Investigation of the chiral cosmological model of f(R, oR) gravity
ΠΠ²ΡΠΎΡ: Chervon S.V., Fomin I.V., Chaadaeva T.I.
ΠΡΡΠ½Π°Π»: ΠΡΠΎΡΡΡΠ°Π½ΡΡΠ²ΠΎ, Π²ΡΠ΅ΠΌΡ ΠΈ ΡΡΠ½Π΄Π°ΠΌΠ΅Π½ΡΠ°Π»ΡΠ½ΡΠ΅ Π²Π·Π°ΠΈΠΌΠΎΠ΄Π΅ΠΉΡΡΠ²ΠΈΡ @stfi
Π ΡΠ±ΡΠΈΠΊΠ°: ΠΡΠ°Π²ΠΈΡΠ°ΡΠΈΡ, ΠΊΠΎΡΠΌΠΎΠ»ΠΎΠ³ΠΈΡ ΠΈ ΡΡΠ½Π΄Π°ΠΌΠ΅Π½ΡΠ°Π»ΡΠ½ΡΠ΅ ΠΏΠΎΠ»Ρ
Π‘ΡΠ°ΡΡΡ Π² Π²ΡΠΏΡΡΠΊΠ΅: 2 (43), 2023 Π³ΠΎΠ΄Π°.
ΠΠ΅ΡΠΏΠ»Π°ΡΠ½ΡΠΉ Π΄ΠΎΡΡΡΠΏ
We study modified f (R, OR) gravity which can be reduced to the chiral cosmological model of the special type. Various types of cosmological solutions are considered based on exact analytical solutions, the slow-roll approximation, the superpotential method, the inclusion of additional material fields and reduction multi-field model to single-field one as well. Thus, this paper presents topical methods for analyzing cosmological models based on an effective multi-field interpretation of the proposed modified gravity.
Chiral cosmological model, π(π , β‘π ) modified gravity, friedman universe
ΠΠΎΡΠΎΡΠΊΠΈΠΉ Π°Π΄ΡΠ΅Ρ: https://sciup.org/142239966
IDR: 142239966 | Π£ΠΠ: 53.1 | DOI: 10.17238/issn2226-8812.2023.2.54-67
ΠΡΡΠ»Π΅Π΄ΠΎΠ²Π°Π½ΠΈΠ΅ ΠΊΠΈΡΠ°Π»ΡΠ½ΠΎΠΉ ΠΊΠΎΡΠΌΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΎΠΉ ΠΌΠΎΠ΄Π΅Π»ΠΈ f(R, oR) Π³ΡΠ°Π²ΠΈΡΠ°ΡΠΈΠΈ
ΠΠ·ΡΡΠ°Π΅ΠΌ ΠΌΠΎΠ΄ΠΈΡΠΈΡΠΈΡΠΎΠ²Π°Π½Π½ΡΡ Π³ΡΠ°Π²ΠΈΡΠ°ΡΠΈΡ f (R, OR), ΠΊΠΎΡΠΎΡΠ°Ρ ΠΌΠΎΠΆΠ΅Ρ Π±ΡΡΡ ΡΠ²Π΅Π΄Π΅Π½Π° ΠΊ ΠΊΠΈΡΠ°Π»ΡΠ½ΠΎΠΉ ΠΊΠΎΡΠΌΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΎΠΉ ΠΌΠΎΠ΄Π΅Π»ΠΈ ΡΠΏΠ΅ΡΠΈΠ°Π»ΡΠ½ΠΎΠ³ΠΎ ΡΠΈΠΏΠ°. Π Π°ΡΡΠΌΠΎΡΡΠ΅Π½Ρ ΡΠ°Π·Π»ΠΈΡΠ½ΡΠ΅ ΡΠΈΠΏΡ ΠΊΠΎΡΠΌΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΈΡ ΡΠ΅ΡΠ΅Π½ΠΈΠΉ, ΠΎΡΠ½ΠΎΠ²Π°Π½Π½ΡΠ΅ Π½Π° ΡΠΎΡΠ½ΡΡ Π°Π½Π°Π»ΠΈΡΠΈΡΠ΅ΡΠΊΠΈΡ ΡΠ΅ΡΠ΅Π½ΠΈΡΡ , ΠΏΡΠΈΠ±Π»ΠΈΠΆΠ΅Π½ΠΈΠΈ ΠΌΠ΅Π΄Π»Π΅Π½Π½ΠΎΠ³ΠΎ ΡΠΊΠ°ΡΡΠ²Π°Π½ΠΈΡ, ΠΌΠ΅ΡΠΎΠ΄Π΅ ΡΡΠΏΠ΅ΡΠΏΠΎΡΠ΅Π½ΡΠΈΠ°Π»Π°, Π²ΠΊΠ»ΡΡΠ΅Π½ΠΈΠΈ Π΄ΠΎΠΏΠΎΠ»Π½ΠΈΡΠ΅Π»ΡΠ½ΡΡ ΠΌΠ°ΡΠ΅ΡΠΈΠ°Π»ΡΠ½ΡΡ ΠΏΠΎΠ»Π΅ΠΉ, Π° ΡΠ°ΠΊΠΆΠ΅ ΡΠ΅Π΄ΡΠΊΡΠΈΠΈ ΠΌΠ½ΠΎΠ³ΠΎΠΏΠΎΠ»Π΅Π²ΠΎΠΉ ΠΌΠΎΠ΄Π΅Π»ΠΈ ΠΊ ΠΎΠ΄Π½ΠΎΠΏΠΎΠ»Π΅Π²ΠΎΠΉ. Π’Π°ΠΊΠΈΠΌ ΠΎΠ±ΡΠ°Π·ΠΎΠΌ, Π² Π΄Π°Π½Π½ΠΎΠΉ ΡΡΠ°ΡΡΠ΅ ΠΏΡΠ΅Π΄ΡΡΠ°Π²Π»Π΅Π½Ρ Π°ΠΊΡΡΠ°Π»ΡΠ½ΡΠ΅ ΠΌΠ΅ΡΠΎΠ΄Ρ Π°Π½Π°Π»ΠΈΠ·Π° ΠΊΠΎΡΠΌΠΎΠ»ΠΎΠ³ΠΈΡΠ΅ΡΠΊΠΈΡ ΠΌΠΎΠ΄Π΅Π»Π΅ΠΉ, ΠΎΡΠ½ΠΎΠ²Π°Π½Π½ΡΠ΅ Π½Π° ΡΡΡΠ΅ΠΊΡΠΈΠ²Π½ΠΎΠΉ ΠΌΠ½ΠΎΠ³ΠΎΠΏΠΎΠ»Π΅Π²ΠΎΠΉ ΠΈΠ½ΡΠ΅ΡΠΏΡΠ΅ΡΠ°ΡΠΈΠΈ ΠΏΡΠ΅Π΄Π»ΠΎΠΆΠ΅Π½Π½ΠΎΠΉ ΠΌΠΎΠ΄ΠΈΡΠΈΡΠΈΡΠΎΠ²Π°Π½Π½ΠΎΠΉ Π³ΡΠ°Π²ΠΈΡΠ°ΡΠΈΠΈ.
Π‘ΠΏΠΈΡΠΎΠΊ Π»ΠΈΡΠ΅ΡΠ°ΡΡΡΡ Investigation of the chiral cosmological model of f(R, oR) gravity
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