The inverse problem for pulsating neutron stars: a 'fingerprint analysis' for the supranuclear equation of state
Kokkotas, K.D., Apostolatos, T.A. and Andersson, N. (2001) The inverse problem for pulsating neutron stars: a 'fingerprint analysis' for the supranuclear equation of state. Monthly Notices of the Royal Astronomical Society, 320, (3), 307-315. (doi:10.1046/j.1365-8711.2001.03945.x).
Full text not available from this repository.
We study the problem of detecting, and inferring astrophysical information from, gravitational waves from a pulsating neutron star. We show that the fluid f and p modes, as well as the gravitational-wave w modes, may be detectable from sources in our own Galaxy, and investigate how accurately the frequencies and damping rates of these modes can be inferred from a noisy gravitational-wave data stream. Based on the conclusions of this discussion we propose a strategy for revealing the supranuclear equation of state using the neutron star fingerprints: the observed frequencies of an f and a p mode. We also discuss how well the source can be located in the sky using observations with several detectors.
|Subjects:||Q Science > QB Astronomy
Q Science > QA Mathematics
Q Science > QC Physics
|Divisions:||University Structure - Pre August 2011 > School of Mathematics > Applied Mathematics
|Date Deposited:||12 May 2006|
|Last Modified:||27 Mar 2014 18:17|
|RDF:||RDF+N-Triples, RDF+N3, RDF+XML, Browse.|
Actions (login required)