Speaker: Johan Samsing (NBIA)
Contact Information:
Title: Towards Probing the Origin of Individual Black Hole Mergers
Abstract: How and where do black hole mergers form in our Universe? After 10 years of GW science with LIGO/Virgo/Kagra, there still seems to be no direct indication of what the underlying astrophysical formation channels are. I will present ideas and ongoing work on how the formation environment can leave observable modulations in the gravitational waveform (GW), from which one can determine the origin of individual GW sources. I further illustrate how a future of strongly lensed GW sources has the potential to provide further insight into the GW source environment that is not possible to measure in any other way. This especially includes the proper motion of the GW source, which can be combined with line-of-sight acceleration measurements, from which one can reconstruct the full orbital trajectory of the GW source.
Visitor's room: 123
If you're not meeting in the visitor's office (Room 123), please indicate your office number.
Monday:
9:30 a.m.: Barak Rom
10:00 a.m.: Yoonsoo Kim
10:30 a.m.: (optionally astro-coffee)
11:00 a.m.: Christian Kragh Jespersen (023A)
11:30 a.m.: Rostom Mbarek
12:00 p.m.: Christian Kragh Jespersen
12:30 p.m.: Wunch
1:00 p.m.: Wunch
1:30 p.m.: Sylvia Biscoveanu
2:00 p.m.: Nils Siemonsen (123)
2:30 p.m.: Yixian Chen
3:00 p.m.: Teagan Clarke
3:30 p.m.: Neta Bahcall (137)
4:00 p.m.: Barak Rom
4:30 p.m.: Barak Rom
Day of week: Monday
Faculty Host: Neta Bahcall
Postdoc Host: Barak Rom
Christian Kragh Jespersen
Yixian Chen
Shaunak Modak
Yoonsoo Kim
Rostom Mbarek
Speaker
STUDENTS HAVE PRIORITY.
PLEASE NO MORE THAN 8 PEOPLE (it is more difficult to properly interact with the speaker in larger groups).