dc.contributor.author | Mahbubani, Rakhi | |
dc.contributor.author | Redi, Michele | |
dc.contributor.author | Tesi, Andrea | |
dc.date.accessioned | 2020-06-09T00:07:10Z | |
dc.date.available | 2020-06-09T00:07:10Z | |
dc.date.issued | 2020-05-15 | |
dc.identifier.citation | Mahbubani , R , Redi , M & Tesi , A 2020 , ' Indirect Detection of Composite (Asymmetric) Dark Matter ' , Physical Review D , vol. 101 , no. 10 , 103037 . https://doi.org/10.1103/PhysRevD.101.103037 | |
dc.identifier.issn | 2470-0010 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/1908.00538v1 | |
dc.identifier.other | ORCID: /0000-0001-6311-4310/work/75617273 | |
dc.identifier.uri | http://hdl.handle.net/2299/22820 | |
dc.description | Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license (https://creativecommons.org/licenses/by/4.0/). Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3. | |
dc.description.abstract | Dark Matter can form bound states upon the emission of quanta of energy equal to the binding energy. The rate of this process is large for strongly-interacting Dark Matter, and further enhanced by long distance effects. The resulting monochromatic and diffuse $\gamma$-rays can be tested in indirect detection experiments. If Dark Matter has electroweak charge, indirect signals include multiple observable photon lines for masses in the TeV range. Else if it couples only via a dark photon portal, diffuse spectra from dwarf galaxies and CMB reionization set powerful limits for masses below a TeV. This mechanism provides a powerful means of probing Asymmetric Dark Matter today. | en |
dc.format.extent | 6 | |
dc.format.extent | 375145 | |
dc.language.iso | eng | |
dc.relation.ispartof | Physical Review D | |
dc.subject | hep-ph | |
dc.subject | astro-ph.CO | |
dc.subject | hep-lat | |
dc.subject | nucl-th | |
dc.title | Indirect Detection of Composite (Asymmetric) Dark Matter | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1103/PhysRevD.101.103037 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |