large acceptance detector (lad) for 12 gev hall c
DESCRIPTION
Large Acceptance Detector (LAD) for 12 GeV Hall C. Exclusive measurements of Short Range Correlations and more. Physics opportunities in Hall C at 12 GeV. Hall C Meeting, Monday, August 4, 2008 Jefferson Lab, Newport News, VA USA. Eli Piasetzky. Tel Aviv University, ISRAEL. - PowerPoint PPT PresentationTRANSCRIPT
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Large Acceptance Detector (LAD) for 12 GeV Hall C
Eli Piasetzky
Tel Aviv University, ISRAEL
Hall C Meeting, Monday, August 4, 2008 Jefferson Lab, Newport News, VA USA
Physics opportunities in Hall C at 12 GeV
Exclusive measurements of Short Range Correlations and more
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e
e’
p,π,…
*
Large solid angle multi particle (charged and neutral) detector
HMS
SHMS
Coverage of a large fraction of the hemisphere (“backward” =4π-forward) consistent with the forward spectrometers.
Ability to detect multi-charge particles with good PID and moderate momentum resolution.
Ability to detect neutrons with high efficiency.
Ability to operate at a luminosity of 1036-1038 cm-2 sec-1 (10-1000 times the planned luminosity for CLAS).
Large Acceptance Detector (LAD)
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The physics driving the LAD detector
Short Range Correlations (SRC)
EMC
Hadronization
Study of GPDs
Nuclear Matter in non - equilibrium condition
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np-SRC dominance ~18 %
12C
Results (summary)
The uncertainties allow a few percent of:
more than 2N correlations
Non - nucleonic degrees of freedom
2N –SRC dominance
18±5%
1±0.3%
12C
Sensitivity required fo the next generation of SRC measurements 0.1 – 1 % of (e, e’ p).[(0.5-5)% of (e,e’p) with Pmiss>300 MeV/c]
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19±4%0.6±0.2%
2N
3N
PR 08-14 / PAC 33
1N >> 2N - SRC >> 3N – SRC.
cure
XB>2
or
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~800 MeV/c~800 MeV/c
~400 MeV/c~400 MeV/c
star geometry
Colinear geometry :
From (e,e’p) + N to (e,e’p)+2N
Exclusive measurement:
From
triple coincidence (2N SRC)
to
4 fold coincidence (3N SRC)
Needs large acceptance multi particle detector
Need to detect two recoil nucleons
0.3-1 GeV/c p and n
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•Are the nucleons in the SRC pair different from free nucleons (e.g size,shape, mass, etc.) ? Are they nucleons ?
For a 1 fm separation, the central density is about 4 times the nuclear central density
1.f
Nucleons
2N-SRC 4o
~1 fm
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Looking for non-nucleonic degrees of freedom
The signature of a non-nucleonic SRC intermediate state is a large branching ratio to a non-nucleonic final state.
... cba NNNSRC
1c,...b, ,0 a
Breaking the pair will yield more backward Δ, π , k
1.f
Nucleons
2N-SRC 5o
~1 fm
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Looking for non-nucleonic degrees of freedom
Expected Δ’s rates 5-10% of recoil N
pnp
nnnn
)(
""
4 fold coincidence
NNN"" ""NN
))((
""00 pp
nnnn
) )((
""0 np
npnp
2 particles in the backward detector
))((or
))((
""0
pp
pp
pppp
ppp
npnp
)(
""0
pnp
pppp
)(
""
3-5 fold coincidence
2-4 particles in the backward detector
Detected by spectrometer
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Title:Search for cumulative Delta 0(1232) and
Delta + + (1232) isobars in neutrino interactions with neon nuclei
Authors: Ammosov, V. V.; Asratyan, A. É.; Burtovoǐ, V. S.; Gapienko, V. A.; Gapienko, G. S.; Gorichev, P. A.; Denisov, A. G.; Zaets, V. G.; Klyukhin, V. I.; Koreshev, V. I.; Kruchinin, S. P.; Kubantsev, M. A.; Makhlyueva, I. V.; Pitukhin, P. V.; Sirotenko, V. I.; Slobodyuk, E. A.; Usubov, Z. U.; Fedotov, A. V.; Shevchenko, V. G.; Shekelyan, V. I.
