Bulletin of the American Physical Society
APS April Meeting 2020
Volume 65, Number 2
Saturday–Tuesday, April 18–21, 2020; Washington D.C.
Session L03: Fast Radio Bursts and Tidal Disruption EventsInvited Live
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Sponsoring Units: DAP Chair: Yuri Levin, Columbia University Room: Washington 2 |
Sunday, April 19, 2020 3:30PM - 4:06PM Live |
L03.00001: The Burgeoning Role of Tidal Disruption Events as Tools for Black Hole Astrophysics Invited Speaker: Sjoert Van Velzen |
Sunday, April 19, 2020 4:06PM - 4:42PM Live |
L03.00002: A Synoptic View of Fast Radio Bursts with CHIME Invited Speaker: Kiyoshi Masui The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is the only radio telescope capable of instantaneously observing hundreds of square degrees with the sensitivity of a 100-meter scale aperture. As a result, its transient search instrument, CHIME/FRB, has detected roughly 700 fast radio bursts (FRBs) in its first year of full operations---increasing the known sample by an order of magnitude. CHIME/FRB thus represents a new era in the study of these enigmatic, extragalactic radio flashes and presents opportunities to use them as probes of the Universe. I will show how CHIME's novel, digitally-driven design, coupled with the availability of mass-produced analogue and digital hardware, has enabled this leap in telescope capabilities. I will then give an overview of CHIME/FRB's most recent results and conclude by describing efforts to augment CHIME's capabilities by adding outrigger telescopes. These outriggers will be located across the continent and will precisely localize FRB sources using very long baseline interferometry. [Preview Abstract] |
Sunday, April 19, 2020 4:42PM - 5:18PM Live |
L03.00003: FRBs and Neutron Stars Invited Speaker: Andrei Beloborodov Cosmological fast radio bursts (FRBs) have ultra-high luminosities (billion times brighter than the sun) and short (millisecond) durations. Their origin is not established. A popular scenario invokes magnetized neutron stars as FRB engines. This talk will discuss FRB physics in this scenario and some general questions regarding propagation of ultra-strong electromagnetic waves through plasma. [Preview Abstract] |
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