Dark nuclei. I. Cosmology and indirect detection
By William Detmold, Matthew McCullough, A. Pochinsky. 2014
139 citations recorded by the source corpus.
In a companion paper Detmold et al. [Phys. Rev. D 90, 114506 (2014)]PRVDAQ1550-799810.1103/PhysRevD.90.114506, lattice field theory methods are used to show that in two-color, two-flavor QCD there are stable nuclear states in the spectrum. As a commonly studied theory of composite dark matter, this motivates the consideration of possible nuclear physics in this and other composite dark sectors. In this work, early Universe cosmology and indirect detection signatures are explored for both symmetric and asymmetric dark matter, highlighting the unique features that arise from considerations of dark nuclei and associated dark nuclear processes. The present day dark matter abundance may be composed of dark nucleons and/or dark nuclei, where the latter are generated through dark nucleosynthesis. For symmetric dark matter, indirect detection signatures are possible from annihilation, dark nucleosynthesis, and dark nuclear capture and we present a novel explanation of the Galactic center gamma ray excess based on the latter. For asymmetric dark matter, dark nucleosynthesis may alter the capture of dark matter in stars, allowing for captured particles to be processed into nuclei and ejected from the star through dark nucleosynthesis in the core. Notably, dark nucleosynthesis realizes a novel mechanism for indirect detection signals of asymmetric dark matter from regions such as the Galactic center, without having to rely on a symmetric dark matter component.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/0e106fe5ae4ae95b37a259f0e713605b32668720
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Citations in the corpus
- A tale of tails: Dark matter interpretations of the Fermi GeV excess in light of background model systematics (2014, methodology): “As for the DM interpretation, there is by now an extensive array of DM scenarios that both can explain the observed emission by DM annihilation while simultaneously being compatible with other direct, indirect and collider constraints [34–81].”