arXiv (All)
open access
Descalarization bursts from Galactic supramassive neutron stars: a kHz continuous-wave target
In massive scalar-tensor gravity, a scalarized neutron star must shed its scalar hair as it collapses into a black hole. Using 3D simulations of a realistic rotating progenitor we show that dispersion stretches the emitted burst into a quasi-monochromatic signal in the kHz frequency range lasting $>
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
- Analyzing GW231109_235456 and understanding its potential implications for population studies, nuclear physics, and multi-messenger astronomy#1014563
- Probing fundamental physics with ALMA2040 mm-wavelength observations of neutron stars#1356925
- Scalarized Hot Neutron Stars Containing Hyperons and $Δ$-Resonances in Different Evolution Regimes#1064879
- Reconstructing Early Primordial Black Hole Domination from Gravitational-Wave Backgrounds#999569
- Probing Neutron Star Equation of State Universality with Gravitational Waves#972067
Record · ID 1247655
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