Roto-Chemical Heating with Fall-Back Disk Accretion in the Neutron Stars Containing Quark Matter
Probing quark matter is one of the important tasks in the studies of neutron stars (NS). Some works explicitly consider the existence of quark matter in the appearance of hybrid star (HS) or pure quark star (QS). In the present work, we study the roto-chemical heating with accretion in HS and QS, an...
Main Authors: | Wei Wei, Xin-Yu Xu, Kai-Tuo Wang, Xiao-Hang Ma |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2020-04-01
|
Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/6/5/62 |
Similar Items
-
Phases of Hadron-Quark Matter in (Proto) Neutron Stars
by: Fridolin Weber, et al.
Published: (2019-07-01) -
Quark Deconfinement in Rotating Neutron Stars
by: Richard D. Mellinger, et al.
Published: (2017-01-01) -
The Structure of the Hadron-Quark Combustion Zone
by: Amir Ouyed, et al.
Published: (2019-06-01) -
Neutron-Star-Merger Equation of State
by: Veronica Dexheimer, et al.
Published: (2019-05-01) -
Hadron–Quark Combustion as a Nonlinear, Dynamical System
by: Amir Ouyed, et al.
Published: (2018-03-01)