Scientific Colloquium
November 16, 2022, 3:00 P.M.
**** PLEASE NOTE
SPECIAL LOCATION****
Building 8, Hinners
Auditorium
RAFFAELLA
MARGUTTI
UNIVERSITY OF CALIFORNIA
BERKELEY
"Mining the Transient Sky in
the Era of Time Domain Multi-Messenger Investigations"
Astronomical transients are
signposts of catastrophic events in space, including the most
extreme stellar deaths, stellar tidal disruptions by
supermassive black holes, and mergers of compact objects. Thanks
to new and improved observational facilities we can now sample
the night sky with unprecedented temporal cadence and
sensitivity across the electromagnetic spectrum and beyond. This
effort has led to the discovery of new types of astronomical
transients, revolutionized our understanding of phenomena that
we thought we already knew, and enabled the first insights into
the physics of neutron star mergers with gravitational waves and
light. In this talk I will review some very recent developments
that resulted from our capability to acquire a truly
panchromatic view of transient astrophysical phenomena. I will
focus on two key areas of ignorance in the field: (i) What are
the progenitors of stellar explosions and what happens in the
last centuries before death? (ii) What is the nature of the
compact objects produced by these explosions and what happens
when compact objects merge? The unique combination of Discovery
Power (guaranteed by planned transient surveys across the
electromagnetic spectrum, combined with efforts in the realm of
artificial intelligence) and Understanding (enabled by
multi-messenger observations) is what positions time-domain
astrophysics for major advances in the near future.
About the Speaker:
Raffaella Margutti received her undergraduate degree in
Astrophysics in 2006 (magna cum laude), and her PhD in Physics
and Astronomy from the University of Milano Bicocca in 2010.
Margutti is a Sloan Fellow in Physics (2019), a CIFAR global
scholar in Gravity and the Extreme Universe (2019), and received
the 2022 New Horizons in Physics Prize for leadership in laying
foundations for electromagnetic observations of sources of
gravitational waves, and leadership in extracting rich
information from the first observed collision of two neutron
stars.
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