Seismic and dynamical solar models i-the impact of the solar rotation history on neutrinos and seismic indicators

Understand

Solar activity and helioseismology show the limitation of the standard solar model and call for the inclusion of dynamical processes in both convective and radiative zones.

• We concentrate here on the radiative zone and first show the sensitivity of boron neutrinos to the microscopic physics included in solar models.
• We confront the neutrino predictions of the seismic model to all the detected neutrino fluxes.
• Then we compute new models of the Sun including a detailed transport of angular momentum and chemicals due to internal rotation that includes meridional circulation and shear induced turbulence.