Numerical Backreaction and Finite-Time Energy Transfer in Post-Recombination Magnetogenesis from Ultralight Dark Matter
Aviv David, Robert Brandenberger
McGill · McGill
hep-ph, astro-ph.CO, gr-qc, hep-th
Submitted: 2026-07-22
Comments: 13 pages, 9 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- 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?
- 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
- Suppressed Magnetogenesis from Ultralight Dark Matter due to Finite Conductivity
- Primordial magnetic fields from pseudo-Goldstone bosons
- Cosmological Magnetic Fields from Primordial Helicity
- N-flationary magnetic fields
- Can slow roll inflation induce relevant helical magnetic fields?
- Consistent generation of magnetic fields in axion inflation models
- 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
- Universe Reheating after Inflation
- Reheating after Inflation
- Towards the Theory of Reheating After Inflation
- Inflaton Decay and Heavy Particle Production with Negative Coupling
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