Primordial magnetic field amplification from turbulent reheating

We analyze the possibility of primordial magnetic field amplification by a stochastic large scale kinematic dynamo during reheating. We consider a charged scalar field minimally coupled to gravity. During inflation this field is assumed to be in its vacuum state. At the transition to reheating the s...

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Detalles Bibliográficos
Autores principales:	Calzetta, E., Kandus, A.
Formato:	JOUR
Materias:	Cosmic magnetic fields theory Magnetohydrodynamics
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_14757516_v2010_n8_p_Calzetta
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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