Topology of nonlinearly charged black hole chemistry via massive gravity

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F62690094%3A18470%2F23%3A50020650" target="_blank" >RIV/62690094:18470/23:50020650 - isvavai.cz</a>

Výsledek na webu

<a href="https://link.springer.com/article/10.1140/epjc/s10052-023-11933-w" target="_blank" >https://link.springer.com/article/10.1140/epjc/s10052-023-11933-w</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1140/epjc/s10052-023-11933-w" target="_blank" >10.1140/epjc/s10052-023-11933-w</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Topology of nonlinearly charged black hole chemistry via massive gravity

Popis výsledku v původním jazyce

The classification of critical points of charged topological black holes (TBHs) in anti-de Sitter spacetime (AdS) under the Power Maxwell Invariant (PMI)-massive gravity is accomplished within the framework of black hole chemistry (BHC). Considering the grand canonical ensemble (GCE), we show that d = 4 black hole have only one topological class, whereas d &gt;= 5 black holes belong to two different topology classes. Furthermore, the conventional critical point characterized by negative topological charge coincides with the maximum extreme point of temperature; and the novel critical point featuring opposite topological charge corresponds to theminimum extreme point of temperature. With increasing pressure, new phases emerge at the novel critical point while disappear from the conventional one. Moreover, a atypical van der Waals (vdW) behavior is found in d &gt;= 6 dimensions, and the anomaly disappears at the traditional critical point. In the limit of nonlinearity parameter s -&gt; 1, different topology classes are only obtained in the GCE and they may not exist within the canonical ensemble. With the absence of electric potential Phi, the neutral TBHs share the same topological classification results as the charged TBHs in the GCE of Maxwell-massive gravity.

Název v anglickém jazyce

Topology of nonlinearly charged black hole chemistry via massive gravity

Popis výsledku anglicky

The classification of critical points of charged topological black holes (TBHs) in anti-de Sitter spacetime (AdS) under the Power Maxwell Invariant (PMI)-massive gravity is accomplished within the framework of black hole chemistry (BHC). Considering the grand canonical ensemble (GCE), we show that d = 4 black hole have only one topological class, whereas d &gt;= 5 black holes belong to two different topology classes. Furthermore, the conventional critical point characterized by negative topological charge coincides with the maximum extreme point of temperature; and the novel critical point featuring opposite topological charge corresponds to theminimum extreme point of temperature. With increasing pressure, new phases emerge at the novel critical point while disappear from the conventional one. Moreover, a atypical van der Waals (vdW) behavior is found in d &gt;= 6 dimensions, and the anomaly disappears at the traditional critical point. In the limit of nonlinearity parameter s -&gt; 1, different topology classes are only obtained in the GCE and they may not exist within the canonical ensemble. With the absence of electric potential Phi, the neutral TBHs share the same topological classification results as the charged TBHs in the GCE of Maxwell-massive gravity.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2023

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

European Physical Journal C

ISSN

1434-6044

e-ISSN

1434-6052

Svazek periodika

83

Číslo periodika v rámci svazku

8

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

15

Strana od-do

"Article Number: 773"

Kód UT WoS článku

001058637000001

EID výsledku v databázi Scopus

2-s2.0-85169545711