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The phase space for the Einstein-Yang-Mills equations and the first law of black hole thermodynamics
School of Science and Technology, University of New England, Armidale, Australia.ORCID-id: 0000-0001-9536-9908
2014 (engelsk)Inngår i: Advances in Theoretical and Mathematical Physics, ISSN 1095-0761, E-ISSN 1095-0753, Vol. 18, nr 4, s. 799-825Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We use the techniques of Bartnik [5] to show that the space of solutions to the Einstein-Yang-Mills constraint equations on an asymptotically flat manifold with one end and zero boundary components, has a Hilbert manifold structure; the Einstein-Maxwell system can be considered as a special case. This is equivalent to the property of linearisation stability, which was studied in depth throughout the 70s [1, 2, 9, 11, 13, 18, 19].

This framework allows us to prove a conjecture of Sudarsky and Wald [22], namely that the validity of the first law of black hole thermodynamics is a suitable condition for stationarity. Since we work with a single end and no boundary conditions, this is equivalent to critical points of the ADM mass subject to variations fixing the Yang-Mills charge corresponding exactly to stationary solutions. The natural extension to this work is to prove the second conjecture from [22], which is the case where an interior boundary is present; this will be addressed in future work.

sted, utgiver, år, opplag, sider
International Press of Boston, Inc. , 2014. Vol. 18, nr 4, s. 799-825
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URN: urn:nbn:se:ltu:diva-95203DOI: 10.4310/atmp.2014.v18.n4.a2ISI: 000346039600002Scopus ID: 2-s2.0-84915813325OAI: oai:DiVA.org:ltu-95203DiVA, id: diva2:1725067
Tilgjengelig fra: 2023-01-10 Laget: 2023-01-10 Sist oppdatert: 2025-10-21bibliografisk kontrollert

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