no code implementations • 7 Jan 2015 • Núria Vinyoles, Aldo Serenelli, Francesco L. Villante, Sarbani Basu, Javier Redondo, Jordi Isern
We present a new statistical analysis that combines helioseismology (sound speed, surface helium and convective radius) and solar neutrino observations (the $^8$B and $^7$Be fluxes) to place upper limits to the properties of non standard weakly interacting particles.
Solar and Stellar Astrophysics
