arXiv (OAI Expanded)
open access
Polarization Formalism for Photon-Gravitational Wave Mixing Around Magnetars
The Gertsenshtein effect can be used to probe the stochastic gravitational wave background at high frequencies, well above the range of standard cosmological sources. In this paper, we revisit the conversion between electromagnetic and gravitational waves in the magnetosphere of magnetars by solving
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
- QCD Crossover Transfer Functions for Scalar-Induced Gravitational Waves in the PTA Band#1077007
- Spectral Fingerprints Beyond Degeneracies in Primordial Gravitational-Wave Sources#1083164
- Angular structure of finite-field vacuum birefringence in magnetars#1143174
- Detecting a large magneto-optical shift in Py/NiO bilayers#1063317
- Induced Scattering of Strong Waves in Pair Plasmas#1069779
Record · ID 1070847
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