Colder Freeze-in Axinos Decaying into Photons
arXiv:1707.02077 · doi:10.1103/PhysRevD.97.055019
Abstract
We point out that 7 keV axino dark matter (DM) in the R-parity violating (RPV) supersymmetric (SUSY) Dine-Fischler-Srednicki-Zhitnitsky model can simultaneously reproduce the 3.5keV X-ray excess, and evade stringent constraints from the Ly-alpha forest data. Peccei-Quinn symmetry breaking naturally generates both axino interactions with minimal SUSY standard model particles and RPV interactions. The RPV interaction introduces an axino-neutrino mixing and provides axino DM as a variant of sterile neutrino DM, whose decay into a monochromatic photon can be detected by X-ray observations. Axinos, on the other hand, are produced by freeze-in processes of thermal particles in addition to the Dodelson-Widrow mechanism of sterile neutrinos. The resultant phase space distribution tends to be colder than the Fermi-Dirac distribution. The inherent entropy production from late-time saxion decay makes axinos even colder. The linear matter power spectrum satisfies even the latest and strongest constraints from the Ly-alpha forest data.
arXiv comment5 pages, 4 figures
References in corpus (35)
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- A Supersymmetry Primer
- Sterile Neutrinos as Dark Matter
- Freeze-In Production of FIMP Dark Matter
- Constraining Warm Dark Matter candidates including sterile neutrinos and light gravitinos with WMAP and the Lyman-alpha forest
- Warm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-alpha forest data
- Detection of An Unidentified Emission Line in the Stacked X-ray spectrum of Galaxy Clusters
- An unidentified line in X-ray spectra of the Andromeda galaxy and Perseus galaxy cluster
- New Constraints on the free-streaming of warm dark matter from intermediate and small scale Lyman- forest data
- The Cosmic Linear Anisotropy Solving System (CLASS) IV: Efficient implementation of non-cold relics
- Lightest sterile neutrino abundance within the nuMSM
- Lyman-alpha Forests cool Warm Dark Matter
- Checking the dark matter origin of 3.53 keV line with the Milky Way center
- Production and Evolution of Perturbations of Sterile Neutrino Dark Matter
- Constraints on 3.55 keV line emission from stacked observations of dwarf spheroidal galaxies
- Axino Mass in Supergravity Models
- Axino Mass
- Cold keV dark matter from decays and scatterings
- Astrophysical constraints on resonantly produced sterile neutrino dark matter
- keV Sterile Neutrino Dark Matter from Singlet Scalar Decays: The Most General Case
- X-ray line signal from 7 keV axino dark matter decay
- X-ray line signal from decaying axino warm dark matter
- Production of Sterile Neutrino Dark Matter and the 3.5 keV line
- Dark matter in the Kim-Nilles mechanism
- Mixed axion/neutralino dark matter in the SUSY DFSZ axion model
- Effective interactions of axion supermultiplet and thermal production of axino dark matter
- Cosmology of the DFSZ axino
- Axino Light Dark Matter and Neutrino Masses with R-parity Violation
- Light Axinos from Freeze-in: production processes, phase space distributions, and Ly- forest constraints
- Structure of Dark Matter Halos in Warm Dark Matter models and in models with Long-Lived Charged Massive Particles
- Axino dark matter in light of an anomalous X-ray line
- Implications of an axino LSP for naturalness
- Axino-Neutrino Mixing in Gauge-Mediated Supersymmetry Breaking Models
- Observation of the new emission line at ~3.5 keV in X-ray spectra of galaxies and galaxy clusters
- Axino as a sterile neutrino and R parity violation
Cited by in corpus (9)
- On UltraViolet Freeze-in Dark Matter during Reheating
- Cold light dark matter in extended seesaw models
- Constraining FIMP from the structure formation of the Universe: analytic mapping from
- MeV-GeV -ray telescopes probing axino LSP/gravitino NLSP as dark matter in the SSM
- Bilinear R-parity violating supersymmetry under the light of neutrino oscillation, higgs and flavor data
- Demystifying Freeze-In Dark Matter at the LHC
- Fingerprint matching of beyond-WIMP dark matter: neural network approach
- WIMP Dark Matter in the USSM
- Fenomenología de modelos supersimétricos: partículas y materia oscura