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Seminario
""The Laser Interferometer Space Antenna""

Relatore: Michele Vallisneri- Caltec, LISA project

Sala Feynman
14 Settembre 2009 ore 15.30

Abstract
Space-based gravitational-wave detectors such as the planned NASA--ESA mission LISA target the low-frequency band between 0.1 mHz and 1 Hz. This band is populated by thousands of detectable astrophysical sources, which will enable many exciting investigations: exploring hierarchical galaxy formation scenarios, sampling the strong-field regime of general-relativistic dynamics, taking a census of Galactic compact binaries, characterizing the nature of the massive objects at galactic centers, and much more.