First Gamma-Ray Spectroscopy of sd -shell Hypernucleus, 21 st , - - PowerPoint PPT Presentation

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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


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SLIDE 1

First Gamma-Ray Spectroscopy of sd-shell Hypernucleus, 𝚳

πŸπŸ˜π†

YANG Seongbae

Department of Physics and Astronomy Seoul National University

21st, November, 2016

  • Neutron Star Matter 2016-

1

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SLIDE 2
  • 1. Introduction

2

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SLIDE 3

Previous Gamm-ray Spectroscopies

β–  Previous Ξ³-ray spectroscopies for s-shell hypernuclei

  • 1. Introdu
  • duction

tion

3

Ξ› 4H

@PLB, 83, 252 (1979)

Ξ› 4He Ξ› 4He

@PRL, 115, 222501 (2015)

*NaI detector *Ge detector

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SLIDE 4

4

@NPA, 835, 3 (2010)

οƒ  The next step is awaited for heavier hypernuclei.

  • 1. Introdu
  • duction

tion

β–  Previous Ξ³-ray spectroscopies for p-shell hypernuclei (Hyperball project)

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SLIDE 5

Gamma-ray Spectroscopy of 𝚳

πŸπŸ˜π†

β–  It is the first Ξ³-ray spectroscopy for sd-shell hypernuclei. β–  Energy spacing of ground state doublet (1/2+, 3/2+)

οƒ  Radial dependency of the Ξ›N spin-spin interaction? οƒ  Ξ›N 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›

  • 1. Introdu
  • duction

tion

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SLIDE 6

Ξ› 4H Ξ› 7Li Ξ› 19F

Four-body Cluster model Wave- function

π’•π‘Άπ’•πœ§ π’’π‘Άπ’•πœ§ (𝒕𝒆)π‘Άπ’•πœ§

N, RMS

radius [fm]

2.5 (0𝑑) 3.0 (0π‘ž1/2) 2.9 (0π‘ž3/2) 3.4 (1𝑑1/2) 3.5 (0π‘ž1/2) 3.3 (0𝑒5/2)

Ξ›, RMS radius [fm]

3.5 (0𝑑) 2.6 (0𝑑) 2.3 (0𝑑) βˆ†πΉπ‘¦ (ground state doublet) 1.1 MeV 0.695 MeV (Ξ”π‘žπ‘‚π‘‡Ξ›=0.43 MeV)

?

6

n n p Ξ› +

4He

n p Ξ› +

16O

n p Ξ› +

@by Millener, private communication @by Millener, private communication

  • 1. Introdu
  • duction

tion

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SLIDE 7
  • 2. Experimental Setup

7

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SLIDE 8

Experimental Setup of J-PARC E13

β–  Reaction: 19F(πΏβˆ’, πœŒβˆ’) Ξ›

19F

β–  K1.8 Beamline : High intensity and high purity πΏβˆ’ beam

οƒ  Intensity of πΏβˆ’ beam: ~350 k/spill οƒ  πΏβˆ’/πœŒβˆ’ = ~2.5 οƒ  1.8 GeV/c beam momentum

β–  SKS & K1.8 Beamline Spectrometers

οƒ  High resolution of missing mass

οƒ  Large acceptance for (πΏβˆ’, πœŒβˆ’)

οƒ  good beam decay suppressor (SP0, SMF)

8

Target:

  • Liquid. H2
  • Liquid. CF4
  • 2. Experi

rime mental tal Setup

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SLIDE 9

β–  Hyperball-J

οƒ  19F(πΏβˆ’, πœŒβˆ’) Ξ›

19F βˆ—, Ξ› 19F βˆ— β†’ 𝛿 + Ξ› 19F

οƒ  ~25 HPGe detectors - βˆ†E ~4.5 keV @ 1MeV οƒ  PWO counters - Fast background suppression

9

@NPA, 835, 3 (2012) *a view of K1.8 experimental hall

Mechanical cooling system Crystal temp. ~70 K

  • 2. Experi

rime mental tal Setup

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SLIDE 10

Data Sample for 𝚳

πŸπŸ˜π†

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

  • Liquid. CF4 (20)

1.8 63 G

10

  • 2. Experi

rime mental tal Setup

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SLIDE 11
  • 3. Analysis

11

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SLIDE 12

Vertex Point (z-direction) and Reaction Angle

β–  CF4 target during physics run

  • 3. Analysi

ysis (K, pi)

*CF4 target real length: 125 mm Reaction angle: 2~12 deg. vertex (z) cut

12

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SLIDE 13

Particle Identification for π‘³βˆ’ and π†βˆ’

M2 distribution of scattered particle β–  At trigger line, Kβˆ’ and Ο€βˆ’ are identified by using AC counters. In addition, M2 is used for identification of Ο€βˆ’.

  • 3. Analysi

ysis (K, pi)

13

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SLIDE 14

Calibration run with CH2 target (6.6 g/cm2)

οƒ  Absolute scale of missing mass: βˆ’0.7

+0.7 MeV level.

