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On the Inationary Origin of Primordial Magnetic Fields
本文正式版本已出版，請見：10.6122/CJP.20140408
並列摘要
Contrary to the conventional wisdom, we find that it is possible to generate coherent magnetic seed fields over a scale of 10 Mpc efficiently via the spinodal instability during primordial inflation, provided that a fast-roll stage is involved before the inflation enters into the slow-roll phase. However, the primordial magnetic field produced in such a mechanism is far too powerful to consistently fit in the energy constraint required by the scalar field driving the cosmic inflation.
並列關鍵字
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延伸閱讀
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