Determining the Neutron Star Equation of State Using the Narrow-Band Gravitational Wave Detector Schenberg

Details Determining the Neutron Star Equation of State Using the Narrow-Band Gravitational Wave Detector Schenberg Determining the Neutron Star Equation of State Using the Narrow-Band Gravitational Wave Detector Schenberg

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mgm..conf.2416d&link_type=abstract

"THE ELEVENTH MARCEL GROSSMANN MEETING On Recent Developments in Theoretical and Experimental General Relativity, Gravitation an

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A new window to the Universe is about to be opened. With the detection of gravitational waves, astrophysicists expect to have the answer to many questions, as well as new ones. There are many detectors all around the world and, soon, even above us. With interferometric or resonant mass detectors, at low and high frequencies, we shall be able to see waves coming from coalescing binary systems, from a cosmological background, from catastrophic events etc...

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