Data analysis of three parameter models of deceleration parameter in FLRW universe
Author:
Publisher
Springer Science and Business Media LLC
Subject
General Physics and Astronomy,Fluid Flow and Transfer Processes
Link
https://link.springer.com/content/pdf/10.1140/epjp/s13360-023-04442-y.pdf
Reference102 articles.
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2. S. Perlmutter, et al., Measurements of the cosmological parameters Omega and Lambda from the first 7 supernovae at z$$>$$=0.35. Astrophys. J. 483, 565 (1997). https://doi.org/10.1086/304265, arXiv:astro-ph/9608192
3. S. Perlmutter, et al., Measurements of $$\Omega$$ and $$\Lambda$$ from 42 high redshift supernovae. Astrophys. J. 517, 565–586 (1999). https://doi.org/10.1086/307221, arXiv:astro-ph/9812133
4. D.N. Vollick, 1/R Curvature corrections as the source of the cosmological acceleration. Phys. Rev. D 68, 063510 (2003). https://doi.org/10.1103/PhysRevD.68.063510. arXiv:astro-ph/0306630,
5. S. Nojiri, S.D. Odintsov, Modified gravity with negative and positive powers of the curvature: Unification of the inflation and of the cosmic acceleration. Phys. Rev. D 68, 123512 (2003). https://doi.org/10.1103/PhysRevD.68.123512. arXiv:hep-th/0307288,
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