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Thermodynamics of Schwarzschild black hole surrounded by quintessence in gravity's rainbow

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dc.rights.license CC BY eng
dc.contributor.author Hamil, B. cze
dc.contributor.author Lütfüoglu, Bekir Can cze
dc.date.accessioned 2025-12-05T12:54:40Z
dc.date.available 2025-12-05T12:54:40Z
dc.date.issued 2023 eng
dc.identifier.issn 0550-3213 eng
dc.identifier.uri http://hdl.handle.net/20.500.12603/1850
dc.description.abstract According to some quantum gravity models, Lorentz invariance can be violated in the Planck energy scale. With this motivation, we analyze the thermal quantities and the stability of Schwarzschild black hole surrounded by quintessence in gravity's rainbow formalism. To do that, we consider the rainbow functions which are motivated by loop quantum gravity and gamma-ray bursts, and we derive Hawking temperature, specific heat, entropy and the equation of state function. We observe that the presence the quintessence matter field and rainbow gravity affect the stability of the black hole. & COPY; 2023 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons .org /licenses /by /4 .0/). Funded by SCOAP3. eng
dc.format p. "Article Number: 116191" eng
dc.language.iso eng eng
dc.publisher Elsevier eng
dc.relation.ispartof Nuclear Physics B, volume 990, issue: MAY eng
dc.subject cosmological constant eng
dc.subject accretion eng
dc.subject dispersion eng
dc.subject universe eng
dc.subject energy eng
dc.title Thermodynamics of Schwarzschild black hole surrounded by quintessence in gravity's rainbow eng
dc.type article eng
dc.identifier.obd 43880198 eng
dc.identifier.wos 001040490900001 eng
dc.identifier.doi 10.1016/j.nuclphysb.2023.116191 eng
dc.publicationstatus postprint eng
dc.peerreviewed yes eng
dc.source.url https://doi.org/10.1016/j.nuclphysb.2023.116191 cze
dc.relation.publisherversion https://doi.org/10.1016/j.nuclphysb.2023.116191 eng
dc.rights.access Open Access eng


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