Modeling the Electromagnetic and Gravitational Radiation from Neutron Stars

Details Modeling the Electromagnetic and Gravitational Radiation from Neutron Stars Modeling the Electromagnetic and Gravitational Radiation from Neutron Stars

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aps..apr.g8007l&link_type=abstract

American Physical Society, APS April Meeting 2012, March 31-Apr 3, 2012, abstract #G8.007

Physics

Scientific paper

The dynamics of magnetized neutron stars both in binaries and in isolation are modeled with a novel numerical approach able to capture the dynamics of the star(s) and of the surrounding plasma. The stellar dynamics incorporate ideal MHD which appropriately models the regime in which the fluid pressure dominates that of the magnetic field, while the stellar exterior is modeled within the force free approach (magnetic pressure largely dominates that of the fluid). The approach is shown to approach certain known solutions. An intense electromagnetic outburst is observed for the collapsing, rotating star. The approach is also applied to the coalescence of a neutron star binary.

Affiliated with

Also associated with

No associations

Rating

Modeling the Electromagnetic and Gravitational Radiation from Neutron Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Modeling the Electromagnetic and Gravitational Radiation from Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling the Electromagnetic and Gravitational Radiation from Neutron Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1366026