Dark matter from dark energy in q-theory
F.R. Klinkhamer, G.E. Volovik

TL;DR
This paper proposes that small spacetime-dependent perturbations of a $q$-field, which helps cancel vacuum energy, can behave as dark matter, providing a new theoretical candidate that may explain dark matter without new particles.
Contribution
It introduces a model where $q$-field perturbations act as dark matter, linking vacuum energy cancellation to dark matter phenomenology.
Findings
$q$-field perturbations behave as pressureless fluid.
Oscillation frequency of $q$-field is at Planck scale.
Implication for dark matter detection efforts.
Abstract
A constant (spacetime-independent) -field may play a crucial role for the cancellation of Planck-scale contributions to the gravitating vacuum energy density. We now show that a small spacetime-dependent perturbation of the equilibrium -field behaves gravitationally as a pressureless perfect fluid. This makes the fluctuating part of the -field a candidate for the inferred dark-matter component of the present universe. For a Planck-scale oscillation frequency of the -field perturbation, the implication would be that direct searches for dark-matter particles would remain unsuccessful in the foreseeable future.
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