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Gravitational self-interactions of a degenerate quantum scalar field

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arxiv 1710.02195 v2 pith:LWBOHTZO submitted 2017-10-05 hep-ph astro-ph.COhep-th

classification hep-phastro-ph.COhep-th
keywords condensatehomogeneousclassicalcondensatesdescriptionfieldquantumcalculate
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We develop a formalism to help calculate in quantum field theory the departures from the description of a system by classical field equations. We apply the formalism to a homogeneous condensate with attractive contact interactions and to a homogeneous self-gravitating condensate in critical expansion. In their classical descriptions, such condensates persist forever. We show that in their quantum description, parametric resonance causes quanta to jump in pairs out of the condensate into all modes with wavector less than some critical value. We calculate in each case the time scale over which the homogeneous condensate is depleted, and after which a classical description is invalid. We argue that the duration of classicality of inhomogeneous condensates is shorter than that of homogeneous condensates.

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  1. Quantum break in models of axion dark matter

    hep-ph 2019-08 conditional novelty 6.0 of 10

    A modified mean-field analysis predicts that axion dark matter can undergo a quantum break into photon pairs, with multi-mode synchronization counteracting red-shift detuning.

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