οƒ  Expected missing mass resolution (FWHM) with CF4 target: 8.7Β±0.4 MeV

  • 3. Analysi

ysis (K, pi)

MPV: 1.1901Β±0.0004Β±0.0001 GeV/𝑑2 FWHM: 0.0060Β±0.0001Β±0.0002 GeV/𝑑2

Ξ£+ g.s. of Ξ›

12C

MPV: -11.06Β±0.18Β±0.21 MeV FWHM: 6.04Β±0.47Β±0.40 MeV

14

*2<ΞΈ<12 *2<ΞΈ<12

1H(πΏβˆ’, πœŒβˆ’)Ξ£+ 12C(πΏβˆ’, πœŒβˆ’) Ξ› 12C

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SLIDE 15

β–  By using Ξ³ rays from normal nuclei, energy resolution (FWHM) and accuracy

  • f absolute energy level are estimated.
  • 3. Analysi

sis (Ξ³ ray)

Analysis for Ξ³ rays

οƒ  Energy Resolution: ~4.5 keV @1.0 MeV (the sum of all germaniums) οƒ  Ξ³ rays were measured under ~0.5 keV accuracy level at E < 3 MeV.

15

Energy Calibration Energy Resolution

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SLIDE 16
  • 4. Results

16

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SLIDE 17
  • B𝚳 Distribution of 𝚳

πŸπŸ˜π† with CF4 target (20 g/cm2)

β–  -21 MeV<-BΞ›<-8 MeV is selected to observe the Ξ³ rays from low lying energy states.

17

Threshold of Ξ›

15N + Ξ±

g.s. of Ξ›

12C

For γ rays from 𝚳

πŸπŸ˜π†

  • 4. Results

lts

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SLIDE 18

Ξ³-ray spectra

β–  Ξ³-ray spectra: energy range: 0~1800 keV and without Doppler shift correction.

18

There are two more peaks.

  • 4. Results

lts

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SLIDE 19

Ξ³(315) and Ξ³(895)

οƒ Energy: 315.5 Β±0.4βˆ’0.5

+0.6 keV

19

οƒ Energy: 895.2 Β±0.3βˆ’0.5

+0.6 keV

Ξ³(315) Ξ³(895)

  • 4. Results

lts

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SLIDE 20

20

β–  At the forward reaction angle, we found two more gamma-ray peaks at 953 keV and 1267 keV. οƒ  The energy difference is consistent with the Ξ³(315) energy. ~313 keV

Ξ³(953) οƒ  E: 952.8 Β±1.2βˆ’0.6

+0.5 keV

Ξ³(1267) οƒ  E: 1265.9 Β± 1.2 Β± 0.7 keV

  • 4. Results

lts

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SLIDE 21
  • 5. Discussion

21

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SLIDE 22

Transition Assignments

22

Ξ³(895) Ξ³(1267) Ξ³(952) Ξ³(315) β–  Based on theoretical calculations, the gamma rays are assigned to their gamma transitions.

  • 5. Discus

ussion sion

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SLIDE 23

Spin-Spin Interaction in sd-shell Hypernuclei

οƒ  The measured energy spacing is well represented by the spin-dependent interaction in p-shell hypernuclei. It also indicates the ΛΣ coupling effect is negligible for the energy spacing. οƒ  The results will be soon published in a major physics journal.

23

Theoretical Calculation Experiment Shell-model with NSC97f model by Umeya and Motoba Shell-model with Ξ›N spin- dependent interaction at p- shell hypernuclei by Millener Δ𝐹(3/2+, 1/2+) [keV] 315.5 Β±0.4βˆ’0.2

+0.3

419 305

  • 5. Discus

ussion sion

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SLIDE 24
  • 6. Summary

24

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SLIDE 25
  • 6. Summar

ary

Summary

β–  A new 𝛿-ray spectroscopy of sd-shell hypernucleus ( Ξ›

19F) via the

(π›¬βˆ’, πœŒβˆ’) reaction with 1.8 GeV/𝑑 beam was performed at the J-PARC K1.8 beamline. β–  Several 𝛿 rays from

Ξ› 19F are observed. The Ξ› 19F(315), Ξ› 19F(895), Ξ› 19F

(953), and

Ξ› 19F(1267) are assigned to the M1(3/2+ β†’ 1/2+), E2(5/2+ β†’

1/2+), E1(1/2βˆ’ β†’ 3/2+), and E1(1/2βˆ’ 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 𝛿 -ray spectroscopy to medium hypernuclei, and it will be a guide for future experiments.

25

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SLIDE 26

*Back Up

26

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SLIDE 27

K1.8 Beamline

β–  K1.8 Beamline : High intensity and high purity πΏβˆ’ beam

οƒ  Intensity of πΏβˆ’ beam: ~350 k/spill οƒ  πΏβˆ’/πœŒβˆ’ = ~2.5 *J-PARC Hadron facility *Back Up Up

27

@PTEP , 2012, 02B009

Proton Beam Secondary Beam

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SLIDE 28

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

Energy calibration

Fit by 1st polynomial Off-beam calibration: Three Ξ³ ray from 238Th source

* Back up up

28

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SLIDE 29

Fit by 1st polynomial In-beam calibration: 10 Ξ³ rays from normal nuclei Fit by 1st polynomial +Exponential functions

* Back up up

29

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SLIDE 30

*Back up up *Background from Ξ›

12C is estimated using calibration data with CH2 target.

  • B𝚳 Distribution of 𝚳

πŸπŸ˜π† with CF2 Target (6.6 g/cm2)

Structure of

Ξ› 19F

30

*Reaction angle, 2<ΞΈ<12