CFT phase transition analysis of charged, rotating black holes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>D</mml:mi><mml:mo>=</mml:mo><mml:mn>4</mml:mn></mml:math>: A holographic thermodynamics approach

We investigate the holographic thermodynamics of 4-D Kerr-Newman anti–de Sitter (AdS) black holes, focusing on the conformal thermal states that are dual to these black holes. We explore the thermodynamic behavior within specific ensembles characterized by fixed sets of variables: <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mo stretchy="false">(</a:mo><a:mi mathvariant="script">Q</a:mi><a:mo>,</a:mo><a:mi mathvariant="script">J</a:mi><a:mo>,</a:mo><a:mi mathvariant="script">V</a:mi><a:mo>,</a:mo><a:mi>C</a:mi><a:mo stretchy="false">)</a:mo></a:math>, <h:math xmlns:h="http://www.w3.org/1998/Math/MathML" display="inline"><h:mrow><h:mo stretchy="false">(</h:mo><h:mi mathvariant="script">Q</h:mi><h:mo>,</h:mo><h:mi mathvariant="normal">Ω</h:mi><h:mo>,</h:mo><h:mi mathvariant="script">V</h:mi><h:mo>,</h:mo><h:mi>C</h:mi><h:mo stretchy="false">)</h:mo></h:mrow></h:math>, <o:math xmlns:o="http://www.w3.org/1998/Math/MathML" display="inline"><o:mrow><o:mo stretchy="false">(</o:mo><o:mi>φ</o:mi><o:mo>,</o:mo><o:mi mathvariant="normal">Ω</o:mi><o:mo>,</o:mo><o:mi mathvariant="script">V</o:mi><o:mo>,</o:mo><o:mi>C</o:mi><o:mo stretchy="false">)</o:mo></o:mrow></o:math>, <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"><u:mrow><u:mo stretchy="false">(</u:mo><u:mi>φ</u:mi><u:mo>,</u:mo><u:mi mathvariant="script">J</u:mi><u:mo>,</u:mo><u:mi mathvariant="script">V</u:mi><u:mo>,</u:mo><u:mi>C</u:mi><u:mo stretchy="false">)</u:mo></u:mrow></u:math>, <ab:math xmlns:ab="http://www.w3.org/1998/Math/MathML" display="inline"><ab:mrow><ab:mo stretchy="false">(</ab:mo><ab:mi mathvariant="script">Q</ab:mi><ab:mo>,</ab:mo><ab:mi mathvariant="normal">Ω</ab:mi><ab:mo>,</ab:mo><ab:mi>p</ab:mi><ab:mo>,</ab:mo><ab:mi>C</ab:mi><ab:mo stretchy="false">)</ab:mo></ab:mrow></ab:math>, and <gb:math xmlns:gb="http://www.w3.org/1998/Math/MathML" display="inline"><gb:mo stretchy="false">(</gb:mo><gb:mi>φ</gb:mi><gb:mo>,</gb:mo><gb:mi mathvariant="normal">Ω</gb:mi><gb:mo>,</gb:mo><gb:mi>p</gb:mi><gb:mo>,</gb:mo><gb:mi>C</gb:mi><gb:mo stretchy="false">)</gb:mo></gb:math>. Here, <lb:math xmlns:lb="http://www.w3.org/1998/Math/MathML" display="inline"><lb:mi>φ</lb:mi></lb:math>, <nb:math xmlns:nb="http://www.w3.org/1998/Math/MathML" display="inline"><nb:mi mathvariant="script">Q</nb:mi></nb:math>, <qb:math xmlns:qb="http://www.w3.org/1998/Math/MathML" display="inline"><qb:mi mathvariant="normal">Ω</qb:mi></qb:math>, <tb:math xmlns:tb="http://www.w3.org/1998/Math/MathML" display="inline"><tb:mi mathvariant="script">J</tb:mi></tb:math>, <wb:math xmlns:wb="http://www.w3.org/1998/Math/MathML" display="inline"><wb:mi>p</wb:mi></wb:math>, <yb:math xmlns:yb="http://www.w3.org/1998/Math/MathML" display="inline"><yb:mi mathvariant="script">V</yb:mi></yb:math>, and <bc:math xmlns:bc="http://www.w3.org/1998/Math/MathML" display="inline"><bc:mi>C</bc:mi></bc:math> represent the electric potential, electric charge, angular velocity, angular momentum, conformal field theory (CFT) pressure, CFT volume, and central charge, respectively. The inclusion of both charge and momentum significantly enriches the regime of phase transitions, leading to a variety of phenomena including first-order van der Waals-type phase transitions, (de)confinement phase transitions, Davies-type phase transitions, and second-order superfluid <dc:math xmlns:dc="http://www.w3.org/1998/Math/MathML" display="inline"><dc:mi>λ</dc:mi></dc:math>-type phase transitions. Notably, the introduction of the CFT pressure variable allows us to identify phase transitions and critical behavior in the <fc:math xmlns:fc="http://www.w3.org/1998/Math/MathML" display="inline"><fc:mo stretchy="false">(</fc:mo><fc:mi mathvariant="script">Q</fc:mi><fc:mo>,</fc:mo><fc:mi mathvariant="normal">Ω</fc:mi><fc:mo>,</fc:mo><fc:mi>p</fc:mi><fc:mo>,</fc:mo><fc:mi>C</fc:mi><fc:mo stretchy="false">)</fc:mo></fc:math> and <lc:math xmlns:lc="http://www.w3.org/1998/Math/MathML" display="inline"><lc:mo stretchy="false">(</lc:mo><lc:mi>φ</lc:mi><lc:mo>,</lc:mo><lc:mi mathvariant="normal">Ω</lc:mi><lc:mo>,</lc:mo><lc:mi>p</lc:mi><lc:mo>,</lc:mo><lc:mi>C</lc:mi><lc:mo stretchy="false">)</lc:mo></lc:math> ensembles, which had not been previously observed. This study underscores the complexity and richness of phase transitions in these systems due to the inclusion of both charge and angular momentum.

