2004/06/30 by L. K. Chavda, Chavda, L. K., Abhijit L. Chavda +1
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #General Physics (physics.gen-ph) #General Relativity and Quantum Cosmology (gr-qc) #Relativity and Gravitational Theory #gr-qc #physics.gen-ph
paper · pdf · doi:10.48550/arxiv.physics/0406159
8 pages,1 Table,PDF.Completely revised.Inapplicability of Rabinowitz' objections demonstrated.Control of Hawking Radiation in an inertial confinement type set up suggested
openalex publication_date 2004/06/30 · arxiv created 2005/10/23 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We prove that the primordial black holes in the early universe did not decay until the gravity decoupled from the other interactions. Rabinowitz' two objections to the formation of Holeums are shown to be inapplicable. We show that primordial black holes having masses beween 8x1018 GeV and 1019 GeV formed gravitational bound states called Holeums when the temperature of the universe was between 1030 K and 1029 K. We prove that the black holes in a fire ball produced in an accelerator such as the LHC, modified into an inertial confinement type set up, will not emit Hawking radiation as long as the fire ball is maintained in thermal equilibrium or is allowed to expand adiabatically.