Experimental perspective on three-dimensional topological semimetals
Topological semimetals (TSMs) are characterized by bulk band crossings in their electronic
structures, which are expected to give rise to gapless electronic excitations and topological …
structures, which are expected to give rise to gapless electronic excitations and topological …
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 …
neutron stars are still uncertain. The extreme conditions encountered in their interiors …
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 …
gravitational waves from the coalescence of a neutron star binary system. The detection of …
Gravitational-wave constraints on the neutron-star-matter Equation of State
The detection of gravitational waves originating from a neutron-star merger, GW170817, by
the LIGO and Virgo Collaborations has recently provided new stringent limits on the tidal …
the LIGO and Virgo Collaborations has recently provided new stringent limits on the tidal …
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 …
state of matter at very high densities from gravitational waves emitted before, during and …
[CITATION][C] Model Comparison from LIGO–Virgo Data on GW170817's Binary Components and Consequences for the Merger Remnant
BP Abbott, R Abbott, TD Abbott, S Abraham… - Default …, 2020 - andrews.elsevierpure.com
Model Comparison from LIGO–Virgo Data on GW170817’s Binary Components and
Consequences for the Merger Remnant — Andrews University Research Portal Skip to main …
Consequences for the Merger Remnant — Andrews University Research Portal Skip to main …
Towards understanding astrophysical effects of nuclear symmetry energy
Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …
Overview of KAGRA: KAGRA science
KAGRA is a newly build gravitational wave observatory, a laser interferometer with 3 km arm
length, located in Kamioka, Gifu, Japan. In this paper, one of a series of articles featuring …
length, located in Kamioka, Gifu, Japan. In this paper, one of a series of articles featuring …
Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections
T Dietrich, T Hinderer, A Samajdar - General Relativity and Gravitation, 2021 - Springer
Gravitational waves emitted from the coalescence of neutron star binaries open a new
window to probe matter and fundamental physics in unexplored, extreme regimes. To extract …
window to probe matter and fundamental physics in unexplored, extreme regimes. To extract …
A long-lived remnant neutron star after GW170817 inferred from its associated kilonova
YW Yu, LD Liu, ZG Dai - The Astrophysical Journal, 2018 - iopscience.iop.org
The successful joint observation of the gravitational wave (GW) event GW170817 and its
multiwavelength electromagnetic counterparts enabled us to witness a definite merger event …
multiwavelength electromagnetic counterparts enabled us to witness a definite merger event …