Ghost Stars in General Relativity

[EN]We explore an idea put forward many years ago by Zeldovich and Novikov concerning the existence of compact objects endowed with arbitrarily small mass. The energy density of such objects, which we call “ghost stars”, is negative in some regions of the fluid distribution, producing a vanishing to...

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Detalhes bibliográficos
Autores: Herrera, Luis, Di Prisco, Alicia, Ospino Zúñiga, Justo Hernán
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Recursos:Universidad de Salamanca (USAL)
Repositorio:GREDOS. Repositorio Institucional de la Universidad de Salamanca
OAI Identifier:oai:gredos.usal.es:10366/162344
Acesso em linha:http://hdl.handle.net/10366/162344
Access Level:acceso abierto
Palavra-chave:Relativistic fluids
Interior solutions
Spherically symmetric sources
Descrição
Resumo:[EN]We explore an idea put forward many years ago by Zeldovich and Novikov concerning the existence of compact objects endowed with arbitrarily small mass. The energy density of such objects, which we call “ghost stars”, is negative in some regions of the fluid distribution, producing a vanishing total mass. Thus, the interior is matched on the boundary surface to Minkowski space–time. Some exact analytical solutions are exhibited and their properties are analyzed. Observational data that could confirm or dismiss the existence of this kind of stellar object are discussed