Secondary Production of Photons from ALP Dark Matter interacting with a Cosmological Magnetic Field
Abdias Aires, Robert Brandenberger, Ashu Kushwaha
astro-ph.CO, gr-qc, hep-ph, hep-th
Submitted: 2026-07-01
Comments: 6 pages
Project page: http://cajihare.github.io/AxionLimits
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Ultra-Light Dark Matter
- Wave Dark Matter
- Primordial magnetic fields from pseudo-Goldstone bosons
- Cosmological Magnetic Fields from Primordial Helicity
- New applications of the chiral anomaly
- Axions, Quantum Mechanical Pumping, and Primeval Magnetic Fields
- Primordial Magnetic Fields, Right Electrons, and the Abelian Anomaly
- Self-consistent evolution of magnetic fields and chiral asymmetry in the early Universe
- Cosmological Magnetic Fields from Ultralight Dark Matter
- Photon Production of Axionic Cold Dark Matter
- Could primordial galactic Magnetic Fields be generated by Charged Ultra-Light Boson Dark Matter?
- N-flationary magnetic fields
- Can slow roll inflation induce relevant helical magnetic fields?
- Consistent generation of magnetic fields in axion inflation models
- Magnetogenesis from axion inflation
- Suppressed Magnetogenesis from Ultralight Dark Matter due to Finite Conductivity
- Parametric Resonance and Backreaction Effects in Magnetogenesis from Ultralight Dark Matter
- Late Time Magnetogenesis from Ultralight Scalar Dark Matter
- Indirect Parametric Resonance of the Electromagnetic Field Driven by an Oscillating SU(2) Dark Matter Condensate
- Direct Collapse Supermassive Black Holes from Ultralight Dark Matter
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