Superfluid Phonons in Neutron Star Core
In neutron stars the nuclear asymmetric matter is expected to undergo phase transitions to a superfluid state. According to simple estimates, neutron matter in the inner crust and just below should be in the s-wave superfluid phase, corresponding to the neutron-neutron <inline-formula><math...
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| Aineistotyyppi: | Artikkeli |
| Kieli: | English |
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MDPI AG
2021-01-01
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| Sarja: | Universe |
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| Linkit: | https://www.mdpi.com/2218-1997/7/1/16 |