[en] Solar evolutionary models are thus far unable to reproduce spectroscopic, helioseismic and neutrino constraints consistently, resulting in the so-called solar modeling problem. In parallel, planet formation models predict that the evolving composition of the protosolar disk, and thus, of the accreted gas by the proto-Sun must have been variable. In this talk, we show that solar evolutionary models including a realistic planet formation scenario lead to an increased core metallicity of up to 5%, implying that accurate neutrino flux measurements are sensitive to the initial stages of the formation of the Solar System. We demonstrate that in addition to macroscopic transport and increased opacities at the base of the convective envelope, the formation history of the Solar System constitutes a key element to resolve the current crisis of solar models.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Kunitomo, Masanobu; Department of Physics, Kurume University, Kurume, Japan
Guillot, Tristan; Laboratoire Lagrange, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Nice cedex 4, France
Buldgen, Gaël ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie ; Département d'Astronomie, Université de Genève, Versoix, Switzerland
Language :
English
Title :
Solar neutrino fluxes show the signature of planet formation processes
Publication date :
2023
Event name :
The 21st Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Event date :
4-8 July, 2022
Main work title :
The 21st Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun