PRIMORDIAL BLACK HOLE FORMATION IN INFLATIONARY PHASE | Zendy

Liao Liu | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

PRIMORDIAL BLACK HOLE FORMATION IN INFLATIONARY PHASE

Author(s) -

Liao Liu

Publication year - 1986

Publication title -

acta physica sinica

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.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research