Positivity of Energy in Einstein-Maxwell Axion-dilaton gravity

Abstract

Avoiding the problem of the existence of asymptotically constant spinors satysfying certain differential equations on a non-compact hypersrface we presented the proof of positivity of the ADM and Bondi energy in Einstein-Maxwell axion-dilaton gravity. In our attitude spinor fields defining the enwergy need only be defined near infinity and there satysfying propagation equations.

11 pages, Latex, to be published in Classical Quantum Gravity

References in corpus (1)

• Positivity of the Bondi Energy in Einstein-Maxwell Axion- Dilaton Gravity

Cited by in corpus (11)

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• Signatures of Einstein-Maxwell dilaton-axion gravity from the observed jet power and the radiative efficiency
• Thin accretion disk and shadow of Kerr-Sen black hole in Einstein-Maxwell-dilaton-axion gravity
• Positive mass theorem in extended supergravities
• Choked accretion onto Kerr-Sen black holes in Einstein-Maxwell-dilaton-axion gravity
• Signatures of Einstein-Maxwell dilaton-axion gravity from the observed quasi-periodic oscillations in black holes
• Observational constraints on the Kerr and its several single-parameter modified spacetimes using quasi-periodic oscillation data
• Static configurations and evolution of higher dimensional brane-dilaton black hole system
• Deciphering signatures of Kerr-Sen black holes in presence of plasma from the Event Horizon Telescope data