期刊文献+

Neutrino energy loss by electron capture on strongly screened iron group nuclei

Neutrino energy loss by electron capture on strongly screened iron group nuclei
原文传递
导出
摘要 The influences on the neutrino energy loss rates in iron group nuclei at the same density are investigated in the presence of strong electron screening and in the absence of electron screening. The results show that at a temperature of 15 × 10^9 K, the neutrino energy loss rates which come from the electron capture process for most iron group nuclei decrease no more than 2 orders of magnitude but for the others (such as ^53,55,56,57,58,59,6o Co, ^56,59Ni) they can decrease about 3 orders of magnitude due to strong electron screening (SES), whereas, at a temperature of 10^9K the neutrino energy loss rates of the most iron group nuclei can be diminished greatly due to the SES. For example, ^61Fe, ^60Fe, and ^62Ni the neutrino energy loss rates decrease about 4, 15 and 16 orders of magnitude and for ^57Cr, ^58Cr, and ^60Cr decrease about 18, 12, and 10 orders of magnitude respectively. According to our calculations the neutrino energy loss rates of nuclei ^58Mn, ^59Mn, ^60Mn, and ^62Mn may decrease about 13 orders of magnitude at a temperature of 10^9 K due to the SES. The influences on the neutrino energy loss rates in iron group nuclei at the same density are investigated in the presence of strong electron screening and in the absence of electron screening. The results show that at a temperature of 15 × 10^9 K, the neutrino energy loss rates which come from the electron capture process for most iron group nuclei decrease no more than 2 orders of magnitude but for the others (such as ^53,55,56,57,58,59,6o Co, ^56,59Ni) they can decrease about 3 orders of magnitude due to strong electron screening (SES), whereas, at a temperature of 10^9K the neutrino energy loss rates of the most iron group nuclei can be diminished greatly due to the SES. For example, ^61Fe, ^60Fe, and ^62Ni the neutrino energy loss rates decrease about 4, 15 and 16 orders of magnitude and for ^57Cr, ^58Cr, and ^60Cr decrease about 18, 12, and 10 orders of magnitude respectively. According to our calculations the neutrino energy loss rates of nuclei ^58Mn, ^59Mn, ^60Mn, and ^62Mn may decrease about 13 orders of magnitude at a temperature of 10^9 K due to the SES.
出处 《Chinese Physics B》 SCIE EI CAS CSCD 2007年第12期3624-3630,共7页 中国物理B(英文版)
基金 Project supported by the National Natural Science Foundation of China (Grant No 10347008).
关键词 neutrino energy loss strong electron screening electron capture neutrino energy loss, strong electron screening, electron capture
  • 相关文献

