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- W3100556327 abstract "We study the non-radial oscillations of relativistic neutron stars, in particular the (fundamental) f-modes, which are believed to be the most relevant for the gravitational wave emission of perturbed isolated stars. The expected frequencies of the f-modes are compared to the sensitivity range of Mario Schenberg, the Brazilian gravitational wave spherical detector." @default.
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- W3100556327 date "2012-01-01" @default.
- W3100556327 modified "2023-09-26" @default.
- W3100556327 title "NON-RADIAL OSCILLATIONS OF NEUTRON STARS AND THE DETECTION OF GRAVITATIONAL WAVES" @default.
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- W3100556327 doi "https://doi.org/10.1142/s2010194512008185" @default.
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