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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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Angular analysis of the B 0 → K *0 μ + μ − decay using 3 fb −1 of integrated luminosity

Roel Aaij, +764 more
TL;DR: An angular analysis of the B0 → K*0(→ K+π−)μ+μ− decay is presented in this paper, where the angular observables and their correlations are reported in bins of q2, the invariant mass squared of the dimuon system.
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Observation of Gravitational Waves from Two Neutron Star–Black Hole Coalescences

Richard J. Abbott, +1695 more
TL;DR: In this article, the authors reported the observation of gravitational waves from two compact binary coalescences in LIGO's and Virgo's third observing run with properties consistent with neutron star-black hole (NSBH) binaries.
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The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914

B. P. Abbott, +961 more
TL;DR: In this paper, the authors report on the constraints these observations place on the rate of binary black hole coalescences, and estimate a 90% credible range of merger rates between $2$--$53 \, \mathrm{Gpc}^{-3} \mathm{yr}^{ −1}$ (comoving frame).
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An upper limit on the stochastic gravitational-wave background of cosmological origin

B. P. Abbott, +667 more
- 20 Aug 2009 - 
TL;DR: In this paper, the authors reported limits on the amplitude of the stochastic gravitational-wave background using the data from a two-year science run of the Laser Interferometer Gravitational-wave Observatory (LIGO).
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GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

B. P. Abbott, +1148 more
TL;DR: In this article, the authors presented the results from three gravitational-wave searches for coalescing compact binaries with component masses above 1, during the first and second observing runs of the Advanced Gravitational-wave detector network.