
Fast radio bursts (FRBs) remain a puzzling phenomenon. Among many unsolved problems, there the a question of periodic activity observed for two sources of repeating bursts. This feature can be an important clue to understanding the physics of these enigmatic sources. Three main hypotheses to explain these 16-day and 160-day periods have been put forwards: orbital periodicity in a binary system; precession of a neutron star; and ultra-long spin. In this seminar, we confront these approaches, inviting three speakers who are proponents of the three competing approaches. We expect that the problem will be elucidated from these different points of view, accounting for all available pieces of information about FRBs. Since the speakers will present their views on these unsolved questions, we hope to have an interesting discussion.
Date: 12 April 2022
Time: 3:00pm CEST | 9:00am EDT | 9:00pm CST Asia
Webinar ID: 836 9329 2513
Webinar Secretariat: universe.webinar@mdpi.com
Cagliari Astronomical Observatory, INAF, Italy;
Graduated from the Astronomy Department of the Bologna University in 2000. Obtained a PhD in Astronomy there in 2003, with a thesis reporting the discovery of the first and only double pulsar system. Currently works as a researcher at the Cagliari Observatory of the National Institute for Astrophysics (INAF) in Italy.
Sternberg Astronomical Institute, Moscow State University, Russia;
Graduated from the Moscow State University in 1995. Obtained PhD there in 1998.
Currently works at the Sternberg Astronomical Institute.
Postdoc at the University of Padua (Italy) in 2002-2004.
Professor of the department of Physics, Moscow State University since 2017.