Long-term evolution of compact-object magnetic fields and ellipticity
Characterize the long-term evolution of compact-object magnetic fields and ellipticities, including the effects of magnetic-field decay and ellipticity evolution on continuous-gravitational-wave detectability and inferred birth magnetic-field distributions.
References
These constraints are conditional on assuming a fixed stellar ellipticity and a fixed magnetic-field decay timescale. However, long-term evolution of both quantities remains poorly understood, and different assumptions could modify the inferred birth magnetic field distribution.
The distribution of ellipticities of compact objects remains uncertain.
Several physical processes can contribute to magnetic-field decay, including Ohmic diffusion, Hall drift, and ambipolar diffusion \citep{GoldreichReisenegger1992,Xie2019TheEM} although estimates of the characteristic decay timescales remain uncertain \citep{Sang1987}.