Non-Maxwellian electromagnetism in astrophysics
Space applications at low radio frequencies
(Sprache: Englisch)
The universe is largely observed with electromagnetic signals - supposedly Maxwellian - though the gravitational wave window was just unbarred. Meanwhile, cosmology is since long confronted with an universe for 96% dark and unknown. Thus, it is pertinent...
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The universe is largely observed with electromagnetic signals - supposedly Maxwellian - though the gravitational wave window was just unbarred. Meanwhile, cosmology is since long confronted with an universe for 96% dark and unknown. Thus, it is pertinent for fundamental physics to start a theoretical and experimental verification of electromagnetism, and its photon messenger. The study discusses nonMaxwellian theories, focusing on testable effects. We deal with a range of applications and assess how alternative electromagnetic theories are helpful. We revise the most notable theories, either non-linear or massive. In the former class, for analysis of the self-force, we consider the radiation of an uniformly accelerating Born-Infeld charge; in the Heisenberg-Euler theory, we find a frequency shift induced by an overcritical magnetic dipole, associated to a magnetar. Being the photon the only massless particle in the Standard Model (SM), we explore SM extensions.
Bibliographische Angaben
- Autor: Luca Bonetti
- 2018, 272 Seiten, Maße: 22 cm, Kartoniert (TB), Englisch
- Verlag: LAP Lambert Academic Publishing
- ISBN-10: 6137344118
- ISBN-13: 9786137344118
Sprache:
Englisch
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