arXiv · 1609.03533
Propagating q-field and q-ball solution
Abstract
One possible solution of the cosmological constant problem involves a so-called $q$-field, which self-adjusts so as to give a vanishing gravitating vacuum energy density (cosmological constant) in equilibrium. We show that this $q$-field can manifest itself in other ways. Specifically, we establish a propagating mode ($q$-wave) in the nontrivial vacuum and find a particular soliton-type solution in flat spacetime, which we call a $q$-ball by analogy with the well-known $Q$-ball solution. Both $q$-waves and $q$-balls are expected to play a role for the equilibration of the $q$-field in the very early universe.
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F. R. Klinkhamer, G. E. Volovik. 2017-05-22. Propagating q-field and q-ball solution. https://doi.org/10.1142/s0217732317501036
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