We study the fermionic vacuum energy of vacua with and without application of an external magnetic field. The energetic difference of two vacua leads to the vacuum decaying and the vacuum energy being released. In the context of quantum field theories, we discuss why and how the vacuum energy can be released by spontaneous photon emission and/or paramagnetically screening the external magnetic field. In addition, we quantitatively compute the vacuum energy released, the paramagnetic screening effect, and the rate and spectrum of spontaneous photon emission. The possibilities of experimentally detecting such an effect of vacuum-energy release and that this effect accounts for the anomalous x-ray pulsar are discussed.
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UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England
Jenkins, Alexander C.
Braden, Jonathan
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Univ Toronto, Canadian Inst Theoret Astrophys, 60 St George St, Toronto, ON M5S 3H8, CanadaUCL, Dept Phys & Astron, London WC1E 6BT, England
Braden, Jonathan
V. Peiris, Hiranya
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UCL, Dept Phys & Astron, London WC1E 6BT, England
Stockholm Univ, Oskar Klein Ctr Cosmoparticle Phys, Dept Phys, AlbaNova, SE-10691 Stockholm, SwedenUCL, Dept Phys & Astron, London WC1E 6BT, England
V. Peiris, Hiranya
Pontzen, Andrew
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UCL, Dept Phys & Astron, London WC1E 6BT, EnglandUCL, Dept Phys & Astron, London WC1E 6BT, England
Pontzen, Andrew
Johnson, Matthew C.
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York Univ, Dept Phys & Astron, Toronto, ON M3J 1P3, Canada
Perimeter Inst Theoret Phys, 31 Caroline St N, Waterloo, ON N2L 2Y5, CanadaUCL, Dept Phys & Astron, London WC1E 6BT, England
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Univ Minnesota, Sch Phys & Astron, William I Fine Theoret Phys Inst, Minneapolis, MN 55455 USAUniv Minnesota, Sch Phys & Astron, William I Fine Theoret Phys Inst, Minneapolis, MN 55455 USA