Authors: A. Beckwith
We introduce a criterion as to the range of HFGW generated by early universe conditions. The 1 to 10 Giga Hertz range is constructed initially starting with what Grupen writes as far as what to expect of GW frequencies which can be detected assuming a sensitivity of h ~ 10-27 . From there we examine the implications of an earlier Hubble parameter at the start of inflation , and a phase transition treatment of pre to post Planckian inflaton physics. We close with an analysis of how gravitational constant G may vary with time , the tie in with the NEC condition and how to select a range of relic GW frequencies.
Comments: 17 pages, one table. Attempt to start preparing for bridge to actual experimental measurements. Based upon some structural considerations as far as space time geometry.
[v1] 22 Feb 2011
Unique-IP document downloads: 65 times
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.