Titlebook: Hadrons and Hadronic Matter; D. Vautherin,F. Lenz,J. W. Negele Book 1990 Plenum Press, New York 1990 astrophysics.hadron.quantum chromodyn

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https://doi.org/10.1007/978-3-642-16753-9of single hadrons is concerned. As the historical development already indicates, compositeness together with a simple picture about the underlying confining dynamics is sufficient for a qualitative understanding of hadronic properties in terms of “constituent” quarks.

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Probing the Quark Structure of Matter, take two divergent paths. The first is to ask what constraints more elementary, phenomenological considerations can put on the structure of the nucleón and therefore on the existing QCD-motivated models. The second is to ask how the consequences of different models might vary for the phenomena mentioned.

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https://doi.org/10.1057/9781137337443elativistic nuclear colhsions. These lectures are aimed primarily at graduate students or young post docs with an interest in learning a little something about these subjects, but who have not been actively involved in research on related problems.

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https://doi.org/10.1007/978-3-319-63820-1ay occur in the cores of neutron stars that a transition (of unknown order) to quark matter might occur; the presence of the quark matter has impact on the maximum possible mass for the star (which is lower because of the quark phase) and on the cooling rate of the neutron star (which is enhanced by