https://doi.org/10.1051/epjconf/201817303003
Model of the Phase Transition Mimicking the Pasta Phase in Cold and Dense Quark-Hadron Matter
1 Joint Institute for Nuclear Research, Joliot-Curie 6, 141980 Dubna, Russia
2 Yerevan State University, Alek Manyukyan 1, 0025 Yerevan, Republic of Armenia
* e-mail: ayriyan@jinr.ru
** e-mail: hovik.grigorian@gmail.com
Published online: 14 February 2018
A simple mixed phase model mimicking so-called “pasta” phases in the quarkhadron phase transition is developed and applied to static neutron stars for the case of DD2 type hadronic and NJL type quark matter models. The influence of the mixed phase on the mass-radius relation of the compact stars is investigated. Model parameters are chosen such that the results are in agreement with the mass-radius constraints.
© The Authors, published by EDP Sciences, 2018
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. (http://creativecommons.org/licenses/by/4.0/).
