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Can Cosmic Rays Interacting With Molecular Clouds Explain The Galactic Center Gamma-Ray Excess?
Chris Gordon, Oscar Macias
The Fermi Large Area Telescope data appear to have an excess of gamma rays from the inner 150 pc of the Galactic Center (GC). The main explanations proposed for this are: an unreso…
Cosmic-Ray Models of the Ridge-Like Excess of Gamma Rays in the Galactic Center
Oscar Macias, Chris Gordon, Roland Crocker +1
The High-Energy Stereoscopic System (HESS) has detected diffuse TeV emission correlated with the distribution of molecular gas along the Ridge at the Galactic Center. Diffuse, non-…
Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data
M. G. Aartsen, M. Ackermann, J. Adams +294
A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial ori…
Multipole analysis of IceCube data to search for dark matter accumulated in the Galactic halo
IceCube Collaboration, M. G. Aartsen, M. Ackermann +299
Dark matter which is bound in the Galactic halo might self-annihilate and produce a flux of stable final state particles, e.g. high energy neutrinos. These neutrinos can be detecte…
Search for non-relativistic Magnetic Monopoles with IceCube
IceCube Collaboration, M. G. Aartsen, R. Abbasi +288
The IceCube Neutrino Observatory is a large Cherenkov detector instrumenting of Antarctic ice. The detector can be used to search for signatures of particle phys…
Letter of Intent: The Precision IceCube Next Generation Upgrade (PINGU)
PINGU Collaboration
The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill array of the IceCube Neutrino Observatory. Leveraging technology proven with IceCube, PINGU w…