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Gravitational Waves: a new window to observe the Universe

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• Current bar detec<strong>to</strong>rs will see gravitational waves if <strong>the</strong>re is<br />

ano<strong>the</strong>r supernova in <strong>the</strong> Galaxy<br />

• Advanced LIGO and VIRGO will probably detect gravitational<br />

waves and may begin <strong>to</strong> do astronomy on compact binaries or<br />

pulsars<br />

• LISA will:<br />

Conclusions<br />

Detect gravitational waves from known sources<br />

Survey all NS-NS binaries in <strong>the</strong> Galaxy<br />

Determine WD-WD statistics <strong>to</strong> inform common-envelope<br />

evolution studies<br />

See mergers of massive black holes in galactic nuclei and<br />

inform models of hierarchal galaxy formation and evolution<br />

Map out <strong>the</strong> field of a black hole (“seeing a black hole”)<br />

Test GR in <strong>the</strong> strong field regime

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