Neutron-star measurements in the multi-messenger Era
S Ascenzi, V Graber, N Rea - Astroparticle Physics, 2024 - Elsevier
Neutron stars are compact and dense celestial objects that offer the unique opportunity to
explore matter and its interactions under conditions that cannot be reproduced elsewhere in …
explore matter and its interactions under conditions that cannot be reproduced elsewhere in …
[HTML][HTML] Searches for continuous gravitational waves from neutron stars: A twenty-year retrospective
K Wette - Astroparticle Physics, 2023 - Elsevier
Seven years after the first direct detection of gravitational waves, from the collision of two
black holes, the field of gravitational wave astronomy is firmly established. A first detection of …
black holes, the field of gravitational wave astronomy is firmly established. A first detection of …
[HTML][HTML] Gravitational waves from neutron-star mountains
F Gittins - Classical and Quantum Gravity, 2024 - iopscience.iop.org
Rotating neutron stars that support long-lived, non-axisymmetric deformations known as
mountains have long been considered potential sources of gravitational radiation. However …
mountains have long been considered potential sources of gravitational radiation. However …
[HTML][HTML] Asteroseismology of Compact Stars
HB Li, Y Gao, L Shao, RX Xu - Universe, 2024 - mdpi.com
Compact stars have been perceived as natural laboratories of matter at an extremely high
density. The uncertainties of the equation of state (EOS) of matter can be constrained by …
density. The uncertainties of the equation of state (EOS) of matter can be constrained by …
GWnext 2024: Meeting Summary
A Torres-Orjuela, V Vazquez-Aceves, R Xu… - arXiv preprint arXiv …, 2024 - arxiv.org
GWnext 2024 was a meeting held in the Kavli Institute for Astronomy and Astrophysics at
Peking University in March $4^\text {th}-8^\text {th} $, 2024. In the meeting researchers at …
Peking University in March $4^\text {th}-8^\text {th} $, 2024. In the meeting researchers at …
Induced polar perturbations with stochastic effects in dense matter relativistic stars: A theoretical probe at intermediate sub-hydro mesoscopic scales
S Satin - International Journal of Modern Physics D, 2024 - ui.adsabs.harvard.edu
A linear response relation between metric and fluid perturbations driven by a background
internal noise source is used as a framework for addressing stochastic effects in order to …
internal noise source is used as a framework for addressing stochastic effects in order to …