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Physical review. D/Physical review. D.
Published
2025-03-28
DOI
https://doi.org/10.1103/physrevd.111.066022
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7
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Black Holes and Theoretical Physics
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article
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article

CFT phase transition analysis of charged, rotating black holes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>D</mml:mi><mml:mo>=</mml:mo><mml:mn>4</mml:mn></mml:math>: A holographic thermodynamics approach

Prabwal Phukon, Abhishek Baruah
7 citations
Physical review. D/Physical review. D.
Black Holes and Theoretical Physics
13.09
article

CFT phase transition analysis of charged, rotating black holes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>D</mml:mi><mml:mo>=</mml:mo><mml:mn>4</mml:mn></mml:math>: A holographic thermodynamics approach

Prabwal Phukon, Abhishek Baruah
article en
7 citations

Abstract

We investigate the holographic thermodynamics of 4-D Kerr-Newman anti–de Sitter (AdS) black holes, focusing on the conformal thermal states that are dual to these black holes. We explore the thermodynamic behavior within specific ensembles characterized by fixed sets of variables: <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mo stretchy="false">(</a:mo><a:mi mathvariant="script">Q</a:mi><a:mo>,</a:mo><a:mi mathvariant="script">J</a:mi><a:mo>,</a:mo><a:mi mathvariant="script">V</a:mi><a:mo>,</a:mo><a:mi>C</a:mi><a:mo stretchy="false">)</a:mo></a:math>, <h:math xmlns:h="http://www.w3.org/1998/Math/MathML" display="inline"><h:mrow><h:mo stretchy="false">(</h:mo><h:mi mathvariant="script">Q</h:mi><h:mo>,</h:mo><h:mi mathvariant="normal">Ω</h:mi><h:mo>,</h:mo><h:mi mathvariant="script">V</h:mi><h:mo>,</h:mo><h:mi>C</h:mi><h:mo stretchy="false">)</h:mo></h:mrow></h:math>, <o:math xmlns:o="http://www.w3.org/1998/Math/MathML" display="inline"><o:mrow><o:mo stretchy="false">(</o:mo><o:mi>φ</o:mi><o:mo>,</o:mo><o:mi mathvariant="normal">Ω</o:mi><o:mo>,</o:mo><o:mi mathvariant="script">V</o:mi><o:mo>,</o:mo><o:mi>C</o:mi><o:mo stretchy="false">)</o:mo></o:mrow></o:math>, <u:math xmlns:u="http://www.w3.org/1998/Math/MathML" display="inline"><u:mrow><u:mo stretchy="false">(</u:mo><u:mi>φ</u:mi><u:mo>,</u:mo><u:mi mathvariant="script">J</u:mi><u:mo>,</u:mo><u:mi mathvariant="script">V</u:mi><u:mo>,</u:mo><u:mi>C</u:mi><u:mo stretchy="false">)</u:mo></u:mrow></u:math>, <ab:math xmlns:ab="http://www.w3.org/1998/Math/MathML" display="inline"><ab:mrow><ab:mo stretchy="false">(</ab:mo><ab:mi mathvariant="script">Q</ab:mi><ab:mo>,</ab:mo><ab:mi mathvariant="normal">Ω</ab:mi><ab:mo>,</ab:mo><ab:mi>p</ab:mi><ab:mo>,</ab:mo><ab:mi>C</ab:mi><ab:mo