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This book provides an introduction to contemporary research in the physics of dense matter, which refers to matter in the density range 500 - 1017 g/cm3. The presentation is intended for the application of dense matter physics to astrophysical problems, such as those manifested in the supernova process and in the structure of the neutron star.
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This book provides an introduction to contemporary research in the physics of dense matter, which refers to matter in the density range 500 - 1017 g/cm3. The presentation is intended for the application of dense matter physics to astrophysical problems, such as those manifested in the supernova process and in the structure of the neutron star.