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超子对中子星的影响

丁文波 杨文华

青岛大学学报(自然科学版)2011,Vol.24Issue(2):20-23,4.
青岛大学学报(自然科学版)2011,Vol.24Issue(2):20-23,4.DOI:10.3969/j.issn.1006-1037.2011.02.005

超子对中子星的影响

Effects of Σ Hyperons on Neutron Stars

丁文波 1杨文华2

作者信息

  • 1. 渤海大学数理学院物理系,辽宁,锦州,121013
  • 2. 青岛大学物理科学学院,山东,青岛,266071
  • 折叠

摘要

Abstract

From the relativistic mean field model and the theory of weak interactions, the effects of ∑ hyperons on neutron stars are studied. Results show that ∑ hyperons have effects on the three meson fields.They change the particle distribution and mass-radius relation of neutron stars. The effects of ∑ on the cooling of neutron stars are obviouly. The density ranges where direct lerca processes of both electorns and muons are allowed can be changed. On the other hand, ∑ hyperons lower the neutrino emissivity obviously, so it maybe not suitable for the fast cooling of neutron stars.

关键词

中子星/∑超子/物态方程/冷却

Key words

neutron stars/ ∑ hyperons/ EoS/ cooling

分类

数理科学

引用本文复制引用

丁文波,杨文华..超子对中子星的影响[J].青岛大学学报(自然科学版),2011,24(2):20-23,4.

青岛大学学报(自然科学版)

1006-1037

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