Holographic Principle bounds on Primordial Black Hole abundances

Details Holographic Principle bounds on Primordial Black Hole abundances Holographic Principle bounds on Primordial Black Hole abundances

2003-01-17

arxiv.org/abs/gr-qc/0301064v1

Class.Quant.Grav. 20 (2003) 813-826

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Latex file, 2 .ps figures. To appear in Classical and Quantum Gravity

Scientific paper

The generalized Second Law of thermodynamics and the Holographic Principle are combined to obtain the maximum mass of black holes formed inside a static spherical box of size $R$ filled with radiation at initial temperature $T_{i}$. The final temperature after the formation of black holes is evaluated, and we show that a critical threshold exists for the radiation to be fully consumed by the process. We next argue that if some form of Holographic Principle holds, upper bounds to the mass density of PBHs formed in the early universe may be obtained. The limits are worked out for inflationary and non-inflationary cosmological models. This method is independent of the known limits based on the background fluxes (from cosmic rays, radiation and other forms of energy) and applies to potentially important epochs of PBH formation, resulting in quite strong constraints to $\Omega_{pbh}$.

Affiliated with

Also associated with

No associations

Rating

Holographic Principle bounds on Primordial Black Hole abundances does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Holographic Principle bounds on Primordial Black Hole abundances, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Holographic Principle bounds on Primordial Black Hole abundances will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-646518