Superradiant and dynamical spin-down of neutron stars with gravitational wave implications
astro-ph.HE, astro-ph.SR, gr-qc
Submitted: 2025-12-26
Updated: 2026-09-24
Terminology
Sources
- Spin evolution of neutron stars
- 45 Years of Rotation of the Crab Pulsar
- Braking Index of Isolated Pulsars
- Supernova Fallback onto Magnetars and Propeller-Powered Supernovae
- Axion superradiance in rotating neutron stars
- Black holes as particle detectors: evolution of superradiant instabilities
- The anti-glitching gamma-ray pulsar PSR J1522-5735
- The McGill Magnetar Catalog
- Beyond the Second Generation of Laser-Interferometric Gravitational Wave Observatories
- Listening to the Universe with Next Generation Ground-Based Gravitational-Wave Detectors
- Discovery of the first anti-glitch event in the rotation-powered pulsar PSR B0540-69
- Pulsar death line revisited -- I. Almost vacuum gap
- Gravitational waves within the magnetar model of superluminous supernovae and gamma-ray bursts
- Gravitational-wave evolution of newborn magnetars with different deformed structure
- Gravitational wave emission from a magnetically deformed non-barotropic neutron star
- Gravitational Waves from Neutron Stars: A Review
- The Structure of a Quasi-Keplerian Accretion Disk around Magnetized Stars
- Short Duration Gamma-Ray Bursts with Extended Emission from Proto-Magnetar Spin-Down
- Characterizing the continuous gravitational-wave signal from boson clouds around Galactic isolated black holes
- Superradiance in rotating stars and pulsar-timing constraints on dark photons
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