A Bozzi
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Explore the profile of A Bozzi including associated specialties, affiliations and a list of published articles.
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Articles
98
Citations
843
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Recent Articles
1.
Acernese F, Agathos M, Ain A, Albanesi S, Allene C, Allocca A, et al.
Phys Rev Lett
. 2023 Aug;
131(4):041403.
PMID: 37566847
In this Letter, we present the design and performance of the frequency-dependent squeezed vacuum source that will be used for the broadband quantum noise reduction of the Advanced Virgo Plus...
2.
Abbott R, Abbott T, Acernese F, Ackley K, Adams C, Adhikari N, et al.
Phys Rev Lett
. 2022 Aug;
129(6):061104.
PMID: 36018635
We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2 M_{⊙} and 1.0 M_{⊙} in Advanced LIGO and Advanced Virgo...
3.
Abbott R, Abbott T, Abraham S, Acernese F, Ackley K, Adams A, et al.
Phys Rev Lett
. 2021 Jul;
126(24):241102.
PMID: 34213926
We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 dataset. Search results are presented for gravitational waves produced by cosmic string loop...
4.
Acernese F, Agathos M, Aiello L, Ain A, Allocca A, Amato A, et al.
Phys Rev Lett
. 2020 Oct;
125(13):131101.
PMID: 33034506
The quantum radiation pressure and the quantum shot noise in laser-interferometric gravitational wave detectors constitute a macroscopic manifestation of the Heisenberg inequality. If quantum shot noise can be easily observed,...
5.
Abbott B, Abbott R, Abbott T, Abraham S, Acernese F, Ackley K, et al.
Living Rev Relativ
. 2020 Oct;
23(1):3.
PMID: 33015351
We present our current best estimate of the plausible observing scenarios for the Advanced LIGO, Advanced Virgo and KAGRA gravitational-wave detectors over the next several years, with the intention of...
6.
Abbott R, Abbott T, Abraham S, Acernese F, Ackley K, Adams C, et al.
Phys Rev Lett
. 2020 Sep;
125(10):101102.
PMID: 32955328
On May 21, 2019 at 03:02:29 UTC Advanced LIGO and Advanced Virgo observed a short duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise ratio of 14.7, and an estimated...
7.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Class Quantum Gravity
. 2020 Sep;
33(13).
PMID: 32908328
On September 14, 2015, a gravitational wave signal from a coalescing black hole binary system was observed by the Advanced LIGO detectors. This paper describes the transient noise backgrounds used...
8.
Abbott B, Abbott R, Abbott T, Abernathy M, Acernese F, Ackley K, et al.
Phys Rev D
. 2020 Aug;
93(12).
PMID: 32818163
On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO) simultaneously observed the binary black hole merger GW150914. We report the results of...
9.
Acernese F, Agathos M, Aiello L, Allocca A, Amato A, Ansoldi S, et al.
Phys Rev Lett
. 2019 Dec;
123(23):231108.
PMID: 31868444
Current interferometric gravitational-wave detectors are limited by quantum noise over a wide range of their measurement bandwidth. One method to overcome the quantum limit is the injection of squeezed vacuum...
10.
Abbott B, Abbott R, Abbott T, Abraham S, Acernese F, Ackley K, et al.
Phys Rev Lett
. 2019 Nov;
123(16):161102.
PMID: 31702344
We present a search for subsolar mass ultracompact objects in data obtained during Advanced LIGO's second observing run. In contrast to a previous search of Advanced LIGO data from the...