Circular Geodesics and Phase Transitions of Charged Black Holes in AdS
Chandrasekhar Bhamidipati, Shrohan Mohapatra
Abstract
Chandrasekhar Bhamidipati, Shrohan Mohapatra
Abstract
The motion of neutral and charged test particles in the gravitational field of a Reissner-Nordstr\{o}m black hole in Anti de Sitter space-time is investigated, concentrating on the case of circular orbits. A classification of circular orbits based on black hole parameters depending on charge Q, mass M and cosmological constant parameter $l$, together with charge to mass ratio $\epsilon=q/m$ of the test particles is presented. The analysis shows the presence of circular orbits at special limiting values, $M_{\rm cr}=4/\sqrt{6} Q$ and $l_{\rm cr}=6 Q$. Thermodynamically, these values are known to occur when the black hole is critical and on the verge of a second order phase transition. We also extend the correspondence of thermodynamics and phase transitions with the radius and impact parameter of circular geodesics, to the case of charged particles.
OpenAlex reports 3 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
The motion of neutral and charged test particles in the gravitational field of a Reissner-Nordstr\{o}m black hole in Anti de Sitter space-time is investigated, concentrating on the case of circular orbits. A classification of circular orbits based on black hole parameters depending on charge Q, mass M and cosmological constant parameter $l$, together with charge to mass ratio $\epsilon=q/m$ of the test particles is presented. The analysis shows the presence of circular orbits at special limiting values, $M_{\rm cr}=4/\sqrt{6} Q$ and $l_{\rm cr}=6 Q$. Thermodynamically, these values are known to occur when the black hole is critical and on the verge of a second order phase transition. We also extend the correspondence of thermodynamics and phase transitions with the radius and impact parameter of circular geodesics, to the case of charged particles.
Key concepts: Physics, Black hole (networking), Circular orbit, Geodesic, RADIUS, Charge (physics), Charged black hole, Test particle