Download - P REX II and CREX
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1/33CREX Workshop Jefferson Lab March 16-19, 2013
PREX II and CREX
Juliette Mammei
208Pb
NASA/CXC/SAO
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2/33CREX Workshop Jefferson Lab March 16-19, 2013
PREX II and CREX
Theory from P. Ring et al. Nucl. Phys. A 624 (1997) 349
208Pb more closely approximates infinite nuclear matter
The 48Ca nucleus is smaller, so can be measured at a Q2 where the figure of merit is higher
and are expected to be correlated, but the correlation depends on the correctness of the models
The structure of 48Ca can be addressed in detailed microscopic models
208nR
48nR
48nR
Measure both and - test nuclear structure models over a large range of A 208nR
48nR
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3/33CREX Workshop Jefferson Lab March 16-19, 2013
Problems during PREX I
• Repeated failures of scattering chamber attachment o-ring – Solution: all metal seals
• Damage to electronics from radiation in Hall– Solution: More rad-hard electronics, better locations Improved shielding design
• Eventual failures of the individual lead targets– Solution: Run with 10 targets!
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4/33CREX Workshop Jefferson Lab March 16-19, 2013
collimator
Downstream face of scattering chamber attachment
Beam pipe through septum
Magnetic shield
Collimator regionThe Enterprise
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5/33CREX Workshop Jefferson Lab March 16-19, 2013
Extend magnetic shield as far upstream and downstream as we can
Metal seals
Decrease the collimator inner diameter and water cool it
Electronics throughout hall replaced and/or moved
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6/33CREX Workshop Jefferson Lab March 16-19, 2013
Background simulations
Geometry in modelled in GEANT4
Physics lists:
• QGSP_BERT_HP
Bertini cascade model for protons, neutrons, pions and kaons (below 10 GeV)
Data driven high precision neutron package to transport neutrons below 20 MeV down to thermal energies
• Standard EM Physics photo- and electro-nuclear (equivalent photon approximation for the latter)
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7/33CREX Workshop Jefferson Lab March 16-19, 2013
Origin of photons hitting a “plane” detector downstream of the septum
Qualitative improvementPREX IPREX II
Collimator bore was not small enough in PREX I to eliminate sources at the end of beampipes; quadrupole field in beampipe exacerbates the problem
decreasing the bore eliminates sources downstream
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8/33CREX Workshop Jefferson Lab March 16-19, 2013
Neutron Energy Spectra
1<E<10 MeV (0.1 MeV bins)
10<E<1050 MeV (10 MeV bins)
0<E<1 MeV (0.01 MeV bins)
“unshielded” neutron rates go up a bit with new bore
Source is localized …
Shield it!
PREX II neutron rates 10x smaller than PREX I
Neu
tron
s per
inci
dent
ele
ctro
n
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9/33CREX Workshop Jefferson Lab March 16-19, 2013
Target PerformanceThree targets, with thin, medium and thick diamond (~0.15 mm) backing on a 0.5 mm thick Pb sheet
Cooled with liquid He (30 W)
Over time, the targets developed thickness non-uniformities which resulted in correlated noise between detectors
→ Synchronize raster to the helicity frequency!
Not synched Synched
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10/33CREX Workshop Jefferson Lab March 16-19, 2013
Target PerformanceX
positi
on o
f ras
ter
Y position of raster
Counts
Targets with thin diamond backing (4.5% bkgd) degraded fastest
Thick diamond (8% bkgd) ran well and did not melt – even at 70 uA!
Trade-off between length of time the target can be used and the amount of bkgd
Solution: Run with 10 targets
(slope from Pb FF)
raster
MELT
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11/33CREX Workshop Jefferson Lab March 16-19, 2013
CREX
• Target design (10x more power – 360 W)• Optimization of the kinematics• Septum design• Backgrounds from 1st excited state (tails larger than in PREX)• Radiation in Hall
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12/33CREX Workshop Jefferson Lab March 16-19, 2013
Target Design
Preliminary
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13/33CREX Workshop Jefferson Lab March 16-19, 2013
22RAFOM
KinematicsPlots vs. central anglebeam energy 2.2 GeV (scaled PREX acceptance)
Asymmetry (ppm)
Rate (Hz) δR (fm)
δA/A(δR/R ~1%)
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14/33CREX Workshop Jefferson Lab March 16-19, 2013
Septum
Same design as for PREX II, but at a higher current density - 1350 A/cm2
With proper cooling, this is not a problem(coils can be run at least as high as 1430 A/cm2)
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15/33CREX Workshop Jefferson Lab March 16-19, 2013
Backgrounds from excited states
We will have a 0.9% background from excited states
Improvement in the hardware optics resolutions will reduce this amount
Assuming calculated Aine~ Aela (with 50% error)→ systematic error contribution = 0.5%
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16/33CREX Workshop Jefferson Lab March 16-19, 2013
Radiation in the Hall
Power from all particles per incident electron for 5% Ca and 8.9% Pb targets.
