{ "id": "1803.07298", "version": "v1", "published": "2018-03-20T08:43:30.000Z", "updated": "2018-03-20T08:43:30.000Z", "title": "Robust Limits on Photon Mass from Statistical Samples of Extragalactic Radio Pulsars", "authors": [ "Jun-Jie Wei", "Xue-Feng Wu" ], "comment": "6 pages, 4 figures, 1 table", "categories": [ "astro-ph.HE", "astro-ph.CO", "gr-qc", "hep-ph" ], "abstract": "The photon zero-mass hypothesis has been investigated for a long time using the frequency-dependent time delays of radio emissions from astrophysical sources. However, the search for a rest mass of the photon has been hindered by the similarity between the frequency-dependent dispersions due to the plasma and nonzero photon mass effects. Here we propose a new method through which the degeneracy of these two effects can be alleviated, by fitting a combination of the dispersion measures of radio sources. This allows us to simultaneously establish a robust limit on the photon mass. Using the observed dispersion measures from two statistical samples of extragalactic pulsars, we show that at the 68\\% confidence level, the constraints on the photon mass can be as low as $m_{\\gamma}\\leq1.5\\times10^{-48}~\\rm kg\\simeq8.4\\times10^{-13}~{\\rm eV}/c^{2}$ for the sample of 22 radio pulsars in the Large Magellanic Cloud and $m_{\\gamma}\\leq1.6\\times10^{-48}~\\rm kg\\simeq8.8\\times10^{-13} {\\rm eV}/c^{2}$ for the other sample of 5 radio pulsars in the Small Magellanic Cloud, which are a factor of $\\sim1$ better than that obtained by a single extragalactic pulsar. Furthermore, the method presented here can also be used when more fast radio bursts with known redshifts are detected in the future.", "revisions": [ { "version": "v1", "updated": "2018-03-20T08:43:30.000Z" } ], "analyses": { "keywords": [ "extragalactic radio pulsars", "robust limit", "statistical samples", "nonzero photon mass effects", "dispersion measures" ], "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable" } } }