arXiv (All)
open access
Causality and perturbative-QCD constraints on first-order phase transitions in neutron stars
Causality bounds the compactness and maximum mass of neutron stars. We generalise this bound to equations of state (EOSs) with a first-order phase transition between maximally stiff phases. In units of the transition energy density, the problem depends only on $q=\ptr/\etr$ and $j=Δ\ve/\etr$. The ma
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
- The presence and order of QCD phase transitions from gravitational-wave observations of neutron star mergers#1402675
- Nonradial oscillations of realistic anisotropic neutron stars: Polar modes#985290
- Classification of $g$-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars#670394
- Classification of $g$-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars#668329
- Recurring region for neutron-star observables#609797
Record · ID 1402909
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