Equations for polar perturbations of slowly rotating neutron stars in a new Gauge

Details Equations for polar perturbations of slowly rotating neutron stars in a new Gauge Equations for polar perturbations of slowly rotating neutron stars in a new Gauge

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hell.confe.128s&link_type=abstract

"5th Hellenic Astronomical Conference, held 20-22 September, 2001 in Crete, Greece. Online at http://www.astro.auth.gr/elaset/he

Astronomy and Astrophysics

Astronomy

Scientific paper

Perturbation equations for slowly rotating relativistic stars were studied until now, in Regge Wheeler Gauge which is good for the axial part of the perturbations. For the polar part of the perturbations though the equations are quite complicated and not straightforward to write them in first order system, suitable for time evolutions. With the new Gauge the polar perturbation equations are much simpler and the trasformation to first order system is very easy.

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