Freeze-in Production of Sterile Neutrino Dark Matter in U(1) Model
arXiv:1607.01469 · doi:10.1088/1475-7516/2016/09/044
Abstract
With the advent of new and more sensitive direct detection experiments, scope for a thermal WIMP explanation of dark matter (DM) has become extremely constricted. The non-observation of thermal WIMP in these experiments has put a strong upper bound on WIMP-nucleon scattering cross section and within a few years it is likely to touch the neutrino floor. Hence in all probability, DM may have some non-thermal origin. In this work we explore in detail this possibility of a non-thermal sterile neutrino DM within the framework of U(1) model. The U(1) model on the other hand is a well-motivated and minimal way of extending the standard model so that it can explain the neutrino masses via Type-I see-saw mechanism. We have shown, besides explaining the neutrino mass, it can also accommodate a non-thermal sterile neutrino DM with correct relic density. In contrast with the existing literature, we have found that decay can also be a dominant production mode of the sterile neutrino DM. To obtain the comoving number density of dark matter, we have solved here a coupled set of Boltzmann equations considering all possible decay as well as annihilation production modes of the sterile neutrino dark matter. The framework developed here though has been done for a U(1) model, can be applied quite generally for any models with an extra neutral gauge boson and a fermionic non-thermal dark matter.
44 pages, 9 eps figures, 2 Tables
References in corpus (20)
- Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC
- Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
- Dark Matter Results from 225 Live Days of XENON100 Data
- Search for high-mass dilepton resonances in pp collisions at sqrt(s) = 8 TeV with the ATLAS detector
- Dark matter production in the early Universe: beyond the thermal WIMP paradigm
- Can sterile neutrinos be the dark matter?
- Exciting Dark Matter and the INTEGRAL/SPI 511 keV signal
- The Minimal Set of Electroweak Precision Parameters
- Realistic sterile neutrino dark matter with keV mass does not contradict cosmological bounds
- keV Sterile Neutrino Dark Matter from Singlet Scalar Decays: Basic Concepts and Subtle Features
- A Dark Matter Progenitor: Light Vector Boson Decay into (Sterile) Neutrinos
- Sterile neutrino dark matter in extension of the standard model and galactic 511 keV line
- MeV sterile neutrinos in low reheating temperature cosmological scenarios
- Nonthermal Two Component Dark Matter Model for Fermi-LAT -ray excess and 3.55 keV X-ray Line
- Class of Higgs-portal Dark Matter models in the light of gamma-ray excess from Galactic center
- Axino Light Dark Matter and Neutrino Masses with R-parity Violation
- 7 keV Scalar Dark Matter and the Anomalous Galactic X-ray Spectrum
- Non-thermal Production of Dark Matter from Late-Decaying Scalar Field at Intermediate Scale
- Sterile Neutrino Dark Matter and Low Scale Leptogenesis from a Charged Scalar
- Sterile neutrino dark matter in warped extra dimensions
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- Dark Matter Relic Abundance and Light Sterile Neutrinos
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- Long lived inert Higgs in fast expanding universe and its imprint on cosmic microwave background
- Freeze-in Dark Matter from a Minimal B-L Model and Possible Grand Unification
- Freeze-in Dark Matter Through Forbidden Channel in
- CMB signature of non-thermal Dark Matter produced from self-interacting dark sector
- Revisiting sterile neutrino dark matter in gauged model
- Non-adiabatic evolution of dark sector in the presence of gauge symmetry
- FIMP dark matter candidate(s) in a model with inverse seesaw mechanism
- Generation of neutrino dark matter, baryon asymmetry, and radiation after quintessential inflation
- Multi-messenger FIMP
- Cosmic Birefringence as a probe of dark matter nature: Sterile neutrino and dipolar dark matter
- Freeze-in sterile neutrino dark matter in a feebly gauged model
- A closer look at the seesaw-dark matter correspondence
- Sterile neutrino dark matter from a TeV Scale Seesaw
- Neutrino flavor mixing with approximate - symmetry within the low-scale minimal linear seesaw model
- Freeze-In Dark Matter and Leptogenesis: a SM route
- Sterile neutrino Dark Matter in the minimal Dirac Seesaw