
Emiss = - Tp - Tr
Emiss (MeV)
2.2 MeV energy separation between the 2 processes
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
5July, 7th, 2004
misspp
)p',p,(ESdΩ
σd K
de'dΩdΩ
σdmissmiss
D
e'
ep2
p'e
5
• Meson Exchange Currents (MEC) and Isobaric Currents (IC) :
• Exchange term :• Final State Interactions (FSI) :
• modify the extracted nuclear information• involve more general cross-section formulation
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
6July, 7th, 2004
• Virtual photon polarization :
- h=0 longitudinal polarization
- h=1 transverse polarizations
qh=0 ε
qh=-1
ε
qh=+1
ε
TT
LT
σ
σinterference terms
Lσ : longitudinal response function coupling to nuclear charge
Tσ : transverse response function coupling to nuclear transverse current
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
7July, 7th, 2004
• Parallel kinematics :
q//pmiss
)cos2 εcos 1)ε(ε εΓ(dE'dΩdΩ
σdTTLTLT σσσσ
p'e
5
ε1
1
Q
q
E
E'Γ
20
)
2
θtan
Q
q2(1ε e2
2
2
) εΓ(dE'dΩdΩ
σdL
p'e
5
σσT pmiss
p’
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
8July, 7th, 2004
)ε(εΓΓ
σ εΓσ εΓσ
)ε(εΓΓ
σ Γσ Γσ
BwFwBwFw
BwFwFwFwBwBwT
BwFwBwFw
BwFwFwBwL
pmiss
(MeV/c)
q
(GeV/c)Fw - Bw
0 1.0 0.7
0 1.5 0.7
0 2.0 0.6
0 3.0 0.5
- 300 1.0 0.4
- 300 2.0 0.7
+ 300 1.0 0.6
• Extracting the response functions :
- forward electron angles : Fw (Fw 1)
- backward electron angles : Bw (Bw 0)at fixed hadronic vertex variables
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
9July, 7th, 2004
- Coincidence experiment => 100% duty cycle- High luminosity (1038 cm-2 s-1) => high beam current and target density-Identification of processes separated by 2.2 MeV at momenta of few GeV => low beam energy dispersion (2.10 -5) and high momentum resolution (2.10 -4)
Jefferson Lab Hall A Basic Equipment
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
10July, 7th, 2004
Duty cycle 100 %
Beam energy 0.8 – 6 GeV
Energy dispersion 2.5 10-5
Beam emittance 2 10-9
Beam current 200 A
Frequency = 1497 MHz 499 MHz in the halls
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
11July, 7th, 2004
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
12July, 7th, 2004
High density : T = 6.3 K P 7.6 or 11 atm = 0.055 or 0.070 g.cm-3
• Density measurements :
- temperature and pressure sensors + state equation of 3He
- elastic electron scattering on 3He at each beam energy
Cylindrical target (tuna can) : = 10.3 cm
Preliminary normalization by density from sensorsSystematic error on density from sensors : 7 %
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
13July, 7th, 2004
• Luminosity monitoring
charge
-e singles nb.rate
L
• Target density stability : max. fluctuation < 3% ( 0.6 %)
corrected for dead time and prescales
refrate_ref
rate ρρL
L
density of the 1st run
density from luminosity monitoring density from P and T sensors
run number
rela
tive
den
sity
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
14July, 7th, 2004
Acceptance Resolution
Momentum ± 5 % 2.5 10-4
Horizontal angle 30 mrad 2.0 mrad
Vertical angle 65 mrad 6.0 mrad
Separates momentum resolution (vertical plane) from vertex position resolution (horizontal plane)
45° vertical deflexion
(FWHM)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
15July, 7th, 2004
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
16July, 7th, 2004
pe > 17 MeV/cp > 4.8 GeV/c
Relative calibration by analysis software
Gas Cerenkov detector Shower counters
Absolute gains calibration (pe = 3581 MeV/c)
preshower and shower counters
-
-
e-e-
Cerenkov (channel) preshower + shower (MeV)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
17July, 7th, 2004
Two planes of 6 scintillator paddles in each arm : S1 and S2 planes
Trigger electronics :
- Coincidence between the 2 PM of the hit paddle.
