Volume 2127: Xiamen-CUSTIPEN Workshop on the Equation of State of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy
Volume 2127: Xiamen-CUSTIPEN Workshop on the Equation of State of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy
By Ang Li, Bao-An Li and Furong Xu
Volume 2127 is the proceedings of Xiamen-CUSTIPEN Workshop on the Equation of State of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy (3–7 January 2019, Xiamen, China)
Title information
The Equation of State (EOS) of matter is the relationship among pressure, density, temperature and composition of the matter. To determine the EOS of dense neutron-rich nuclear matter has been a longstanding goal of both astrophysics and nuclear physics. Articles in this proceeding of the Xiamen-CUSTIPEN Workshop on the EOS of Dense Neutron-Rich Nuclear Matter in the Era of Gravitational Waves summarize the latest development in this field. The main topics include
- EOS of Neutron-Rich Matter from Nuclear Theories and Terrestrial Experiments
- Properties of Neutron Stars from Theories and Observations
- Impacts of Nuclear EOS on the Evolution Dynamics and Products of Compact Binaries
- Imprints of Nuclear EOS on Gravitational Waves from Various Sources
- Nature of Dense Matter and Synthesis of Heavy Elements in the Cosmos
- Isospin Dependence of Strong Interactions and Correlations in Dense Matter
These proceedings will be of interest to: Researchers and graduate students in nuclear astrophysics, gravitational waves and nuclear physics.
For further information about this volume: Please view the table of contents available on AIP Publishing's Scitation platform: Volume 2127 table of contents.
