Evolutions of Magnetized Neutron Stars

Details Evolutions of Magnetized Neutron Stars Evolutions of Magnetized Neutron Stars

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aps..aprt11005l&link_type=abstract

American Physical Society, 2009 APS April Meeting, May 2-5, 2009, abstract #T11.005

Physics

Scientific paper

Magnetized neutron stars, whether considered individually or within compact binary systems, demonstrate a number of interesting dynamical effects and may represent an important source of observable gravitational waves. In addition, isolated, rotating, magnetized stars serve as a good testbed for a necessarily complex, distributed adaptive mesh refinement (AMR) code. As initial data, we use fully consistent, magnetized, rotating stellar configurations generated with the Lorene toolkit. Here results are presented which (i) demonstrate convergence and stability of the code, (ii) show the evolution of stable and unstable magnetized stars, and (iii) study the effects of a scheme to track the leakage of neutrinos.

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