Thermodynamics and Geometrical Optics of Reissner Nordstrom de Sitter Black Holes in Noncommutative Geometry

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Main Authors: Sereewat, Phongsakorn, Senjaya, David, Burikham, Piyabut
Format: Preprint
Published: 2026
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author Sereewat, Phongsakorn
Senjaya, David
Burikham, Piyabut
author_facet Sereewat, Phongsakorn
Senjaya, David
Burikham, Piyabut
contents We investigate the thermodynamic, optical, and dynamical properties of Reissner-Nordstrom-de Sitter black holes in a noncommutative spacetime with a minimal length scale Theta. Within a two-horizon framework, we formulate an effective first law of thermodynamics and introduce an entropy capturing correlations between the event and cosmological horizons. Imposing the lukewarm condition, where both horizons share a common temperature, uniquely determines the entropy correction and yields closed-form expressions for thermodynamic quantities. The analysis reveals a noncommutativity-induced second-order phase transition, emphasizing the role of short-distance structure. On the optical side, we study photon motion and weak gravitational lensing, showing that noncommutativity modifies the effective potential and critical impact parameter. Using the Gauss-Bonnet method, we derive the weak deflection angle and analyze the effects of charge and cosmological constant. We further connect geometry and dynamics through the Lyapunov exponent and quasinormal modes, showing systematic impacts on orbital instability and damping.
format Preprint
id arxiv_https___arxiv_org_abs_2603_20824
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Thermodynamics and Geometrical Optics of Reissner Nordstrom de Sitter Black Holes in Noncommutative Geometry
Sereewat, Phongsakorn
Senjaya, David
Burikham, Piyabut
High Energy Physics - Theory
We investigate the thermodynamic, optical, and dynamical properties of Reissner-Nordstrom-de Sitter black holes in a noncommutative spacetime with a minimal length scale Theta. Within a two-horizon framework, we formulate an effective first law of thermodynamics and introduce an entropy capturing correlations between the event and cosmological horizons. Imposing the lukewarm condition, where both horizons share a common temperature, uniquely determines the entropy correction and yields closed-form expressions for thermodynamic quantities. The analysis reveals a noncommutativity-induced second-order phase transition, emphasizing the role of short-distance structure. On the optical side, we study photon motion and weak gravitational lensing, showing that noncommutativity modifies the effective potential and critical impact parameter. Using the Gauss-Bonnet method, we derive the weak deflection angle and analyze the effects of charge and cosmological constant. We further connect geometry and dynamics through the Lyapunov exponent and quasinormal modes, showing systematic impacts on orbital instability and damping.
title Thermodynamics and Geometrical Optics of Reissner Nordstrom de Sitter Black Holes in Noncommutative Geometry
topic High Energy Physics - Theory
url https://arxiv.org/abs/2603.20824