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      Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light

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      Nature Photonics

      Springer Science and Business Media LLC

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          Quantum-mechanical noise in an interferometer

           Carlton Caves (1981)
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            LIGO: The Laser Interferometer Gravitational-Wave Observatory.

            The goal of the Laser Interferometer Gravitational-Wave Observatory (LIGO) Project is to detect and study astrophysical gravitational waves and use data from them for research in physics and astronomy. LIGO will support studies concerning the nature and nonlinear dynamics of gravity, the structures of black holes, and the equation of state of nuclear matter. It will also measure the masses, birth rates, collisions, and distributions of black holes and neutron stars in the universe and probe the cores of supernovae and the very early universe. The technology for LIGO has been developed during the past 20 years. Construction will begin in 1992, and under the present schedule, LIGO's gravitational-wave searches will begin in 1998.
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              Advanced LIGO: the next generation of gravitational wave detectors

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                Author and article information

                Journal
                Nature Photonics
                Nature Photon
                Springer Science and Business Media LLC
                1749-4885
                1749-4893
                August 2013
                July 21 2013
                August 2013
                : 7
                : 8
                : 613-619
                10.1038/nphoton.2013.177
                © 2013

                http://www.springer.com/tdm

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