Abstract
Despite many decades of study the physical origin of "dark matter" in the Universe remains elusive. In this letter we calculate the properties of a completely new dark matter candidate - Bose-Einstein condensates formed from a recently discovered bosonic particle in the light-quark sector, the $\mathbf{ d^*(2380)}$ hexaquark. In this first study, we show stable $\mathbf{ d^*(2380)}$ Bose-Einstein condensates could form in the primordial early universe, with a production rate sufficiently large that they are a plausible new candidate for dark matter. Some possible astronomical signatures of such dark matter are also presented.
Original language | English |
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Article number | 03LT01 |
Number of pages | 10 |
Journal | Journal of Physics G: Nuclear and Particle Physics |
Volume | 47 |
Issue number | 3 |
Early online date | 12 Feb 2020 |
DOIs | |
Publication status | Published - Mar 2020 |
Bibliographical note
© 2020 The Author(s)Keywords
- Hexaquark
- dark matter