Revisiting the Constraint on the Equation of State of Neutron Stars Based on Binary Neutron Star Mergers
The merger of a neutron star (NS)–NS binary can form different productions of compact remnants, among which a supramassive NS (SMNS) can create an internal plateau, and the following steep decay marks the collapse of the SMNS. The proportion of the SMNS and the corresponding collapse time are often...
I tiakina i:
| Ngā kaituhi matua: | , , , |
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| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
IOP Publishing
2024-01-01
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| Rangatū: | The Astrophysical Journal |
| Ngā marau: | |
| Urunga tuihono: | https://doi.org/10.3847/1538-4357/ad4452 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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