Testing the evolution of the absolute magnitude of type Ia supernovae and cosmological parameters

Mahtessian, A. P.; Karapetian, G. S.; Hovhannisyan, M. A.; Movsisyan, V. H.; Mahtessian, L. A.

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Title: Testing the evolution of the absolute magnitude of type Ia supernovae and cosmological parameters

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2579-2276

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484-489

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Computer simulations show that, in estimating cosmological parameters, the best agreement between theory and observation is achieved by assuming the evolution of the absolute magnitude of type Ia supernovae. This requires only 0.3m of evolution for the time corresponding to z = 1. This leads to zero density of hidden energy in the Universe.

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oai:arar.sci.am:296456

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Communications of the Byurakan Astrophysical Observatory (ComBAO) is a peer-reviewed scientific journal, which publishes research in observational and theoretical astronomy/astrophysics and presents recent advances in these fields. It is being published by the NAS RA V. Ambartsumian Byurakan Astrophysical Observatory (BAO) in English in electronic form. The journal publishes original papers, review papers, brief reports, book reviews, special communications, observational and theoretical results in various fields of astronomy and related sciences, and some editorial notes, including anniversaries and obituaries. Under the heading “Legacy”, the renewed magazine will republish some old articles of high value in English. The heading “Guest articles” will bring to the attention of readers the articles of researchers who are not employees of BAO. ComBAO was founded in 1946 and regularly published in 1946-1990. However, the publication was interrupted because of the economic situation after the disintegration of the Soviet Union in 1991.

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Astronomy cosmological models supernovae dark energy dark matter general

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Aug 1, 2024

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Jan 10, 2022

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https://arar.sci.am/publication/323724

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Mahtessian, A. P., Testing the evolution of the absolute magnitude of type Ia supernovae and cosmological parameters	Aug 1, 2024

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Title: Testing the evolution of the absolute magnitude of type Ia supernovae and cosmological parameters

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