Pair neutrino energy loss for nuclei 56Fe at the late stages of stellar evolution

Get Citation
LIU Jing-Jing and LUO Zhi-Quan. Pair neutrino energy loss for nuclei 56Fe at the late stages of stellar evolution[J]. Chinese Physics C, 2008, 32(8): 617-619. doi: 10.1088/1674-1137/32/8/005
LIU Jing-Jing and LUO Zhi-Quan. Pair neutrino energy loss for nuclei 56Fe at the late stages of stellar evolution[J]. Chinese Physics C, 2008, 32(8): 617-619.  doi: 10.1088/1674-1137/32/8/005 shu
Milestone
Received: 2007-08-13
Revised: 2007-09-23
Article Metric

Article Views(2936)
PDF Downloads(628)
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:

Pair neutrino energy loss for nuclei 56Fe at the late stages of stellar evolution

    Corresponding author: LIU Jing-Jing,

Abstract: 

Based on the Weinberg-Salam theory, the pair neutrino energy loss rates for nuclei 56Fe are canvassed for the wide range of density and temperature. The results of ours (QLJ) are compared with those of Beaudet G, Petrosian V and Salpeter E. E's (QBPS), and it shows that the pair neutrino energy loss rates of QBPS are always larger than QLJ .The QBPS is 12.57%, 12.86%, 14.99%, 19.80% times higher than QLJ corresponding to the temperature T9=0.385, 1.0, 5.0, 10, respectively.

    HTML

Reference (1)

目录

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return