Speaker
Mr
Андрей Юдин
(ИТЭФ)
Description
We show that the unusual thermodynamic properties of matter within the region of twophase coexistence in hybrid stars result in a change of the standard condition for beginning of convection. In particular, the thermal flux transported by convection may be directed towards the stellar center in this region. We consider favourable circumstances leading to such an effect of "inverse convection" and its influence on the thermal evolution of hybrid stars.