stretchy="false">)</ab:mo></ab:mrow></ab:math>, and <gb:math xmlns:gb="http://www.w3.org/1998/Math/MathML" display="inline"><gb:mo stretchy="false">(</gb:mo><gb:mi>φ</gb:mi><gb:mo>,</gb:mo><gb:mi mathvariant="normal">Ω</gb:mi><gb:mo>,</gb:mo><gb:mi>p</gb:mi><gb:mo>,</gb:mo><gb:mi>C</gb:mi><gb:mo stretchy="false">)</gb:mo></gb:math>. Here, <lb:math xmlns:lb="http://www.w3.org/1998/Math/MathML" display="inline"><lb:mi>φ</lb:mi></lb:math>, <nb:math xmlns:nb="http://www.w3.org/1998/Math/MathML" display="inline"><nb:mi mathvariant="script">Q</nb:mi></nb:math>, <qb:math xmlns:qb="http://www.w3.org/1998/Math/MathML" display="inline"><qb:mi mathvariant="normal">Ω</qb:mi></qb:math>, <tb:math xmlns:tb="http://www.w3.org/1998/Math/MathML" display="inline"><tb:mi mathvariant="script">J</tb:mi></tb:math>, <wb:math xmlns:wb="http://www.w3.org/1998/Math/MathML" display="inline"><wb:mi>p</wb:mi></wb:math>, <yb:math xmlns:yb="http://www.w3.org/1998/Math/MathML" display="inline"><yb:mi mathvariant="script">V</yb:mi></yb:math>, and <bc:math xmlns:bc="http://www.w3.org/1998/Math/MathML" display="inline"><bc:mi>C</bc:mi></bc:math> represent the electric potential, electric charge, angular velocity, angular momentum, conformal field theory (CFT) pressure, CFT volume, and central charge, respectively. The inclusion of both charge and momentum significantly enriches the regime of phase transitions, leading to a variety of phenomena including first-order van der Waals-type phase transitions, (de)confinement phase transitions, Davies-type phase transitions, and second-order superfluid <dc:math xmlns:dc="http://www.w3.org/1998/Math/MathML" display="inline"><dc:mi>λ</dc:mi></dc:math>-type phase transitions. Notably, the introduction of the CFT pressure variable allows us to identify phase transitions and critical behavior in the <fc:math xmlns:fc="http://www.w3.org/1998/Math/MathML" display="inline"><fc:mo stretchy="false">(</fc:mo><fc:mi mathvariant="script">Q</fc:mi><fc:mo>,</fc:mo><fc:mi mathvariant="normal">Ω</fc:mi><fc:mo>,</fc:mo><fc:mi>p</fc:mi><fc:mo>,</fc:mo><fc:mi>C</fc:mi><fc:mo stretchy="false">)</fc:mo></fc:math> and <lc:math xmlns:lc="http://www.w3.org/1998/Math/MathML" display="inline"><lc:mo stretchy="false">(</lc:mo><lc:mi>φ</lc:mi><lc:mo>,</lc:mo><lc:mi mathvariant="normal">Ω</lc:mi><lc:mo>,</lc:mo><lc:mi>p</lc:mi><lc:mo>,</lc:mo><lc:mi>C</lc:mi><lc:mo stretchy="false">)</lc:mo></lc:math> ensembles, which had not been previously observed. This study underscores the complexity and richness of phase transitions in these systems due to the inclusion of both charge and angular momentum.

Physical review. D/Physical review. D.Vol. 111(6)
Dibrugarh University (IN)
Openalex Percentile: Top 2%
Black Holes and Theoretical Physics
13.09
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