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DTSTART;TZID=Atlantic/Canary:20180904T123000
DTEND;TZID=Atlantic/Canary:20180904T133000
UID:iactalks-1188
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/1188
CREATED:2018-09-04T12:30:00+01:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:Non-Maxwellian electromagnetism in astrophysics and cosmology
DESCRIPTION:Non-Maxwellian electromagnetism in astrophysics and cosmology\n
 Dr. Alessandro D.A.M. Spallicci\n\nInexplicable observations on the Univer
 se prompt cosmologists to propose either ad hoc explanationsas dark matter
  and energy maintaining general relativity entirely valid, or to propose a
 lternatives togeneral relativity, without evoking dark ingredients [7]. Bu
 t for the former investigation track,experimental confirmations are missin
 g, and for the latter general relativity continues to predictobservations 
 with exactitude.Confronted with this dichotomy, and with a multi-parametri
 sed cosmology, we consider legitimate alsoto investigate on the nature of 
 the main messenger from the Universe, light, that we stick so far tointerp
 ret as Maxwellian. But the photon in the Standard Model singles out as the
  only massless freeparticle, and the waves emerge from a linear theory of 
 the XIX century. What if light were to bedescribed by a different theory?R
 esults on testing non-Maxwellian electromagnetism (either massive initiate
 d by de Broglie and Procaor non-linear by Born and Infeld, Heisenberg and 
 Euler) include setting photon mass upper limits fromthe modified Amp&egrav
 e;re law in solar wind through the Cluster spacecraft [8], or from frequen
 cy dependentgroup velocities of photons from Fast Radio Bursts [2,5]. Futu
 re nanosatellite swarms operating in anew radio-astronomy window, 10 KHz -
  10 MHz, [1] might provide a significant contribution.De Broglie formulate
 d a photon mass already in 1922 and in the later year he estimated such ma
 ss to belower than 10 -53 kg, surprisingly close to the actual limits esta
 blished by the Particle Data Group.Meanwhile, an effective photon mass eme
 rges when Lorentz symmetry is broken in (possibly Super-Symmetrised) Stand
 ard Model Extensions, as well as bi-refringence and dissipation [3,4].Non-
 linear effects as polarisation dependent frequency shifts in strong magnet
 ic field in Magnetars havebeen analysed too [6], but we are now progressin
 g in modelling a general non-linear electromagnetismLagrangian and look wh
 ether wave dissipation in vacuum may occur, possibly in presence of abackg
 round field. When wave dissipation is transferred into photon energy descr
 iption, we cannot avoidconsidering, additional, non-cosmological redshifts
 .\n&nbsp;\n[1] Bentum M.J., Bonetti L., Spallicci A.D.A.M., 2017. Adv. Sp.
  Res., 59, 736.[2] Bonetti L., Ellis J., Mavromatos N.E., Sakharov A.S., S
 arkisyan-Grinbaum E.K.G., Spallicci A.D.A.M., 2016. Phys. Lett.B, 757, 548
 .[3] Bonetti L., dos Santos Filho L.R., Helay&euml;l-Neto J.A., Spallicci 
 A.D.A.M., 2017. Phys. Lett. B, 764, 203.[4] Bonetti L., dos Santos Filho L
 .R., Helay&euml;l-Neto J.A., Spallicci A.D.A.M., 2017. arXiv:1709.04995[5]
  Bonetti L., Ellis J., Mavromatos N.E., Sakharov A.S., Sarkisyan-Grinbaum 
 E.K.G., Spallicci A.D.A.M., 2017. Phys. Lett.B, 768, 326.[6] Bonetti L., P
 erez Bergliaffa S.E., Spallicci A.D.A.M., 2017, 14 th Marcel Grossmann Mee
 ting, 12-18 July 2015 Roma, M.Bianchi, R.T. Jantzen, R. Ruffini Eds., Worl
 d Scientific, 3531.[7] Capozziello S., Prokopec T., Spallicci A.D.A.M., 20
 17. Aims and Scopes of the Special Issue: Foundations of Astrophysicsand C
 osmology, Volume 47, Issue 6.[8] Retin&ograve; A., Spallicci A.D.A.M., Vai
 vads A., 2016. Astropart. Phys., 82, 49.
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