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A Study of the Isoscalar Giant Monopole ResonanceSummary and Current Status

A Study of the Isoscalar Giant Monopole Resonance: Summary and Current Status [The nuclear matter equation of state (EOS) plays an important role in our understanding of nuclear bulk properties, as well as processes taking place in the stellar environments (i.e. dynamics of supernovae collapse and structure of neutron stars). The EOS also sheds light on the phase transitions taking place in the heavy ion collision reactions. Its exact determination is being pursued extensively, both experimentally and theoretically. Nuclear incompressibility is an important parameter of the nuclear matter EOS. The centroid energy of one of the nuclear compression modes – the isoscalar Giant Monopole Resonance (ISGMR) – is a direct experimental tool to constrain the value of nuclear matter incompressibility.] http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png

A Study of the Isoscalar Giant Monopole ResonanceSummary and Current Status

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Publisher
Springer International Publishing
Copyright
© Springer International Publishing Switzerland 2016
ISBN
978-3-319-22206-6
Pages
73 –76
DOI
10.1007/978-3-319-22207-3_6
Publisher site
See Chapter on Publisher Site

Abstract

[The nuclear matter equation of state (EOS) plays an important role in our understanding of nuclear bulk properties, as well as processes taking place in the stellar environments (i.e. dynamics of supernovae collapse and structure of neutron stars). The EOS also sheds light on the phase transitions taking place in the heavy ion collision reactions. Its exact determination is being pursued extensively, both experimentally and theoretically. Nuclear incompressibility is an important parameter of the nuclear matter EOS. The centroid energy of one of the nuclear compression modes – the isoscalar Giant Monopole Resonance (ISGMR) – is a direct experimental tool to constrain the value of nuclear matter incompressibility.]

Published: Dec 25, 2015

Keywords: Symmetry Energy; Giant Resonance; Centroid Energy; Supernova Collapse; Nuclear Matter Equation

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