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
Lưu vào:
| Tác giả chính: | , , |
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| Định dạng: | Bài trích |
| Ngôn ngữ: | eng |
| Nhà xuất bản: |
The European Physical Journal A
2021
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| Truy cập trực tuyến: | 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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| Tóm tắt: | 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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