QCD coupling constant ($α_c$) and nonzero value of strange quark mass ($m_s\neq 0$) dependent stable stellar structure admitting observational results

Similar Items

• Influence of density-dependent bag function $B(n)$ on strange stars for non-zero strange quark mass ($m_s\neq0$) in $f(R,T)$ gravity consistent with observational validation
  by: Roy, Rohit, et al.
  Published: (2025)
• Impact of non-zero strange quark mass $(m_{s}\neq0)$ in $f(R,T)$ gravity admitting observational results of strange stars
  by: Bhattacharjee, Debadri, et al.
  Published: (2024)
• 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
  by: Chattopadhyay, Pradip Kumar, et al.
  Published: (2025)
• Hybrid compact stars with finite strange quark mass and dark energy: implications for astrophysical observations
  by: Roy, Rohit, et al.
  Published: (2024)
• The quark-mass dependence of the potential energy between static colour sources in the QCD vacuum with light and strange quarks
  by: Bulava, John, et al.
  Published: (2024)