Scholarlink

Equation of State of the coupled dark energy can be expressed in terms of the ration of total pressure to the vacuum energy density. Here in this article the stability of the saddle points are produced for different types of functions which can be considered to produce the quintessence models. Chosen functions are further tested with CPL parameterization to fit them for dark energy models.

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

Coupled Dark Energy Models and CPL Parameterization to Explain Chosen Equations of State

  • 会议论文

  • 发表日期：

    2025年

查看全文
  • Sovan Ghosh

摘要

Equation of State of the coupled dark energy can be expressed in terms of the ration of total pressure to the vacuum energy density. Here in this article the stability of the saddle points are produced for different types of functions which can be considered to produce the quintessence models. Chosen functions are further tested with CPL parameterization to fit them for dark energy models.