Effect of Generalized Uncertainty Principle on Main-Sequence Stars and White Dwarfs

Abstract

This paper addresses the effect of generalized uncertainty principle, emerged by a different approaches of quantum gravity within Planck scale, on thermodynamic properties of photon, non-relativistic ideal gases and degenerate fermions. A modification in pressure, particle number and energy density are calculated. Astrophysical objects such as main sequence stars and white dwarfs are examined and discussed as an application. A modification in Lane-Emden equation due to a change in a polytropic relation caused by the presence of quantum gravity, is investigated. The applicable range of quantum gravity parameters is estimated. The bounds in the perturbed parameters are relatively large but it may be considered reasonable values in the astrophysical regime.

12 pages. arXiv admin note: text overlap with arXiv:1301.6133 by other authors

References in corpus (6)

• Universality of Quantum Gravity Corrections
• Natural extension of the Generalised Uncertainty Principle
• Statistical physics in deformed spaces with minimal length
• Analysis of White Dwarfs with Strange-Matter Cores
• White dwarfs as test objects of Lorentz violations
• The Minimal Length and the Quantum Partition Functions

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