## 13 Citations

### Gravitational waves from neutron star mergers and their relation to the nuclear equation of state

- PhysicsProgress in Particle and Nuclear Physics
- 2019

### Spectral classification of gravitational-wave emission and equation of state constraints in binary neutron star mergers

- PhysicsJournal of Physics G: Nuclear and Particle Physics
- 2019

The first detection of gravitational waves from a binary neutron star merger (GW170817) and the accompanying electromagnetic emission has impressively advanced our understanding of the merger process…

### Neutron star matter as a relativistic Fermi liquid

- PhysicsPhysical Review C
- 2019

The equation of state (EoS) of neutron star matter, constrained by the existence of two-solar-mass stars and gravitational wave signals from neutron star mergers, is analysed using the Landau theory…

### From QCD symmetries to nuclei and neutron stars

- PhysicsInternational Journal of Modern Physics E
- 2018

Global symmetries and symmetry breaking patterns of QCD with light quarks, in particular chiral symmetry, provide basic guidance not only for low-energy hadron physics but also for nuclear forces and…

### Quarkyonic Matter and Neutron Stars.

- PhysicsPhysical review letters
- 2019

This work makes a simple model of quarkyonic matter and shows that generically the sound velocity is a nonmonotonic function of density-it reaches a maximum at relatively low density, decreases, and then increases again to its asymptotic value of 1/sqrt[3].

### Gravitational waves from binary neutron stars

- PhysicsArabian Journal of Mathematics
- 2022

I review the current global status of research on gravitational waves emitted from mergers of binary neutron star systems, focusing on general-relativistic simulations and their use to interpret data…

### A Pedagogical Discussion of Quarkyonic Matter and Its Implication for Neutron Stars

- Physics
- 2020

This paper is a brief pedagogical review of the ideas that motivate the concept of Quarkyonic Matter. If Nc is the number of quark colors, baryonic matter at very high density and low temperature…

### Excluded-volume model for quarkyonic matter. II. Three-flavor shell-like distribution of baryons in phase space

- Physics
- 2020

We extend the excluded volume model of iso-spin symmetric two-flavor dense Quarkyonic matter including strange baryons and quarks and address its implications for neutron stars. The effective size of…

### Fluctuations and phases in baryonic matter

- PhysicsThe European Physical Journal A
- 2021

The phase structure of baryonic matter is investigated with focus on the role of fluctuations beyond the mean-field approximation. The prototype test case studied is the chiral nucleon-meson model,…

### Excluded-volume model for quarkyonic matter: Three-flavor baryon-quark mixture

- Physics
- 2020

The single-flavor excluded-volume model based on the effective size of baryons reproduces the hard-soft density evolution of the equation of state (EoS) required by the recent studies of GW170817.…

## References

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- PhysicsScience
- 2004

Observations that include studies of pulsars in binary systems, thermal emission from isolated neutron stars, glitches from pulsars, and quasi-periodic oscillations from accreting neutron stars provide information about neutron star masses, radii, temperatures, ages, and internal compositions.

### EQUATION OF STATE AND NEUTRON STAR PROPERTIES CONSTRAINED BY NUCLEAR PHYSICS AND OBSERVATION

- Physics
- 2013

Microscopic calculations of neutron matter based on nuclear interactions derived from chiral effective field theory, combined with the recent observation of a 1.97 ± 0.04 M☉ neutron star, constrain…

### Shapiro delay measurement of a two solar mass neutron star

- Physics
- 2010

Neutron stars are composed of the densest form of matter known to exist in our universe, and thus provide a unique laboratory for exploring the properties of cold matter at supranuclear density.…

### Binary neutron star mergers: a review of Einstein’s richest laboratory

- PhysicsReports on progress in physics. Physical Society
- 2017

The recent progress in understanding what could be considered Einstein's richest laboratory is reviewed, highlighting in particular the numerous significant advances of the last decade in models, techniques and results for fully general-relativistic dynamical simulations.

### A two-solar-mass neutron star measured using Shapiro delay

- PhysicsNature
- 2010

Radio timing observations of the binary millisecond pulsar J1614-2230 that show a strong Shapiro delay signature are presented and the pulsar mass is calculated to be (1.97 ± 0.04)M⊙, which rules out almost all currently proposed hyperon or boson condensate equations of state.

### Holographic Quark Matter and Neutron Stars.

- PhysicsPhysical review letters
- 2016

It is predicted that no quark matter exists inside neutron stars because the Tolman-Oppenheimer-Volkov equations with the resulting hybrid EOSs find maximal stellar masses in excess of two solar masses.

### Gravitational-Wave Constraints on the Neutron-Star-Matter Equation of State.

- PhysicsPhysical review letters
- 2018

It is concluded that the maximal radius of a 1.4-solar-mass neutron star is 13.6 km, and that the smallest allowed tidal deformability of a similar-mass star is Λ(1.4 M_{⊙})=120.4%.

### Neutron star structure from QCD

- Physics
- 2015

Abstract.In this review article, we argue that our current understanding of the thermodynamic properties of cold QCD matter, originating from first principles calculations at high and low densities,…

### Using Gravitational-wave Observations and Quasi-universal Relations to Constrain the Maximum Mass of Neutron Stars

- Physics
- 2017

Combining the GW observations of merging systems of binary neutron stars and quasi-universal relations, we set constraints on the maximum mass that can be attained by nonrotating stellar models of…

### CONSTRAINING NEUTRON STAR MATTER WITH QUANTUM CHROMODYNAMICS

- Physics
- 2014

In recent years, there have been several successful attempts to constrain the equation of state of neutron star matter using input from low-energy nuclear physics and observational data. We…