Origin of the heaviest elements: The rapid neutron-capture process-Reference-Cited by-同舟云学术

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

Published:2021-02-01 Issue:1 Volume:93 Page:
ISSN:0034-6861
Container-title:Reviews of Modern Physics
language:en
Short-container-title:Rev. Mod. Phys.

Author:

Cowan John J.^ORCID,Sneden Christopher^ORCID,Lawler James E.^ORCID,Aprahamian Ani^ORCID,Wiescher Michael^ORCID,Langanke Karlheinz,Martínez-Pinedo Gabriel^ORCID,Thielemann Friedrich-Karl^ORCID

Funder

National Aeronautics and Space Administration

National Science Foundation

Deutsche Forschungsgemeinschaft

H2020 European Research Council

Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung

Extreme Matter Institute

COST Actions NewCompstar

Publisher

American Physical Society (APS)

Subject

General Physics and Astronomy

Link

http://harvest.aps.org/v2/journals/articles/10.1103/RevModPhys.93.015002/fulltext

Reference945 articles.

1. Multi-messenger Observations of a Binary Neutron Star Merger

2. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

3. On the Progenitor of Binary Neutron Star Merger GW170817

4. Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817

5. Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

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