arXiv (All)
open access
Structure and astrophysical properties of dark energy admixed neutron stars
The presence of a dark energy (DE) core, made of a Chaplygin dark fluid, is capable of influencing the diverse observable properties of neutron stars (NSs). However, there is also the possibility that NSs could contain a mixture of ordinary nuclear matter and DE. In this perspective, we propose an e
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
- Gravitational Imprints of Dark Energy in Neutron Stars#1061817
- Pulse profiles of accreting neutron stars - A review of analysis methods, observations, and theoretical models#662068
- Pulse profiles of accreting neutron stars - A review of analysis methods, observations, and theoretical models#661018
- Three-dimensional orbital-free density functional theory description of nuclear pasta in the inner crust of neutron stars#1035508
- Thermal conduction and thermopower of a warm neutron star crust in magnetic fields#1049709
Record · ID 1036280
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