Search for long-lived staus using neutrino telescopes

We present a novel search strategy for long-lived charged particles with neutrino telescopes. Specifically, we consider long-lived staus produced in atmospheric air showers, which reach the IceCube Neutrino Observatory producing detectable track signatures. We show that their reconstructed energy peaks sharply at $700$ GeV, making energy cuts an efficient technique for background reduction. Using one year of IceCube data from 2012, and conservative assumptions on the detection efficiency, we obtain the lower limit $m_{\tilde \tau}\geq 120$ GeV at the 95\% C.L. assuming Drell-Yan production. For ten years of IceCube data, which have already been collected, we forecast a lower limit $m_{\widetilde \tau }\geq 430$ GeV. We also comment on the prospects of improving the sensitivity to long-lived staus with future neutrino telescopes.