arXiv (All)
open access
Dirac stars in modified $F(R)$ gravity
We study Dirac mini-stars in modified $R^2$ gravity, where gravity is sourced by both linear and nonlinear spinor fields. Two-dimensional (2D) and three-dimensional (3D) profiles of the mini-star mass are constructed as functions of the spinor frequency (for the 2D profiles) and the central value of
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
- Nonlinear Degrees of Freedom of Born-Infeld New Massive Gravity#1070289
- Classical Dirac particle: Mass and Spin invariance and radiation reaction#1248318
- Experimental constraints on the spin and parity of the Λc(2880)+#630539
- Parity-Anomalous Hall Response of Chiral Lifshitz Fermions#1297369
- Scattering, bound states, and resonances in the one-dimensional Dirac equation via supersymmetric quantum mechanics#924105
Record · ID 1343788
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