Massive Neutron Stars with Hadron-Quark Transition Core : phenomenological approach by "3-window model"
Nuclear Theory
2015-12-29 v1
Abstract
By a new approach introducing a "3-window model" and constructing phenomenologically an equation of state for the hadron-quark (HQ) transition region, possible maximum mass of neutron stars (NSs) is discussed. It is found that neutron stars (NSs) with HQ transition core are able to have a mass exceeding two-solar mass, consistent with massive NSs recently observed.
Keywords
Cite
@article{arxiv.1512.08350,
title = {Massive Neutron Stars with Hadron-Quark Transition Core : phenomenological approach by "3-window model"},
author = {Tatsuyuki Takatsuka and Kota Masuda and Tetsuo Hatsuda},
journal= {arXiv preprint arXiv:1512.08350},
year = {2015}
}
Comments
3 pages, 1 figure