2017
DOI: 10.1016/j.asr.2016.10.018
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Dispersion by pulsars, magnetars, fast radio bursts and massive electromagnetism at very low radio frequencies

Abstract: International audienceOur understanding of the universe relies mostly on electromagnetism. As photons are the messengers, fundamental physics is concerned in testing their properties. Photon mass upper limits have been earlier set through pulsar observations, but new investigations are offered by the excess of dispersion measure (DM), sometimes observed with pulsar and magnetar data at low frequencies, or with the fast radio bursts (FRBs), of yet unknown origin. Arguments for the excess of DM do not reach a co… Show more

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Cited by 33 publications
(32 citation statements)
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“…Thirdly, the massive photon group velocity differs from c by a quantity proportional to the inverse of the frequency squared [9][10][11]23]. Such a dependence has been analysed recently with the signals from Fast Radio Bursts (FRBs) [79][80][81][82][83][84][85][86][87][88].…”
Section: Time Dilation and Supernovaementioning
confidence: 99%
“…Thirdly, the massive photon group velocity differs from c by a quantity proportional to the inverse of the frequency squared [9][10][11]23]. Such a dependence has been analysed recently with the signals from Fast Radio Bursts (FRBs) [79][80][81][82][83][84][85][86][87][88].…”
Section: Time Dilation and Supernovaementioning
confidence: 99%
“…Here n is average electron density along the line-ofsight, m e and e is the mass and charge of the electron. Equation (5) also implies that higher frequency radio photons pass through the ISM faster than lower frequency ones (see e.g., Bentum et al 2016). …”
Section: Velocity Dispersion From the Plasma Effectmentioning
confidence: 99%
“…Thereby, the photons emitted towards the end of the burst will employ more time than the initial photons to reach an observer. Incidentally, the dependence of the group velocity on the frequency allows us to set upper limits on the photon mass from Fast Radio Bursts (FRBs) [19][20][21][22][23].…”
Section: Conclusion Discussion and Perspectivesmentioning
confidence: 99%