Muonphilic dark matter explanation of gamma-ray galactic center excess: a comprehensive analysis
- Location
-
Deutsche Nationalbibliothek Frankfurt am Main
- ISSN
-
1029-8479
- Extent
-
Online-Ressource
- Language
-
Englisch
- Notes
-
online resource.
- Bibliographic citation
-
Muonphilic dark matter explanation of gamma-ray galactic center excess: a comprehensive analysis ; volume:2022 ; number:7 ; day:20 ; month:7 ; year:2022 ; pages:1-28 ; date:7.2022
Journal of high energy physics ; 2022, Heft 7 (20.7.2022), 1-28, 7.2022
- Creator
-
Abdughani, Murat
Fan, Yi-Zhong
Lu, Chih-Ting
Tang, Tian-Peng
Tsai, Yue-Lin Sming
- Contributor
-
SpringerLink (Online service)
- DOI
-
10.1007/JHEP07(2022)127
- URN
-
urn:nbn:de:101:1-2022100520094631989301
- Rights
-
Open Access; Der Zugriff auf das Objekt ist unbeschränkt möglich.
- Last update
-
15.08.2025, 7:28 AM CEST
Data provider
This object is provided by:
Deutsche Nationalbibliothek. If you have any questions about the object, please contact the data provider.
Deutsche Nationalbibliothek. If you have any questions about the object, please contact the data provider.
Associated
- Abdughani, Murat
- Fan, Yi-Zhong
- Lu, Chih-Ting
- Tang, Tian-Peng
- Tsai, Yue-Lin Sming
- SpringerLink (Online service)
Other Objects (12)
Dark matter annihilation into right-handed neutrinos and the galactic center gamma-ray excess
Gamma-ray excess and the minimal dark matter model
Interpretations of galactic center gamma-ray excess confronting the PandaX-II constraints on dark matter-neutron spin-dependent scatterings in the NMSSM
Hidden Higgs portal vector dark matter for the Galactic center gamma-ray excess from the two-step cascade annihilation, and muon g − 2
Collider probes of singlet fermionic dark matter scenarios for the Fermi gamma-ray excess
Galactic gamma ray excess and dark matter phenomenology in a U(1) B−L model
Diffuse Gamma-Ray Emission from the Galactic Centre with H.E.S.S.
A potentially detectable gamma-ray line in the Fermi Galactic center excess — in light of one-step cascade annihilations of secluded (vector) dark matter via the Higgs portal
Scalar dark matter explanation of the excess in the Belle II B + → K ++ invisible measurement
HESS and Fermi Surveys of the Galactic Gamma-ray Source Population
Modelling the galactic population of very-high-energy gamma-ray sources
Diphoton excess through dark mediators
Dark matter annihilation into right-handed neutrinos and the galactic center gamma-ray excess
Gamma-ray excess and the minimal dark matter model
Interpretations of galactic center gamma-ray excess confronting the PandaX-II constraints on dark matter-neutron spin-dependent scatterings in the NMSSM
Hidden Higgs portal vector dark matter for the Galactic center gamma-ray excess from the two-step cascade annihilation, and muon g − 2
Collider probes of singlet fermionic dark matter scenarios for the Fermi gamma-ray excess
Galactic gamma ray excess and dark matter phenomenology in a U(1) B−L model
Diffuse Gamma-Ray Emission from the Galactic Centre with H.E.S.S.
A potentially detectable gamma-ray line in the Fermi Galactic center excess — in light of one-step cascade annihilations of secluded (vector) dark matter via the Higgs portal
Scalar dark matter explanation of the excess in the Belle II B + → K ++ invisible measurement
HESS and Fermi Surveys of the Galactic Gamma-ray Source Population
Modelling the galactic population of very-high-energy gamma-ray sources
Diphoton excess through dark mediators
Dark matter annihilation into right-handed neutrinos and the galactic center gamma-ray excess
Gamma-ray excess and the minimal dark matter model
Interpretations of galactic center gamma-ray excess confronting the PandaX-II constraints on dark matter-neutron spin-dependent scatterings in the NMSSM
Hidden Higgs portal vector dark matter for the Galactic center gamma-ray excess from the two-step cascade annihilation, and muon g − 2
Collider probes of singlet fermionic dark matter scenarios for the Fermi gamma-ray excess
Galactic gamma ray excess and dark matter phenomenology in a U(1) B−L model
Diffuse Gamma-Ray Emission from the Galactic Centre with H.E.S.S.
A potentially detectable gamma-ray line in the Fermi Galactic center excess — in light of one-step cascade annihilations of secluded (vector) dark matter via the Higgs portal
Scalar dark matter explanation of the excess in the Belle II B + → K ++ invisible measurement
HESS and Fermi Surveys of the Galactic Gamma-ray Source Population
Modelling the galactic population of very-high-energy gamma-ray sources