Applying Friedmann models to describe the evolution of the Universe based on data from the SAI Supernovae Catalog
- Authors: Gavrikov A.S.1, Saha B.1,2, Rikhvitsky V.S.2
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Affiliations:
- Peoples’ Friendship University of Russia (RUDN University)
- Joint Institute for Nuclear Research
- Issue: Vol 28, No 2 (2020)
- Pages: 120-130
- Section: Mathematical models in Physics
- URL: https://journals.rcsi.science/2658-4670/article/view/315317
- DOI: https://doi.org/10.22363/2658-4670-2020-28-2-120-130
- ID: 315317
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Abstract
In the recent years thanks to the modern and sophisticated technologies the astronomers and astrophysicists were able to look deep into the Universe. This vast data poses some new problem to the cosmologists. One of the problems is to develop an adequate theory. Another one is to fit the theoretical results with the observational one. In this report within the scope of the isotropic and homogeneous Friedman-Lemaitre-Robertson-Walker (FLRW) cosmological model we study the evolution of the Universe filled with dust or cosmological constant. The reason to consider this model is the present universe surprisingly homogeneous and isotropic in large scale. We also compare our results with the data from the SAI Supernovae Catalog. Since the observational data are given in terms of Hubble constant (????) and redshift (????) we rewrite the corresponding equations as a functions of ????. The task is to find the set of parameters for the mathematical model of an isotropic and homogeneous Universe that fits best with the astronomical data obtained from the study of supernovae: magnitude (????), redshift (????).
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About the authors
Arsenii S. Gavrikov
Peoples’ Friendship University of Russia (RUDN University)
Author for correspondence.
Email: gavrikov.997755@gmail.com
Student of the Institute of Physical Research and Technologies
6, Miklukho-Maklaya St., Moscow, 117198, Russian FederationBijan Saha
Peoples’ Friendship University of Russia (RUDN University); Joint Institute for Nuclear Research
Email: bijan64@mail.ru
Doctor of Physical and Mathematical Sciences, assistant professor of the Institute of Physical Research and Technologies of Peoples’ Friendship University of Russia (RUDN University), leading researcher at the Laboratory of Information Technologies of The Joint Institute for Nuclear Research
6, Miklukho-Maklaya St., Moscow, 117198, Russian Federation; 6, Joliot-Curie St., Dubna, Moscow region, 141980, Russian FederationVictor S. Rikhvitsky
Joint Institute for Nuclear Research
Email: rqvtsk@mail.ru
Master of physical and mathematical Sciences, Leading programmer of the Laboratory of Information Technologies
6, Joliot-Curie St., Dubna, Moscow region, 141980, Russian FederationReferences
- A. Riess, A. Filippenko, Challis, and et al., “Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant,” The Astronomical Journal, vol. 116, p. 1009, 1998. doi: 10.1086/300499.
- A. G. Riess, L.-G. Strolger, J. Tonry, S. Casertano, and et al., “Type Ia Supernova Discoveries at z > 1 from the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution,” The Astrophysical Journal, vol. 607, no. 2, pp. 665-687, Jun. 2004. doi: 10.1086/383612.
- S. Perlmutter, G. Aldering, G. Goldhaber, and et al., “Measurements of Ω and Λ from 42 High-Redshift Supernovae,” The Astrophysical Journal, vol. 517, no. 2, pp. 565-586, Jun. 1999. doi: 10.1086/307221.
- S. Perlmutter and et al., “Discovery of a supernova explosion at half the age of the Universe,” Nature, vol. 391, pp. 51-54, 1998. DOI: 10.1038/ 34124.
- C. L. Bennett et al., “First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results,” The Astrophysical Journal Supplement Series, vol. 148, no. 1, pp. 1-27, Sep. 2003. doi: 10.1086/377253.
- B. Saha, “Nonlinear spinor field in Bianchi type-I cosmology: Inflation, isotropization, and late time acceleration,” Phys. Rev. D, vol. 74, Dec. 2006. doi: 10.1103/PhysRevD.74.124030.
- A. Pradhan and B. Saha, “Accelerating dark energy models of the universe in anisotropic Bianchi type space-times and recent observations,” Physics of Particles and Nuclei, vol. 46, Mar. 2015. DOI: 10.1134/ S1063779615030028.
- B. Saha, “Spinor Field Nonlinearity and Space-Time Geometry,” Physics of Particles and Nuclei, vol. 49, pp. 146-212, Mar. 2018. DOI: 10.1134/ S1063779618020065.
- O. Bartunov, D. Tsvetkov, and N. Pavlyuk, “Sternberg Astronomical Institute Supernova Catalogue, and Radial Distribution of Supernovae in Host Galaxies,” in Proceedings of the International Astronomical Union, vol. 2, Aug. 2006, pp. 316-316. doi: 10.1017/S1743921307010812.
- O. Bartunov, D. Tsvetkov, and N. Pavlyuk, “SAI Supernova Catalog,” Accessed: 2020-03-01.
- A. Friedman, “Über die Krümmung des Raumes,” Z. Phys., vol. 10, pp. 377-386, Dec. 1922. doi: 10.1007/BF01332580.
- G. Lemaître, “L’Univers en expansion,” Annales de la Societe Scietifique de Bruxelles, vol. 53, p. 51, Jan. 1933.
- H. Robertson, “Kinematics and World-Structure,” The Astrophysical Journal, vol. 82, p. 284, Oct. 1935. doi: 10.1086/143681.
- H. Robertson, “Kinematics and World-Structure II.,” The Astrophysical Journal, vol. 83, p. 187, Apr. 1936. doi: 10.1086/143716.
- H. Robertson, “Kinematics and World-Structure III.,” The Astrophysical Journal, vol. 83, p. 257, May 1936. doi: 10.1086/143726.
- A. G. Walker, “On Milne’s Theory of World-Structure,” Proceedings of the London Mathematical Society, vol. 42, pp. 90-127, Jan. 1937.
- A. Liddle, An Introduction to Modern Cosmology (2nd ed.) Wiley, 2003, 189 pp.
- P. Ade, “Planck 2015 results. XIII. Cosmological parameters,” Astronomy & Astrophysics, vol. 594, Oct. 2016. doi: 10.1051/0004-6361/ 201525830.
- B. Saha and V. S. Rikhvitsky, “Nonlinear spinor fields in LRS Bianchi type-I space-time: Theory and observation,” Gravitation and Cosmology, vol. 23, no. 4, pp. 329-336, Oct. 2017. DOI: 10.1134/ s0202289317040193.
- M. O. Farooq, D. Mania, and B. Ratra, “Observational constraints on non-flat dynamical dark energy cosmological models,” Astrophysics and Space Science, vol. 357, Aug. 2013. doi: 10.1007/s10509-015-2319-2.
- M. O. Farooq, “Observational constraints on dark energy cosmological model parameters,” Sep. 2013. arXiv: 1309.3710.
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