Мақаланы E-mail арқылы жіберу Loop Quantum Cosmology and Probability of Inflation
- Авторлар: Vereshchagin G.1,2,3, Bedić S.1
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Мекемелер:
- ICRANet
- ICRA and University of Rome “Sapienza”
- ICRANet-Minsk, Institute of Physics
- Шығарылым: Том 62, № 12 (2018)
- Беттер: 959-964
- Бөлім: Article
- URL: https://ogarev-online.ru/1063-7729/article/view/192152
- DOI: https://doi.org/10.1134/S1063772918120326
- ID: 192152
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Аннотация
We study the measure on the set of initial conditions in remote past for Loop Quantum Cosmology with massive scalar field motivated by various choices of the measure present in the literature. The main finding of the paper is existence of an attractor at contracting phase of the universe, which, in addition to the well known attractor at expanding phase, predicts a very specific duration of inflationary stage with the number of e-foldings about 140.
Авторлар туралы
G. Vereshchagin
ICRANet; ICRA and University of Rome “Sapienza”; ICRANet-Minsk, Institute of Physics
Хат алмасуға жауапты Автор.
Email: veresh@icra.it
Италия, Pescara, 65122; piazza Aldo Moro 5, Rome, 00185; Nezavisimosti ave. 68, Minsk, 220072
S. Bedić
ICRANet
Email: veresh@icra.it
Италия, Pescara, 65122
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