Correlation Analysis of Decaying Sterile Neutrino Dark Matter in the Context of the SRG Mission
arXiv:2211.05919 · doi:10.1088/1475-7516/2023/02/055
Abstract
We provide a correlation analysis of signatures associated with traces of the dark matter decay and the galaxy spatial distribution according to the 2MRS catalog of galaxies. Signature data analysis plays an important role in the context of current and future observations and cosmological constraints. Attention is paid to the constraints that can be obtained for decaying sterile neutrinos when analyzing observations in the context of the Spectr-Roentegn-Gamma (SRG) mission. We study the correlation spectra of dark matter and galaxies, which can be obtained both for the eROSITA telescope and for the first time for the ART-XC telescope. The analysis is carried out both within the framework of the Limber approximation and within the framework of the extended Limber approximation, which makes it possible to more accurately study the power spectra in the region of small multipoles. We calculate the power spectra in both approaches and examine the contribution of different ranges of multipoles to the resulting constraints on sterile neutrino parameters.
arXiv comment19 pages, 3 figures
References in corpus (54)
- A Universal Density Profile from Hierarchical Clustering
- Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
- Halo Models of Large Scale Structure
- Sterile Neutrinos as Dark Matter
- Analytic model for galaxy and dark matter clustering
- The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests
- The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass
- Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
- The eROSITA X-ray telescope on SRG
- A New Dark Matter Candidate: Non-thermal Sterile Neutrinos
- Detection of An Unidentified Emission Line in the Stacked X-ray spectrum of Galaxy Clusters
- The 2MASS Redshift Survey - Description and Data Release
- An unidentified line in X-ray spectra of the Andromeda galaxy and Perseus galaxy cluster
- Sterile Neutrino Hot, Warm, and Cold Dark Matter
- The properties of warm dark matter haloes
- Extended Limber Approximation
- eROSITA Science Book: Mapping the Structure of the Energetic Universe
- The Halo Occupation Distribution and the Physics of Galaxy Formation
- Sterile Neutrino Dark Matter
- The SRG X-ray orbital observatory, its telescopes and first scientific results
- A White Paper on keV Sterile Neutrino Dark Matter
- The MSM, Inflation, and Dark Matter
- Direct Detection of Warm Dark Matter in the X-ray
- An accurate physical model for halo concentrations
- Constraints on sterile neutrino as a dark matter candidate from the diffuse X-ray background
- Where to find a dark matter sterile neutrino?
- Checking the dark matter origin of 3.53 keV line with the Milky Way center
- Peculiar velocities of galaxies and clusters
- New Constraints on Sterile Neutrino Dark Matter from M31 Observations
- (Almost) Closing the MSM Sterile Neutrino Dark Matter Window with NuSTAR
- The ART-XC telescope on board the SRG observatory
- Remarks on the KARMEN Anomaly
- Searching for decaying dark matter in deep XMM-Newton observation of the Draco dwarf spheroidal
- Long-Exposure NuSTAR Constraints on Decaying Dark Matter in the Galactic Halo
- eROSITA on SRG
- Constraints on parameters of radiatively decaying dark matter from the galaxy cluster 1E0657-56
- The halo model in a massive neutrino cosmology
- Dark matter searches in the gamma-ray extragalactic background via cross-correlations with galaxy catalogues
- Particle dark matter searches in the anisotropic sky
- Relic Gravity Waves and 7 keV Dark Matter from a GeV scale inflaton
- Mapping dark matter in the gamma-ray sky with galaxy catalogs
- Imprint of galaxy clustering in the cosmic gamma-ray background
- Substructure and the halo model of large-scale structure
- Angular power spectrum of galaxies in the 2MASS Redshift Survey
- The Signature of Large Scale Structures on the Very High Energy Gamma-Ray Sky
- Power spectrum tomography of dark matter annihilation with local galaxy distribution
- Searches for sterile neutrinos and axionlike particles from the Galactic halo with eROSITA
- Angular Correlations of the MeV Cosmic Gamma Ray Background
- The role of the eROSITA all-sky survey in searches for sterile neutrino dark matter
- Searching for Sterile Neutrino with X-ray Intensity Mapping
- Angular Power Spectra with Finite Counts
- Induced resonance makes light sterile neutrino Dark Matter cool
- Towards Testing Sterile Neutrino Dark Matter with Spectrum-Roentgen-Gamma Mission
- New constraints on sterile neutrino dark matter from the Galactic Center