This work is motivated by the sign problem in a logarithmic parameter of black hole entropy
and the existing more massive white dwarfs than the Chandrasekhar mass limit. We
examine the quadratic, linear, and linear–quadratic generalized uncertainty principle (GUP)
models within the virtue of recent masses and radii of white dwarfs. We consider the
modification generated by introducing the minimal length on the degenerate Fermi gas
equation of state (EoS) and the hydrostatic equation. For the latter, we applied Verlinde's …

This work is motivated by the sign problem in a logarithmic parameter of black hole entropy
and the existing more massive white dwarfs than the Chandrasekhar mass limit. We
examine the quadratic, linear, and linear-quadratic generalized uncertainty principle (GUP)
models within the virtue of recent masses and radii of white dwarfs. We consider the
modification generated by introducing the minimal length proposal on the degenerate Fermi
gas equation of state (EOS) and on the hydrostatic equation. For the latter, we applied …