Publication:
Journal of Experimental and Theoretical Physics Letters, Vol. 40, p.1041
Publication Date:
09/1984
Expected Δ’s rates 5-10% of recoil N
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Δ
Kinematics
pede22 =)( mppq fd
pΔ=640 MeV/c
With SHMS(e) and HMS(p) acceptancesand Γ=110 MeV
Needs large acceptance multi particle detector
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Extrapolation factor ~10
)',()/',( 1212 peeCppeeC
Measured ratio
Extrapolated ratio
The limited acceptance allows determination of only two components of the pair c.m. momentum with very limited acceptance.
Even the triple coincidence SRC experiment could be done better with a larger acceptance detector.
R.B. Wiringa, R. Schiavilla, Steven C. Pieper, J. Carlson . Jun 2008. arXiv:0806.1718 [nucl-th]
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A large acceptance detector allows tagging of the DIS event
EMC
High nuclear density tagging :
A recoil high momentum nucleon to the backward hemisphere is a signature of 2N-SRC i.e large local nuclear density.
Due to the dominance of np-SRC pairs: a recoil neutron tags the proton structure function a recoil proton tags the neutron structure function
Flavor tagging :
Identifying a π + or π - with a large z can point to the flavor of the struck quark ( u or d).
Recoil and forward tagging allows the study of u, d in p, n
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Hadronization
Measure the multiplicity and the type of emitted particles in a large acceptance “backward direction ” in coincidence with the forward (large z) leading π +, π -, k +, k - particle.
Difference in hadronization of different quarks
Difference between hadronization in free space and the nuclear medium
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GPDs
NN *
Hall C np *
With a large acceptance detector:
NL*
)(* NNL low mass πN system- a test of chiral symmetry
)(* KNL
With a deuteron one can measure simultaneously both protons and neutrons by detecting the recoil neutron or proton, respectively ?
Hall B
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Nuclear Matter in non - equilibrium condition
Using hard processes to remove a single or a few nucleons from the nucleus creates a non-stable state.
How does such a non-stable state decay to a stable system?
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Large solid angle- 4π – non-symmetric opening in the forward hemisphere
Large (full) luminosity
Can operate in coincidence with small solid angle, high resolution spectrometer / spectrometers
Multi particle detection
Particle ID
pe
e’
*
Δp
Large Acceptance Detector
Cover up to ~1800
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P
SHMS @5.50HMS @ 120
TOF CountersTarget Chamber
TOF Counters
Phase space coverage
TOF
CLAS Large –angle TOF scintillators
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Beam in
Beam View
Add two sectors at beam high
Phase space coverage
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Beam Left View
Sector #1
Sector #2
Sector #3
Sector 1: 82-1420
Sector 2: 97-1290
Sector 3: 117-1720
Polar angle acceptance
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Beam Right View
Sector #4
Sector #5
Sector #6
Polar angle acceptanceSector 4: 75-1420
Sector 5: 97-1060
Sector 6: 77-1030
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1420
1720n-detectors
n-de
tect
ors
Sector #1
Sector #3
Sector #4 Sector #6
Sectors 2 and 5 are not shown
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5
PID
22 X (370-450) X 5.08 cm3
10x(10-25)x(100-160) cm3
~140 counters
With ~ 80 counters / layer we can cover the beam height ±80 cm behind sectors 3 and 6.
neutron detection
5cm
10 cm
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π
p
d
~140 counters
beam
TOF
PID
22 X 370-450 X 5.08 cm3
at about 4 m from the target
PID can be better done by a partial acceptance (sectors 3 and 6) where more than one counter is on the line of sight.
