Higher derivative contributions to black hole thermodynamics at NNLO

Abstract In an effective theory of gravity, thermodynamic quantities of black holes receive corrections from the infinite series of higher derivative terms. At the next to leading order, these can be obtained by using only the leading order solution. In this paper, we push forward this property to t...

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Main Authors: Liang Ma, Yi Pang, H. Lü
Format: Article
Language:English
Published: SpringerOpen 2023-06-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP06(2023)087
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author Liang Ma
Yi Pang
H. Lü
author_facet Liang Ma
Yi Pang
H. Lü
author_sort Liang Ma
collection DOAJ
description Abstract In an effective theory of gravity, thermodynamic quantities of black holes receive corrections from the infinite series of higher derivative terms. At the next to leading order, these can be obtained by using only the leading order solution. In this paper, we push forward this property to the next to next to leading order. We propose a formula which yields the Euclidean action of asymptotically flat black holes at the next to next to leading order using only the solution up to and including the next to leading order. Other conserved quantities are derived from the Euclidean action via standard thermodynamic relation. We verify our formula in examples of D-dimensional pure gravity and Einstein-Maxwell theory extended by 4- and 6-derivative terms. Based on our formula, we also prove that for asymptotically flat black holes, the physical quantities are invariant under field redefinitions.
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spelling doaj.art-276ae382d15c448f88574974db481a6f2023-09-24T11:06:22ZengSpringerOpenJournal of High Energy Physics1029-84792023-06-012023613910.1007/JHEP06(2023)087Higher derivative contributions to black hole thermodynamics at NNLOLiang Ma0Yi Pang1H. Lü2Center for Joint Quantum Studies and Department of Physics, School of Science, Tianjin UniversityCenter for Joint Quantum Studies and Department of Physics, School of Science, Tianjin UniversityCenter for Joint Quantum Studies and Department of Physics, School of Science, Tianjin UniversityAbstract In an effective theory of gravity, thermodynamic quantities of black holes receive corrections from the infinite series of higher derivative terms. At the next to leading order, these can be obtained by using only the leading order solution. In this paper, we push forward this property to the next to next to leading order. We propose a formula which yields the Euclidean action of asymptotically flat black holes at the next to next to leading order using only the solution up to and including the next to leading order. Other conserved quantities are derived from the Euclidean action via standard thermodynamic relation. We verify our formula in examples of D-dimensional pure gravity and Einstein-Maxwell theory extended by 4- and 6-derivative terms. Based on our formula, we also prove that for asymptotically flat black holes, the physical quantities are invariant under field redefinitions.https://doi.org/10.1007/JHEP06(2023)087Black HolesClassical Theories of Gravity
spellingShingle Liang Ma
Yi Pang
H. Lü
Higher derivative contributions to black hole thermodynamics at NNLO
Journal of High Energy Physics
Black Holes
Classical Theories of Gravity
title Higher derivative contributions to black hole thermodynamics at NNLO
title_full Higher derivative contributions to black hole thermodynamics at NNLO
title_fullStr Higher derivative contributions to black hole thermodynamics at NNLO
title_full_unstemmed Higher derivative contributions to black hole thermodynamics at NNLO
title_short Higher derivative contributions to black hole thermodynamics at NNLO
title_sort higher derivative contributions to black hole thermodynamics at nnlo
topic Black Holes
Classical Theories of Gravity
url https://doi.org/10.1007/JHEP06(2023)087
work_keys_str_mv AT liangma higherderivativecontributionstoblackholethermodynamicsatnnlo
AT yipang higherderivativecontributionstoblackholethermodynamicsatnnlo
AT hlu higherderivativecontributionstoblackholethermodynamicsatnnlo