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Black Holes and Inflation
Author(s) -
GonzálezDíaz P. F.
Publication year - 1988
Publication title -
annalen der physik
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.009
H-Index - 68
eISSN - 1521-3889
pISSN - 0003-3804
DOI - 10.1002/andp.19885000404
Subject(s) - physics , black hole (networking) , white hole , primordial black hole , gravitational collapse , charged black hole , scalar field , planck , extremal black hole , rotating black hole , inflation (cosmology) , virtual black hole , classical mechanics , gravitation , theoretical physics , astrophysics , quantum mechanics , binary black hole , schwarzschild radius , gravitational wave , entropy (arrow of time) , routing protocol , routing (electronic design automation) , computer science , link state routing protocol , computer network , angular momentum
A model for black hole collapse and evaporation in which the black hole is supposed to be an excited state of one of the Planck black holes pervading the structure of spacetime is discussed. By assuming a Coleman‐Weinberg gravitational effective potential for a scalar field inside the collapse matter, it is shown that the black hole state cannot be attained neither through bubble tunneling nor by the rolling down of the field.