Single event
S1 & S2 & 45° track
Relative calibration by analysis software
Coincidence event
Electron event & Hadron eventS1 ADC (channel) S1 ADC (channel)
xrot (m)
S1
AD
C (
chan
nel)
S1
AD
C (
chan
nel)
xrot (m)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
18July, 7th, 2004
VDC tracks detector variables
Spectrometer focal plane variables
Spectrometer target variables
Vertex variables
detector position offsets / focal plane
spectrometer absolute position / hall
spectrometer optics tensor + beam position
• In each detection arm :
)Φ , y,θ ,(xfpfpfpfp
δ) ,Φ , y,θ ,(xtgtgtgtg
variableslkinematica
(react_z) positionvertex
)Φ , y,θ ,(xdetdetdetdet
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
19July, 7th, 2004
ztg
ytg
beam
scattered e-
tg
ytg
react_z
target
Transverse position tensor coefficients optimized from vertex position along beam line (react_z)
Scattering off 4 targets : - carbon foil at z = 0 - aluminum foils at z = ± 2 cm
z = ± 5 cm z = ± 7.5 cm
zlab
ylab
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
20July, 7th, 2004
before after
Low electronmomentum
High protonmomentum
hadron react_z (cm) hadron react_z (cm)
Ph = 2999 MeV/c
Ph = 1295 MeV/c
electron react_z (cm)
Pe = 694 MeV/c
Pe = 3850 MeV/c
electron react_z (cm)electron react_z (cm)
hadron react_z (cm)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
21July, 7th, 2004
Momentum tensor coefficients optimized on missing energy spectra : remove dependence on dispersive variables (xfp, fp)
Em
iss (
MeV
)
Em
iss (
MeV
)
hadron rot (rad) hadron rot (rad)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
22July, 7th, 2004
- May not point at the hall center- Angle orientation may be different from floor marks
Use scattering off carbon foil at z = 0
electron react_z (mm) electron react_z (mm)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
23July, 7th, 2004
- Background rejection => experimental 3He(e,e’p) events
- 2-bbu and 3-bbu separation- Radiative corrections- Phase space calculation=> Monte Carlo Simulation
Data Analysis and Simulation
=> Simulated 3He(e,e’p) events
3He(e,e’p)dCross-sections=>
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
24July, 7th, 2004
• Corrected time of coincidence : tc_cor
Time of coincidence window width = 12 ns
2 ns beam structure
resolution 0.6 ns
tc (ns) tc_cor (ns)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
25July, 7th, 2004
signal in the Cerenkov detector+ signal in the showers
e-
-
-
e-
shower (MeV)
pres
how
er (
MeV
)
shower (MeV)
pres
how
er (
MeV
)
tc_cor (ns)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
26July, 7th, 2004
| react_z | < 4 cm cut on the arm with best resolution on react_z
| react_ze arm – react_zh arm | < 2 cm
electron react_z (cm) electron react_z - hadron react_z (cm)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
27July, 7th, 2004
p
d
+
before cuts after cuts
No need to remove deuterons or pions
hadron hadron
hadr
on S
2 A
DC
hadr
on S
2 A
DC
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
28July, 7th, 2004
pmiss
bq
p'pq
q
Parallel configuration : q//pmiss
Cone aperture = 45 °
bq (°) bq (°)bq (°)
pmiss=+300 MeV/cpmiss=0 MeV/c pmiss=-300 MeV/c
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
29July, 7th, 2004
Subtraction of missing energy spectra :accidbbu-2
12/50 – SS
12nsΔt
50nsΔtΔt
bbu2
f2f1before accidental subtractionafter accidental subtraction
tc_cor (ns) Emiss (MeV)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
30July, 7th, 2004
Emiss (MeV)Emiss (MeV)
Emiss (MeV) Emiss (MeV)
pmiss = 0 MeV/c
pmiss = +300 MeV/c
forward backward
forward backward
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
31July, 7th, 2004
• Limit simulated and experimental phase space to the same volume
• Optimize statistics by considering maximal phase space volume
Cuts on target variables :
tgtgtgy,Φ ,θ δ,
(same cuts for both arms)
ytg (m) tg (rad)
tg (
rad)
tg (
rad)
tg (
rad)
tg (
rad)
(R-function defined by M. Rvachev)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
32July, 7th, 2004
• Angular resolutions : FWHM tg = 2 mrad
FWHM tg = 4 mrad
• Transverse position resolution : fitted from ytg distributions on scattering off carbon foils data
1.4 mm < FWHM ytg < 9.7 mm
Carbon foil data Quasi-elastic 3He data
data simulation
ytg (mm)electron react_z - hadron react_z (cm)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
33July, 7th, 2004
• Adjusted in the simulation to get same resolution on missing energy for 2-bbu as experimental resolution same momentum resolution for electron and hadron arms.
