How the HESS J1731-347 object could be explained using K− condensation
The recent observation of a compact star with a mass of M=0.77−0.17+0.20M⊙ and a radius of R=10.4−0.78+0.86 km, located within the supernova remnant HESS J1731-347, has substantially reinforced the evidence for the presence of exotic matter in neutron stars core. This finding has markedly enhanced o...
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| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Elsevier
2025-01-01
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| Series: | Physics Letters B |
| Subjects: | |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269324007433 |
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