The Glow of Axion Quark Nugget Dark Matter: (II) Galaxy Clusters

Abstract

(abridged) We analyze the emission of axion quark nuggets in a large sample of 161 simulated galaxy clusters using the SLOW simulation. These clusters are divided into a sub-sample of 150 galaxy clusters, ordered in five mass bins ranging from $0.8$ to $31.7\times 10^{14}{M}_{\odot }$, along with 11 cross-identified galaxy clusters from observations. We investigate dark matter-baryonic matter interactions in galaxy clusters in their present stage at redshift $z=0$ by assuming all dark matter consists of axion quark nuggets. The resulting electromagnetic signatures are compared to thermal Bremsstrahlung and non-thermal cosmic ray synchrotron emission in each galaxy cluster. We further investigate individual frequency bands imitating the observable range of the WMAP, Planck, Euclid, and XRISM telescopes for the most promising cross-identified galaxy clusters hosting detectable signatures of axion quark nugget emission. We propose that the Fornax and Virgo clusters represent the most promising candidates to search for axion quark nugget emission signatures.

22 pages, 14 figures

References in corpus (31)

• Color superconductivity in dense quark matter
• Measurement of the permanent electric dipole moment of the neutron
• Diffuse Radio Emission from Galaxy Clusters
• The dark-matter axion mass
• Simulation techniques for cosmological simulations
• Radio halos in a mass-selected sample of 75 galaxy clusters. II. Statistical analysis
• The Axion Quark Nugget Dark Matter Model: Size Distribution and Survival Pattern
• The Young and the Wild: What happens to Protoclusters forming at z = 4?
• Diffuse cosmic gamma-rays at 1-20 MeV: A trace of the dark matter?
• Width of the 511 KeV Line from the Bulge of the Galaxy
• Solar Extreme UV radiation and quark nugget dark matter model
• Simulating the LOcal Web (SLOW): I. Anomalies in the local density field
• Narrow head-tail radio galaxies at very high resolution
• Two striking head-tail galaxies in the galaxy cluster IIZW108: insights into transition to turbulence, magnetic fields and particle re-acceleration
• Radiation from matter-antimatter annihilation in the quark nugget model of dark matter
• The ANITA Anomalous Events and Axion Quark Nuggets
• The mysterious diffuse UV radiation and Axion Quark Nugget dark matter model
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• Structure Formation Paradigm and Axion Quark Nugget dark matter model
• Radio impulsive events in quiet solar corona and Axion Quark Nugget Dark Matter
• The Mysterious Bursts observed by Telescope Array and Axion Quark Nuggets
• Thermal and annihilation radiation in the quark nugget model of dark matter
• A new catalogue of head-tail radio galaxies from LoTSS DR1
• The Merger Dynamics of the Galaxy Cluster Abell 1775: New Insights from Chandra and XMM-Newton for a Cluster Simultaneously Hosting a WAT and a NAT Radio Sources
• Results of search for magnetized quark-nugget dark matter from radial impacts on Earth
• Radio frequency emissions from dark-matter-candidate magnetized quark nuggets interacting with matter
• Clusters' far-reaching influence on narrow-angle tail radio galaxies
• Limits on Magnetized Quark-Nugget Dark Matter from Episodic Natural Events
• Radiation from cold molecular clouds and Sun chromosphere produced by anti-quark nugget dark matter
• The Glow of Axion Quark Nugget Dark Matter: (I) Large Scale Structures
• A Search for Magnetized Quark Nuggets (MQNs), a Candidate for Dark Matter, Accumulating in Iron Ore

Cited by in corpus (3)

• The Glow of Axion Quark Nugget Dark Matter: (I) Large Scale Structures
• Cosmological Zoom-In Simulation of Odd Radio Circles as Merger-Driven Shocks in Galaxy Groups
• The Glow of Axion Quark Nugget Dark Matter: (IV) CMB Spectral and Anisotropy Signatures