arXiv (OAI Expanded)open access
Classification of $g$-modes for neutron stars with a strong transition: Novel universal relation including slow stable hybrid stars
high energy physics - phenomenology, high energy astrophysical phenomena, general relativity and quantum cosmology, nuclear theory
This document is indexed with metadata only — full text is not available in the archive for this record.
Open the official source ↗
Record · ID 668329
Retrieved via
Conceptio — every document is proof-bundled with source, license, and retrieval metadata.