From hadrons to quarks in neutron stars: a review

G Baym, T Hatsuda, T Kojo, PD Powell… - Reports on Progress …, 2018 - iopscience.iop.org
In recent years our understanding of neutron stars has advanced remarkably, thanks to
research converging from many directions. The importance of understanding neutron star …

Neutron-star tidal deformability and equation-of-state constraints

K Chatziioannou - General Relativity and Gravitation, 2020 - Springer
Despite their long history and astrophysical importance, some of the key properties of
neutron stars are still uncertain. The extreme conditions encountered in their interiors …

Modified gravity and cosmology

EN Saridakis, R Lazkoz, V Salzano, PV Moniz… - 2021 - Springer
The dawn of the twenty-first century came with very positive prospects for gravity, cosmology,
and astrophysics. Technological progress made it possible for cosmology to enter to its …

Heavy baryons in compact stars

A Sedrakian, JJ Li, F Weber - Progress in Particle and Nuclear Physics, 2023 - Elsevier
We review the physics of hyperons and Δ-resonances in dense matter in compact stars. The
covariant density functional approach to the equation of state and composition of dense …

Masses, radii, and the equation of state of neutron stars

F Özel, P Freire - Annual Review of Astronomy and Astrophysics, 2016 - annualreviews.org
We summarize our current knowledge of neutron-star masses and radii. Recent
instrumentation and computational advances have resulted in a rapid increase in the …

The equation of state of hot, dense matter and neutron stars

JM Lattimer, M Prakash - Physics Reports, 2016 - Elsevier
Recent developments in the theory of pure neutron matter and experiments concerning the
symmetry energy of nuclear matter, coupled with recent measurements of high-mass …

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

L Baiotti - Progress in Particle and Nuclear Physics, 2019 - Elsevier
In this article, I introduce ideas and techniques to extract information about the equation of
state of matter at very high densities from gravitational waves emitted before, during and …

GW170817: Measurements of neutron star radii and equation of state

BP Abbott, R Abbott, TD Abbott, F Acernese, K Ackley… - Physical review …, 2018 - APS
On 17 August 2017, the LIGO and Virgo observatories made the first direct detection of
gravitational waves from the coalescence of a neutron star binary system. The detection of …

Time-domain effective-one-body gravitational waveforms for coalescing compact binaries with nonprecessing spins, tides, and self-spin effects

A Nagar, S Bernuzzi, W Del Pozzo… - Physical Review D, 2018 - APS
We present TEOBResumS, a new effective-one-body (EOB) waveform model for
nonprecessing (spin-aligned) and tidally interacting compact binaries. Spin-orbit and spin …

Black hole perturbation theory and gravitational self-force

A Pound, B Wardell - Handbook of Gravitational Wave Astronomy, 2022 - Springer
Much of the success of gravitational-wave astronomy rests on perturbation theory.
Historically, perturbative analysis of gravitational-wave sources has largely focused on post …