# Antisolar differential rotation of slowly rotating cool stars

@inproceedings{Rudiger2019AntisolarDR,
title={Antisolar differential rotation of slowly rotating cool stars},
author={Guenther Rudiger and Manfred Kuker and Petri J. K{\"a}pyl{\"a} and Klauss G. Strassmeier},
year={2019}
}
It is well-known that rotating stellar convection transports angular momentum equatorward while a thermal energy flows poleward producing warm poles. The characteristic equatorial acceleration of the solar rotation law is a consequence of these phenomena. New numerical box simulations confirm the cross correlations $\langle u_r u_\theta\rangle$ and $\langle u_\theta u_\phi\rangle$ to be anticorrelated but their signs prove to be different for slow and fast rotation. The explanation is that… CONTINUE READING

## Differential rotation and stellar convection. Sun and the solar stars

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