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A Search for Neutrino Emission from Fast Radio Bursts with Six Years of IceCube Data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +320
We present a search for coincidence between IceCube TeV neutrinos and fast radio bursts (FRBs). During the search period from 2010 May 31 to 2016 May 12, a total of 29 FRBs with 13…
Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption
IceCube Collaboration, M. G. Aartsen, M. Ackermann +314
Neutrinos interact only very weakly, so they are extremely penetrating. However, the theoretical neutrino-nucleon interaction cross section rises with energy such that, at energies…
Search for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger Observatory
A. Albert, M. Andre, M. Anghinolfi +1931
The Advanced LIGO and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst (GRB) that followed the merg…
The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part V: Solar flares, Supernovae, Event reconstruction, Education & Outreach
IceCube Collaboration, M. G. Aartsen, M. Ackermann +312
Papers on solar flares, supernovae, event reconstruction and education & outreach, submitted to the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the…
The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part IV: Searches for Beyond the Standard Model Physics
IceCube Collaboration, M. G. Aartsen, M. Ackermann +312
Papers on searches for beyond the standard model physics, submitted to the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the IceCube Collaboration
The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part III: Cosmic Rays
IceCube Collaboration, M. G. Aartsen, M. Ackermann +312
Papers on cosmic-ray measurements submitted to the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the IceCube Collaboration
The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part II: Properties of the Atmospheric and Astrophysical Neutrino Flux
IceCube Collaboration, M. G. Aartsen, M. Ackermann +312
Papers on the properties of the atmospheric and astrophysical neutrino flux submitted to the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the IceCube…
The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part I: Searches for the Sources of Astrophysical Neutrinos
IceCube Collaboration, M. G. Aartsen, M. Ackermann +312
Papers on the searches for the sources of astrophysical neutrinos, submitted to the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the IceCube Collabor…
Search for Nonstandard Neutrino Interactions with IceCube DeepCore
IceCube Collaboration, M. G. Aartsen, M. Ackermann +317
As atmospheric neutrinos propagate through the Earth, vacuum-like oscillations are modified by Standard-Model neutral- and charged-current interactions with electrons. Theories bey…
Neutrino Interferometry for High-Precision Tests of Lorentz Symmetry with IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +319
Lorentz symmetry is a fundamental space-time symmetry underlying the Standard Model of particle physics and gravity. However, unified theories, such as string theory, allow for vio…
Constraints on Galactic Neutrino Emission with Seven Years of IceCube Data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +309
The origins of high-energy astrophysical neutrinos remain a mystery despite extensive searches for their sources. We present constraints from seven years of IceCube Neutrino Observ…
Measurement of Atmospheric Neutrino Oscillations at 6-56 GeV with IceCube DeepCore
IceCube Collaboration, M. G. Aartsen, M. Ackermann +314
We present a measurement of the atmospheric neutrino oscillation parameters using three years of data from the IceCube Neutrino Observatory. The DeepCore infill array in the center…
Search for Neutrinos from Dark Matter Self-Annihilations in the center of the Milky Way with 3 years of IceCube/DeepCore
IceCube Collaboration, M. G. Aartsen, M. Ackermann +310
We present a search for a neutrino signal from dark matter self-annihilations in the Milky Way using the IceCube Neutrino Observatory (IceCube). In 1005 days of data we found no si…
Search for astrophysical sources of neutrinos using cascade events in IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +310
The IceCube neutrino observatory has established the existence of a flux of high-energy astrophysical neutrinos inconsistent with the expectation from atmospheric backgrounds at a…
Search for High-energy Neutrinos from Gravitational Wave Event GW151226 and Candidate LVT151012 with ANTARES and IceCube
A. Albert, M. Andre, M. Anghinolfi +1410
The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up…
Extending the search for muon neutrinos coincident with gamma-ray bursts in IceCube data
M. G. Aartsen, M. Ackermann, J. Adams +305
We present an all-sky search for muon neutrinos produced during the prompt -ray emission of 1172 gamma-ray bursts (GRBs) with the IceCube Neutrino Observatory. The detection of…
Multiwavelength follow-up of a rare IceCube neutrino multiplet
M. G. Aartsen, M. Ackermann, J. Adams +501
On February 17 2016, the IceCube real-time neutrino search identified, for the first time, three muon neutrino candidates arriving within 100 s of one another, consistent with comi…
Search for sterile neutrino mixing using three years of IceCube DeepCore data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +305
We present a search for a light sterile neutrino using three years of atmospheric neutrino data from the DeepCore detector in the energy range of approximately GeV. DeepCor…
Neutrinos and Cosmic Rays Observed by IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +303
The core mission of the IceCube Neutrino observatory is to study the origin and propagation of cosmic rays. IceCube, with its surface component IceTop, observes multiple signatures…