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Автор Michał Artymowski
Автор Zygmunt Lalak
Дата выпуска 2011-09-01
dc.description In the context of the Loop Quantum Cosmology we have analysed the holonomy correction to the classical evolution of the simplified Bianchi I model in the presence of vector fields. For the Universe dominated by a massive vector field or by a combination of a scalar field and a vector field a smooth transition between Kasner-like and Kasner-unlike solutions for a Bianchi I model has been demonstrated. In this case a lack of initial curvature singularity and a finite maximal energy density appear already at the level of General Relativity, which simulates a classical Big Bounce.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Vector fields and Loop Quantum Cosmology
Тип paper
DOI 10.1088/1475-7516/2011/09/017
Electronic ISSN 1475-7516
Журнал Journal of Cosmology and Astroparticle Physics
Том 2011
Первая страница 17
Последняя страница 017
Аффилиация Michał Artymowski; Institute of Theoretical Physics, Faculty of Physics, University of Warsaw, ul. Hoża 69, 00-681 Warszawa, Poland
Аффилиация Zygmunt Lalak; Institute of Theoretical Physics, Faculty of Physics, University of Warsaw, ul. Hoża 69, 00-681 Warszawa, Poland
Выпуск 09

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