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Luminosity: singles rates
3 1033 cm-2 sec-1 ----> 1 kHz/m2 (The large counters are ~ 1m2 )
6 1036 cm-2 sec-1 ----> 2 MHz
(the planned luminosity for 12GeV CLAS is 1035)
(The Hall A E01-015 luminosity was 5·1037 )
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Luminosity: rates
6 1036 cm-2 sec-1 / 5 1037 cm-2 sec-1 = 1 / 10
Rate of (e,e’p) with Pmiss=300-600 MeV/c, Hall A experiment E01-015: 0.2 Hz
LAD: (e, e’ppp) ~ 0.2 ·1% ·0.1 → ~1 events / hr
~100 events / week(e,e’p) rate
(e,e’ppp)/(e,e’p)
Luminosities ratio
(higher rates taking into account the spectrometers solid angles)
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Luminosity: Signal/BG
TOF corrected by the momentum determination based on Eloss
Pmis=“300” MeV/c
Pmis=“400” MeV/c
Pmis=“500” MeV/c
(Signal : BG= 1.5:1)
(Signal : BG= 2.3:1)
(Signal : BG= 4:1)
Δt~15 nsecHall A experiment E01-015
12 37 sec10 5.1 cmLN
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For each pair of identified protons with momentum within physically possible range calculate:
21 ppprecoil
Only pairs with missp-
recoilp
Luminosity: number of pairs
Average number of hits per event:
2MHz ·15 nsec = 3% 3%·140 = 4 hits/event (6 pairs/event)
are relevant
BigBite is ~100msr, assuming 1Sr / 2π i.e <1 pair on average
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Luminosity: Signal/BG
(e, e’pp)/(e,e’p) Hall A experiment E01-015:
5.1155
%10
sin,
,
nsMHtRR
fR
BG
signal
Zglesepe
epe
(e, e’ppp)/(e,e’p) in LAD Hall C:
(assuming the worst case: that an individual recoil proton does not have any directional correlation with Pmiss.)
'8)152(
140'
)(
'
22sin,
,f
nsMH
f
tRRN
fR
BG
signal
Zglesepe
epe
To be sensitive to 1% of the (e, e’p) we need to be sensitive to about 5% of the (e,e’p) with Pmiss between 300 -600 MeV/c (the spectrometer based trigger) .
4.0'8 fBG
signal
(calculation for a single counter:)
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What can be done with LAD that cannot be done with the planned 12 GeV CLAS ?
Up to ~100x the planned luminosity for the 12 GeV CLAS (1035).
Backward coverage up to 1720 (the planned 12 GeV CLAS covers up to 1350 )
Possible trigger by two high resolution spectometers
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A physics proposals on SRC to the next PAC
Conceptual detector design
2008
Simulations
Other proposals ?
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Acknowledgment
Stepan Stepanyan
Sebastian Kuhn
Steve Wood
Rolf Ent
Discussions and ideas exchange with:
Larry Weinstein
Preliminary design
Mike Fowler
Dave Kashy
Paul Brindza
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How to relate what we learned about SRC in nuclei to the dynamics of neutron star formation and structure ?
SRC
in nuclei
NN interaction: what is the role played by the repulsive core ?
•Are the nucleons in the SRC pair different from free nucleons (e.g size,shape, mass, etc.) ? Are they nucleons ?
What is the role played by short range correlation of more than two nucleons ?
SRC in nuclei
Roadmap
1.f
Nucleons
2N-SRC
1.7f
o = 0.16 GeV/fm3
5o
~1 fm 1.7 fm
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π
pd
beam
beam
~200 counters
20 cm
5 cmAlso E vs. ΔE
PID
TOF
ΔE
n-detection efficiency ~20% +15%(?)
LACLAC
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Short Range Correlations (SRC)
EMC
Hadronization
Study of GPDs
Nuclear Matter in non - equilibrium condition
2-3 physics proposals to the 12 GeV PAC
Conceptual detector design
2008
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Large Angle Calorimeter (LAC)
2 mm lead foil
1.5 cm plastic Scintillator
33 layers
neutron momentum [GeV/c]
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Improve n-detection
For the new 12 GeV clas:
The current magnet, Drift chambers, and scintillator counters are not to be used.
The CLAS as a 4π-forward detector
Need new power supplies, and electronics
Require a careful, non trivial dismount of the current detector at Hall B and non trivial setup at hall c.
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The CLAS as a 4π-forward detector
TOF CER CAL
DC1DC2DC3
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CLAS 3-D View
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How to relate what we learned about SRC in nuclei to the dynamics of neutron star formation and structure ?
