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Paul Seidel

Researcher at University of Jena

Publications -  367
Citations -  6934

Paul Seidel is an academic researcher from University of Jena. The author has contributed to research in topics: Josephson effect & Thin film. The author has an hindex of 28, co-authored 364 publications receiving 5591 citations. Previous affiliations of Paul Seidel include Schiller International University & Roma Tre University.

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The Einstein Telescope: a third-generation gravitational wave observatory

M. Punturo, +134 more
TL;DR: The third-generation ground-based observatory Einstein Telescope (ET) project as discussed by the authors is currently in its design study phase, and it can be seen as the first step in this direction.
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Sensitivity studies for third-generation gravitational wave observatories

Stefan Hild, +141 more
TL;DR: In this article, a special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates, including the most relevant fundamental noise contributions.
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Scientific objectives of Einstein Telescope

Bangalore Suryanarayana Sathyaprakash, +225 more
TL;DR: The advanced interferometer network will herald a new era in observational astronomy, and there is a very strong science case to go beyond the advanced detector network and build detectors that operate in a frequency range from 1 Hz to 10 kHz, with sensitivity a factor 10 better in amplitude as discussed by the authors.
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The third generation of gravitational wave observatories and their science reach

M. Punturo, +133 more
TL;DR: The status of the project Einstein Telescope (ET), a design study of a third-generation gravitational wave observatory, is reported in this paper, where an overview of the possible science reaches and the technological progress needed to realize a third generation observatory are discussed.
Journal ArticleDOI

Sensitivity Studies for Third-Generation Gravitational Wave Observatories

Stefan Hild, +141 more
TL;DR: In this article, a special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates, including the most relevant fundamental noise contributions.