What is LIGO ?

LIGO (the Laser Interferometer Gravitational-Wave Observatory) is a cutting-edge project to detect gravitational waves directly for the first time. These waves, predicted by Einstein's general theory of relativity, are emitted when matter moves in certain ways; in a sense they are the "echo" of a rapidly-changing gravitational field. Black holes and neutron stars are expected to emit gravitational waves when they orbit closely, merge, or are perturbed; collapsing massive stars and possibly other astrophysical sources should also emit gravitational waves through a number of physical mechanisms that have been modeled but not yet confirmed. Upgrades to the three LIGO detectors in the U.S. and its sister detectors Virgo and GEO600 in Europe, currently in progress, will reach sensitivity levels at which gravitational-wave signals are expected to be detected regularly. Measurements of the waves themselves will also determine their properties (polarization components, etc.) and thereby test the theory of general relativity. LIGO thus sits at the interface between physics and astronomy, and between experiment and theory.

University of Maryland physicists, including professors Peter Shawhan (in the Gravitation Experiment group) and Alessandra Buonanno (in the Gravitation Theory group) plus postdocs and students, are active members of the LIGO Scientific Collaboration, especially in the areas of analyzing the data to search for and interpret "burst" and "inspiral" signals.

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A few selected papers