Dark nuclei. I. Cosmology and indirect detection
Name
PhysRevD.90.115013.pdf
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641.37 KB
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Adobe PDF
Checksum (MD5)
7779010789497dc7dd8b5d6498a549f5
Author(s)
Detmold, William
Pochinsky, Andrew
McCullough, Matthew P.
Date Issued
December 2014
Journal
Physical Review D
Publisher
American Physical Society
Citation
Detmold, William, Matthew McCullough, and Andrew Pochinsky. "Dark nuclei. I. Cosmology and indirect detection." Phys. Rev. D 90, 115013 (December 2014). © 2014 American Physical Society
Version
Final published version
Abstract
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.
MIT Department
Massachusetts Institute of Technology. Center for Theoretical Physics
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
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DOI of Published Version
https://doi.org/10.1103/PhysRevD.90.115013
