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Timothy Evans

Researcher at CERN

Publications -  785
Citations -  85465

Timothy Evans is an academic researcher from CERN. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 105, co-authored 704 publications receiving 70620 citations. Previous affiliations of Timothy Evans include California Institute of Technology & University of Oxford.

Papers
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Journal ArticleDOI

Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo’s third observing run

Richard J. Abbott, +1681 more
- 15 Jul 2021 - 
TL;DR: In this article, the authors report results of a search for an isotropic gravitational-wave background (GWB) using data from Advanced LIGO's and Advanced Virgo's third observing run (O3) combined with upper limits from the earlier O1 and O2 runs.
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Limits on gravitational-wave emission from selected pulsars using LIGO data.

B. P. Abbott, +407 more
TL;DR: The unprecedented sensitivity of the detectors allows us to set strain upper limits as low as a few times 10(-24), which translate into limits on the equatorial ellipticities of the pulsars, which are smaller than 10(-5) for the four closest pulsars.
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Measurements of the S-wave fraction in B 0 → K + π − μ + μ − decays and the B 0 → K ∗ (892) 0 μ + μ − differential branching fraction

Roel Aaij, +762 more
TL;DR: In this article, a measurement of the differential branching fraction of the decay B0→K∗(892)0μ+μ− is presented together with a determination of the S-wave fraction of B 0→K+π−μ +μ− decays.
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Search for A^{'}→μ^{+}μ^{-} Decays.

Roel Aaij, +906 more
TL;DR: In this article, both prompt-like and long-lived dark photons, A^{'}, produced in proton-proton collisions at a center-of-mass energy of 13 TeV, were searched using a data sample corresponding to an integrated luminosity of 5.5
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First search for gravitational waves from known pulsars with Advanced LIGO

B. P. Abbott, +999 more
TL;DR: In this article, the results of searches for gravitational waves from 200 pulsars using data from the first observing run of the Advanced LIGO detectors were presented, and they were able to set the most constraining upper limits yet on their gravitational-wave amplitudes and ellipticities.