kin # FWHM
16 4.8 10-4
01 4.0 10-4
18 4.8 10-4
20 5.2 10-4
22 6.2 10-4
24 5.2 10-4
26 4.3 10-4
kin # FWHM
17 6.5 10-4
03 6.3 10-4
19 5.8 10-4
21 4.4 10-4
23 7.0 10-4
25 6.5 10-4
27 8.0 10-4
4 10-4 < FWHM < 8 10-4
data simulation
Emiss (MeV)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
34July, 7th, 2004
’
By fitting simulated missing energy spectrum to experimental data
• takes into account 3-bbu contribution (1 % systematic error on subtraction)• simulates energy losses and radiative effects• extracts unradiated cross-section averaged on phase-space
Two theoretical models :
- unit cross-section
- PWIA model )S(pσdΩdΩde'
σdmisscc1
pe
5
Emiss (MeV)
Emiss (MeV)
data
simulation
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
35July, 7th, 2004
• Experimental data analysis shows reliable background control and pretty good transport variables resolutions
• Simulation reproduces rather well kinematical variables resolutions => used to extract unradiated cross-section averaged on phase-space
• Possible improvements could come from spectrometer optics optimization, simulated resolutions and absolute normalization by density from elastic data.
• Systematic error on preliminary cross-sections is 8.8 % (mainly due to target density)
Preliminary results
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
36July, 7th, 2004
De Forest / Salme PWIALaget PWIALaget full calculation
pmiss (MeV/c) pmiss (MeV/c)cr
oss-
sect
ion
(b.
MeV
-1.s
r-2)
cros
s-se
ctio
n (
b.M
eV-1.s
r-2)
Backwardelectron angles
Forward electron angles
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
37July, 7th, 2004
De Forest / Salme PWIALaget PWIALaget full calculation
Pmiss (MeV/c)
cros
s-se
ctio
n (
b.M
eV-1.s
r-2)
Pmiss (MeV/c)
cros
s-se
ctio
n (
b.M
eV-1.s
r-2)
Salmewave function Urbanna
Paris
Forward electron angles
Backward electron angles
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
38July, 7th, 2004
De Forest / Salme PWIALaget PWIA
Pmiss (MeV/c)
cros
s-se
ctio
n (
b.M
eV-1.s
r-2)
Pmiss (MeV/c)
cros
s-se
ctio
n (
b.M
eV-1.s
r-2)
Salmewave function Urbanna
Paris
Forward electron angles
Backward electron angles
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
39July, 7th, 2004
• and q matching for forward and backward kinematics• 50 MeV/c pmiss bins• achieving forward and backward cross-sections
De Forest / SalmePWIA
Sensitivity to interference terms and imperfect (, q) matching
Pmiss (MeV/c) Pmiss (MeV/c)
L (b
.sr-2
)
T (b
.sr-2
)
E. Penel-Nottaris
Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
40July, 7th, 2004
•Preliminary results show unexpected effects for forward electron angles kinematics at pmiss = 0 and rather good agreement for the other kinematics that should constraint theoretical models.• Elastic data analysis would allow final cross-sections extraction.• Longitudinal and transverse separation looks promising
• Very interesting results on perpendicular kinematics (2-bbu and 3-bbu) that constrained models.
• Other experiments at Jlab study few body interactions models through (e,e’p)
Overview on E89-044 resultsParallel kinematics