期刊文献+

The β Decay of ^21N

The β Decay of ^21N
下载PDF
导出
摘要 The β-delayed neutron and γ energy spectra taken from the decay of neutron-rich nucleus ^21N were measured by using the β - γ and β - n coincidence detection method. Thirteen new neutron groups ranging from 0.28 MeV to 4.98 MeV and with a total branching ratio of 88.7±4.2% were observed and presented. One γ transition with an energy of 1222 keV emitted from the excited state of ^21O and four γ transitions with energies of 1674, 2397, 2780, and 3175keV emitted from the excited states of ^20O were identified in the β decay chain of ^21N. The β decay half-life for ^21N is determined to be 82.9±1.9ms. The uncertainty of half-life is much smaller than the previous result. The β-delayed neutron and γ energy spectra taken from the decay of neutron-rich nucleus ^21N were measured by using the β - γ and β - n coincidence detection method. Thirteen new neutron groups ranging from 0.28 MeV to 4.98 MeV and with a total branching ratio of 88.7±4.2% were observed and presented. One γ transition with an energy of 1222 keV emitted from the excited state of ^21O and four γ transitions with energies of 1674, 2397, 2780, and 3175keV emitted from the excited states of ^20O were identified in the β decay chain of ^21N. The β decay half-life for ^21N is determined to be 82.9±1.9ms. The uncertainty of half-life is much smaller than the previous result.
出处 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第6期1992-1995,共4页 中国物理快报(英文版)
基金 Supported by the National Basic Research Programme of China under Grant Nos 2007CB815000 and 2005CB724800, the National Natural Science Foundation of China under Grant Nos 10775003,10475004, 10405001, 10221003 and J0730316.
关键词 supernova explosion proto-neutron star shock wave supernova explosion, proto-neutron star, shock wave
  • 相关文献

参考文献22

  • 1Buta A et al 2000 Nucl. Instrum. Methods A 455 412
  • 2Perrot F et al 2006 Phys. Rev. C 74 014313
  • 3Nummela S et al 2001 Phys. Rev. C 63 044316
  • 4Grevy S et al 2004 Nucl.Phys. A 734 369
  • 5Sumithrarachchi C S et al 2007 Phys. Rev. C 75 024305
  • 6Sumithrarachchi C S et al 2006 Phys. Rev. C 74 024322
  • 7Scheller K W et al 1994 Phys. Rev. C 49 1
  • 8Scheller K W et al 1995 Nucl. Phys. A 582 109
  • 9Harkewicz R et al 1991 Phys. Rev. C 44 6
  • 10Ozawa A et al 1995 Nucl. Phys. A 592 244

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部