Please use this identifier to cite or link to this item:
http://hdl.handle.net/2248/3902
Title: | Nuclear matter in the derivative scalar coupling model. Energy per nucleon and a finite temperature equation of state |
Authors: | Datta, B Sahu, P. K |
Keywords: | Scalar coupling model Nucleon Binding energy Supernova |
Issue Date: | 2-Dec-1993 |
Publisher: | Elsevier Science B.V. |
Citation: | Physics Letters B, Vol. 318, No. 2, pp. 277 - 280 |
Abstract: | We calculate an equation of state of nuclear matter based on the derivative scalar coupling model proposed by Zimanyi and Moszkowski, using improved values of the saturation density and binding energy. Comparison of this model's prediction for the energy per nucleon is made with available estimates from heavy-ion collision data and with the theoretical requirement for a prompt type II supernova bounce. We also derive a finite temperature equation of state for nuclear matter based on this model |
Description: | Restricted Access |
URI: | http://hdl.handle.net/2248/3902 |
ISSN: | 0370-2693 |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Nuclear matter in the derivative scalar coupling model. Restricted Access | Restricted Access | 286.23 kB | Adobe PDF | View/Open Request a copy |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.