QCD equations of state and speed of sound in neutron stars
Abstract Neutron stars are cosmic laboratories to study dense matter in quantum chromodynamics (QCD). The observable mass-radius relations of neutron stars are determined by QCD equations of state and can reflect the properties of QCD phase transitions. In the last decade, there have been historical...
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| Format: | Article |
| Language: | English |
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Springer
2021-04-01
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| Series: | AAPPS Bulletin |
| Online Access: | https://doi.org/10.1007/s43673-021-00011-6 |