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 elements

A Arcones, FK Thielemann - The Astronomy and Astrophysics Review, 2023 - Springer
What is the origin of the oxygen we breathe, the hydrogen and oxygen (in form of water
H2O) in rivers and oceans, the carbon in all organic compounds, the silicon in electronic …

A kilonova as the electromagnetic counterpart to a gravitational-wave source

SJ Smartt, TW Chen, A Jerkstrand, M Coughlin… - Nature, 2017 - nature.com
Gravitational waves were discovered with the detection of binary black-hole mergers and
they should also be detectable from lower-mass neutron-star mergers. These are predicted …

Binary neutron star mergers: mass ejection, electromagnetic counterparts, and nucleosynthesis

D Radice, A Perego, K Hotokezaka… - The Astrophysical …, 2018 - iopscience.iop.org
We present a systematic numerical relativity study of the mass ejection and the associated
electromagnetic transients and nucleosynthesis from binary neutron star (NS) mergers. We …

Illuminating gravitational waves: A concordant picture of photons from a neutron star merger

MM Kasliwal, E Nakar, LP Singer, DL Kaplan, DO Cook… - Science, 2017 - science.org
Merging neutron stars offer an excellent laboratory for simultaneously studying strong-field
gravity and matter in extreme environments. We establish the physical association of an …

Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger

I Arcavi, G Hosseinzadeh, DA Howell, C McCully… - Nature, 2017 - nature.com
The merger of two neutron stars has been predicted to produce an optical–infrared transient
(lasting a few days) known as a 'kilonova', powered by the radioactive decay of neutron-rich …

The combined ultraviolet, optical, and near-infrared light curves of the kilonova associated with the binary neutron star merger GW170817: unified data set, analytic …

VA Villar, J Guillochon, E Berger… - The Astrophysical …, 2017 - iopscience.iop.org
We present the first effort to aggregate, homogenize, and uniformly model the combined
ultraviolet, optical, and near-infrared data set for the electromagnetic counterpart of the …

Gigaelectronvolt emission from a compact binary merger

A Mei, B Banerjee, G Oganesyan, OS Salafia… - Nature, 2022 - nature.com
An energetic γ-ray burst (GRB), GRB 211211A, was observed on 11 December 2021,.
Despite its long duration, typically associated with bursts produced by the collapse of …

Black holes, gravitational waves and fundamental physics: a roadmap

L Barack, V Cardoso, S Nissanke… - … and quantum gravity, 2019 - iopscience.iop.org
70 AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France

Swift and NuSTAR observations of GW170817: Detection of a blue kilonova

PA Evans, SB Cenko, JA Kennea, SWK Emery… - Science, 2017 - science.org
With the first direct detection of merging black holes in 2015, the era of gravitational wave
(GW) astrophysics began. A complete picture of compact object mergers, however, requires …