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MG12 - Talk detail
 

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 Participant 

Visinescu, Anca

Institution

National Institute for Physics and Nuclear Engineering - "Horia Hulubei" , IFIN-HH  - Magurele MG - 6 - Bucharest - Romania - Romania

Session

Talk

Abstract

COT4

Bianchi type-I cosmological string model in the presence of a magnetic field: classical an quantum loop approaches

Cosmic strings are expected generically formed in the Early Universe as topological defects as a result of a series of phase transitions related to the spontaneous breaking of internal symmetry. A Bianchi type-I cosmological string model in the presence of a magnetic field is investigated. A few plausibly assumptions are introduced and their outcomes are discussed using numerical and qualitative analyzes. Quantum effects of a cosmological string are examined in the framework of loop quantum cosmology.

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