[HTML][HTML] Gravitational-wave physics and astronomy in the 2020s and 2030s

M Bailes, BK Berger, PR Brady, M Branchesi… - Nature Reviews …, 2021 - nature.com
The 100 years since the publication of Albert Einstein's theory of general relativity saw
significant development of the understanding of the theory, the identification of potential …

The faintest dwarf galaxies

JD Simon - Annual Review of Astronomy and Astrophysics, 2019 - annualreviews.org
The lowest luminosity (L) Milky Way satellite galaxies represent the extreme lower limit of the
galaxy luminosity function. These ultra-faint dwarfs are the oldest, most dark matter …

Constraints on the dense matter equation of state and neutron star properties from NICER's mass–radius estimate of PSR J0740+ 6620 and multimessenger …

G Raaijmakers, SK Greif, K Hebeler… - The Astrophysical …, 2021 - iopscience.iop.org
In recent years our understanding of the dense matter equation of state (EOS) of neutron
stars has significantly improved by analyzing multimessenger data from radio/X-ray pulsars …

Bayesian inference for compact binary coalescences with bilby: validation and application to the first LIGO–Virgo gravitational-wave transient catalogue

IM Romero-Shaw, C Talbot… - Monthly Notices of …, 2020 - academic.oup.com
Gravitational waves provide a unique tool for observational astronomy. While the first LIGO–
Virgo catalogue of gravitational-wave transients (GWTC-1) contains 11 signals from black …

Binary black hole population properties inferred from the first and second observing runs of Advanced LIGO and Advanced Virgo

BP Abbott, R Abbott, TD Abbott… - The Astrophysical …, 2019 - iopscience.iop.org
The second LIGO/Virgo observing run (O2) spanned 9 months between 2016 November
and 2017 August, building on the first, 4-month run (O1) in 2015. The LIGO/Virgo …

Identification of strontium in the merger of two neutron stars

D Watson, CJ Hansen, J Selsing, A Koch, DB Malesani… - Nature, 2019 - nature.com
Half of all of the elements in the Universe that are heavier than iron were created by rapid
neutron capture. The theory underlying this astrophysical r-process was worked out six …

Multimessenger constraints on the neutron-star equation of state and the Hubble constant

T Dietrich, MW Coughlin, PTH Pang, M Bulla, J Heinzel… - Science, 2020 - science.org
Observations of neutron-star mergers with distinct messengers, including gravitational
waves and electromagnetic signals, can be used to study the behavior of matter denser than …

Origin of the heaviest elements: The rapid neutron-capture process

JJ Cowan, C Sneden, JE Lawler, A Aprahamian… - Reviews of Modern …, 2021 - APS
The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …

Origin of the heavy elements in binary neutron-star mergers from a gravitational-wave event

D Kasen, B Metzger, J Barnes, E Quataert… - Nature, 2017 - nature.com
The cosmic origin of elements heavier than iron has long been uncertain. Theoretical
modelling,,,,,, shows that the matter that is expelled in the violent merger of two neutron stars …