P J Veitch
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Explore the profile of P J Veitch including associated specialties, affiliations and a list of published articles.
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42
Citations
567
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Recent Articles
1.
Jia W, Xu V, Kuns K, Nakano M, Barsotti L, Evans M, et al.
Science
. 2024 Sep;
385(6715):1318-1321.
PMID: 39298573
The Heisenberg uncertainty principle dictates that the position and momentum of an object cannot be simultaneously measured with arbitrary precision, giving rise to an apparent limitation known as the standard...
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.
Jia W, Yamamoto H, Kuns K, Effler A, Evans M, Fritschel P, et al.
Phys Rev Lett
. 2021 Dec;
127(24):241102.
PMID: 34951783
High-quality optical resonant cavities require low optical loss, typically on the scale of parts per million. However, unintended micron-scale contaminants on the resonator mirrors that absorb the light circulating in...
4.
Ciobanu A, Brown D, Veitch P, Ottaway D
J Opt Soc Am A Opt Image Sci Vis
. 2021 Oct;
38(9):1293-1303.
PMID: 34613136
Fabry-Perot cavities are central to many optical measurement systems. In high-precision experiments, such as aLIGO and AdVirgo, coupled cavities are often required, leading to complex optical behavior. We show, for...
5.
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...
6.
Whittle C, Hall E, Dwyer S, Mavalvala N, Sudhir V, Abbott R, et al.
Science
. 2021 Jun;
372(6548):1333-1336.
PMID: 34140386
The motion of a mechanical object, even a human-sized object, should be governed by the rules of quantum mechanics. Coaxing them into a quantum state is, however, difficult because the...
7.
Ciobanu A, Brown D, Veitch P, Ottaway D
Appl Opt
. 2020 Nov;
59(31):9884-9895.
PMID: 33175829
Precise mode matching is needed to maximize performance in coupled cavity interferometers such as Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO). In this paper, we present a new mode matching sensing...
8.
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...
9.
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...
10.
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...