Gup-corrected black holes: thermodynamic properties, evaporation time and shadow constraint from EHT observations of M87*and Sgr A*
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F62690094%3A18470%2F24%3A50021721" target="_blank" >RIV/62690094:18470/24:50021721 - isvavai.cz</a>
Result on the web
<a href="https://link.springer.com/article/10.1140/epjp/s13360-024-05561-w" target="_blank" >https://link.springer.com/article/10.1140/epjp/s13360-024-05561-w</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1140/epjp/s13360-024-05561-w" target="_blank" >10.1140/epjp/s13360-024-05561-w</a>
Alternative languages
Result language
angličtina
Original language name
Gup-corrected black holes: thermodynamic properties, evaporation time and shadow constraint from EHT observations of M87*and Sgr A*
Original language description
In this manuscript, we implement the generalized uncertainty principle (GUP) with linear and quadratic moment for Schwarzschild black hole metric in order to study the influence of quantum effect on the thermodynamics and evaporation of black hole. To this end, we first derive the GUP-modified Hawking temperature of a black hole in the semi-classical framework. Due to the existence of the GUP effect, there is a maximum Hawking temperature. We determine the entropy, heat capacity and Helmholtz free energy with heuristic analysis that investigates the particle absorbed by black hole. Furthermore, we also verify that these quantities are modified by the GUP, the influence of quantum effect on the black hole phase transition is discussed in detail. Then, we analyze the black hole evaporation process in the mentioned framework and examine the obtained results by graphical methods and compare them with each other. We likewise explore the behavior of the event horizon radius, photon sphere radius, and shadow silhouette when influenced by the GUP-corrected Schwarzschild black hole (GCSBH) parameters. We intend to establish restrictions for alpha by utilizing the event horizon telescope (EHT) data for M87* and Sagittarius A* (Sgr A*). Our findings show that Sgr A* provides more robust constraints. As the parameter beta grows, the range of constraints for alpha expands. For Sgr A* one, we find that the shadow radius is close to the observed value at smaller values of alpha.
Czech name
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2024
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
The European physical journal plus
ISSN
2190-5444
e-ISSN
2190-5444
Volume of the periodical
139
Issue of the periodical within the volume
8
Country of publishing house
DE - GERMANY
Number of pages
14
Pages from-to
"Article Number: 759"
UT code for WoS article
001298032500001
EID of the result in the Scopus database
2-s2.0-85201936483