EPJ Web Conf.
Volume 168, 2018Joint International Conference of ICGAC-XIII and IK-15 on Gravitation, Astrophysics and Cosmology
|Number of page(s)||4|
|Published online||09 January 2018|
Role of strangeness to the neutron star mass and cooling
Department of Physics, Pusan National University, Busan 46241, Korea
2 Cyclotron Institute, Texas A&M University, College Station, TX 77843, USA
3 Department of Physics Education, Daegu University, Gyeongsan 38453, Korea
4 Department of Physics, Ulsan National Institue of Science and Technology (UNIST), Ulsan 44919, Korea
* e-mail: email@example.com
Published online: 9 January 2018
Neutron star provides unique environments for the investigation of the physics of extreme dense matter beyond normal nuclear saturation density. In such high density environments, hadrons with strange quarks are expected to play very important role in stabilizing the system. Kaons and hyperons are the lowest mass states with strangeness among meson and bayron families, respectively. In this work, we investigate the role of kaons and hyperons to the neutron star mass, and discuss their role in the neutron star cooling.
© 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/).
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