×
近期发现有不法分子冒充我刊与作者联系,借此进行欺诈等不法行为,请广大作者加以鉴别,如遇诈骗行为,请第一时间与我刊编辑部联系确认(《中国物理C》(英文)编辑部电话:010-88235947,010-88236950),并作报警处理。
本刊再次郑重声明:
(1)本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
(2)本刊采编系统作者中心是投稿的唯一路径,该系统为ScholarOne远程稿件采编系统,仅在本刊投稿网网址(https://mc03.manuscriptcentral.com/cpc)设有登录入口。本刊不接受其他方式的投稿,如打印稿投稿、E-mail信箱投稿等,若以此种方式接收投稿均为假冒。
(3)所有投稿均需经过严格的同行评议、编辑加工后方可发表,本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿,并收取发表费用,均为假冒。
                  
《中国物理C》(英文)编辑部
2024年10月30日

Effects of ultra-strong magnetic field on electron capture rates of 55Co and 56Ni in the magnetar surrounding

  • The electron capture rates of 55Co and 56Ni in the ultra-strong magnetic field at four typical temperature-density points have been calculated using the nuclear shell model and Landau energy levels quantized approximate correction. The results show that the electron capture rates of 55Co and 56Ni are increased greatly in the ultra-strong magnetic field, and even exceed two orders of magnitude in the range from 4.414× 1013G to 2.207× 1017G. The change rate of electron abundance, Ýe, of 55Co and 56Ni under the condition of B=4.414× 1015G in the magnetar surrounding has been calculated and discussed, the proportions of Ýe of 55Co and 56Ni in the total Ýe have been reduced by 50 percent in all more than the condition without a magnetic field.
      PCAS:
  • 加载中
  • [1] Fassio-Canuto L. Phys. Rev., 1969, 187: 2138-2146[2] Horiuchi S, Suwa Y, Takami H et al. Mon. Not. R. Astron. Soc., 2008, 391: 1893-1899[3] Woods P M, Thompson C. Camb. Astroph. Seri., 2006, 39: 547-586[4] PENG Q H. Nucl. Phys. A, 2004, 738: 515-518[5] WANG K, LUO Z Q, LI Y L. Chin. Phys. Lett., 2012, 29: 049701[6] LIU M Q, ZHANG J, LUO Z Q. Astron. Astrphy., 2007, 463: 261-264[7] Nabi J U, Rahman M U. Phys. Lett. B, 2005, 612: 190-196[8] Nabi J U. Phys. Scri., 2010, 81: 025901[9] Langanke K, Martinez-Pinedo G. Phys. Lett. B, 1998, 436: 19-24[10] Aufderheide M B, Fushiki I, Woosley S E et al. Astrophys. J., 1994, 91: 389[11] Fuller G M, Flower W A, Newman W J. Astrophys. J. Suppl. S., 1980, 42: 447[12] Fuller G M, Flower W A, Newman W J. Astrophys. J., 1982, 252: 715[13] Fuller G M, Flower W A, Newman W J. Astrophys. J. Suppl. S., 1982, 48: 279[14] LUO Z Q. Journal of Sichuan University (Natural Science Edit ion), 2001, 38: 596-599
  • 加载中

Get Citation
DU Jun, LUO Zhi-Quan and LI Ping-Ping. Effects of ultra-strong magnetic field on electron capture rates of 55Co and 56Ni in the magnetar surrounding[J]. Chinese Physics C, 2014, 38(1): 015102. doi: 10.1088/1674-1137/38/1/015102
DU Jun, LUO Zhi-Quan and LI Ping-Ping. Effects of ultra-strong magnetic field on electron capture rates of 55Co and 56Ni in the magnetar surrounding[J]. Chinese Physics C, 2014, 38(1): 015102.  doi: 10.1088/1674-1137/38/1/015102 shu
Milestone
Received: 2013-03-19
Revised: 1900-01-01
Article Metric

Article Views(1469)
PDF Downloads(219)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Effects of ultra-strong magnetic field on electron capture rates of 55Co and 56Ni in the magnetar surrounding

    Corresponding author: LUO Zhi-Quan,

Abstract: The electron capture rates of 55Co and 56Ni in the ultra-strong magnetic field at four typical temperature-density points have been calculated using the nuclear shell model and Landau energy levels quantized approximate correction. The results show that the electron capture rates of 55Co and 56Ni are increased greatly in the ultra-strong magnetic field, and even exceed two orders of magnitude in the range from 4.414× 1013G to 2.207× 1017G. The change rate of electron abundance, Ýe, of 55Co and 56Ni under the condition of B=4.414× 1015G in the magnetar surrounding has been calculated and discussed, the proportions of Ýe of 55Co and 56Ni in the total Ýe have been reduced by 50 percent in all more than the condition without a magnetic field.

    HTML

Reference (1)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return