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| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Ngo Hai Tan | - |
| dc.contributor.author | Dao T. Khoa | - |
| dc.contributor.author | Doan Thi Loan | - |
| dc.date.accessioned | 2021-09-10T04:46:51Z | - |
| dc.date.available | 2021-09-10T04:46:51Z | - |
| dc.date.issued | 2021 | - |
| dc.identifier.uri | https://link.springer.com/article/10.1140%2Fepja%2Fs10050-021-00467-y | - |
| dc.identifier.uri | https://dlib.phenikaa-uni.edu.vn/handle/PNK/2735 | - |
| dc.description.abstract | 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 | vi |
| dc.language.iso | eng | vi |
| dc.publisher | The European Physical Journal A | vi |
| dc.title | Equation of state of asymmetric nuclear matter and the tidal deformability of neutron star | vi |
| dc.type | Bài trích | vi |
| eperson.identifier.doi | https://doi.org/10.1140/epja/s10050-021-00467-y | - |
| Appears in Collections | Bài báo khoa học | |
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