First Gamma-Ray Spectroscopy of sd-shell Hypernucleus, π³
πππ
YANG Seongbae
Department of Physics and Astronomy Seoul National University
21st, November, 2016
- Neutron Star Matter 2016-
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First Gamma-Ray Spectroscopy of sd -shell Hypernucleus, 21 st , - - PowerPoint PPT Presentation
First Gamma-Ray Spectroscopy of sd -shell Hypernucleus, 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
21st, November, 2016
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β Previous Ξ³-ray spectroscopies for s-shell hypernuclei
tion
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@PLB, 83, 252 (1979)
@PRL, 115, 222501 (2015)
*NaI detector *Ge detector
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@NPA, 835, 3 (2010)
tion
β Previous Ξ³-ray spectroscopies for p-shell hypernuclei (Hyperball project)
πππ
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 ΞN spin-spin interaction? ο ΞN spin-dependent interaction with different wave-function? low-lying energy levels of Ξ
19F
*A. Umeya and T. Motoba NPA 116, 122501 (2016). 5
Spin-spin interaction
16O
n p Ξ + Ξ
tion
Ξ 4H Ξ 7Li Ξ 19F
Four-body Cluster model Wave- function
N, RMS
radius [fm]
2.5 (0π‘) 3.0 (0π1/2) 2.9 (0π3/2) 3.4 (1π‘1/2) 3.5 (0π1/2) 3.3 (0π5/2)
Ξ, RMS radius [fm]
3.5 (0π‘) 2.6 (0π‘) 2.3 (0π‘) βπΉπ¦ (ground state doublet) 1.1 MeV 0.695 MeV (ΞπππΞ=0.43 MeV)
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n n p Ξ +
4He
n p Ξ +
16O
n p Ξ +
@by Millener, private communication @by Millener, private communication
tion
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β Reaction: 19F(πΏβ, πβ) Ξ
19F
β K1.8 Beamline : High intensity and high purity πΏβ beam
ο Intensity of πΏβ beam: ~350 k/spill ο πΏβ/πβ = ~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 (πΏβ, πβ)
ο good beam decay suppressor (SP0, SMF)
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Target:
rime mental tal Setup
β Hyperball-J
ο 19F(πΏβ, πβ) Ξ
19F β, Ξ 19F β β πΏ + Ξ 19F
ο ~25 HPGe detectors - βE ~4.5 keV @ 1MeV ο PWO counters - Fast background suppression
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@NPA, 835, 3 (2012) *a view of K1.8 experimental hall
Mechanical cooling system Crystal temp. ~70 K
rime mental tal Setup
πππ
β 05.2015~06.2015 at the J-PARC K1.8 Beamline Data Target (Thickness [g/cm2]) Momentum [GeV/c] Number of K Beam through . 1.37, 1.5, and 1.8 . Ξ£+ and Ξ
12C
CH2 (6.6) 1.8 0.6 G
Ξ 19F
CF2 (6.6) 1.8 2.3 G Physics Run
1.8 63 G
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rime mental tal Setup
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β CF4 target during physics run
ysis (K, pi)
*CF4 target real length: 125 mm Reaction angle: 2~12 deg. vertex (z) cut
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M2 distribution of scattered particle β At trigger line, Kβ and Οβ are identified by using AC counters. In addition, M2 is used for identification of Οβ.
ysis (K, pi)
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ο Absolute scale of missing mass: β0.7
+0.7 MeV level.
ο Expected missing mass resolution (FWHM) with CF4 target: 8.7Β±0.4 MeV
ysis (K, pi)
MPV: 1.1901Β±0.0004Β±0.0001 GeV/π2 FWHM: 0.0060Β±0.0001Β±0.0002 GeV/π2
12C
MPV: -11.06Β±0.18Β±0.21 MeV FWHM: 6.04Β±0.47Β±0.40 MeV
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*2<ΞΈ<12 *2<ΞΈ<12
1H(πΏβ, πβ)Ξ£+ 12C(πΏβ, πβ) Ξ 12C
β By using Ξ³ rays from normal nuclei, energy resolution (FWHM) and accuracy
sis (Ξ³ ray)
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.
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Energy Calibration Energy Resolution
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πππ with CF4 target (20 g/cm2)
β -21 MeV<-BΞ<-8 MeV is selected to observe the Ξ³ rays from low lying energy states.
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Threshold of Ξ
15N + Ξ±
g.s. of Ξ
12C
For Ξ³ rays from π³
πππ
lts
β Ξ³-ray spectra: energy range: 0~1800 keV and without Doppler shift correction.
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There are two more peaks.
lts
ο Energy: 315.5 Β±0.4β0.5
+0.6 keV
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ο Energy: 895.2 Β±0.3β0.5
+0.6 keV
Ξ³(315) Ξ³(895)
lts
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β At the forward reaction angle, we found two more gamma-ray peaks at 953 keV and 1267 keV. ο The energy difference is consistent with the Ξ³(315) energy. ~313 keV
Ξ³(953) ο E: 952.8 Β±1.2β0.6
+0.5 keV
Ξ³(1267) ο E: 1265.9 Β± 1.2 Β± 0.7 keV
lts
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Ξ³(895) Ξ³(1267) Ξ³(952) Ξ³(315) β Based on theoretical calculations, the gamma rays are assigned to their gamma transitions.
ussion sion
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.
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Theoretical Calculation Experiment Shell-model with NSC97f model by Umeya and Motoba Shell-model with ΞN spin- dependent interaction at p- shell hypernuclei by Millener ΞπΉ(3/2+, 1/2+) [keV] 315.5 Β±0.4β0.2
+0.3
419 305
ussion sion
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ary
19F) via the
Ξ 19F are observed. The Ξ 19F(315), Ξ 19F(895), Ξ 19F
Ξ 19F(1267) are assigned to the M1(3/2+ β 1/2+), E2(5/2+ β
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β K1.8 Beamline : High intensity and high purity πΏβ beam
ο Intensity of πΏβ beam: ~350 k/spill ο πΏβ/πβ = ~2.5 *J-PARC Hadron facility *Back Up Up
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@PTEP , 2012, 02B009
Proton Beam Secondary Beam
Energy of Ξ³ ray is calibrated through two steps.
Fit by 1st polynomial Off-beam calibration: Three Ξ³ ray from 238Th source
* Back up up
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Fit by 1st polynomial In-beam calibration: 10 Ξ³ rays from normal nuclei Fit by 1st polynomial +Exponential functions
* Back up up
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*Back up up *Background from Ξ
12C is estimated using calibration data with CH2 target.
πππ with CF2 Target (6.6 g/cm2)
Ξ 19F
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*Reaction angle, 2<ΞΈ<12