Gravity and On-Shell Probe Actions
arXiv:1602.07177 · doi:10.1007/JHEP08(2016)047
Abstract
In any gravitational theory and in a wide class of background space-times, we argue that there exists a simple, yet profound, relation between the on-shell Euclidean gravitational action and the on-shell Euclidean action of probes. The probes can be, for instance, charged particles or branes. The relation is tightly related to the thermodynamic nature of gravity. We provide precise checks of the relation in several examples, which include both asymptotically flat and asymptotically AdS space-times, with particle, D-brane and M-brane probes. Perfect consistency is found in all cases, including in a highly non-trivial example including α'-corrections.
45 pages, 1 figure; v2: list of references updated; v3: typos corrected, a few explanations and a remark on bubbling geometries added, published version
References in corpus (11)
- Exact half-BPS Type IIB interface solutions I: Local solution and supersymmetric Janus
- Holographic Wilson Loops
- Quantum corrections to eta/s
- On gravitational description of Wilson lines
- Universality of Gravity from Entanglement
- Holographic Black Hole Chemistry
- Cold Black Holes in the Harlow-Hayden Approach to Firewalls
- A Holographic Bound on Cosmic Magnetic Fields
- Phase with no mass gap in non-perturbatively gauge-fixed Yang--Mills theory
- Localised anti-branes in non-compact throats at zero and finite T
- From black holes to flux throats: polarization can resolve the singularity
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