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We present a new statistical analysis that combines helioseismology and solar neutrino observations to place upper limits to the properties of non standard weakly interacting particles. We present two applications to test the method: the well studied case of axions and the more novel case of low mass hidden photons. For axions we obtain an upper limit at 3 for the axion-photon coupling constant of g₀\, <\, 4. 1 10^-10 GeV^-1. For hidden photons we obtain the most restrictive upper limit available accross a wide range of masses for the product of the kinetic mixing and mass of m < 1. 8 10^-12 eV at 3. Both cases improve the previous solar constraints based on the Standard Solar Models.
Vinyoles et al. (Thu,) studied this question.
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