CERN Accelerating science

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1.
Tests of General Relativity with GWTC-3 / LIGO Scientific Collaboration
The ever-increasing number of detections of gravitational waves (GWs) from compact binaries by the Advanced LIGO and Advanced Virgo detectors allows us to perform ever-more sensitive tests of general relativity (GR) in the dynamical and strong-field regime of gravity. [...]
arXiv:2112.06861 ; LIGO-P2100275.
- 41 p.
Fulltext
2.
Search for Subsolar-Mass Binaries in the First Half of Advanced LIGO’s and Advanced Virgo’s Third Observing Run / LIGO Scientific Collaboration
We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2 $M_\odot$ and 1.0 $M_\odot$ in Advanced LIGO and Advanced Virgo data collected between 1 April 2019 1500 UTC and 1 October 2019 1500 UTC. We extend previous analyses in two main ways: we include data from the Virgo detector and we allow for more unequal mass systems, with mass ratio $q \geq 0.1$. [...]
arXiv:2109.12197; LIGO-P2100163-v8.- 2022-08-05 - 16 p. - Published in : Phys. Rev. Lett. 129 (2022) 061104 Fulltext: PDF;
3.
First joint observation by the underground gravitational-wave detector KAGRA with GEO 600 / KAGRA Collaboration
We report the results of the first joint observation of the KAGRA detector with GEO600. KAGRA is a cryogenic and underground gravitational-wave detector consisting of a laser interferometer with three-kilometer arms, and located in Kamioka, Gifu, Japan. [...]
arXiv:2203.01270; LIGO-P2100286.- 2022-06-14 - 37 p. - Published in : PTEP 2022 (2022) 063F01 Fulltext: 2203.01270 - PDF; document - PDF;
4.
Investigation of magnetic noise in Advanced Virgo / Cirone, A. (Genoa U. ; INFN, Genoa) ; Fiori, I. (EGO, Pisa) ; Paoletti, F. (INFN, Pisa) ; Perez, M.M. (Barcelona, IFAE) ; Rodríguez, A.R. (CERN ; Erice, Majorana Ctr.) ; Swinkels, B.L. (NIKHEF, Amsterdam) ; Vazquez, A.M. (Mexico U.) ; Gemme, G. (Enrico Fermi Ctr., Rome ; Genoa U. ; INFN, Genoa) ; Chincarini, A. (INFN, Genoa)
The Advanced Virgo (AdV) sensitivity might be influenced by the effects of environmental noise, in particular magnetic noise (MN). In order to show the impact on the gravitational-wave strain signal h(t) and on the AdV sensitivity, we must understand the coupling between the environmental magnetic activity and the strain. [...]
arXiv:1908.11174.- 2019-10-18 - 14 p. - Published in : Class. Quantum Gravity 36 (2019) 225004

See also: similar author names
42 Swinkels, B
19 Swinkels, B L
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