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Black hole chemistry, the cosmological constant and the embedding tensor

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arxiv 2203.13588 v2 pith:JDNS3IJN submitted 2022-03-25 hep-th gr-qc

classification hep-thgr-qc
keywords constantstheoriesconstantcontextembeddingsupergravitytensorthem
verification ladder T0 review T1 audit T2 compute T3 formal
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We study black-hole thermodynamics in theories that contain dimensionful constants such as the cosmological constant or coupling constants in Wald's formalism. The most natural way to deal with these constants is to promote them to scalar fields introducing a (d-1)-form Lagrange multiplier that forces them to be constant on-shell. These (d-1)-form potentials provide a dual description of them and, in the context of superstring/supergravity theories, a higher-dimensional origin/explanation. In the context of gauged supergravity theories, all these constants can be collected in the embedding tensor. We show in an explicit 4-dimensional example that the embedding tensor can also be understood as a thermodynamical variable that occurs in the Smarr formula in a duality-invariant fashion. This establishes an interesting link between black-hole thermodynamics, gaugings and compactifications in the context of superstring/supergravity theories.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Thermodynamics of charged rotating black strings in extended phase space

    gr-qc 2025-01 conditional novelty 6.0 of 10

    Charged rotating AdS black strings show a specific-heat divergence that is interpreted as a second-order, Van der Waals-like critical point, while uncharged strings show no such criticality.

  2. Komar charge of N = 2 supergravity and its superspace generalization

    hep-th 2024-12 conditional novelty 6.0 of 10

    The authors derive an on-shell closed, supersymmetric and duality-invariant generalized Komar 2-form for minimal N=2, d=4 supergravity in superspace, with a component-formalism confirmation.

  3. On the thermodynamics of the black holes of the Cano-Ruip\'erez 4-dimensional string effective action

    hep-th 2024-11 conditional novelty 6.0 of 10

    The paper derives a Smarr formula and no-hair theorems for string-corrected black holes, with the string length acting as a thermodynamic variable.

  4. Black hole solutions in theories of supergravity

    hep-th 2024-12 unverdicted

    A review of the history of black hole solutions in supergravity, from early no-superhair theorems to attractor mechanics and alpha-prime corrections.

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