Characterisation of dark energy in General Relativity using supernovae data

Details Characterisation of dark energy in General Relativity using supernovae data Characterisation of dark energy in General Relativity using supernovae data

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf..673f&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

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Scientific paper

Using the supernovae data, one will show how to characterize the dark energy properties within the framework of the General Relativity with massive scalar field. To proceed, one will consider various forms of its state equation according to the redshift. One will see that it is degenerated on the contrary to other observational (redshifts of the dark energy domination and expansion acceleration) and theoretical (scalar field potential) data.

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