On the oscillation-driven cosmological expansion at the post-inflationary stage


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The dynamics of the inflaton scalar field oscillating around a minimum of singular potentials in the expanding Universe is studied. Asymptotic formulas are obtained, describing the cosmological expansion at late times. The problem of stability of the considered oscillanions as well as a related phenomenon of field fragmentation are briefly discussed.

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V. Koutvitsky

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation (IZMIRAN) of the Russian Academy of Sciences

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Email: vak@izmiran.ru
俄罗斯联邦, Troitsk, Moscow oblast, 108840

E. Maslov

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation (IZMIRAN) of the Russian Academy of Sciences

Email: vak@izmiran.ru
俄罗斯联邦, Troitsk, Moscow oblast, 108840

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