Imagen de Portada

Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Mehta, Harsh, Mukherjee, Suvodip
Formato:	Preprint
Publicado:	2025
Materias:	Cosmology and Nongalactic Astrophysics High Energy Astrophysical Phenomena
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
por: Mehta, Harsh, et al.
Publicado: (2024)

The Prospect from the Upcoming CMB Experiment LiteBIRD to Discover Axion-like Particles Using Milky Way
por: Mehta, Harsh, et al.
Publicado: (2025)

A Diffused Background from Axion-like Particles in the Microwave Sky
por: Mehta, Harsh, et al.
Publicado: (2024)

Detecting Axion-like particles using Cosmic Variance Cancellation with CMB and Radio surveys
por: Mehta, Harsh, et al.
Publicado: (2026)

Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion
por: Fiorillo, Damiano F. G., et al.
Publicado: (2026)

Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap
por: Afroz, Samsuzzaman, et al.
Publicado: (2025)

A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
por: Mehta, Harsh, et al.
Publicado: (2024)

Are all Binary Black Holes Detected by LIGO-Virgo-KAGRA Following the Universal Time-Delay Distributions? Probably Not
por: Afroz, Samsuzzaman, et al.
Publicado: (2025)

The Glow of Axion Quark Nugget Dark Matter: (II) Galaxy Clusters
por: Sommer, Julian S., et al.
Publicado: (2024)

A New Gravitational Wave Probe to the Nature of Dark Energy from the Aging of the Universe
por: Mukherjee, Suvodip
Publicado: (2024)

The First Upper Bound on the Non-Stationary Gravitational Wave Background and its Implication on the High Redshift Binary Black Hole Merger Rate
por: Sah, Mohit Raj, et al.
Publicado: (2025)

Is the Binary Black Hole Population Inference from Gravitational-Wave Data Robust?
por: Das, Upasana, et al.
Publicado: (2026)

Phase Space of Binary Black Holes from Gravitational Wave Observations to Unveil its Formation History
por: Afroz, Samsuzzaman, et al.
Publicado: (2024)

The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
por: Dehghani, Amir, et al.
Publicado: (2024)

Gravitational Wave Burst from Bremsstrahlung in Milky Way Can Discover Sub-Solar Dark Matter in Near Future
por: Afroz, Samsuzzaman, et al.
Publicado: (2025)

The Phase Space of Low-Mass Binary Compact Objects from LIGO-Virgo-KAGRA Catalog: Hints on the Chances of Different Formation Scenarios
por: Afroz, Samsuzzaman, et al.
Publicado: (2025)

How lonely are the Binary Compact Objects Detected by the LIGO-Virgo-KAGRA Collaboration?
por: Giri, Devesh, et al.
Publicado: (2026)

BBH-Genesis: Disentangling Binary Black Hole Formation Channels with GWTC-4
por: Padhyegurjar, Shaunak, et al.
Publicado: (2026)

Constraints on Axion-Photon Mixing from Fast Radio Burst Dispersion Measures
por: Muthusami, Gunalan, et al.
Publicado: (2026)

False Alarm Rates in Detecting Gravitational Wave Lensing from Astrophysical Coincidences: Insights with Model-Independent Technique GLANCE
por: Chakraborty, Aniruddha, et al.
Publicado: (2025)

Axion-Photon Conversion Signals from Neutron Stars with Spacetime Curvature Accounted for in the Magnetosphere Model
por: Satherley, Jesse, et al.
Publicado: (2024)

The First Model-Independent Chromatic Microlensing Search: No Evidence in the Gravitational Wave Catalog of LIGO-Virgo-KAGRA
por: Chakraborty, Aniruddha, et al.
Publicado: (2025)

The First Model-Independent Upper Bound on Micro-lensing Signature of the Highest Mass Binary Black Hole Event GW231123
por: Chakraborty, Aniruddha, et al.
Publicado: (2025)

Discovering the Dispersion of Gravitational Waves using Multi-Band Observation including Deci-Hertz: A Unique Probe to Cosmic Acceleration
por: Praveen, Adith, et al.
Publicado: (2025)

Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference
por: Müller, Michael, et al.
Publicado: (2024)

$μ$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals
por: Chakraborty, Aniruddha, et al.
Publicado: (2024)

Axion-Like Particle Dark Matter Intensity Mapping: A New Probe via Cross-Correlation with Galaxy Surveys
por: Guo, Wen-Qing
Publicado: (2026)

NuSTAR Observations of the Galaxy Cluster Abell 3667
por: Mirakhor, Mohammad S., et al.
Publicado: (2025)

A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background
por: Kuralkar, Hardik Jitendra, et al.
Publicado: (2025)

Electron-Ion Equilibration in the Merging Galaxy Cluster A665
por: Norseth, Christian, et al.
Publicado: (2025)

Forecasting the FRB Population Observed Through Galaxy Cluster Lenses
por: Sammons, Mawson W, et al.
Publicado: (2025)

Increase in the Brightness of the Cosmic Radio Background toward Galaxy Clusters
por: Grebenev, S. A., et al.
Publicado: (2024)

Adiabatic Axion-Photon Mixing Near Neutron Stars
por: Tjemsland, Jonas, et al.
Publicado: (2023)

Modeling Gravitational Wave Bias from 3D Power Spectra of Spectroscopic Surveys
por: Hosseini, Dorsa Sadat, et al.
Publicado: (2025)

Imprints of Supermassive Black Hole Evolution on the Spectral and Spatial Anisotropy of Nano-Hertz Stochastic Gravitational-Wave Background
por: Sah, Mohit Raj, et al.
Publicado: (2024)

Environmental Dependence of Type Ia Supernovae in Low-Redshift Galaxy Clusters
por: Larison, Conor, et al.
Publicado: (2023)

Cross-correlating dark sirens and galaxies: constraints on $H_0$ from GWTC-3 of LIGO-Virgo-KAGRA
por: Mukherjee, Suvodip, et al.
Publicado: (2022)

Numerical Analysis of Resonant Axion-Photon Mixing: Part I
por: Ginés, Estanis Utrilla, et al.
Publicado: (2024)

Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
por: Mehta, Harsh, et al.
Publicado: (2025)

Cross Calibration of Galaxy Cluster Temperatures Measured with NuSTAR, XMM-Newton, and Chandra
por: Lopez, Fiona, et al.
Publicado: (2025)