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PRIMORDIAL BLACK HOLE FORMATION IN INFLATIONARY PHASE
Author(s) -
Li-Zhi Liao
Publication year - 1986
Publication title -
wuli xuebao
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.199
H-Index - 47
ISSN - 1000-3290
DOI - 10.7498/aps.35.375
Subject(s) - physics , primordial black hole , homogeneous , black hole (networking) , phase (matter) , universe , astrophysics , theoretical physics , quantum mechanics , thermodynamics , binary black hole , gravitational wave , routing protocol , computer science , link state routing protocol , computer network , routing (electronic design automation)
In the inflationary phase of our universe, the true vacuum bubbles, appearing during the non-homogeneous phase transition, may collapse into primordial black holes. The lowest mass limit of them is 104g, and they may accompanied by t'Hooft-polyakov rno-nopoles. This result may have certain observational significance as compared with that of Carr, Hwaking and Wu.

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