Heating after higher dimensional inflation

Details Heating after higher dimensional inflation Heating after higher dimensional inflation

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988nuphb.297..697s&link_type=abstract

Nuclear Physics B, Volume 297, Issue 4, p. 697-720.

Physics

Nuclear Physics

17

Scientific paper

Within the context of a class of higher dimensional models of gravity,
we investigate the heating of the universe following an inflationary
phase. High temperatures, typically on the order of 1017 GeV
can be achieved. This allows for a subsequent production of baryon
asymmetry and, if existing, superheavy cosmic strings.

Affiliated with

Also associated with

No associations

Rating

Heating after higher dimensional inflation 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 Heating after higher dimensional inflation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Heating after higher dimensional inflation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1227536