Timothy Evans

TL;DR: A search for the stochastic background with the latest data from the LIGO and Virgo detectors shows no evidence of a stochastically gravitational-wave signal, and the limits in these four bands are the lowest direct measurements to date on the stoChastic background.

TL;DR: In this paper, a search for a long-lived scalar particle χ is performed, looking for the decay B+→K+χ with χ→μ+μ− in pp collision data corresponding to an integrated luminosity of 3fb−1, collected by the LHCb experiment at centre-of-mass energies of s√=7 and 8TeV.

TL;DR: In this paper, a search for gravitational wave bursts using data from the first science run of the Laser Interferometer Gravitational Wave Observatory (LIGO) detectors was reported. But their search focused on bursts with durations ranging from 4 to 100 ms, and with significant power in the LIGO sensitivity band of 150 to 3000 Hz.

TL;DR: In this paper, a search for short-duration gravitational-wave bursts with arbitrary waveform in the 64-1600 Hz frequency range appeared in all three LIGO interferometers.

TL;DR: In this article, the authors reported a search for gravitational waves from the inspiral, merger and ringdown of binary black holes with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010.