Extragalactic photon-ALP conversion at CTA energies
- Max-Planck-Inst. fur Physik, Munich (Germany)
- Max-Planck-Inst. fur Physik, Munich (Germany); SLAC National Accelerator Lab., Menlo Park, CA (United States)
Magnetic fields in extragalactic space between galaxy clusters may induce conversions between photons and axion-like particles (ALPs), thereby shielding the photons from absorption on the extragalactic background light. For TeV gamma rays, the oscillation length (losc) of the photon-ALP system becomes inevitably of the same order as the coherence length of the magnetic field l and the length over which the field changes significantly (transition length lt) due to refraction on background photons. We derive exact statistical evolution equations for the mean and variance of the photon and ALP transfer functions in the non-adiabatic regime (losc ~ l >> lt). We also make analytical predictions for the transfer functions in the quasi-adiabatic regime (losc <t). Our results are important in light of the upcoming Cherenkov Telescope Array (CTA), and may also be applied to models with non-zero ALP masses.
- Research Organization:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Organization:
- USDOE; German Research Foundation (DFG); European Union (EU)
- Grant/Contract Number:
- AC02-76SF00515; EXC 153; H2020-MSCAITN- 2015/674896-ELUSIVES
- OSTI ID:
- 1360940
- Report Number(s):
- SLAC-PUB-16842
- Journal Information:
- Journal of Cosmology and Astroparticle Physics, Vol. 2017, Issue 01; ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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