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D. Passuello

Researcher at Istituto Nazionale di Fisica Nucleare

Publications -  18
Citations -  12112

D. Passuello is an academic researcher from Istituto Nazionale di Fisica Nucleare. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 10, co-authored 18 publications receiving 9981 citations.

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Journal ArticleDOI

Observation of Gravitational Waves from a Binary Black Hole Merger

B. P. Abbott, +1011 more
TL;DR: This is the first direct detection of gravitational waves and the first observation of a binary black hole merger, and these observations demonstrate the existence of binary stellar-mass black hole systems.
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Astrophysical implications of the binary black hole merger gw150914

B. P. Abbott, +964 more
TL;DR: The discovery of the GW150914 with the Advanced LIGO detectors provides the first observational evidence for the existence of binary black-hole systems that inspiral and merge within the age of the Universe as mentioned in this paper.
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 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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GW150914: The Advanced LIGO Detectors in the Era of First Discoveries

B. P. Abbott, +958 more
TL;DR: Following a major upgrade, the two advanced detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO) held their first observation run between September 2015 and January 2016, and observed a transient gravitational-wave signal determined to be the coalescence of two black holes.
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.