Conveners
Plenary: Gravitational Wave
- Chang Sub Shin (Institute for Basic Science)
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Prof. A. Gopakumar (Tata Institute of Fundamental Research, Mumbai)14/06/2023, 11:00
Supermassive Black Holes (SMBHs) thrive at the centres of massive galaxies and galaxy mergers
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can lead to SMBH binaries with orbital periods of years. Such systems emit nano-hertz
gravitational waves (GWs) which can be detected by employing networks of precisely
timed milli-second pulsars.
The rapidly maturing Pulsar Timing Arrays like NANOGrav, EPTA, InPTA, CPTA and PPTA, are... -
Tjonnie Li (KU Leuven)14/06/2023, 11:30
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Myungshin Im (Seoul National University)14/06/2023, 12:00Plenary invited
The 2017 detection of the binary neutron star (BNS) merger event in both gravitational wave (GW) and electromagnetic wave (EM), GW170817, has shown the great potential for multi-messenger astronomy, allowing us to understand the link between neutron star mergers and gamma-ray bursts, physical mechanisms and environments of the EM counterpart, kilonova (KN), and cosmology with GW sources. Yet,...
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