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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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Search for gravitational waves from low mass binary coalescences in the first year of LIGO's S5 data

B. P. Abbott, +516 more
- 05 Jun 2009 - 
TL;DR: In this article, the authors search for gravitational waves from coalescing low mass compact binary systems with a total mass between 2M and 35Mz-sun and a minimum component mass of 1M_([sun]) using data from the first year of the fifth science run of the three LIGO detectors.
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First search for gravitational waves from known pulsars with advanced LIGO

B. P. Abbott, +1039 more
TL;DR: In this paper, 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.
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Constraints on cosmic strings using data from the first Advanced LIGO observing run

B. P. Abbott, +1042 more
- 08 May 2018 - 
TL;DR: In this article, an analysis conducted to specifically search for gravitational-wave bursts from cosmic string loops in the data of Advanced LIGO 2015-2016 observing run (O1) was conducted.
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Evidence of a J/psi Lambda structure and observation of excited Xi(-) states in the Xi(-)(b) -> J/psi Lambda K- decay

Roel Aaij, +968 more
TL;DR: The first evidence of a structure in the LHC invariant mass distribution was obtained from an amplitude analysis of J/psi{\Lambda}K^-$decays.
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All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

B. P. Abbott, +1225 more
- 08 Jul 2019 - 
TL;DR: In this article, the results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast spinning neutron stars with an asymmetry around their rotation axis, were presented.