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.
