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https://hdl.handle.net/2440/134489
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Type: | Journal article |
Title: | The role of baryon structure in neutron stars |
Author: | Motta, T.F. Thomas, A.W. |
Citation: | Modern Physics Letters A, 2022; 37(1):1-30 |
Publisher: | World Scientific Publishing |
Issue Date: | 2022 |
ISSN: | 0217-7323 1793-6632 |
Statement of Responsibility: | Theo F. Motta and Anthony W. Thomas |
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. |
Keywords: | Equation of state; dense matter; neutron stars; hadron structure; change of hadron structure in-medium; quarks; mean-fields |
Rights: | Copyright Status Unknown |
DOI: | 10.1142/S0217732322300014 |
Grant ID: | http://purl.org/au-research/grants/arc/DP180100497 http://purl.org/au-research/grants/arc/CE200100008 |
Published version: | http://dx.doi.org/10.1142/s0217732322300014 |
Appears in Collections: | Physics publications |
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