Coulomb Dissociation of 26 Ne

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Coulomb Dissociation of 26 Ne Nakamura-laboratory Kazuhiro Ishikawa 02M01020

description

Coulomb Dissociation of 26 Ne. Nakamura-laboratory Kazuhiro Ishikawa 02M01020. Contents. Motivation Introduction Experimental Setup Data Analysis Results and Discussions Conclusion. Motivation. Search for the Soft Dipole Resonance (SDR) in 26 Ne. Coulomb Dissociation - PowerPoint PPT Presentation

Transcript of Coulomb Dissociation of 26 Ne

Page 1: Coulomb Dissociation of  26 Ne

Coulomb   Dissociation of 26Ne

Nakamura-laboratory

Kazuhiro Ishikawa

02M01020

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Contents

Motivation Introduction Experimental Setup Data Analysis Results and Discussions Conclusion

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Motivation

Coulomb Dissociation Nuclear Breakup

Search for the Soft Dipole Resonance (SDR) in 26Ne

Breakup

Develop a method to distinguish two components

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Introduction

RIPS

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Neutron-rich nuclei

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Giant Dipole Resonance (GDR) versusSoft Dipole Resonance (SDR)

stable nucleiE1 strength is almost exhausted by Giant Dipole Resonance (GDR).

Ex=80A-1/3 MeV (~ 20 MeV 20Ne)

unstable nuclei low lying E1 strength

Soft Dipole Resonance (SDR)

PredictionLow Ex (  8 MeV

26Ne)

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In the case of 26Ne

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Experimental MethodCoulomb DissociationUsing High Z

target

Cross section = photon number × B(E1)

Calculated by equivalent photon method

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Experimental Setup

DALI

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Experimental Setup

Reaction TargetPb: Coulomb DissociationAl : Nuclear Breakup

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Data Analysis

Silicon

Strip Detector

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Particle Identification Upstream of the Target

Pulse Height versus TOFΔE ~ Z2/v2=Z2TOF2

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Particle Identification Downstream of the Target

ΔE=Z2/v2

Ekin=Av2/2 EkinΔE ~ AZ2 A: mass Z: charge

ΔE=ΔEX + ΔEY

Ekin=E+ΔE

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Mass Spectrum of Ne Fragments

AZ2 ~ ΔEE’kin=ΔE(E+ΔE/2)b (Z=10)b=0.75

Select specific mass   Reaction Cross Section Angular Distribution

Neutron Tagged

Removal of beam contaminants

Selecting of Angle(1~6 degree)Selecting of Angle(1~6 degree)

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Results and Discussions

Neutron Counter

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Reaction Cross Section

Run 26Ne+pb

26Ne+Al

25Ne 119(2) 10(0.3)24Ne 211(3) 29(0.6)23Ne 167(3) 22(0.5)22Ne 197(3) 31(0.7)

Cross Section (mb)

ε : εn~30%

PbPb

AlAl

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Cross Section Ratio Ratio for 25Ne is high!

1. Coulomb dissociation for 25Ne2. Hindrance of σσ (Al)(Al) for 25Ne , 25Ne+Al→24Ne+n+x

%56)24(σ

)25(σ%34

)24(σ

)25(σ

pb

pb

Al

Al

(Al)/(Pb)

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Angular Distribution of Ne Fragments

Two components are seen.

Al Pb

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Estimation of the width by the fragmentation model

)2

exp(2

2

FE

ACd

dF

220

2

)1(

)1(

1

)(D

p

FF

p

FpF

pAA

AA

A

AAA

0 =87 MeV/c D =200~300 MeV/c

AP : Projectile massAF : Fragment mass

EF : Fragment energy

AP : Projectile massAF : Fragment mass

EF : Fragment energy

From Fermi motionFrom Fermi motion Target DeflectionTarget Deflection

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Wide

Narrow

This result for wide is agreement with Goldhaber model.

σ ⊥(M

eV/c

)σ ⊥

(MeV

/c)

Al wide +Pb wide×

Al narrow *Pb narrow■

Al wide +Pb wide×

Al narrow *Pb narrow■

(Pb)(Al) DD

(Pb)(Al) DD

MeV/c 267(5)(Al)D σc262(5)MeV/(Pb)D

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Conclusion

Electronics

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for 25Ne Large Coulomb dissociation for the 26Ne+Pb→25Ne+n

reaction Angular distributions Two components

(narrow ,wide)

1. wide component : In agreement with fragmentation model (nuclear component)

2. narrow component : Further investigations are necessary (Coulomb component?)

(Al)/Pb)(

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Special thanks toR332n Collaborators Julien GibelinB, Koichi YoshidaE, Takashi NakamuraA, Dider BeaumelB, Nori AoiE,

Hidetada BabaD, Yorick BlumefeldB, Zoltan ElekesE, Naoki FukudaE, Tomoko GomiD, Yosuke KondoA, Akito SaitoD, Yositeru SatoA, Eri TakeshitaD, Satoshi TakeuchiE, Takashi TeranisiC, Yasuhiro ToganoD, Victor LimaB, Yoshiyuki YanagisawaE, Attukalathil Mayyan VinodkumarA, Toshiyuki KuboE, Tohru MotobayashiE

A: Department of Physics. Tokyo Institute of TechnologyB: Institut de Physique Nuclaire, Orsay, FranceC: University of Tokyo (CNS), Riken CampusD: Department of Physics, Rikkyo UniversityE: The Institute of Physics and Chemical Research (Riken)Nakamura-laboratoryTakashi Sugimoto, Nobuyuki Matsui, Masako Ohara, Takumi Nakabayashi, Yoshiko

Hashimoto