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Thomas Eberl

Researcher at University of Erlangen-Nuremberg

Publications -  222
Citations -  8540

Thomas Eberl is an academic researcher from University of Erlangen-Nuremberg. The author has contributed to research in topics: Neutrino & Neutrino detector. The author has an hindex of 44, co-authored 204 publications receiving 7415 citations. Previous affiliations of Thomas Eberl include Max Planck Society & Spanish National Research Council.

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Letter of intent for KM3NeT 2.0

S. Adrián-Martínez, +246 more
- 24 Jun 2016 - 
TL;DR: In this article, the main objectives of the KM3NeT Collaboration are (i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and (ii) the determination of the mass hierarchy of neutrinos.
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ANTARES: the first undersea neutrino telescope

M. Ageron, +287 more
TL;DR: The ANTARES Neutrino Telescope was completed in May 2008 and is the first operational neutrino telescope in the Mediterranean Sea as mentioned in this paper, where the main purpose of the detector is to perform neutrinos astronomy and the apparatus also offers facilities for marine and Earth sciences.
Journal ArticleDOI

Letter of Intent for KM3NeT 2.0

S. Adrián-Martínez, +245 more
TL;DR: In this paper, the main objectives of the KM3NeT Collaboration are the discovery and subsequent observation of high-energy neutrino sources in the Universe and the determination of the mass hierarchy of neutrinos.
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The high-acceptance dielectron spectrometer HADES

G. Agakichiev, +217 more
TL;DR: HADES as discussed by the authors is a versatile magnetic spectrometer aimed at studying dielectron production in pion, proton and heavy-ion-induced collisions, which includes a ring imaging gas Cherenkov detector for electron-hadron discrimination, a tracking system consisting of a set of 6 superconducting coils producing a toroidal field and drift chambers, and a multiplicity and electron trigger array for additional electron hadron discrimination.
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Black Hole-Neutron Star Mergers as Central Engines of Gamma-Ray Bursts

TL;DR: Hydrodynamic simulations of the merger of stellar mass black hole-neutron star binaries are compared with mergers of binary neutron stars and the use of a physical nuclear equation of state allows us to include the effects of neutrino emission.