arXiv (All)
open access
Probing fundamental physics with ALMA2040 mm-wavelength observations of neutron stars
Bursty or (rotation-induced) pulsed coherent radio emission from pulsars, magnetars, and fast radio transients originates in some of the most extreme environments in the Universe. However, the exact physical mechanism behind the scenes remains poorly understood. ALMA2040 will allow for systematic ex
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
- Descalarization bursts from Galactic supramassive neutron stars: a kHz continuous-wave target#1247655
- Recurring region for neutron-star observables#609797
- General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars#173223
- Trace Anomaly and Effective Topological Sources in Neutron Stars#659029
- Trace Anomaly and Effective Topological Sources in Neutron Stars#656893
Record · ID 1356925
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