arXiv (All)
open access
Continuous Gravitational Waves from Thermo-Elastic Mountains in Ultraluminous X-ray Pulsars
Fast-spinning, nonaxisymmetrically deformed neutron stars (NSs) are promising targets for continuous gravitational-wave (CGW) searches with current and next-generation ground-based detectors. Ultraluminous X-ray pulsars (ULXPs), characterized by super-Eddington accretion and strong magnetic fields,
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Detailed characterisation of the orbital parameters and eclipses of 'black widow' pulsars by radio timing and use of this new population of fast pulsars for the detection of the gravitational wave background#173060
- Empirical determination of the Galactic neutron star--black hole merger rate using StarTrack models#1130372
- Weak in the Presence of Beauty: Gravitational waves from the mergers of black holes and neutron stars as a messenger#1122507
- Red noise and evolving signals: a complete frequentist approach to supermassive black hole binary searches with pulsar timing arrays#1063940
- Astrophysics with continuous gravitational waves#294816
Record · ID 1202718
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive