Investigations of spinodal dynamics in asymmetric nuclear matter within a stochastic relativistic model
dc.citation.epage | 11 | en_US |
dc.citation.issueNumber | 3 | en_US |
dc.citation.spage | 1 | en_US |
dc.citation.volumeNumber | 49 | en_US |
dc.contributor.author | Yilmaz, O. | en_US |
dc.contributor.author | Ayik, S. | en_US |
dc.contributor.author | Acar, F. | en_US |
dc.contributor.author | Saatci, S. | en_US |
dc.contributor.author | Gokalp, A. | en_US |
dc.date.accessioned | 2015-07-28T11:56:53Z | |
dc.date.available | 2015-07-28T11:56:53Z | |
dc.date.issued | 2013 | en_US |
dc.department | Department of Physics | en_US |
dc.description.abstract | Early development of spinodal instabilities and density correlation functions in asymmetric nuclear matter are investigated in the stochastic extension of the Walecka-type relativistic mean field including coupling with rho meson. Calculations are performed under typical conditions encountered in heavy-ion collisions and in the crusts of neutron stars. In general, growth of instabilities occur relatively slower for increasing charge asymmetry of matter. At higher densities around rho = 0.4 rho(0) fluctuations grow relatively faster in the quantal description than those found in the semi-classical limit. Typical sizes of early condensation regions extracted from density correlation functions are consistent with those found from dispersion relations of the unstable collective modes. | en_US |
dc.identifier.doi | 10.1140/epja/i2013-13033-8 | en_US |
dc.identifier.eissn | 1434-601X | |
dc.identifier.issn | 1434-6001 | |
dc.identifier.uri | http://hdl.handle.net/11693/11110 | |
dc.language.iso | English | en_US |
dc.publisher | Springer-Verlag | en_US |
dc.relation.isversionof | http://dx.doi.org/10.1140/epja/i2013-13033-8 | en_US |
dc.source.title | European Physical Journal A : Hadrons and Nuclei | en_US |
dc.subject | Mean-field Theory | en_US |
dc.subject | Instabilities | en_US |
dc.subject | Density | en_US |
dc.title | Investigations of spinodal dynamics in asymmetric nuclear matter within a stochastic relativistic model | en_US |
dc.type | Article | en_US |
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