Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....5.3033t&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
Scientific paper
Quintessential inflation explains both inflation and present accelerated expansion. In this model these two accelerated expansion is driven by a single scalar field. We construct a model based on an exponential potential. We consider two kinds of reheating process. One is the ordinary reheating in quintessential inflation, using gravitational particle creation. The other is the instant preheating which is much more effective. We calculate the relic gravitational waves produced during inflation in our model. We find that the spectrum of the gravitational waves is quite sensitive to the reheating process. Conversely, the detection or non-detection of primordial gravitational waves at ˜100MHz would have profound implications for the inflationary cosmology.
Chiba Takeshi
Sasaki Makoto
Tashiro Hiroyuki
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