Kaluza-Klein (KK) axions appear in theories with extra dimensions as higher mass, significantly shorter lifetime, excitations of the Peccei-Quinn axion. When produced in the Sun, they would remain gravitationally trapped in the solar system, and their decay to a pair of photons could provide an explanation of the solar corona heating problem. A low-density detector would discriminate such a signal from the background, by identifying the separation of the interaction point of the two photons. The NEWS-G collaboration uses large volume Spherical Proportional Counters, gas-filled metallic spheres with a spherical anode in their centre. After observation of a single axion-like event in a 42 day long run with the SEDINE detector, a $90%$ C.L. upper limit of $g_{agammagamma}<7.76cdot10^{-13},GeV^{-1}$ is set on the axion-photon coupling for a KK axion density on Earth of $n_{a}=4.07cdot10^{13},m^{-3}$ and two extra dimensions of size $R = 1,eV^{-1}$.
Download