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Charged cosmological dust solutions of the coupled Einstein and Maxwell equations
Author(s) -
Joel Spruck,
Yisong Yang
Publication year - 2010
Publication title -
discrete and continuous dynamical systems
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.289
H-Index - 70
eISSN - 1553-5231
pISSN - 1078-0947
DOI - 10.3934/dcds.2010.28.567
Subject(s) - physics , naked singularity , gravitation , point particle , schwarzschild radius , limit (mathematics) , black hole (networking) , space (punctuation) , general relativity , gravitational singularity , classical mechanics , charge (physics) , einstein , maxwell's equations , distribution (mathematics) , mathematical physics , mathematical analysis , quantum mechanics , mathematics , computer network , routing protocol , routing (electronic design automation) , computer science , link state routing protocol , linguistics , philosophy
It is well known through the work of Majumdar, Papapetrou, Hartle, andHawking that the coupled Einstein and Maxwell equations admit a static multipleblackhole solution representing a balanced equilibrium state of finitely manypoint charges. This is a result of the exact cancellation of gravitationalattraction and electric repulsion under an explicit condition on the mass andcharge ratio. The resulting system of particles, known as an extremely chargeddust, gives rise to examples of spacetimes with naked singularities. In thispaper, we consider the continuous limit of theMajumdar--Papapetrou--Hartle--Hawking solution modeling a space occupied by anextended distribution of extremely charged dust. We show that for a givensmooth distribution of matter of finite ADM mass there is a continuous familyof smooth solutions realizing asymptotically flat space metrics.

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