First Gamma-Ray Spectroscopy of sd -shell Hypernucleus, π³ ππ π 21 st , November, 2016 -Neutron Star Matter 2016- YANG Seongbae Department of Physics and Astronomy Seoul National University 1
1. Introduction 2
1. Introdu oduction tion Previous Gamm-ray Spectroscopies β Previous Ξ³ -ray spectroscopies for s- shell hypernuclei *NaI detector 4 H *Ge detector Ξ 4 He 4 He Ξ Ξ @PRL, 115, 222501 (2015) @PLB, 83, 252 (1979) 3
1. Introdu oduction tion β Previous Ξ³ -ray spectroscopies for p- shell hypernuclei (Hyperball project) @NPA, 835, 3 (2010) ο The next step is awaited for heavier hypernuclei. 4
1. Introdu oduction tion Gamma-ray Spectroscopy of π³ ππ π β It is the first Ξ³ -ray spectroscopy for sd -shell hypernuclei. β Energy spacing of ground state doublet (1/2 + , 3/2 + ) ο Radial dependency of the Ξ N spin-spin interaction? ο Ξ N spin-dependent interaction with different wave-function? Ξ p + 16 O Spin-spin interaction n Ξ low-lying energy levels of Ξ 19 F *A. Umeya and T. Motoba NPA 116, 122501 (2016). 5
1. Introdu oduction tion 4 H 7 Li 19 F Ξ Ξ Ξ Four-body p p p + Ξ + Ξ n + Ξ 4 He 16 O Cluster n n n model Wave- π πΆ π π§ π πΆ π π§ (ππ) πΆ π π§ function 3.4 ( 1π‘ 1/2 ) 3.0 ( 0π 1/2 ) N, RMS 3.5 ( 0π 1/2 ) 2.5 ( 0π‘ ) 2.9 ( 0π 3/2 ) radius [fm] 3.3 ( 0π 5/2 ) @by Millener, private communication Ξ , RMS 3.5 ( 0π‘ ) 2.6 ( 0π‘ ) 2.3 ( 0π‘ ) radius [fm] @by Millener, private communication ? βπΉ π¦ 0.695 MeV (ground 1.1 MeV ( Ξ π π π Ξ =0.43 MeV) state doublet) 6
2. Experimental Setup 7
2. Experi rime mental tal Setup Experimental Setup of J-PARC E13 β Reaction: 19 F(πΏ β , π β ) Ξ 19 F β K1.8 Beamline : High intensity and high purity πΏ β beam ο Intensity of πΏ β beam: ~350 k/spill ο πΏ β / π β = ~2.5 ο 1.8 GeV/c beam momentum β SKS & K1.8 Beamline Spectrometers ο High resolution of missing mass ο Large acceptance for (πΏ β , π β ) ο good beam decay suppressor (SP0, SMF) Target: Liquid. H 2 Liquid. CF 4 8
2. Experi rime mental tal Setup β Hyperball-J 19 F β β πΏ + 19 F β , Ξ ο 19 F(πΏ β , π β ) Ξ 19 F Ξ ο ~25 HPGe detectors - βE ~4.5 keV @ 1MeV ο PWO counters - Fast background suppression Mechanical cooling system Crystal temp. ~70 K *a view of K1.8 experimental hall @NPA, 835, 3 (2012) 9
2. Experi rime mental tal Setup Data Sample for π³ ππ π β 05.2015~06.2015 at the J-PARC K1.8 Beamline Target Momentum Data Number of K (Thickness [g/cm 2 ]) [GeV/c] Beam 1.37, 1.5, . . through and 1.8 Ξ£ + and Ξ CH 2 (6.6) 1.8 0.6 G 12 C CF 2 (6.6) 1.8 2.3 G 19 F Ξ Physics Run Liquid. CF 4 (20) 1.8 63 G 10
3. Analysis 11
3. Analysi ysis (K, pi) Vertex Point (z-direction) and Reaction Angle β CF 4 target during physics run vertex (z) cut Reaction angle: 2~12 deg. *CF 4 target real length: 125 mm 12
3. Analysi ysis (K, pi) Particle Identification for π³ β and π β β At trigger line, K β and Ο β are identified by using AC counters. In addition, M 2 is used for identification of Ο β . M 2 distribution of scattered particle 13
3. Analysi ysis (K, pi) Calibration run with CH 2 target (6.6 g/cm 2 ) 1 H(πΏ β , π β )Ξ£ + 12 C(πΏ β , π β ) Ξ 12 C *2< ΞΈ <12 *2< ΞΈ <12 Ξ£ + g.s. of Ξ 12 C MPV: 1.1901 Β± 0.0004 Β± 0.0001 GeV/π 2 MPV: -11.06 Β± 0.18 Β± 0.21 MeV FWHM: 0.0060 Β± 0.0001 Β± 0.0002 GeV/π 2 FWHM: 6.04 Β± 0.47 Β± 0.40 MeV +0.7 MeV level. ο Absolute scale of missing mass: β0.7 ο Expected missing mass resolution (FWHM) with CF 4 target: 8.7 Β± 0.4 MeV 14
