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

dc.contributor.authorHamil, B.
dc.contributor.authorLütfüoglu, Bekir Can
dc.date.accessioned2025-12-05T12:54:40Z
dc.date.available2025-12-05T12:54:40Z
dc.date.issued2023
dc.description.abstractAccording 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.formatp. &quot;Article Number: 116191&quot;
dc.identifier.doi10.1016/j.nuclphysb.2023.116191
dc.identifier.issn0550-3213
dc.identifier.obd43880198
dc.identifier.urihttp://hdl.handle.net/20.500.12603/1850
dc.identifier.wos001040490900001
dc.language.isoeng
dc.peerreviewedyes
dc.publicationstatuspostprint
dc.publisherElsevier
dc.relation.ispartofNuclear Physics B, volume 990, issue: MAYeng
dc.relation.publisherversionhttps://doi.org/10.1016/j.nuclphysb.2023.116191
dc.rights.accessOpen Access
dc.rights.licenseCC BY
dc.source.urlhttps://doi.org/10.1016/j.nuclphysb.2023.116191
dc.subjectcosmological constanteng
dc.subjectaccretioneng
dc.subjectdispersioneng
dc.subjectuniverseeng
dc.subjectenergyeng
dc.titleThermodynamics of Schwarzschild black hole surrounded by quintessence in gravity's rainboweng
dc.typearticle

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