Equation of state of asymmetric nuclear matter and the tidal deformability of neutron star
Neutron star (NS) is a unique astronomical compact object where the four fundamental interactions have been revealed from the observation and studied in different ways. While the macroscopic properties of NS like mass and radius can be determined within t
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| Main Authors: | , , |
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| Format: | Bài trích |
| Language: | eng |
| Published: |
The European Physical Journal A
2021
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| Online Access: | https://link.springer.com/article/10.1140%2Fepja%2Fs10050-021-00467-y https://dlib.phenikaa-uni.edu.vn/handle/PNK/2735 https://doi.org/10.1140/epja/s10050-021-00467-y |
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| Summary: | Neutron star (NS) is a unique astronomical compact object where the four fundamental interactions have been revealed from the observation and studied in different ways. While the macroscopic properties of NS like mass and radius can be determined within t |
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