Journal
PHYSICAL REVIEW D
Volume 81, Issue 12, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.81.124023
Keywords
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Funding
- National Science Foundation [PHY-0803629, PHY-0653369, CCF-0832966, PHY-0803615, CCF-0833090, PHY-0803624, PHY-040027]
- NSERC
- Division Of Physics
- Direct For Mathematical & Physical Scien [0803615] Funding Source: National Science Foundation
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We study the evolution of magnetized and rigidly rotating neutron stars within a fully general relativistic implementation of ideal magnetohydrodynamics with no assumed symmetries in three spatial dimensions. The stars are modeled as rotating, magnetized polytropic stars, and we examine diverse scenarios to study their dynamics and stability properties. In particular, we concentrate on the stability of the stars and possible critical behavior. In addition to their intrinsic physical significance, we use these evolutions as further tests of our implementation, which incorporates new developments to handle magnetized systems.
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