SRC
in nuclei
NN interaction: what is the role played by the repulsive core ?
•Are the nucleons in the SRC pair different from free nucleons (e.g size,shape, mass, etc.) ? Are they nucleons ?
What is the role played by short range correlation of more than two nucleons ?
SRC in nuclei
Roadmap
1.f
Nucleons
2N-SRC
1.7f
o = 0.16 GeV/fm3
5o
~1 fm 1.7 fm
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12C:
18±4.5 %
0.95 ± 0.2 %
0.95 ± 0.2 %
2N-SRCnp-SRC
pp-SRC
nn-SRC
20±4.5 %
80±4.5%
The uncertainties allow a few percent of:
more than 2N correlations
Non nucleonic degrees of freedom
A single “particle” in an average potential
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Identifying Future Experiments
Looking for SRC with more than 2 nucleons:
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Identifying Future Experiments
Looking for SRC with more than 2 nucleons:
The problems:
The cross sections are small.
1N >> 2N - SRC >> 3N – SRC.
star geometry :What is the signature for 3N correlation ?
Questions
What is the difference from two 2N correlations ?
What is the expected isospin structure of the 3N ?
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Identifying Future Experiments
Looking for SRC with more than 2 nucleons:
The problems:
The cross sections are small.
1N >> 2N - SRC >> 3N – SRC.
The cure for 1N background is : large pmiss and/or large XB
The cure for 2N-SRC:
XB>2 or
suppression of the 2N-SRC at prel=300-600 MeV/c for nn or pp pairs.
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Identifying Future Experiments
Looking for SRC with more than 2 nucleons:
Colinear geometry :
Initial configurations
~800 MeV/c~800 MeV/c
The signal of today is tomorrow’s background
The 2N-SRC interaction is suppressed, opening a window of opportunity to identify 3N correlation.
~400 MeV/c~400 MeV/c
A very strong isospin dependence is expected for the 2N part. For the 3N?
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Identifying Future Experiments
Looking for SRC with more than 2 nucleons:
Colinear geometry
~800 MeV/c~800 MeV/c
FSI are strong function of θ
SRC are not
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Identifying Future Experiments
Looking for non-nucleonic degrees of freedom
The signature of a non-nucleonic SRC intermediate state is a large branching ratio to a non nucleonic final state.
... cba NNNSRC
1c,...b, ,0 a
Breaking the pair will yield more backward Δ, π , k
1.f
Nucleons
2N-SRC 5o
~1 fm
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Looking for non-nucleonic degrees of freedom
In coincidence with (e, e’p), as a function of the missing momentum we want to detect;
p, n, π-, π+ k - triple coincidence
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Identifying Future Experiments
Looking for non-nucleonic degrees of freedom
pΔ0 p π - p
“np” pn
“pp” pp
pΔ+ p π+ n
p 0
n 4 fold coincidence
Expected rates 5-10% of recoil N
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Δ
Kinematics
pede22 =)( mppq fd
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p
e
e’
*n or p
p
Pm =
“30
0”,”
400”
,”50
0” M
eV/c
99 ±50
P =
300
-600
MeV
/c
Ee = 4.627 GeV
Ee’ = 3.724 GeV
Q2=2 (GeV/c)2
qv=1.65 GeV/c
50.40
19.50
40.1 ,35.8 ,32.00
p = 1.45,1.42,1.36 GeV/c
The selected kinematics for E01-015
X=1.245Increasing, energy, ω,NΔ ?
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p
e
e’
*Δ
p
Ee = 11 GeV
Ee’ = 9.8 GeV
Q2=2.5 (GeV/c)2
qv=1.65 GeV/c
48.50
8.80
34 0
p = 1.32 GeV/c
The selected kinematics
X=1.12
Increasing, energy and ω, NΔ
Pmiss =770 MeV/c
PΔ =770 MeV/c
Cannot produce backward going Δ.
