Testing AN Inflation Model with a Massive Nonminimal Scalar Field

Details Testing AN Inflation Model with a Massive Nonminimal Scalar Field Testing AN Inflation Model with a Massive Nonminimal Scalar Field

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cosm.conf..307n&link_type=abstract

COSMO-2000 . Proceedings of the Fourth International Workshop on Particle Physics and the Early Universe . Held 4-8 September 20

Physics

Scientific paper

The power spectra of the scalar- and tensor-type structures generated in an inflation model based on a massive nonminimally coupled scalar field are derived. The contributions of these structures to the anisotropy of the cosmic microwave background radiation are compared with the four-year COBE DMR data. The constraints on the expansion rate during the inflation period, and the relative amount of the tensor-type contribution to the quadrupole of the CMBR temperature anisotropy are provided.

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