Generalized Komar charges and Smarr formulas for black holes and boson stars
Romina Ballesteros, Tomás Ortín
SciPost Phys. Core 8, 038 (2025) · published 24 April 2025
- doi: 10.21468/SciPostPhysCore.8.2.038
- Submissions/Reports
-
Abstract
The standard Komar charge is a (d−2)-form that can be defined in spacetimes admitting a Killing vector and which is closed when the vacuum Einstein equations are satisfied. Its integral at spatial infinity (the Komar integral) gives the conserved charge associated to the Killing vector, and, due to its on-shell closedness, the same value (expressed in terms of other physical variables) is obtained integrating over the event horizon (if any). This equality is the basis of the Smarr formula. This charge can be generalized so that it still is closed on-shell in presence of matter and its integrals give generalizations of the Smarr formula. We show how the Komar charge and other closed (d−2)-form charges can be used to prove non-existence theorems for gravitational solitons and boson stars. In particular, we show how one can deal with generalized symmetric fields (invariant under a combination of isometries and other global symmetries) and how the generalized symmetric Ansatz permits to evade the non-existence theorems.
Authors / Affiliations: mappings to Contributors and Organizations
See all Organizations.- 1 2 Romina Ballesteros,
- 2 Tomás Ortín
- 1 Instituto de Física Teórica / Institute for Theoretical Physics [IFT]
- 2 Pontificia Universidad Católica de Valparaíso / Pontificial Catholic University of Valparaiso [PUCV]
- Agencia Estatal de Investigación
- Agencia Nacional de Investigación y Desarrollo [ANID]
- Ministerio de Ciencia e Innovación (through Organization: Ministerio de Ciencia, Innovación y Universidades / Ministry of Science, Innovation and Universities)
- Pontificia Universidad Católica de Valparaíso / Pontificial Catholic University of Valparaiso [PUCV]