2023
DOI: 10.1103/physrevd.108.043033
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Astrophysically sourced quantum coherent photonic signals

Arjun Berera,
Jaime Calderón-Figueroa,
Liang Chen
et al.
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“…In ref. [24], the cross section for the elastic scattering of two axions due to self-interactions is given by σ SI ≈ 8πm a /(32πf 2 a ) for the conventional axion potential, while the stimulated emission cross section is calculated in [25] with the result as σ SE ∼ (λ 0 /2π) 2 (λ 0 /τ a ), where λ 0 denotes the wavelength of the incident photon and τ a as the axion lifetime. As JCAP05(2024)132 a consequence, the ratio of these two cross sections is σ SI /σ SE ∼ 10 −47 with benchmark parameter values.…”
Section: Jcap05(2024)132mentioning
confidence: 99%
“…In ref. [24], the cross section for the elastic scattering of two axions due to self-interactions is given by σ SI ≈ 8πm a /(32πf 2 a ) for the conventional axion potential, while the stimulated emission cross section is calculated in [25] with the result as σ SE ∼ (λ 0 /2π) 2 (λ 0 /τ a ), where λ 0 denotes the wavelength of the incident photon and τ a as the axion lifetime. As JCAP05(2024)132 a consequence, the ratio of these two cross sections is σ SI /σ SE ∼ 10 −47 with benchmark parameter values.…”
Section: Jcap05(2024)132mentioning
confidence: 99%