Scholarlink

Abstract <p>In disk accretion of gas onto a neutron star, high densities and temperatures are expected. The objective of the quantitative accretion model is to obtain boundary layer gas parameters during the development of small-scale instability. For critical accretion of incident matter on a neutron star, we have discussed the possibility of nucleosynthesis.</p>

错误：搜索内容不能为空，请输入英文关键词
错误：关键词超出字数限制，请精简
高级检索

Critical Accretion to Neutron Star with an Evaluation of Nucleosynthesis

  • 期刊论文

  • 发表日期：

    2025年11月1日

查看全文
  • A. G. Aksenov,
  • V. M. Chechetkin

摘要

Abstract

In disk accretion of gas onto a neutron star, high densities and temperatures are expected. The objective of the quantitative accretion model is to obtain boundary layer gas parameters during the development of small-scale instability. For critical accretion of incident matter on a neutron star, we have discussed the possibility of nucleosynthesis.