From inflation to acceleration, with phantom and canonical scalar fields in non-flat universe

Details From inflation to acceleration, with phantom and canonical scalar fields in non-flat universe From inflation to acceleration, with phantom and canonical scalar fields in non-flat universe

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phlb..666..288s&link_type=abstract

Physics Letters B, Volume 666, Issue 4, p. 288-298.

Physics

12

Scientific paper

Motivated by the recent work of Elizalde et al. [E. Elizalde, S. Nojiri, S.D. Odintsov, D. Saez Gomez, V. Faraoni, Phys. Rev. D 77 (2008) 106005], we generalize their work to the non-flat case. We consider a universe filled with matter and show that it is possible to obtain both inflation and accelerated expansion at late times by using a single scalar field. Realistic examples are worked out in order to illustrate this fact. Then we extend the problem to the interacting case.

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