Sensing the Undetected
Szabolcs Márka[1]
LIGO[2] Laboratory[3], California Institute of Technology, Pasadena, California, USA
Abstract
Interferometric
gravitational wave detectors are in their commissioning or construction phase in
North America, Europe, and Japan. Once completed, this worldwide network of
detectors will be capable of detecting gravitational waves with great detail and
sensitivity. Their long-term ambition reaches well beyond the first direct
detection of gravitational waves; they promise the dawn of a new field, the
gravitational wave astronomy. The majority of these detectors are complete
enough that running for extended periods is a routine exercise and short-term
scientific results are promised. In this talk, I will summarize the status of
the various detectors currently being developed with special emphasis on the
LIGO Project. I will also explain
the fundamental limiting factors and the scientific reach of these instruments,
outlining what gravitational-wave astronomy is likely to teach us about the
universe. I will also point out the potential future, and benefits of
collaboration amongst gravitational wave detectors.
[1] smarka@ligo.caltech.edu; phone 1 626 395 2005; www.ligo.caltech.edu/~smarka; Address: Szabolcs Márka, LIGO Laboratory, California Institute of Technology, MS 18-34, Pasadena, CA 91125, USA
[2] Detailed information about the Laser Interferometer Gravitational Wave Observatory (LIGO) is available at http://www.ligo.caltech.edu.
[3] Detailed information about the LIGO Scientific Collaboration (LSC) is available at http://www.ligo.org.