{ "id": "1605.01043", "version": "v1", "published": "2016-05-03T19:44:50.000Z", "updated": "2016-05-03T19:44:50.000Z", "title": "Searches for Axion-Like Particles with NGC1275: Observation of Spectral Modulations", "authors": [ "Marcus Berg", "Joseph P. Conlon", "Francesca Day", "Nicholas Jennings", "Sven Krippendorf", "Andrew J. Powell", "Markus Rummel" ], "comment": "37 pages, 17 figures", "categories": [ "astro-ph.HE", "hep-ph" ], "abstract": "Axion-like particles (ALPs) can induce localised O(10%) oscillatory modulations in the spectra of photon sources passing through astrophysical magnetic fields. Ultra-deep Chandra observations of the Perseus cluster contain over $5 \\times 10^5$ counts from the central NGC1275 AGN and represent a dataset of extraordinary quality for ALP searches. We use these to search for X-ray spectral irregularities from the AGN. The absence of irregularities at the O(30%) level allows us to place leading constraints on the ALP-photon mixing parameter $g_{a\\gamma\\gamma} \\lesssim 1.5 - 5.4 \\times 10^{-12} {\\rm GeV}^{-1}$ for $m_a \\lesssim 10^{-12}$eV, depending on assumptions on the magnetic field realisation along the line of sight. At O(10%) level two modulations are present at high statistical significance, an excess in the 2-2.2 keV region and a deficit at 3.4-3.5 keV. We are unable to account for these through conventional instrumental or astrophysical processes and, interpreted as a signal, they would correspond to an ALP-photon coupling in the range $g_{a \\gamma \\gamma} \\sim 1-5 \\times 10^{-12} {\\rm GeV}^{-1}$.", "revisions": [ { "version": "v1", "updated": "2016-05-03T19:44:50.000Z" } ], "analyses": { "keywords": [ "axion-like particles", "spectral modulations", "x-ray spectral irregularities", "magnetic field realisation", "central ngc1275 agn" ], "note": { "typesetting": "TeX", "pages": 37, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1454386 } } }