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Relevance of photon-photon dispersion within the jet for blazar axionlike particle searches

Abstract:
Axionlike particles (ALPs) could mix with photons in the presence of astrophysical magnetic fields. Searching for this effect in gamma-ray observations of blazars has provided some of the strongest constraints on ALP parameter space so far. Previously, photon-photon dispersion of gamma rays off of the cosmic microwave background has been shown to be important for these calculations and is universally included in ALP-photon mixing models. Here, we assess the effects of dispersion off of other photon fields within the blazar (produced by the accretion disk, the broad line region, the dust torus, starlight, and the synchrotron field) by modeling the jet and fields of the flat spectrum radio quasar 3C454.3 and propagating ALPs through the model both with and without the full dispersion calculation. We find that the full dispersion calculation can strongly affect the mixing, particularly at energies above 100 GeV—often reducing the ALP-photon conversion probability. This could have implications for future searches planned with, e.g., the Cherenkov Telescope Array, particularly those looking for a reduced opacity of the Universe at the highest energies.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1103/PhysRevD.105.023017

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Exeter College
Role:
Author
ORCID:
0000-0002-9975-1829


More from this funder
Grant:
ST/W508019/1
ST/S002952/1
ST/L006499/1
ST/V006355/1
ST/M00757X/1
ST/S002618/1
ST/V001477/1


Publisher:
American Physical Society
Journal:
Physical Review D More from this journal
Volume:
105
Issue:
2
Article number:
023017
Publication date:
2022-01-18
Acceptance date:
2021-12-14
DOI:
EISSN:
2470-0029
ISSN:
2470-0010


Language:
English
Keywords:
Pubs id:
1240348
Local pid:
pubs:1240348
Deposit date:
2022-04-28

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