dark matter-philic Higgs for 3.5 keV X-ray signal
arXiv:1407.6827 · doi:10.1016/j.physletb.2015.02.014
Abstract
We suggest a new model of 7 keV right-handed neutrino dark matter inspired by a recent observation of 3.5 keV X-ray line signal in the XMM-Newton observatory. It is difficult to derive the tiny masses with a suitable left-right mixing of the neutrino in a framework of ordinary simple type-I seesaw mechanism. We introduce a new Higgs boson, a dark matter-philic Higgs boson, in which the smallness of its vacuum expectation value can be achieved. We investigate suitable parameter regions where the observed dark matter properties are satisfied. We find that the vacuum expectation value of dark matter-philic Higgs boson should be about 0.17 GeV.
10 pages, 1 figure, v2:references added, minor changes, v3:published version
References in corpus (23)
- Can sterile neutrinos be the dark matter?
- Can sterile neutrinos be ruled out as warm dark matter candidates?
- Realistic sterile neutrino dark matter with keV mass does not contradict cosmological bounds
- The Poker Face of the Majoron Dark Matter Model: LUX to keV Line
- The 7 keV axion dark matter and the X-ray line signal
- A 3.55 keV Photon Line and its Morphology from a 3.55 keV ALP Line
- Soft L_e-L_mu-L_tau flavour symmetry breaking and sterile neutrino keV Dark Matter
- Sterile neutrino dark matter in extension of the standard model and galactic 511 keV line
- X-ray line signal from decaying axino warm dark matter
- Generating X-ray lines from annihilating dark matter
- X-ray Lines from Dark Matter: The Good, The Bad, and The Unlikely
- 3.5 keV X-rays as the "21 cm line" of dark atoms, and a link to light sterile neutrinos
- 3.55 keV photon lines from axion to photon conversion in the Milky Way and M31
- 7 keV Scalar Dark Matter and the Anomalous Galactic X-ray Spectrum
- keV Photon Emission from Light Nonthermal Dark Matter
- 3.55 keV X-ray Line Signal from Excited Dark Matter in Radiative Neutrino Model
- A Dynamical Framework for KeV Dirac Neutrino Warm Dark Matter
- SUSY in the sky or a keV signature of sub-GeV gravitino dark matter
- 7 keV Dark Matter as X-ray Line Signal in Radiative Neutrino Model
- Natural -ray Lines from the Low Scale Supersymmetry Breaking
- 3.5 keV X-ray line and R-Parity Conserving Supersymmetry
- 3.5 keV Galactic Emission Line as a Signal from the Hidden Sector
- 3.55 keV X-ray Line Interpretation in Radiative Neutrino Model