Radiative bound-state-formation cross-sections for dark matter interacting via a Yukawa potential
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Publication:680696
DOI10.1007/JHEP04(2017)077zbMath1378.85006arXiv1611.01394OpenAlexW3104995897MaRDI QIDQ680696
Kalliopi Petraki, Marieke Postma, Jordy De Vries
Publication date: 23 January 2018
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1611.01394
Unified quantum theories (81V22) Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)
Related Items (7)
Probability density of the Yukawa particle at the origin: numerical calculation and analytical solution ⋮ Saha equilibrium for metastable bound states and dark matter freeze-out ⋮ Effects of QCD bound states on dark matter relic abundance ⋮ Complete analytical solution to the quantum Yukawa potential ⋮ On quantum and classical treatments of radiative recombination ⋮ Bound-state formation, dissociation and decays of darkonium with potential non-relativistic Yukawa theory for scalar and pseudoscalar mediators ⋮ Bound states of pseudo-Dirac dark matter
Uses Software
Cites Work
- Unnamed Item
- Diurnal modulation signal from dissipative hidden sector dark matter
- Relic densities including Sommerfeld Enhancements in the MSSM
- Model-independent implications of the \(e^{\pm }\), \(\bar{p}\) cosmic ray spectra on properties of Dark Matter
- Inverse compton constraints on the dark matter \(e^{\pm }\) excesses
- Dark-matter bound states from Feynman diagrams
- Über die Beugung und Bremsung der Elektronen
- Journey to the Bound States
- Mirror dark matter: Cosmology, galaxy structure and direct detection
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