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Study of Giant resonances in Hot Nuclei produced in Heavy Ion Fusion Reactions

Research Project

Project/Area Number 02640219
Research Category

Grant-in-Aid for General Scientific Research (C)

Allocation TypeSingle-year Grants
Research Field 核・宇宙線・素粒子
Research InstitutionTokyo Institute of Technology

Principal Investigator

KASAGI Jirohta  Tokyo Inst. of Tech., Ass. Professor, 理学部, 助教授 (10016181)

Co-Investigator(Kenkyū-buntansha) MURAKAMI Takeshi  Tokyo Inst. of Tech, Research Ass., 理学部, 助手 (20166250)
Project Period (FY) 1990 – 1991
Project Status Completed (Fiscal Year 1991)
Budget Amount *help
¥2,800,000 (Direct Cost: ¥2,800,000)
Fiscal Year 1991: ¥500,000 (Direct Cost: ¥500,000)
Fiscal Year 1990: ¥2,300,000 (Direct Cost: ¥2,300,000)
KeywordsGiant Resonance / Hot Nuclei / Heavy Ion Reaction / Fusion Reaction / High Energy gamma rays / Level Density / Limiting Temperature / Statistical Model / γ線多重度
Research Abstract

1. We have studied properties of hot nuclei by using ^<40>Ar+Ni, ^<92>Mo, and ^<122>Sn reactions with E/A=21 and 26 MeV by using the RIKEN Ring Cyclotron. Fusion reaction process was selected to study level densities and giant dipole resonances in hot nuclei. It was found that neutron energy spectra measured in coincidence with fusion residues were reproduced with the level density parameter a=A/(9<plus-minus>1). However, yields of the GDR decay gamma rays do not increase above E_x-250 MeV. The limiting temperature for the GDR gamma -ray decay were deduced as T_c-17A^<-1/3> for 80 < A < 150. It is highly desirable to continue the systematic study in order to answer the question whether the collective motion of the nucleus disappears at the high temperature or the hot nucleus is cooled down by particle evaporations before it emitts gamma rays.
2. In order to investigate the dependence of giant dipole resonances on the excitation energy and the angular momentum, high energy gamma rays were measured in ^<100>Mo+^<32>S reaction with E=150, 180 and 210 MeV using the tandem accelerator at JAERI. The result shows that the GDR width depends strongly on the thermal excitation energy for E_x > 100 MeV and an empirical formula GAMMA =4.5+0.035E_x+1.6x10^<-8>E_x^4 obtained in the previous work at RIKEN can explain the data very well.

Report

(3 results)
  • 1991 Annual Research Report   Final Research Report Summary
  • 1990 Annual Research Report
  • Research Products

    (13 results)

All Other

All Publications (13 results)

  • [Publications] K.Yoshida,et al.: "Excitation Energy Dependence of the Giant Dipcle Resonance in Hot Nuclei" Phys.Lett.245B. 7-12 (1990)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] J.Kasagi,et al.: "Excitation Energy and Spin Dependence of the Giant Dipole Resonance at Finite Temperature" Nucl.Phys.(1992)

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] K.Yoshida,et al.: "Neatron Emission for the Fusion of ^<40>Ar+Ni, ^<92>Mo, ^<122>Sn Reactions at E/A = 26 Mev" Phys.Rev.

    • Description
      「研究成果報告書概要(和文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] K. Yoshida, J. Kasagi, H. Hama, M. Sakurai, M. Kodama, K. Furutaka, K. Ieki, W. Galster, T. Kubo and M. Ishihara: ""Excitation Energy Dependence of the Giant Dipole Resonance in Hot Nuclei"" Phys. Lett.245B. 7-12 (1990)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] J. Kasagi, K. Yoshida, H. Hama, M. Sakurai, M. Kodama, K. Furutaka, K. Ieki, W. Galster, T. Kubo, M. Ishihara and A. Galonsky: ""Gamma-Ray and Neutron Emission from Hot Nuclei"" Proc. of the 2nd IN2P3-Riken Symposium on Heavy Ion Collisions, Obernai, France. World Scientific Pub. 304-313 (1990)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] J. Kasagi, K. Furutaka, T. Murakami, A. Yajima, M. Ohshima, S. Niiya, H. Tominaga, K. Yoshida, H. Hama, K. Ieki, W. Galster, T. Kubo, M. Ishihara and A. Galonsky: ""Excitation Energy and Spin Dependence of the Giant Dipole Resonance at Finite Temperature"" Nucl. Phys.(1992)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] K. Yoshida, J. Kasagi, H. Hama, M. Sakurai, M. Kodama, K. Furutaka, K. Ieki, W. Galster, T. Kubo, M. Ishihara and A. Galonsky: ""Neutron Emission for the Fusion of ^<40>Ar+Ni, ^<92>Mo, ^<122>Sn Reactions at E/A=26 MeV"" Phys. Rev. C.

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] J. Kasagi: ""Disappearance of the Giant Dipole Resonance in Hot Nuclei"" Proc. of the International symposium on Towards a Unified Picture of Dynamics, Nikko, Japan. AIP Conference Proceedings. (1992)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] J. Kasagi: ""Gamma-Ray Emission from Hot Nuclei"" Proc. of the Tours symposium on Nuclear Physics, Tours, France. World Scientific Pub. (1992)

    • Description
      「研究成果報告書概要(欧文)」より
    • Related Report
      1991 Final Research Report Summary
  • [Publications] J.Kasagi他: "Excitation energy and spin dependence of the giant dipole resonance at finite temperatare" Nucl.Phys.

    • Related Report
      1991 Annual Research Report
  • [Publications] K.Yoshida,J.Kasagi他: "Neution emission for the fusion of ^<40>Ar+Ni,^<92>Mo,^<122>Sn reactions at E/A=26 MeV" Phys.Rev.C.

    • Related Report
      1991 Annual Research Report
  • [Publications] J.Kasagi: "Disappearance of the giant dipole resonance in hot nuclei" AIP Conference Proceedings.

    • Related Report
      1991 Annual Research Report
  • [Publications] K.Yoshida,J.Kasagi et al.: "Excitation Energy Dependenee of the Giant Dipole Resonance in Hot Naclei" Phys.Lett.245B. 7-12 (1990)

    • Related Report
      1990 Annual Research Report

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Published: 1990-04-01   Modified: 2016-04-21  

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