Anisotropic convection in rotating proto-neutron stars

@article{Miralles2004AnisotropicCI,
  title={Anisotropic convection in rotating proto-neutron stars},
  author={J. A. Miralles and Jos{\'e} A. Pons and Vadim A. Urpin},
  journal={arXiv: Astrophysics},
  year={2004}
}
We study the conditions for convective instability in rotating, non-magnetic proto--neutron stars. The criteria that determine stability of nascent neutron stars are analogous to the Solberg--Hoiland conditions but including the presence of lepton gradients. Our results show that, for standard angular velocity profiles, convectively unstable modes with wave-vectors parallel to the rotation axis are suppressed by a stable angular momentum profile, while unstable modes with wave-vectors… Expand

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