Backgrounds from radiation in hall are 10x smaller than PREX II
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17/33CREX Workshop Jefferson Lab March 16-19, 2013
PREX II and CREX
Table 1 –Proposed data for PREX II and CREX.
Table 2 –Systematic errors for PREX II and CREX.
These numbers are based on experience from PREX-I
C-REX is a standard energy (2.2 GeV)1-pass beam is easy to schedule – standard equipment (HRS, etc.)
48nR
208nR ±0.05 fm
± 0.03 fm
Uncertainty in:
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18/33CREX Workshop Jefferson Lab March 16-19, 2013
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19/33CREX Workshop Jefferson Lab March 16-19, 2013
Spokespeople
PREX IIK. Kumar R. MichaelsK. PaschkeP.A. SouderG.M. Urciuoli
CREXJ. MammeiR. MichaelsK. PaschkeS. RiordanP.A.SouderD. McNulty
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20/33CREX Workshop Jefferson Lab March 16-19, 2013
Extra Slides
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21/33CREX Workshop Jefferson Lab March 16-19, 2013
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22/33CREX Workshop Jefferson Lab March 16-19, 2013
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23/33CREX Workshop Jefferson Lab March 16-19, 2013
Incident particle:
1 GeV (p or e-)
Damage-weighted energy spectra
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24/33CREX Workshop Jefferson Lab March 16-19, 2013
Physics Lists
"Like QGSP, but using Geant4 Bertini cascade for primary protons, neutrons, pions and kaons below ~10GeV. In comparison to experimental data we find improved agreement to data compared to QGSP which uses the low energy parameterised (LEP) model for all particles at these energies. The Bertini model produces more secondary neutrons and protons than the LEP model, yielding a better agreement to experimental data. "
QGSP is the basic physics list applying the quark gluon string model for high energy interactions of protons, neutrons, pions, and kaons and nuclei. The high energy interaction creates an exited nucleus, which is passed to the precompound model modeling the nuclear de-excitation.
data driven high precision neutron package (NeutronHP) to transport neutrons below 20 MeV down to thermal energies.
http://www.slac.stanford.edu/comp/physics/geant4/slac_physics_lists/ilc/LHEPlistdoc.html
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25/33CREX Workshop Jefferson Lab March 16-19, 2013
46
2524.638
17.018
R = 3.0
o-ring nominal dimensions shown; septum o-ring extends ±1 cm and sc o-ring extends ±0.5 cm around that in plane, and both are 2 cm thick in the z direction
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26/33CREX Workshop Jefferson Lab March 16-19, 2013
85.82214.351
collimator
septum o-ring scattering chamber o-ring
flange(Al – PREX I, SS – PREX II )
plane detectorplane detector
septum
vacuum attachments
hut(polyethylene)
cylinder(polyethylene)
target
opening in scattering chamber
septum pipe
52.075.08
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27/33CREX Workshop Jefferson Lab March 16-19, 2013
Possible Future Program
Nucleus E (GeV) dRN / RN
208Pb 1 1 %
48Ca 2.2 (1-pass) 0.4 %
48Ca 2.6 2 %
40Ca 2.2 (1-pass) 0.6 %
tin isotope 1.8 0.6 %
tin isotope 2.6 1.6 %
Each point 30 days, statistical error only
Not yet proposed
Shufang Ban, C.J. Horowitz, R. Michaels J. Phys. G39 014104 (2012)
• relate the measurement to 3-nucleon forces (other nuclei)• and constrain the surface thickness (add’l higher energy point)
Additional measurements would allow us to:
To be proposed
Approved
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28/33CREX Workshop Jefferson Lab March 16-19, 2013
PREx Apparatus
YYYYAmeas