Energetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star
(2017)
Ultrahigh-energy cosmic rays from tidally-ignited white dwarfs
Physical Review D American Physical Society 96:10 (2017) 103003
Abstract:
Ultrahigh-energy cosmic rays (UHECRs) can be accelerated by tidal disruption events of stars by black holes. We suggest a novel mechanism for UHECR acceleration wherein white dwarfs (WDs) are tidally compressed by intermediate-mass black holes (IMBHs), leading to their ignition and subsequent explosion as a supernova. Cosmic rays accelerated by the supernova may receive an energy boost when crossing the accretion-powered jet. The rate of encounters between WDs and IMBHs can be relatively high, as the number of IMBHs may be substantially augmented once account is taken of their likely presence in dwarf galaxies. Here we show that this kind of tidal disruption event naturally provides an intermediate composition for the observed UHECRs, and suggest that dwarf galaxies and globular clusters are suitable sites for particle acceleration to ultrahigh energies.Paving the way to simultaneous multi-wavelength astronomy
New Astronomy Reviews Elsevier 79 (2017) 26-48
Radio Transients in the Era of Multi-Messenger Astrophysics
Proceedings of the International Astronomical Union Cambridge University Press (CUP) 14:S339 (2017) 207-214
The reverberation signatures of rotating disc winds in active galactic nuclei
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 471:4 (2017) 4798-4811