Hypernuclei: A very quick introduction Electroproduction of hypernuclei The experimental Program at Jefferson Lab Update on the analysis of O and Be targets Update on the analysis of Elementary Production Hall A Collaboration Meeting Jefferson Lab, 13-14 December 2007 Francesco Cusanno INFN Rome (Italy) Armando Acha FIU (Miami FL)
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Hypernuclei: A very quick introduction Electroproduction of hypernuclei The experimental Program at Jefferson Lab Update on the analysis of O and Be targets.
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Hypernuclei: A very quick introduction
Electroproduction of hypernuclei
The experimental Program at Jefferson Lab
Update on the analysis of O and Be targets
Update on the analysis of Elementary Production
Hall A Collaboration Meeting Jefferson Lab, 13-14 December 2007
: I=0, q=0 n = pSpectroscopy of mirror hypernuclei reveal n ≠ p 0 mixing and N-N coupling
What do we learn from hypernuclear spectroscopy Hypernuclei and the -N interaction
“weak coupling model”
(parent nucleus) ( hyperon) (doublet state)
JA 1 (s shell) JHyp JA 1 12
VN = V0(r) + V (r)s
s N + V (r)
N
s + VN (r)
N
s N + VT (r)S12
S SNT
J 12
J
J 12
(A-1)A
SN
, S , T
Split by N spindependent interaction
HypernuclearFine Structure
Low-lying levels of Hypernuclei
Each of the 5 radial integral (V, , S, SN, T) can be phenomenologically determined from the low lying level structure of p-shell hypernuclei
V
ELECTROproduction of Hypernuclei
Hypernuclear physics accesses information on the nature of the force between
nucleons and strange baryons, i.e. the -N interaction. The nucleus provides a unique
laboratory for studying such interaction.
The characteristics of the Jefferson Lab. electron beam, together with those of the experimental equipments, offer a unique opportunity to study hypernuclear spectroscopy via electromagnetic induced reactions. A new experimental approach: alternative to the hadronic induced reactions studied so far.
The experimental program at Jefferson Lab, in Hall A and in Hall C, has completed its first part of measurements, performing high-resolution hypernuclear spectroscopy on light (p-shell) and medium heavy targets
Different approach:
Hall C : Low Luminosity (thin targets low current) Large Acceptance
Hall A : Small Acceptance - High Luminosity
JLAB Hall A Experiment E94-107
1616O(e,e’KO(e,e’K++))1616NN
1212C(e,e’KC(e,e’K++))1212
Be(e,e’KBe(e,e’K++))99LiLi
H(e,e’KH(e,e’K++))00
Ebeam = 4.016, 3.777, 3.656 GeV
Pe= 1.80, 1.57, 1.44 GeV/c Pk= 1.96 GeV/c
e = K = 6°
W 2.2 GeV Q2 ~ 0.07 (GeV/c)2
Beam current : <100 A Target thickness : ~100 mg/cm2
Counting Rates ~ 0.1 – 10 counts/peak/hour
A.Acha, H.Breuer, C.C.Chang, E.Cisbani, F.Cusanno, C.J.DeJager, R. De Leo, R.Feuerbach, S.Frullani, F.Garibaldi*, D.Higinbotham, M.Iodice, L.Lagamba,
J.LeRose, P.Markowitz, S.Marrone, R.Michaels, Y.Qiang, B.Reitz, G.M.Urciuoli, B.Wojtsekhowski, and the Hall A Collaboration
E94107 COLLABORATION
Results on 12C target
Analysis of the reaction 12C(e,e’K)12B
Results published: M.Iodice et al., Phys. Rev. Lett. E052501, 99 (2007).Results published: M.Iodice et al., Phys. Rev. Lett. E052501, 99 (2007).
Results on 12C target – Hypernuclear Spectrum of 12B
G.S. width is 1150 keV; an unresolved doublet?What would separation be between two 670 keV peaks? ~650 keV (theory predicts only 140)
Narrowest peak is doublet at 10.93 MeV experiment resolution < 700 keV
670 keVFWHM
Results from the 9Be target
Analysis of the reaction 9Be(e,e’K)9Li (very preliminary) C
ou
nts
/ 2
00 k
eV
Missing energy (MeV)
Cou
nts
/ 2
00 k
eV
0
1.6
0 2 4 6 8 10 12
Millener w.f.'s
Red line: Benhold-Mart (K MAID)
Blue line: Saghai Saclay-Lyon (SLA)
Curves are normalized on g.s. peak.
Red line: Benhold-Mart (K MAID)
Blue line: Saghai Saclay-Lyon (SLA)
Curves are normalized on g.s. peak.
Black line: Millener wave function
Results from the 9Be target
Analysis of the reaction 9Be(e,e’K)9Li (very preliminary)
Missing energy (MeV)
Cou
nts
0
1.6
0 2 4 6 8 10 12
Millener w.f.'s
Preliminary Results on the WATERFALL target
Analysis of the reaction 16O(e,e’K)16N
and 1H(e,e’K)(elementary reaction)
Be windows H2O “foil”
H2O “foil”
the WATERFALLWATERFALL target: provides 16O and H targets
1H (e,e’K)1H (e,e’K)
16O(e,e’K)16N16O(e,e’K)16N
1H (e,e’K)1H (e,e’K)
Energy Calibration Run
Preliminary Results on the WATERFALL target - 16O and H spectra
Excitation Energy (MeV)N
b/sr
2 G
eV
MeV
Water thickness from elastic cross section on H Fine determination of the particle momenta and beam energy
using the Lambda peak reconstruction (resolution vs position)
Fit to the data: Fit 4 regions with 4 Voigt functions 2
/ndf = 1.19 Theoretical model superimposed curve based on :
i) SLA p(e,e’K+) (elementary process)ii) N interaction fixed parameters from KEK and
BNL 16O spectra
Results on 16O target – Hypernuclear Spectrum of 16N
- Peak Search :Identified 4 regions with excess counts above background
Binding Energy B=13.66±0.25 MeVMeasured for the first time with this level of accuracy (ambiguous interpretation from emulsion data; interaction involving production on n more difficult to normalize)
Results on 16O target – Hypernuclear Spectrum of 16N
11
11.5
12
12.5
13
13.5
14
14.5
0 1 2 3 4 5
Serie1
E94-107
(+,K+)
(K-,-) (K-,-)
[2] O. Hashimoto, H. Tamura,Part Nucl Phys 57, 564 (2006)
[3] private communication from D. H. Davis, D. N. Dovee, fit of data from Phys Lett B 79, 157 (1978) [4] private communication from H. Tamura, erratum on Prog Theor Phys Suppl 117, 1 (1994)
[2] [3] [4]
Comparison with the mirror nucleus 16ODifference expected: 400 – 500 keV
p(e,e'K+) on WaterfallProduction run
p(e,e'K+) on LH2 Cryo TargetCalibration run
Work on normalizations, acceptances, efficiencies still underway
Expected data from theProposal E07-012 to study the angular dependence of p(e,e’K) and 16O(e,e’K)16N at Low Q2