参考文献17

  • 1Fuller G M, Fowler W A and Newman M J 1980 AP. J. 42 447.
  • 2Fuller G M, Fowler W A and Newman M J 1982 AP. J. 252 715.
  • 3Fuller G M, Fowler W A and Newman M J 1982 AP. J. 48 279.
  • 4Fuller G M, Fowler W A and Newman M J 1985 AP. J. 293 1.
  • 5Itoh N, Nishikawa A and Kohyama Y 1996 AP. J. 470 1015.
  • 6Itoh N, Hayashi H, Nishikawa A and Kohyama Y 1996 AP. J. 102 411.
  • 7Esposito S, Mangano G and Miele G 2003 Nuclear Physics. B 658 217.
  • 8Gutierrez J, Garcia-Berro E, Iben I, Isern J, Labay J and Canal R 1996 ApJ 459 701.
  • 9Bravo E and Garcie-Senz D 1999 MNRAS 307 984.
  • 10Luo Z Q and Peng Q H 1996 Science in China 26 665.
  • 1阿秒电子捕获[J].激光与光电子学进展,2008,45(2):39-39.
  • 2Zhang Ruitian,Ma Xinwen,Zhang Shaofen,Zhu Xiaolong,Feng Wentian,Guo Dalong,Li Bin,Liu Huiping,Wang Jianguo,Yan Shuncheng,Zhang Pengju,Wang Qian.Electron Capture to Continuum of Transfer Ionization in 30 keV/u He2+ on Argon Collision[J].IMP & HIRFL Annual Report,2011(1):179-179.
  • 3陈百鸣.发现微中子的质量[J].发现.图形科普,2000(4):12-17.
  • 4Wang Yuyu Zhao Yongtao Cheng Rui Zhou Xianming Lei Yu Wang Xing Xu Ge Sun Yuanpo Xiao Guoqing.Energy Loss of Low Energy H, He and O Ions in Carbon Foils[J].IMP & HIRFL Annual Report,2011(1):43-43.
  • 5洪峰笑.物理世界11个未解之谜[J].发现.图形科普,2002(8):36-41.
  • 6都有为.自旋——未来的科技明星[J].科技导报,2014,32(25):1-1.
  • 7刘晶晶.Bremsstrahlung neutrino energy loss for ^(24)Mg,^(28)Si,^(32)S,^(40)Ca,^(56)Fe in strong electron screening[J].Chinese Physics C,2010,34(2):171-176.
  • 8刘晶晶.The competition of neutrino energy loss due to the pair, photo-, plasma process at the late stages of stellar evolution[J].Chinese Physics C,2009,33(1):15-19.
  • 9K.A.Olive,K.Agashe,C.Amsler,M.Antonelli,J.-F.Arguin,D.M.Asner,H.Baer,H.R.Band,R.M.Barnett,T.Basaglia,C.W.Bauer,J.J.Beatty,V.I.Belousov,J.Beringer,G.Bernardi,S.Bethke,H.Bichsel,O.Biebe,E.Blucher,S.Blusk,G.Brooijmans,O.Buchmueller,V.Burkert,M.A.Bychkov,R.N.Cahn,M.Carena,A.Ceccucci,A.Cerr,D.Chakraborty,M.-C.Chen,R.S.Chivukula,K.Copic,G.Cowan,O.Dahl,G.D'Ambrosio,T.Damour,D.de Florian,A.de Gouvea,T.DeGrand,P.de Jong,G.Dissertor,B.A.Dobrescu,M.Doser,M.Drees,H.K.Dreiner,D.A.Edwards,S.Eidelman,J.Erler,V.V.Ezhela,W.Fetscher,B.D.Fields,B.Foster,A.Freitas,T.K.Gaisser,H.Gallagher,L.Garren,H.-J.Gerber,G.Gerbier,T.Gershon,T.Gherghetta,S.Golwala,M.Goodman,C.Grab,A.V.Gritsan,C.Grojean,D.E.Groom,M.Grnewald,A.Gurtu,T.Gutsche,H.E.Haber,K.Hagiwara,C.Hanhart,S.Hashimoto,Y.Hayato,K.G.Hayes,M.Heffner,B.Heltsley,J.J.Hernandez-Rey,K.Hikasa,A.Hocker,J.Holder,A.Holtkamp,J.Huston,J.D.Jackson,K.F.Johnson,T.Junk,M.Kado,D.Karlen,U.F.Katz,S.R.Klein,E.Klempt,R.V.Kowalewski,F.Krauss,M.Kreps,B.Krusche,Yu.V.Kuyanov,Y.Kwon,O.Lahav,J.Laiho,P.Langacker,A.Liddle,Z.Ligeti,C.-J.Lin,T.M.Liss,L.Littenberg,K.S.Lugovsky,S.B.Lugovsky,F.Maltoni,T.Mannel,A.V.Manohar,W.J.Marciano,A.D.Martin,A.Masoni,J.Matthews,D.Milstead,P.Molaro,K.Monig,F.Moortgat,M.J.Mortonson,H.Murayama,K.Nakamura,M.Narain,P.Nason,S.Navas,M.Neubert,P.Nevski,Y.Nir,L.Pape,J.Parsons,C.Patrignani,J.A.Peacock,M.Pennington,S.T.Petcov,Kavli IPMU,A.Piepke,A.Pomarol,A.Quadt,S.Raby,J.Rademacker,G.Raffel,B.N.Ratcliff,P.Richardson,A.Ringwald,S.Roesler,S.Rolli,A.Romaniouk,L.J.Rosenberg,J,L.Rosner,G.Rybka,C.T.Sachrajda,Y.Sakai,G.P.Salam,S.Sarkar,F.Sauli,O.Schneider,K.Scholberg,D.Scott,V.Sharma,S.R.Sharpe,M.Silari,T.Sjostrand,P.Skands,J.G.Smith,G.F.Smoot,S.Spanier,H.Spieler,C.Spiering,A.Stahl,T.Stanev,S.L.Stone,T.Sumiyoshi,M.J.Syphers,F.Takahashi,M.Tanabashi,J.Terning,L.Tiator,M.Titov,N.P.Tkachenko,N.A.Tornqvist,D.Tovey,G.Valencia,G.Venanzoni,M.G.Vincter,P.Vogel,A.Vogt,S.P.Wakely,W.Walkowiak,C.W.Walter,D.R.Ward,G.Weiglein,D.H.Weinberg,E.J.Weinberg,M.White,L.R.Wiencke,C.G.Wohl,L.Wolfenstein,J.Womersley,C.L.Woody,R.L.Workman,A.Yamamoto,W.-M.Yao,G.P.Zeller,O.V.Zenin,J.Zhang,R.-Y.Zhu,F.Zimmermann,P.A.Zyla,G.Harper,V.S.Lugovsky,P.Schaffner.COMMONLY USED RADIOACTIVE SOURCES[J].Chinese Physics C,2014,38(9):466-466.
  • 10张富祥,金尚宪.电子屏蔽和离子间关联对Pd-D系统中氘核聚变率的影响[J].科学通报,1992,37(14):1276-1279.

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