Journal
PHYSICAL REVIEW D
Volume 81, Issue 12, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.81.123002
Keywords
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Funding
- Georgian National Science Foundation [GNSF ST08/4-422]
- Department of Energy [DOE DE-FG03-99EP41043]
- Swiss National Science Foundation SCOPES [128040]
- NASA Astrophysics Theory Program [NNXlOAC85G]
- European Research Council [227952]
- Swedish Research Council [621-2007-4064]
- ICTP associate membership program
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We perform direct numerical simulations of forced and freely decaying 3D magnetohydrodynamic turbulence in order to model magnetic field evolution during cosmological phase transitions in the early Universe. Our approach assumes the existence of a magnetic field generated either by a process during inflation or shortly thereafter, or by bubble collisions during a phase transition. We show that the final configuration of the magnetic field depends on the initial conditions, while the velocity field is nearly independent of initial conditions.
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