Saved in:
Bibliographic Details
Main Authors: Liang, Guanming, Caldwell, Robert R.
Format: Preprint
Published: 2024
Subjects:
Online Access:https://arxiv.org/abs/2408.08356
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866916733674061824
author Liang, Guanming
Caldwell, Robert R.
author_facet Liang, Guanming
Caldwell, Robert R.
contents We present a novel candidate for cold dark matter consisting of condensed Cooper pairs in a theory of interacting fermions with broken chiral symmetry. Establishing the thermal history from the early radiation era to the present, the fermions are shown to behave like standard radiation at high temperatures, but then experience a critical era decaying faster than radiation, akin to freeze-out, which sets the relic abundance. Through a second-order phase transition, fermion-antifermion pairs condense and the system asymptotes toward zero temperature and pressure. By the present era, the nonrelativistic, massive condensate decays slightly faster than in the standard scenario--a unique prediction that may be tested by combined measurements of the cosmic microwave background and large scale structure. We also show that in the case of massive fermions, the phase transition is frustrated, and instead leaves a residual, long-lived source of dark energy.
format Preprint
id arxiv_https___arxiv_org_abs_2408_08356
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Cold Dark Matter Based on an Analogy with Superconductivity
Liang, Guanming
Caldwell, Robert R.
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
We present a novel candidate for cold dark matter consisting of condensed Cooper pairs in a theory of interacting fermions with broken chiral symmetry. Establishing the thermal history from the early radiation era to the present, the fermions are shown to behave like standard radiation at high temperatures, but then experience a critical era decaying faster than radiation, akin to freeze-out, which sets the relic abundance. Through a second-order phase transition, fermion-antifermion pairs condense and the system asymptotes toward zero temperature and pressure. By the present era, the nonrelativistic, massive condensate decays slightly faster than in the standard scenario--a unique prediction that may be tested by combined measurements of the cosmic microwave background and large scale structure. We also show that in the case of massive fermions, the phase transition is frustrated, and instead leaves a residual, long-lived source of dark energy.
title Cold Dark Matter Based on an Analogy with Superconductivity
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2408.08356