More on cold dark matter from q-theory
classification
🌀 gr-qc
astro-ph.COhep-th
keywords
behavescoldcold-dark-mattercomponentconsidercontextcosmiccosmological
read the original abstract
We consider the rapidly-oscillating part of a $q$-field in a cosmological context and find that its energy density behaves in the same way as a cold-dark-matter component, namely proportional to the inverse cube of the cosmic scale factor.
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