Expand description
Helpers for dark photon (γ ↔ A’) conversion in the narrow-width approximation.
The canonical way to model γ ↔ A’ resonant conversion in the PDE solver is
crate::energy_injection::InjectionScenario::DarkPhotonResonance, which
takes (ε, m_{A’}) and internally calls gamma_con / resonance_redshift
to install the impulsive depletion
Δn(x) = -[1 - exp(-γ_con/x)] × n_pl(x) at z_start = z_res.
The 1/x factor in that IC captures the frequency dependence of the conversion probability P(x) ∝ 1/ω for ultrarelativistic photons.
References:
- Mirizzi, Redondo & Sigl (2009), JCAP 0903, 026
- Chluba, Cyr & Johnson (2024), MNRAS 535, 1874
- Arsenadze et al. (2025), JHEP 03, 018
Functions§
- dln_
omega_ pl_ sq_ dlna - |d ln ω_pl² / d ln a| at redshift
z. Centered finite difference in z. - gamma_
con - NWA dark-photon conversion parameter γ_con (dimensionless).
- plasma_
frequency_ ev - Photon plasma frequency ω_pl (in eV) at redshift
z. - resonance_
redshift - Resonance redshift
z_reswhere ω_pl(z_res) = m.