3. Analysi sis ( Ξ³ ray ) Analysis for Ξ³ rays β By using Ξ³ rays from normal nuclei, energy resolution (FWHM) and accuracy of absolute energy level are estimated. Energy Resolution Energy Calibration ο Energy Resolution: ~4.5 keV @1.0 MeV (the sum of all germaniums) ο Ξ³ rays were measured under ~0.5 keV accuracy level at E < 3 MeV. 15
4. Results 16
4. Results lts - B π³ Distribution of π³ ππ π with CF 4 target (20 g/cm 2 ) β -21 MeV<- B Ξ <-8 MeV is selected to observe the Ξ³ rays from low lying energy states. Threshold of Ξ 15 N + Ξ± g.s. of Ξ 12 C For Ξ³ rays from π³ ππ π 17
4. Results lts Ξ³ -ray spectra β Ξ³ -ray spectra: energy range: 0~1800 keV and without Doppler shift correction. There are two more peaks. 18
4. Results lts Ξ³ (315) and Ξ³ (895) Ξ³ (315) Ξ³ (895) +0.6 keV +0.6 keV ο Energy: 315.5 Β±0.4 β0.5 ο Energy: 895.2 Β±0.3 β0.5 19
4. Results lts β At the forward reaction angle, we found two more gamma-ray peaks at 953 keV and 1267 keV. Ξ³ (953) +0.5 keV ο E: 952.8 Β±1.2 β0.6 ~313 keV Ξ³ (1267) ο E: 1265.9 Β± 1.2 Β± 0.7 keV ο The energy difference is consistent with the Ξ³ (315) energy. 20
5. Discussion 21
5. Discus ussion sion Transition Assignments β Based on theoretical calculations, the gamma rays are assigned to their gamma transitions. Ξ³ (952) Ξ³ (1267) Ξ³ (895) Ξ³ (315) 22
5. Discus ussion sion Spin-Spin Interaction in sd -shell Hypernuclei Shell-model Shell-model with Ξ N spin- Theoretical with NSC97f model dependent Experiment Calculation by Umeya and interaction at p - Motoba shell hypernuclei by Millener ΞπΉ ( 3/2 + , 1/2 + ) 419 305 +0.3 315.5 Β±0.4 β0.2 [keV] ο The measured energy spacing is well represented by the spin-dependent interaction in p -shell hypernuclei. It also indicates the ΞΞ£ coupling effect is negligible for the energy spacing. ο The results will be soon published in a major physics journal. 23
6. Summary 24
6. Summar ary Summary β A new πΏ -ray spectroscopy of sd-shell hypernucleus ( Ξ 19 F ) via the (π¬ β , π β ) reaction with 1.8 GeV/π beam was performed at the J-PARC K1.8 beamline. β Several πΏ rays from 19 F are observed. The 19 F (315), 19 F (895), 19 F Ξ Ξ Ξ Ξ 19 F (1267) are assigned to the M1(3/2 + β 1/2 + ) , E2(5/2 + β (953), and Ξ 1/2 + ) , E1(1/2 β β 3/2 + ) , and E1(1/2 β β 1/2 + ) transitions, respectively. β The measured energy spacing (315 keV) between the ground state doublet is well represented by the spin-dependent interaction at p- shell hypernuclei. β It is meaningful to extend the πΏ -ray spectroscopy to medium hypernuclei, and it will be a guide for future experiments. 25
*Back Up 26
*Back Up Up K1.8 Beamline β K1.8 Beamline : High intensity and high purity πΏ β beam ο Intensity of πΏ β beam: ~350 k/spill ο πΏ β / π β = ~2.5 *J-PARC Hadron facility Secondary Beam Proton Beam 27 @PTEP , 2012, 02B009
* Back up up Energy calibration Energy of Ξ³ ray is calibrated through two steps. 1. Off-beam calibration: spill-off condition for each runs 2. In-beam calibration: spill-on condition Off-beam calibration: Three Ξ³ ray from 238 Th source Fit by 1 st polynomial 28
* Back up up In-beam calibration: 10 Ξ³ rays from normal nuclei Fit by 1 st polynomial Fit by 1 st polynomial +Exponential functions 29
*Back up up - B π³ Distribution of π³ ππ π with CF 2 Target (6.6 g/cm 2 ) *Reaction angle, 2< ΞΈ <12 Structure of 19 F Ξ *Background from Ξ 12 C is estimated using calibration data with CH 2 target. 30
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