This paper shows how entropy generation from numerical density calculations of relic gravitons can be measured via the Li‐Baker high‐frequency gravity wave (HFGW) detector, and suggests the implications this has for the physics of early‐universe phase transitions. This paper indicates the role of Ng’s revised statistics in gravitational wave physics detection and the application of Baumann et al. (2007) formalism of reduction of rank‐two tensorial contributions to density wave physics, using the HFGW approximation directly at the beginning as well as Li’s treatment of energy density explicitly. This formalism is a way to refine and add more capacity to the Li‐Baker HFGW detector in reconstructing early‐universe conditions at the onset of the big bang.
Relic High Frequency Gravitational waves from the Big Bang and How to Detect Them
SPACE, PROPULSION & ENERGY SCIENCES INTERNATIONAL FORUM: SPESIF‐2009 ; 2009 ; Huntsville (Alabama)
AIP Conference Proceedings ; 1103 , 1 ; 571-581
2009-03-16
11 pages
Conference paper
Electronic Resource
English
Relic High Frequency Gravitational Waves from the Big Bang and How to Detect Them
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