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S. Birindelli

Researcher at University of Nice Sophia Antipolis

Publications -  23
Citations -  5269

S. Birindelli is an academic researcher from University of Nice Sophia Antipolis. The author has contributed to research in topics: Gravitational wave & Gravitational-wave observatory. The author has an hindex of 17, co-authored 23 publications receiving 4105 citations.

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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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Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors

J. Abadie, +722 more
TL;DR: In this paper, Kalogera et al. presented an up-to-date summary of the rates for all types of compact binary coalescence sources detectable by the initial and advanced versions of the ground-based gravitational-wave detectors LIGO and Virgo.
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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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Virgo: a laser interferometer to detect gravitational waves

T. Accadia, +341 more
TL;DR: Virgo as discussed by the authors is a very large Michelson interferometer with 3 km-long arms, built at Cascina, near Pisa (Italy), with a detailed description of all its different elements is given.
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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.