Finite Temperature Considerations in the Structure of Quadratic GUP-modified White Dwarfs
arXiv:2210.09886 · doi:10.1142/S0218271823500499
Abstract
In quantum gravity phenomenology, the effect of the generalized uncertainty principle (GUP) on white dwarfs has been given much attention in the literature. However, these studies assume a zero temperature equation of state (EoS), consequently excluding young white dwarfs whose initial temperatures are substantially high. To that cause, this paper calculates the Chandrasekhar EoS and resulting mass-radius relations of finite temperature white dwarfs modified by the quadratic GUP, an approach that extends Heisenberg's uncertainty principle by a quadratic term in momenta. The EoS was first approximated by treating the quadratic GUP parameter as perturbative, causing the EoS to exhibit expected thermal deviations at low pressures, and conflicting behaviors at high pressures, depending on the order of approximation. We then proceeded with a full numerical simulation of the modified EoS, and showed that in general, finite temperatures cause the EoS at low pressures to soften, while the quadratic GUP stiffens the EoS at high pressures. This modified EoS was then applied to the Tolman-Oppenheimer-Volkoff equations and its classical approximation to obtain the modified mass-radius relations for general relativistic and Newtonian white dwarfs. The relations for both cases were found to exhibit the expected thermal deviations at small masses, where low-mass white dwarfs are shifted to the high-mass regime at large radii, while high-mass white dwarfs acquire larger masses, beyond the Chandrasekhar limit. Additionally, we find that for sufficiently large values of the GUP parameter and temperature, we obtain mass-radius relations that are completely removed from the ideal case, as high-mass deviations due to GUP and low-mass deviations due to temperature are no longer mutually exclusive.
References in corpus (16)
- Universality of Quantum Gravity Corrections
- Discreteness of Space from the Generalized Uncertainty Principle
- White Dwarf Mass Distribution in the SDSS
- Quantum-corrected black hole thermodynamics to all orders in the Planck length
- GUP parameter from quantum corrections to the Newtonian potential
- Minimal Length Uncertainty Relation and gravitational quantum well
- A Higher Order GUP with Minimal Length Uncertainty and Maximal Momentum II: Applications
- Minimal Length in Quantum Gravity, Equivalence Principle and Holographic Entropy Bound
- Measurements of Physical Parameters of White Dwarfs: A Test of the Mass-Radius Relation
- Analysis of White Dwarfs with Strange-Matter Cores
- White dwarfs as test objects of Lorentz violations
- The generalized uncertainty principle effect in acoustic black holes
- On the Chandrasekhar Limit in Generalized Uncertainty Principles
- Thermodynamics of Bardeen regular black hole with generalized uncertainty principle
- A framework for nonrelativistic isotropic models based on generalized uncertainty principles
- White-dwarfs equation of state and structure: The effect of temperature