Discovery of the First Antiglitch Event in the Rotation-powered Pulsar PSR B0540-69
Using data from the Neutron star Interior Composition ExploreR observatory, we identified a
permanent spin frequency decrease of Δν=−(1.04±0.07)× 10− 7 Hz around MJD 60132 in …
permanent spin frequency decrease of Δν=−(1.04±0.07)× 10− 7 Hz around MJD 60132 in …
Glitching pulsars as gravitational wave sources
B Haskell, DI Jones - Astroparticle Physics, 2024 - Elsevier
Spinning neutron stars, when observed as pulsars, are seen to undergo occasional spin-up
events known as glitches. Despite several decades of study, the physical mechanisms …
events known as glitches. Despite several decades of study, the physical mechanisms …
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 …
High priority targets for transient gravitational waves from glitching pulsars
Glitching pulsars are expected to be important sources of gravitational waves. In this paper,
we explore six different models that propose the emission of transient continuous waves …
we explore six different models that propose the emission of transient continuous waves …