Dispersion by pulsars, magnetars, fast radio bursts and massive electromagnetism at very low radio frequencies

详细信息    查看全文

• 作者：Mark J. Bentum^a ; ^b ; ^{m.j.bentum@utwente.nl} ; Luca Bonetti^c ; ^d ; ^e ; ^{luca.bonetti@cnrs-orleans.fr} ; Alessandro D.A.M. Spallicci^c ; ^d ; ^e ; ^{spallicci@cnrs-orleans.fr} ;
• 关键词：Photons ; Radio astronomy ; Satellites ; Pulsars ; Magnetars ; Fast radio bursts
• 刊名：Advances in Space Research
• 出版年：2017
• 出版时间：15 January 2017
• 年：2017
• 卷：59
• 期：2
• 页码：736-747
• 全文大小：498 K
• 卷排序：59

文摘

Our 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 consensus, but are not mutually exclusive. Thus, we remind that for massive electromagnetism, dispersion goes as the inverse of the frequency squared. Thereby, new avenues are offered also by the recently operating ground observatories in 10–80 MHz domain and by the proposed Orbiting Low Frequency Antennas for Radio astronomy (OLFAR). The latter acts as a large aperture dish by employing a swarm of nano-satellites observing the sky for the first time in the 0.1–15 MHz spectrum. The swarm must be deployed sufficiently away from the ionosphere to avoid distorsions from terrestrial interference, especially during solar maxima, and offer stable conditions for calibration during observations.