Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Wijngaarden, Marcella"'
Autor:
Hourihane, Sophie, Chatziioannou, Katerina, Wijngaarden, Marcella, Davis, Derek, Littenberg, Tyson, Cornish, Neil
Publikováno v:
Phys. Rev. D 106, 042006 15 August 2022
The increasing sensitivity of gravitational-wave detectors has brought about an increase in the rate of astrophysical signal detections as well as the rate of "glitches"; transient and non-Gaussian detector noise. Temporal overlap of signals and glit
Externí odkaz:
http://arxiv.org/abs/2205.13580
Autor:
Wijngaarden, Marcella, Chatziioannou, Katerina, Bauswein, Andreas, Clark, James A., Cornish, Neil J.
The gravitational wave signal emitted during the coalescence of two neutron stars carries information about the stars' internal structure. During the long inspiral phase the main matter observable is the tidal interaction between the binary component
Externí odkaz:
http://arxiv.org/abs/2202.09382
Publikováno v:
Phys. Rev. D 103, 044013 (2021)
Transient non-gaussian noise in gravitational wave detectors, commonly referred to as glitches, pose challenges for inference of the astrophysical properties of detected signals when the two are coincident in time. Current analyses aim towards modeli
Externí odkaz:
http://arxiv.org/abs/2101.01200
Autor:
Wijngaarden, Marcella, Chatziioannou, Katerina, Bauswein, Andreas, Clark, James A., Cornish, Neil J.
Publikováno v:
Physical Review D
Physical review / D 105(10), 104019 (2022). doi:10.1103/PhysRevD.105.104019
Physical review / D 105(10), 104019 (2022). doi:10.1103/PhysRevD.105.104019
The gravitational wave signal emitted during the coalescence of two neutron stars carries information about the stars' internal structure. During the long inspiral phase the main matter observable is the tidal interaction between the binary component
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69c356c5f40bfd457e9b4ca9ae3fb9c9
https://resolver.caltech.edu/CaltechAUTHORS:20220228-183339664
https://resolver.caltech.edu/CaltechAUTHORS:20220228-183339664
Neutron stars host a range of interesting matter states from matter at supranuclear densities in their cores to possible neutron superfluidity and exotic nucleonic matter in their crusts. In this thesis, I use two distinct approaches probing differen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______348::c51787a4533e9d02751e4b260d7700fc
https://eprints.soton.ac.uk/467476/
https://eprints.soton.ac.uk/467476/
Autor:
Wijngaarden, Marcella J.P.1,2 (AUTHOR) M.J.P.Wijngaarden@soton.ac.uk, Wijnands, Rudy2 (AUTHOR), Ootes, Laura S.2 (AUTHOR), Parikh, Aastha S.2 (AUTHOR), Page, Dany3 (AUTHOR), Weltevrede, P. (AUTHOR), Perera, B.B.P. (AUTHOR), Preston, L.L. (AUTHOR), Sanidas, S. (AUTHOR)
Publikováno v:
Proceedings of the International Astronomical Union. Jul2017, Vol. 13 Issue S337, p229-232. 4p.
