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pro vyhledávání: '"Scott, Susan"'
We present the results of two searches for gravitational waves from the post-merger remnants of the binary neutron star coalescence events GW170817 and GW190425. The searches are fully coherent over 1800~s of data from the 2nd (for GW170817) and 3rd
Externí odkaz:
http://arxiv.org/abs/2403.11392
Publikováno v:
Phys. Rev. D 108, 123045 (2023)
In this work we characterise the performance of a new search technique designed to be sensitive to the remnants of binary neutron star systems. Sensitivity estimates of the new method on simulated data are competitive against those of other work. Pre
Externí odkaz:
http://arxiv.org/abs/2310.12463
Publikováno v:
Monthly Notices of the Royal Astronomical Society 527, 10564-10574 (2024)
Precise measurement of stellar properties through the observation of continuous gravitational waves from spinning non-axisymmetric neutron stars can shed light onto new physics beyond terrestrial laboratories. Although hitherto undetected, prospects
Externí odkaz:
http://arxiv.org/abs/2309.01133
Autor:
Kaur, Tejinder, Kersting, Magdalena, Adams, Kyla, Blair, David, Treagust, David, Popkova, Anastasia, Boublil, Shon, Santoso, Jesse, Ju, Li, Zadnik, Marjan, Wood, David, Horne, Elaine, McGoran, Darren, Scott, Susan, Venville, Grady
Recent years have seen a growing interest in modernizing physics and science curricula around the world. While many science educators and curriculum developers design instructional resources to successfully introduce topics of Einsteinian physics to
Externí odkaz:
http://arxiv.org/abs/2306.17344
Publikováno v:
International Journal of Modern Physics D 32, 2341005 (2023)
Neutron stars are one of the most mysterious wonders in the Universe. Their extreme densities hint at new and exotic physics at work within. Gravitational waves could be the key to unlocking their secrets. In particular, a first detection of gravitat
Externí odkaz:
http://arxiv.org/abs/2305.06606
Ultralight bosons are predicted in many extensions to the Standard Model and are popular dark matter candidates. The black hole superradiance mechanism allows for these particles to be probed using only their gravitational interaction. In this scenar
Externí odkaz:
http://arxiv.org/abs/2305.00401
Detection of continuous gravitational waves from rapidly-spinning neutron stars opens up the possibility of examining their internal physics. We develop a framework that leverages a future continuous gravitational wave detection to infer a neutron st
Externí odkaz:
http://arxiv.org/abs/2209.10981