A Secular Quark Gluon Plasma Phase Preceding Black HoleFormation
Conference
·
OSTI ID:891221
As spherical collapse of very massive stars would tend to the formation of Black Holes with an Event Horion having a gravitational red-shift of z = {infinity}, the pressure of gravitationally trapped radiation would increase as {approx} (1 + z){sup 2}. Consequently catastrophic collapse must change into a secular collapse as the radioactive luminosity would attain its Eddington value. Since the local temperature of the collapsing body is found to be {approx} 250 MeV, the stellar mass Black Hole Candidates could be in this intermediate state of a hot Quark Gluon Plasma.
- Research Organization:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Organization:
- USDOE Director. Office of Science. Office of AdvancedScientific Computing Research. Office of Nuclear Physics
- DOE Contract Number:
- DE-AC02-05CH11231
- OSTI ID:
- 891221
- Report Number(s):
- LBNL-59320; R&D Project: NTCOST; BnR: KB0301020; TRN: US0605323
- Resource Relation:
- Conference: Marcel Grossman Meeting on General Relativity,Berlin, Germany, July 23 - 29, 2006
- Country of Publication:
- United States
- Language:
- English
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