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Modelling magnetically deformed neutron stars · Around

2007

Modelling magnetically deformed neutron stars

Haskell, B., Samuelsson, L., Glampedakis, K. et al.

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Rotating deformed neutron stars are important potential sources for groundbased gravitational-wave interferometers such as LIGO, GE0600 and VIRGO.

One mechanism that may lead to significant non-asymmetries is the internal magnetic field.
It is well known that a magnetic star will not be spherical and, if the magnetic axis is not aligned with the spin axis, the deformation will lead to the emission of gravitational waves.
The aim of this paper is to develop a formalism that would allow us to model magnetically deformed stars, using both realistic equations of state and field configurations.

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