Constraining solar hidden photons using HPGe detector

Abstract In this Letter we report on the results of our search for photons from a U(1) gauge factorin the hidden sectorof the full theory. With our experimental setup we observe the single spectrum in a HPGe detector arising as a result of the photoelectric-like absorption of hidden photons emitted from the Sun on germanium atoms inside the detector. The main ingredient of the theory used in our analysis, a severely constrained kinetic mixing from the two U(1) gauge factorsand massive hidden photons, entails both photon into hidden state oscillations and a minuscule coupling of hidden photons to visible matter, of which the latter our experimental setup has been designed to observe. On a theoretical side, full account was taken of the effects of refraction and damping of photons while propagating in Sunʼs interior as well as in the detector. We exclude hidden photons with kinetic couplings χ > ( 2.2 × 10 − 13 – 3 × 10 − 7 ) in the mass region 0.2 eV ≲ m γ ′ ≲ 30 keV . Our constraints on the mixing parameter χ in the mass region from 20 eV up to 15 keV prove even slightly better then those obtained recently by using data from the CAST experiment, albeit still somewhat weaker than those obtained from solar and HB stars lifetime arguments.