Fluctuations in the composition of nuclear pasta in symmetric nuclear matter at finite temperature

Celso C. Barros, Jr., Débora P. Menezes, and Francesca Gulminelli
Phys. Rev. C 101, 035211 – Published 30 March 2020

Abstract

The equilibrium distributions of the different pasta geometries and their linear sizes are calculated from the mean field Gibbs energy functional in symmetric nuclear matter at finite temperature. The average sizes and shapes coincide approximately with the ones predicted by a standard pasta calculation in the coexisting phase approximation, but fluctuations are additionally calculated and seen to increase with temperature and baryonic density. The different pasta shapes are shown to coexist in a wide domain of density and temperature, in qualitative agreement with the findings of large scale molecular dynamics simulations, but with a much less expensive computational cost.

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  • Received 6 November 2019
  • Revised 5 February 2020
  • Accepted 19 February 2020

DOI:https://doi.org/10.1103/PhysRevC.101.035211

©2020 American Physical Society

Physics Subject Headings (PhySH)

Nuclear Physics

Authors & Affiliations

Celso C. Barros, Jr.1, Débora P. Menezes1, and Francesca Gulminelli2

  • 1Depto de Física, CFM, Universidade Federal de Santa Catarina Florianópolis, SC, CP. 476, CEP 88.040, 900, Brazil
  • 2CNRS and ENSICAEN, UMR6534, LPC, 14050 Caen cédex, France

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Issue

Vol. 101, Iss. 3 — March 2020

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