Energy Emission by Quantum Systems in an Expanding FRW Metric

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dc.creatorSheehan, D. P.
dc.creatorKriss, V. G.
dc.date2004-11-11
dc.date.accessioned2026-07-07T02:15:46Z
dc.date.available2026-07-07T02:15:46Z
dc.descriptionBound quantum mechanical systems not expanding with the comoving frame of an expanding, flat FRW metric are found to release energy at a rate linearly proportional to the local Hubble constant ($H_{o}$) and the systems' binding energy ($E_{b}$); {\em i.e.}, $\dot{E} = H_{o} E_{b}$. Three exemplary quantum systems are examined. For systems with early cosmological condensation times | notably hadrons | time-integrated energy release could have been significant and could account for an appreciable fraction of the dark matter inventory.
dc.description12 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0411299
dc.identifierhttp://arxiv.org/abs/astro-ph/0411299
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8535
dc.subjectAstrophysics
dc.titleEnergy Emission by Quantum Systems in an Expanding FRW Metric
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