Effects of Differential Rotation on the Maximum Mass of Neutron Stars
Hyukjin Kwon, Jinho Kim, Kazuyuki Sekizawa
astro-ph.HE, gr-qc, nucl-th
Submitted: 2026-07-10
Comments: 17 pages, 11 figures, 4 tables, Submitted to Physical Review D
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- GW190814: Gravitational Waves from the Coalescence of a 23 M$_\odot$ Black Hole with a 2.6 M$_\odot$ Compact Object
- Multi-pomeron repulsion and the Neutron-star mass
- Impact of hyperon mixing on neutron star structure based on Skyrme-type equations of state: Systematic analysis of $\Lambda NN$ and $\Lambda\Lambda N$ three-body forces with Bayesisan inference
- Too massive neutron stars: The role of dark matter?
- Constraining the mass of fermionic dark matter from its feeble interaction with hadronic matter via dark mediators in neutron stars
- Comparing Models of Rapidly Rotating Relativistic Stars Constructed by Two Numerical Methods
- The bar-mode instability in differentially rotating neutron stars: Simulations in full general relativity
- AthenaK: A Performance-Portable Version of the Athena++ AMR Framework
- Differentially-rotating neutron star models with a parametrized rotation profile
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