Abstract
The LIGO interferometers are operating as gravitational wave observatories, with a noise level near an order of magnitude of the goal and the first scientific data recently taken. This data has been analyzed for four different categories of gravitational wave sources; millisecond bursts, inspiralling binary neutron stars, periodic waves from a known pulsar, and stochastic background. Research and development is also underway for the next generation LIGO detector, Advanced LIGO.
Original language | English |
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Title of host publication | The Tenth Marcel Grossmann Meeting |
Subtitle of host publication | On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories |
Publisher | World Scientific Publishing Co. |
Pages | 308-336 |
Number of pages | 29 |
Volume | 1 |
ISBN (Electronic) | 9789812704030 |
ISBN (Print) | 9789812566676 |
DOIs | |
State | Published - 1 Jan 2006 |
Bibliographical note
Publisher Copyright:© 2005 by World Scientific Publishing Co. Pte. Ltd. All rights reserved.