This work summarizes a novel dataset, searching for starting track events, whereas a neutrino interacts within the fiducial volume of the detector producing a muon track.

This work summarizes a novel dataset, searching for starting track events, whereas a neutrino interacts within the fiducial volume of the detector producing a muon track.

Newly developed methods, techniques, and simulations are vital to the success of this work and are presented along the way to the final result.

This work revisits the HESE sample analysis with an additional 4.5 years of data, newer glacial ice models, and improved systematics treatment.

This study presents the results of different searches for correlations between very high-energy neutrino candidates detected by IceCube and the highest-energy cosmic rays measured by the Pierre Auger Observatory and the Telescope Array.

The research presented here focuses on improving IceCube's sensitivity to southern sky sources by selecting for starting tracks, which are created by muon neutrinos that interact inside of the IceCube detector volume.

The work presented here is about an improved analysis to observe astrophysical tau neutrinos using novel observation techniques, a critical key in measuring the astrophysical neutrino flavor ratio.

We present a simple physical model in which high-energy cosmic rays are confined within the volumes of radio galaxies, where they interact with gas to generate the observed diffuse fluxes of neutrinos and gamma rays.