Abstract
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.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
