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L. Köpke

Researcher at University of Mainz

Publications -  955
Citations -  86932

L. Köpke is an academic researcher from University of Mainz. The author has contributed to research in topics: Large Hadron Collider & Neutrino. The author has an hindex of 136, co-authored 950 publications receiving 81787 citations. Previous affiliations of L. Köpke include West University of Timișoara & University of Oregon.

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Book ChapterDOI

Status of the Neutrino Telescope AMANDA: Monopoles and WIMPS

TL;DR: The neutrino telescope AMANDA has been set up at the geographical South Pole as the first step to a neutrinos telescope of the scale of one cubic kilometer, which is the canonical size for a detector sensitive to Neutrinos from Active Galactic Nuclei (AGN), Gamma Ray Bursts (GRB) and Topological Defects (TD).
Posted Content

All-flavor constraints on nonstandard neutrino interactions and generalized matter potential with three years of IceCube DeepCore data

Rasha Abbasi, +369 more
TL;DR: In this paper, the authors report constraints on nonstandard neutrino interactions (NSI) from the observation of atmospheric neutrinos with IceCube, limiting all individual coupling strengths from a single dataset.
Journal ArticleDOI

Summary of working group 4: High energy neutrino telescopes

TL;DR: The field of high-energy neutrino astronomy is rapidly developing and a number of new experiments are currently being deployed and developed Additionally, the recent successes of TeV gamma-ray astronomy have exciting implications for future neutrinos telescopes as mentioned in this paper.

The IceCube prototype string in Amanda The Amanda Collaboration, M. Ackermann, J. Ahrens, X. Bai, M. Bartelt, S.W. Barwick, R. Bay, T. Becka, J.K. Becker, K.H. Becker, E. Bernardini, D. Bertrand, D.J. Boersma, S. Boser, O. Botner, A. Bouchta, O. Bouhali, J. Braun, C. Burgess, T. Burgess, T. Castermans,

Search for Diffuse Fluxes of Extraterrestrial Muon-Neutrinos with the AMANDA Detectors

TL;DR: The AMANDA neutrino detector has been in operation since the start of the austral winter of 1997 as mentioned in this paper, and the analysis of the initial year of data taking has produced a 90% confidence level upper limit on an E−2 flux of muon-neutrinos, at the earth, at a level EΦ(E) = 8.4×10−7 cm−2 s−1 sr−1GeV.