Michele Vallisneri (Caltech/JPL, IPhT)
The detection of gravitational waves (GWs) with ground-based interferometers opened a revolutionary vista on the Universe, upending our notions about the origin of stellar-mass black holes, and offering a spectacular multimessenger view of a binary neutron-star merger and of the ensuing radiation across the electromagnetic band.
From a fundamental-physics standpoint, GWs provide experimental access to the strong-field regime of general relativity and to precision tests of modified gravity.
This whirlwind tour of GW science is meant to give theoretical physicists and non-GW astrophysicists an appreciation of current topics of GW research, as well as an entry point to connect their work with GW applications or observations.
The five lectures will cover:
- GW propagation and detection
- GW generation and waveform models
- Astrophysical GW sources, with focus on the LIGO-Virgo catalog
- GW data analysis, with focus on tests of GR
- Cosmology and cosmography with GWs