Structure Factors for Hot Neutron Matter from <i>Ab Initio</i> Lattice Simulations with High-Fidelity Chiral Interactions-Reference-Cited by-同舟云学术

Structure Factors for Hot Neutron Matter from Ab Initio Lattice Simulations with High-Fidelity Chiral Interactions

Published:2024-06-05 Issue:23 Volume:132 Page:
ISSN:0031-9007
Container-title:Physical Review Letters
language:en
Short-container-title:Phys. Rev. Lett.

Author:

Ma Yuan-Zhuo¹²^ORCID,Lin Zidu³^ORCID,Lu Bing-Nan⁴^ORCID,Elhatisari Serdar⁵⁶^ORCID,Lee Dean²^ORCID,Li Ning⁷^ORCID,Meißner Ulf-G.⁶⁸⁹^ORCID,Steiner Andrew W.³¹⁰^ORCID,Wang Qian¹^ORCID

Affiliation:

1. South China Normal University

2. Michigan State University

3. University of Tennessee

4. Graduate School of China Academy of Engineering Physics

5. Gaziantep Islam Science and Technology University

6. Universität Bonn

7. Sun Yat-Sen University

8. Forschungszentrum Jülich

9. Tbilisi State University

10. Oak Ridge National Laboratory

Funder

National Natural Science Foundation of China

China Postdoctoral Science Foundation

National Science Foundation

Office of Nuclear Energy

National Safety Academic Fund

U.S. Department of Energy

H2020 European Research Council

Deutsche Forschungsgemeinschaft

Chinese Academy of Sciences

Volkswagen Foundation

Ministerium für Kultur und Wissenschaft des Landes Nordrhein-Westfalen

Natural Science Foundation of Guangdong Province

South China Normal University

Gauss Centre for Supercomputing

Jülich Supercomputing Centre, Forschungszentrum Jülich

Michigan State University

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevLett.132.232502/fulltext

Reference61 articles.

1. ASCERTAINING THE CORE COLLAPSE SUPERNOVA MECHANISM: The State of the Art and the Road Ahead

2. Neutrino opacities in nuclear matter

3. Colloquium: Perspectives on core-collapse supernova theory

4. Core-collapse supernova explosion theory

5. Effects of nuclear forces on neutrino opacities in hot nuclear matter