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https://hdl.handle.net/2440/134489
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DC Field | Value | Language |
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dc.contributor.author | Motta, T.F. | - |
dc.contributor.author | Thomas, A.W. | - |
dc.date.issued | 2022 | - |
dc.identifier.citation | Modern Physics Letters A, 2022; 37(1):1-30 | - |
dc.identifier.issn | 0217-7323 | - |
dc.identifier.issn | 1793-6632 | - |
dc.identifier.uri | https://hdl.handle.net/2440/134489 | - |
dc.description.abstract | Understanding the equation of state of dense nuclear matter is a fundamental challenge for nuclear physics. It is an especially timely and interesting challenge as we have reached a period where neutron stars, which contain the most dense nuclear matter in the Universe, are now being studied in completely new ways, from gravitational waves to satellite-based telescopes. We review the theoretical approaches to calculating this equation of state which involve a change in the structure of the baryons, along with their predictions for neutron star properties. | - |
dc.description.statementofresponsibility | Theo F. Motta and Anthony W. Thomas | - |
dc.language.iso | en | - |
dc.publisher | World Scientific Publishing | - |
dc.rights | Copyright Status Unknown | - |
dc.source.uri | http://dx.doi.org/10.1142/s0217732322300014 | - |
dc.subject | Equation of state; dense matter; neutron stars; hadron structure; change of hadron structure in-medium; quarks; mean-fields | - |
dc.title | The role of baryon structure in neutron stars | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1142/S0217732322300014 | - |
dc.relation.grant | http://purl.org/au-research/grants/arc/DP180100497 | - |
dc.relation.grant | http://purl.org/au-research/grants/arc/CE200100008 | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Thomas, A.W. [0000-0003-0026-499X] | - |
Appears in Collections: | Physics publications |
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