Interpretation of the Observed Magnitude—Redshift Relation for Type la Supernovae

Details Interpretation of the Observed Magnitude—Redshift Relation for Type la Supernovae Interpretation of the Observed Magnitude—Redshift Relation for Type la Supernovae

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010arep...54..537k&link_type=abstract

Astronomy Reports, Volume 54, Issue 6, pp.537-549

Astronomy and Astrophysics

Astronomy

Scientific paper

Theoretical magnitude—redshift relations calculated for the well known ΛCDM model and the C model, which differs in its description of the repulsive force, are compared with the observed ( m - M) ( z) relation for Type Ia supernovae. The predictions of the ΛCDM and C models for the ( m - M)( z) relation differ little at redshifts z ≤ 2, and both qualitatively correctly describe the observed dependence. However, the two models differ appreciably at redshifts z ≥ 3. Studies of the ( m - M)( z) relation at redshifts z ≥ 3 may make it possible to approach a better understanding of the nature of the cosmological repulsive forces.

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