AXIS Could Have Accessed Dark Matter Decays
astro-ph.CO, astro-ph.GA, astro-ph.HE, hep-ex, hep-ph
Submitted: 2026-08-28
Updated: 2026-10-22
Comments: 8 pages, 5 figures
Project page: https://cajohare.github.io/AxionLimits
License: http://creativecommons.org/licenses/by/4.0/
The gist: The Advanced X-ray Imaging Satellite (AXIS) was a mission concept designed to improve upon the sensitivity and spatial resolution of the Chandra X-ray Observatory and XMM-Newton.
Abstract
The Advanced X-ray Imaging Satellite (AXIS) was a mission concept designed to improve upon the sensitivity and spatial resolution of the Chandra X-ray Observatory and XMM-Newton. Although AXIS was not selected for implementation, the concept study defined a mature instrument design with low-background, arcsecond imaging over the 0.3 - 10 keV energy range, a large effective area, and a wide field of view. These capabilities provide a useful benchmark for the dark matter decay sensitivity of future X-ray observatories. We estimate the reach of a future AXIS-like instrument for narrow photon lines from decaying keV-scale dark matter, including axion-like particles and sterile neutrinos. For Galactic center observations, we find projected lifetime sensitivities of order 10 31 s, improving upon existing limits by up to an order of magnitude over part of the keV mass range.
Sources
- A History of Dark Matter
- Axion Dark Matter
- Sterile neutrinos in cosmology
- The Advanced X-ray Imaging Satellite
- Overview of the Advanced X-ray Imaging Satellite (AXIS)
- Line Emission Mapper (LEM): Probing the physics of cosmic ecosystems
- TASI Lectures on Indirect Searches For Dark Matter
- Listening to the Universe through Indirect Detection
- PPPC 4 DM ID: A Poor Particle Physicist Cookbook for Dark Matter Indirect Detection
- Limits from the grave: resurrecting Hitomi for decaying dark matter and forecasting leading sensitivity for XRISM
- Probing The Longest Dark Matter Lifetimes with the Line Emission Mapper
- Handling the Uncertainties in the Galactic Dark Matter Distribution for Particle Dark Matter Searches
- Status, Challenges and Directions in Indirect Dark Matter Searches
- A Universal Density Profile from Hierarchical Clustering
- A deep search for decaying dark matter with XMM-Newton blank-sky observations
- The dark matter profile of the Milky Way inferred from its circular velocity curve
- Constraining Light Dark Matter with Diffuse X-Ray and Gamma-Ray Observations
- HI4PI: A full-sky HI survey based on EBHIS and GASS
- A High Spectral Resolution Observation of the Soft X-ray Diffuse Background with Thermal Detectors
- Resolving the extragalactic hard X-ray background
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation