Scientific Programme
Lectures
schedule
December 12th-16th 2016
Registration & Inaugural Session (12.12.2016) |
09:00 |
Lunch Break |
13:00 - 14:00 |
Coffee / Tea Break |
11:00 - 11:30 & 15:30 - 16:00 |
Tentative Lecture Schedules
09:30 - 11:00 |
11:30 - 13:00 |
14:00 - 15:30 |
16:00 - 17:00 |
|
12/12/2016 |
Lecture 1 (Raychaudhury) |
Lecture 1 (Ajith) |
Lecture 2 (Ajith) |
Discussions |
13/12/2016 |
Lecture 1 (Adhikari) |
Lecture 2 (Adhikari) |
Lecture 1 (Arun) |
Discussions |
14/12/2016 |
Lecture 2 (Arun) |
Lecture 3 (Adhikari) |
Lecture 3 (Ajith) |
Lecture 4 (Ajith) |
15/12/2016 |
Lecture 5 (Ajith) |
Lecture 4 (Adhikari) |
Lecture 3 (Arun) |
Lecture 4 (Arun) |
16/12/2016 |
Tutorial (Gupta) |
Tutorial (Gupta) |
Lecture 1 (Chatterjee) |
Closing Session |
Topics covereD
Binary Black Hole Physics: Modelling compact binary mergers: Overview, Basics of PN theory, PN structure of gravitational waveform, Physical effects encoded in gravitational waveforms, Testing strong-field gravity using gravitational waveforms (theoretical aspects), Astrophysical aspects of binary black holes as discovered by aLIGO
GW Data Analysis: Basics of GW theory, sources and detection, Basics of signal detection: Noise, stationary processes, power spectrum estimation, Maximum likelihood estimation, matched filtering, template banks, Bayesian inference: Parameter estimation, model selection, Real examples: Tests of general relativity, astrophysical model selection, neutron star equation of state
GW Instrumentation : Optical Response of Complex Interferometers, Major Noise Sources in Interferometers, The Quantum Rao Bound, Future Interferometers, Challenges for LIGO India
Tutorial : Dr. Anuradha Gupta (IUCAA)
GW Data Analysis: Basics of GW theory, sources and detection, Basics of signal detection: Noise, stationary processes, power spectrum estimation, Maximum likelihood estimation, matched filtering, template banks, Bayesian inference: Parameter estimation, model selection, Real examples: Tests of general relativity, astrophysical model selection, neutron star equation of state
GW Instrumentation : Optical Response of Complex Interferometers, Major Noise Sources in Interferometers, The Quantum Rao Bound, Future Interferometers, Challenges for LIGO India
Tutorial : Dr. Anuradha Gupta (IUCAA)