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Quasi-normal modes and fermionic vacuum decay around a Kerr black hole

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arxiv 1809.03480 v2 pith:L5PIIJZG submitted 2018-09-10 gr-qc hep-th

classification gr-qchep-th
keywords decayvacuumfermionkerrmodesquasi-normalanalogousanalyze
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We analyze the instability of the non-rotating fermion vacuum in Kerr spacetimes. We describe how the co-rotating Fermi sea is formed as a result of a spontaneous vacuum decay. Most significantly, and drawing upon intuition gained from analogous electrodynamic processes in supercritical fields, we show that this decay process is encoded entirely in a subset of quasi-normal fermion modes.

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Cited by 1 Pith paper

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  1. Revisiting the fermionic quasi-bound states around Schwarzschild black holes with improved analytic spectrum

    gr-qc 2025-01 conditional novelty 5.0 of 10

    Fermionic quasibound-state energies around Schwarzschild black holes are derived analytically with a first-order matching scheme and a higher-order angular correction that improves agreement with numerics.

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