Maximum mass limit of strange stars in quadratic curvature-matter coupled gravity

Documents similaires

• The role of finite value of strange quark mass $(m_{s}\neq0)$ and baryon number density $(n)$ on the stability and maximum mass of strange stars
  par: Chattopadhyay, Pradip Kumar, et autres
  Publié: (2025)
• Impact of non-zero strange quark mass $(m_{s}\neq0)$ in $f(R,T)$ gravity admitting observational results of strange stars
  par: Bhattacharjee, Debadri, et autres
  Publié: (2024)
• Maximum mass of singularity-free anisotropic compact stars in Rastall theory of gravity
  par: Biswas, Sourav, et autres
  Publié: (2025)
• ACT DR6 Leads to Stronger Evidence for Dynamical Dark Matter
  par: Wang, Deng, et autres
  Publié: (2025)
• Perturbed $f(R)$ gravity coupled with neutrinos: exploring cosmological implications
  par: Yarahmadi, Muhammad, et autres
  Publié: (2024)