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Hermann Kolanoski

Researcher at Humboldt University of Berlin

Publications -  1314
Citations -  102570

Hermann Kolanoski is an academic researcher from Humboldt University of Berlin. The author has contributed to research in topics: Large Hadron Collider & Neutrino. The author has an hindex of 145, co-authored 1279 publications receiving 96152 citations. Previous affiliations of Hermann Kolanoski include Uppsala University & University of California, Davis.

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Search for quark contact interactions in dijet angular distributions in pp collisions at √s = 7 TeV measured with the ATLAS detector

Georges Aad, +3166 more
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Observation of charmless B meson decays

H. Albrecht, +77 more
- 28 Jul 1988 - 
TL;DR: In this paper, it was shown that the charmless decays of B mesons into the final states ppπ± and ppπ+π− are not the result of penguin-type processes.
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Measurement of the differential cross-section of highly boosted top quarks as a function of their transverse momentum in s =8 TeV proton-proton collisions using the ATLAS detector

Georges Aad, +2858 more
- 26 Feb 2016 - 
TL;DR: The differential cross-section for pair production of top quarks with high transverse momentum is measured in 20.3 fb(-1) of proton-proton collisions at a center-of-mass energy of 8 TeV as mentioned in this paper.
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Transverse momentum, rapidity, and centrality dependence of inclusive charged-particle production in sNN=5.02 TeV p + Pb collisions measured by the ATLAS experiment

Georges Aad, +2845 more
- 10 Dec 2016 - 
TL;DR: In this paper, the per-event charged particle yield as a function of the charged-particle transverse momentum and rapidity is performed using p+Pbp+Pb collision data collected by the ATLAS experiment at the LHC at a centre-of-mass energy of sqrt (SNN) = 5.01 TeV.
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Anisotropy in Cosmic-Ray Arrival Directions in the Southern Hemisphere with Six Years of Data from the IceCube Detector

M. G. Aartsen, +314 more
- 03 Mar 2016 - 
TL;DR: In this paper, a detailed analysis of the cosmic-ray arrival direction anisotropy in the TeV to PeV energy range was performed using high-statistics data from the IceCube Neutrino Observatory.