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Автор Mohammad A. Ganjali
Дата выпуска 2005-09-01
dc.description In this paper, we study the generation of a large scale magnetic field with amplitude of order μG in an inflationary model which has been introduced in [1]. This inflationary model based on existence of a speed limit for inflaton field. Generating a mass for inflaton at scale above the φ<sub>IR</sub>, breaks the conformal triviality of the Maxwell equation and causes to originate a magnetic field during the inflation. The amplitude strongly depends on the details of reheating stage and also depends on the e-foldings parameter N. We find the amplitude of the primordial magnetic field at decoupling time in this inflationary background using late time behavior of the theory.
Формат application.pdf
Издатель Institute of Physics Publishing
Название DBI with primordial magnetic field in the sky
Тип paper
DOI 10.1088/1126-6708/2005/09/004
Electronic ISSN 1029- 8479
Print ISSN 1126-6708
Журнал Journal of High Energy Physics
Том 2005
Первая страница 4
Последняя страница 004
Выпуск 09

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