Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of TurinIT1.2k papers
- University of ManchesterGB1.1k papers
- University of FerraraIT1.1k papers
- Budker Institute of Nuclear PhysicsRU1.1k papers
- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di FrascatiIT1k papers
- Centre National de la Recherche ScientifiqueFR1k papers
- Johannes Gutenberg University MainzDE1k papers
- University of PerugiaIT1k papers
- Uppsala UniversitySE912 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di FerraraIT903 papers
- University of GroningenNL898 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR888 papers
27 papers · 2 filters
Searches for Relativistic Magnetic Monopoles in IceCube
IceCube Collaboration, M. G. Aartsen, K. Abraham +306
Various extensions of the Standard Model motivate the existence of stable magnetic monopoles that could have been created during an early high-energy epoch of the Universe. These p…
Energy loss of intergalactic pair beams: Particle-in-Cell simulation
Andreas Kempf, Patrick Kilian, Felix Spanier
The change of the distribution function of electron-positron pair beams determines whether GeV photons can be produced as secondary radiation from TeV photons. We will discuss the…
Cosmic ray transport and anisotropies to high energies
P. L. Biermann, L. I. Caramete, A. Meli +4
A model is introduced, in which the irregularity spectrum of the Galactic magnetic field beyond the dissipation length scale is first a Kolmogorov spectrum at small scal…
The IceCube Neutrino Observatory - Contributions to ICRC 2015 Part II: Atmospheric and Astrophysical Diffuse Neutrino Searches of All Flavors
The IceCube Collaboration, M. G. Aartsen, K. Abraham +312
Papers on atmospheric and astrophysical diffuse neutrino searches of all flavors submitted to the 34th International Cosmic Ray Conference (ICRC 2015, The Hague) by the IceCube Col…
Wide-Band, Low-Frequency Pulse Profiles of 100 Radio Pulsars with LOFAR
M. Pilia, J. W. T. Hessels, B. W. Stappers +84
LOFAR offers the unique capability of observing pulsars across the 10-240 MHz frequency range with a fractional bandwidth of roughly 50%. This spectral range is well-suited for stu…
Gamma-ray emitting supernova remnants as the origin of Galactic cosmic rays?
Julia Becker Tjus, Björn Eichmann, Mike Kroll +1
The origin of cosmic rays is one of the long-standing mysteries in physics and astrophysics. Simple arguments suggest that a scenario of supernova remnants (SNRs) in the Milky Way…
The Radio-Gamma Correlation In Starburst Galaxies
Björn Eichmann, Julia Becker Tjus
We present a systematic study of the non-thermal electron-proton plasma and its emission processes in starburst galaxies in order to explain the correlation between the luminosity…
Search for Astrophysical Tau Neutrinos in Three Years of IceCube Data
IceCube Collaboration, M. G. Aartsen, K. Abraham +310
The IceCube Neutrino Observatory has observed a diffuse flux of TeV-PeV astrophysical neutrinos at 5.7σ significance from an all-flavor search. The direct detection of tau neutrino…
Search for Transient Astrophysical Neutrino Emission with IceCube-DeepCore
M. G. Aartsen, K. Abraham, M. Ackermann +309
We present the results of a search for astrophysical sources of brief transient neutrino emission using IceCube and DeepCore data acquired between May 15th 2012 and April 30th 2013…
A combined maximum-likelihood analysis of the high-energy astrophysical neutrino flux measured with IceCube
IceCube Collaboration, M. G. Aartsen, K. Abraham +310
Evidence for an extraterrestrial flux of high-energy neutrinos has now been found in multiple searches with the IceCube detector. The first solid evidence was provided by a search…
Evidence for Astrophysical Muon Neutrinos from the Northern Sky with IceCube
IceCube Collaboration, M. G. Aartsen, K. Abraham +309
Results from the IceCube Neutrino Observatory have recently provided compelling evidence for the existence of a high energy astrophysical neutrino flux utilizing a dominantly South…
Search for Dark Matter Annihilation in the Galactic Center with IceCube-79
IceCube Collaboration, M. G. Aartsen, K. Abraham +310
The Milky Way is expected to be embedded in a halo of dark matter particles, with the highest density in the central region, and decreasing density with the halo-centric radius. Da…
Characterization of the Atmospheric Muon Flux in IceCube
IceCube Collaboration, M. G. Aartsen, K. Abraham +312
Muons produced in atmospheric cosmic ray showers account for the by far dominant part of the event yield in large-volume underground particle detectors. The IceCube detector, with…
Detection of a Type IIn Supernova in Optical Follow-up Observations of IceCube Neutrino Events
M. G. Aartsen, K. Abraham, M. Ackermann +331
The IceCube neutrino observatory pursues a follow-up program selecting interesting neutrino events in real-time and issuing alerts for electromagnetic follow-up observations. In Ma…
Probing Atmospheric Electric Fields in Thunderstorms through Radio Emission from Cosmic-Ray-Induced Air Showers
P. Schellart, T. N. G. Trinh, S. Buitink +71
We present measurements of radio emission from cosmic ray air showers that took place during thunderstorms. The intensity and polarization patterns of these air showers are radical…
Shock formation in electron-ion plasmas: mechanism and timing
Anne Stockem Novo, Antoine Bret, Ricardo A. Fonseca +1
We analyse the full shock formation process in electron-ion plasmas in theory and simulations. It is accepted that electromagnetic shocks in initially unmagnetised relativistic pla…
Measurement of the Atmospheric Spectrum with IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +308
We present a measurement of the atmospheric spectrum at energies between 0.1 TeV and 100 TeV using data from the first year of the complete IceCube detector. Atmospheric $ν_e…
Diffusive cosmic ray acceleration at relativistic shock waves with magnetostatic turbulence
Reinhard Schlickeiser
The analytical theory of diffusive cosmic ray acceleration at parallel stationary shock waves with magnetostatic turbulence is generalized to arbitrary shock speeds , inc…
Discovery of variable VHE gamma-ray emission from the binary system 1FGL J1018.6-5856
H. E. S. S. Collaboration, :, A. Abramowski +230
Re-observations with the H.E.S.S. telescope array of the very-high-energy (VHE) source HESS J1018-589 A coincident with the Fermi-LAT -ray binary 1FGL J1018.6-5856 have resulted…
Searches for Time Dependent Neutrino Sources with IceCube Data from 2008 to 2012
M. G. Aartsen, M. Ackermann, J. Adams +304
In this paper searches for flaring astrophysical neutrino sources and sources with periodic emission with the IceCube neutrino telescope are presented. In contrast to time integrat…
Constraints on an Annihilation Signal from a Core of Constant Dark Matter Density around the Milky Way Center with H.E.S.S
HESS Collaboration, A. Abramowski, F. Aharonian +223
An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data acquired in dedicated ON/OFF observations of the Galactic center region with H.…
Cosmic rays in astrospheres
Klaus Scherer, Ausgusts van der Schyff, Dominik Bomans +7
Cosmic rays passing through large astrospheres can be efficiently cooled inside these "cavities" in the interstellar medium. Moreover, the energy spectra of these energetic particl…
Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +300
A diffuse flux of astrophysical neutrinos above has been observed at the IceCube Neutrino Observatory. Here we extend this analysis to probe the astrophysical f…
The exceptionally powerful TeV gamma-ray emitters in the Large Magellanic Cloud
H. E. S. S. Collaboration, :, A. Abramowski +226
The Large Magellanic Cloud, a satellite galaxy of the Milky Way, has been observed with the High Energy Stereoscopic System (H.E.S.S.) above an energy of 100 billion electron volts…