An Asymptotically Causal Metamodel for Neutron Star Equations of State
nucl-th, astro-ph.HE
Submitted: 2026-03-31
Updated: 2026-08-27
Terminology
Sources
- PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
- The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
- A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- The Radius of PSR J0740+6620 from NICER with NICER Background Estimates
- An updated mass-radius analysis of the 2017-2018 NICER data set of PSR J0030+0451
- Constraining the dense matter equation of state with new NICER mass-radius measurements and new chiral effective field theory inputs
- A NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Properties of the binary neutron star merger GW170817
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- A Horizon Study for Cosmic Explorer: Science, Observatories, and Community
- The Science of the Einstein Telescope
- Binary neutron-star mergers: a review of Einstein's richest laboratory
- The Dynamics of Binary Neutron Star Mergers and of GW170817
- Constraining the equation of state in neutron-star cores via the long-ringdown signal
- Neutron stars - cooling and transport
- Constraints on the dense matter equation of state from young and cold isolated neutron stars
- Insights into the physics of neutron star interiors from pulsar glitches
- Gravitational-wave constraints on the neutron-star-matter Equation of State
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