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Combined dark matter searches towards dwarf spheroidal galaxies with Fermi-LAT, HAWC, H.E.S.S., MAGIC, and VERITAS
Celine Armand, Eric Charles, Mattia di Mauro +13
Cosmological and astrophysical observations suggest that 85\% of the total matter of the Universe is made of Dark Matter (DM). However, its nature remains one of the most challengi…
Searching for eV-scale sterile neutrinos with eight years of atmospheric neutrinos at the IceCube neutrino telescope
M. G. Aartsen, R. Abbasi, M. Ackermann +373
We report in detail on searches for eV-scale sterile neutrinos, in the context of a 3+1 model, using eight years of data from the IceCube neutrino telescope. By analyzing the recon…
An eV-scale sterile neutrino search using eight years of atmospheric muon neutrino data from the IceCube Neutrino Observatory
M. G. Aartsen, R. Abbasi, M. Ackermann +373
The results of a 3+1 sterile neutrino search using eight years of data from the IceCube Neutrino Observatory are presented. A total of 305,735 muon neutrino events are analyzed in…
Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data
M. G. Aartsen, M. Ackermann, J. Adams +331
The Neutrino Mass Ordering (NMO) remains one of the outstanding questions in the field of neutrino physics. One strategy to measure the NMO is to observe matter effects in the osci…
Measurement of Atmospheric Tau Neutrino Appearance with IceCube DeepCore
M. G. Aartsen, M. Ackermann, J. Adams +327
We present a measurement of atmospheric tau neutrino appearance from oscillations with three years of data from the DeepCore sub-array of the IceCube Neutrino Observatory. This ana…
Measurements using the inelasticity distribution of multi-TeV neutrino interactions in IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +330
Inelasticity--the fraction of a neutrino's energy transferred to hadrons--is a quantity of interest in the study of astrophysical and atmospheric neutrino interactions at multi-TeV…
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 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…
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 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…
Very High-Energy Gamma-Ray Follow-Up Program Using Neutrino Triggers from IceCube
IceCube Collaboration, M. G. Aartsen, K. Abraham +537
We describe and report the status of a neutrino-triggered program in IceCube that generates real-time alerts for gamma-ray follow-up observations by atmospheric-Cherenkov telescope…
PINGU: A Vision for Neutrino and Particle Physics at the South Pole
Gen2 Collaboration
The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on t…
Searches for Sterile Neutrinos with the IceCube Detector
The IceCube Collaboration
The IceCube neutrino telescope at the South Pole has measured the atmospheric muon neutrino spectrum as a function of zenith angle and energy in the approximate 320 GeV to 20 TeV r…
Determining neutrino oscillation parameters from atmospheric muon neutrino disappearance with three years of IceCube DeepCore data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +301
We present a measurement of neutrino oscillations via atmospheric muon neutrino disappearance with three years of data of the completed IceCube neutrino detector. DeepCore, a regio…
Measurement of Atmospheric Neutrino Oscillations with IceCube
The IceCube Collaboration
We present the first statistically significant detection of neutrino oscillations in the high-energy regime ( 20 GeV) from an analysis of IceCube Neutrino Observatory data colle…
Measurement of the Atmospheric flux in IceCube
IceCube Collaboration, M. G. Aartsen, R. Abbasi +274
We report the first measurement of the atmospheric electron neutrino flux in the energy range between approximately 80 GeV and 6 TeV, using data recorded during the first year of o…
Search for Neutrinos from Annihilating Dark Matter in the Direction of the Galactic Center with the 40-String IceCube Neutrino Observatory
The IceCube collaboration, R. Abbasi, Y. Abdou +269
A search for muon neutrinos from dark matter annihilations in the Galactic Center region has been performed with the 40-string configuration of the IceCube Neutrino Observatory usi…
Observation of an Anisotropy in the Galactic Cosmic Ray arrival direction at 400 TeV with IceCube
IceCube Collaboration, R. Abbasi, Y. Abdou +258
In this paper we report the first observation in the Southern hemisphere of an energy dependence in the Galactic cosmic ray anisotropy up to a few hundred TeV. This measurement was…
The AMANDA Neutrino Telescope
F. Halzen
With an effective telescope area of order m for TeV neutrinos, a threshold near 50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector r…
The AMANDA Neutrino Telescope and the Indirect Search for Dark Matter
F. Halzen
With an effective telescope area of order 10^4 m^2, a threshold of ~50 GeV and a pointing accuracy of 2.5 degrees, the AMANDA detector represents the first of a new generation of h…