Cannot produce larger momentum difference between the recoil Δ and the struck nucleon.p
ee’
*
Δ p
p = 1.32 GeV/c
Pmiss =1.32 GeV/c
PΔ =770 MeV/c
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Ee= 11.00000 Eout= 9.960000 theta_e = 8.200000 Q2= 2.240232 x= 1.147892
input angle of (qe) and (qp) planes 0.0000000E+00 theta of q: -51.20859
The format of the following output is:
type of the particle, momentum, angle vs q, angle vs e, azimuthal angle in lab
knock-out nucleon 1.200000 5.490372 45.71821 180.0000 missing 0.6385024 169.6408 118.4322 0.0000000E+00
recoil 0.6385024 10.35917 61.56776 180.0000 tet between recoil and scattred proton -15.84955
pmiss in the q direction 0.6280947
Ee= 11.00000 Eout= 9.790000 theta_e = 8.800000 Q2= 2.535372 x= 1.116600 input angle of (qe) and (qp) planes 0.0000000E+00 theta of q: -48.49650 The format of the following output is: type of the particle, momentum, angle vs q, angle vs e, azimuthal angle in lab knock-out nucleon 1.328000 13.52419 34.97231 180.0000 missing 0.7737520 156.3361 107.8397 0.0000000E+00 recoil 0.7737520 23.66388 72.16035 180.0000 tet between recoil and scattred proton -37.18803 pmiss in the q direction 0.7086919
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p
e
e’
*Δ
pPm
= “
640
MeV
/c
1000
Ee = 11 GeV
Ee’ = 9 GeV
Q2=2 (GeV/c)2
qv=2.5 GeV/c
31.50
8.20
16.60
p = 2.3 GeV/c
The selected kinematics for the measurement
X=0.5
P Δ=
“640
MeV
/c
Ee= 11.00000 Eout= 9.000000 theta_e = 8.200000 Q2= 2.024307 x= 0.5393709 input angle of (qe) and (qp) planes 0.0000000E+00 theta of q: -31.53330 The format of the following output is: type of the particle, momentum, angle vs q, angle vs e, azimuthal angle in lab knock-out nucleon 2.300000 14.94191 16.59142 179.9802 missing 0.6368749 111.3839 79.85064 0.0000000E+00 recoil 0.6368749 68.61605 100.1494 180.0000 tet between recoil and scattred proton -83.55794 pmiss in the q direction 0.2322146
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pΔ=640 MeV/c
With SHMS(e) and HMS(p) acceptancesand Γ=110 MeV
With SHMS(e) and HMS(p) acceptances
Needs large acceptance multi particle detector
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Large solid angle- 4π – non symmetric gape at the forward hemisphere
Large (full) luminosity
Can operate in coincidence with small solid angle high resolution spectrometer / spectrometers
Multi particle detection
Particle ID
pe
e’
*
Δp
The LargeAcceptanceMINUSFORWARD detector
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CLAS12
Solenoid
Toro
id
Cal
orim
eter
CF 4
Cer
enko
v
Toroidal field < 45o
Solenoidal field 45 < < 135o
DC TOF
CO2 Cer
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SRC
in nuclei
•Are the nucleons in the SRC pair different from free nucleons (e.g size,shape, mass, etc.) ? Are they nucleons ?
What is the role played by short range correlation of more than two nucleons ?
SRC in nuclei
Roadmap
1.f
Nucleons
2N-SRC
1.7f
o = 0.16 GeV/fm3
5o
~1 fm 1.7 fm
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12C:
18±4.5 %
0.95 ± 0.2 %
0.95 ± 0.2 %
2N-SRCnp-SRC
pp-SRC
nn-SRC
20±4.5 %
80±4.5%
The uncertainties allow a few percent of:
more than 2N correlations
Non nucleonic degrees of freedom
A single “particle” in an average potential
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LAC
TOF scintillators
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Singles rates
3 1033 cm-2 sec-1 ----> 1 kHz/m2 (The large counters are ~ 1m2 )
6 1036 cm-2 sec-1 ----> 2 MHz
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PRELIMINARY
12C
12C12C
12C
?
?
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Proposal : same luminosity as before
i.E : 30 microA on 0.25 mm 12C at 20 deg
12 37 sec10 5.1 cmLN
Can the chambers at 100 deg hold such luminosity?
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Sector #2
Sector #1
Sector #3
Sector #4
Sector #5
Sector #6