scholarly journals On parametrized cold dense matter equation-of-state inference

2018 ◽  
Vol 478 (1) ◽  
pp. 1093-1131 ◽  
Author(s):  
Thomas E Riley ◽  
Geert Raaijmakers ◽  
Anna L Watts
Keyword(s):  
Equation Of State ◽  
Dense Matter ◽  
Cold Dense Matter ◽  
State Inference

scholarly journals Equation of state constraints for the cold dense matter inside neutron stars using the cooling tail method

2016 ◽  
Vol 591 ◽  
pp. A25 ◽  
Author(s):  
J. Nättilä ◽  
A. W. Steiner ◽  
J. J. E. Kajava ◽  
V. F. Suleimanov ◽  
J. Poutanen
Keyword(s):  
Equation Of State ◽  
Neutron Stars ◽  
State Constraints ◽  
Dense Matter ◽  
Cold Dense Matter

An Equation of State of Cold Dense Matter

1975 ◽  
Vol 53 (3) ◽  
pp. 891-893 ◽  
Author(s):  
A. Nishimura ◽  
Y. Yamaguchi
Keyword(s):  
Equation Of State ◽  
Dense Matter ◽  
Cold Dense Matter

scholarly journals Role of Δs in determining the properties of neutron stars in parameterized hydrostatic equilibrium

2019 ◽  
Vol 28 (09) ◽  
pp. 1950122 ◽  
Author(s):  
Debashree Sen
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Dense Matter ◽  
Hydrostatic Equilibrium ◽  
Chiral Model ◽  
Equilibrium Conditions ◽  
Self Gravity ◽  
Cold Dense Matter ◽  
Baryonic Mass

The possible existence of [Formula: see text] resonances is inspected in the cold dense matter of neutron star (NS) core in the presence of hyperons. The diverse effects of variation in [Formula: see text] mass on their formation and the equation of state (EoS) are studied in this work with an effective chiral model and the resultant NS properties are calculated with the help of parameterized Tolman–Oppenheimer–Volkoff (PTOV) equations to bring out the two important features of pressure in the context of massive NSs. The [Formula: see text] puzzle is re-explored and resolved taking into account the concept of modified/parametrized inertial pressure and self-gravity in case of massive pulsars like PSR J1614−2230 and PSR J0348-0432. It is seen that although the presence of exotic matter like the hyperons and [Formula: see text] softens the EoS considerably, their presence in massive NSs can be successfully explained with the theory of parametrized hydrostatic equilibrium conditions. The results of this work also satisfy the constraints on [Formula: see text] and [Formula: see text] from the gravitational wave (GW170817) detection of binary NS merger. The constraint on baryonic mass from PSR J0737-3039 is also satisfied with the solutions of the PTOV equations for all the [Formula: see text] masses considered.

scholarly journals Probing the neutron star interior and the Equation of State of cold dense matter with the SKA

2015 ◽  
Author(s):  
Anna Watts ◽  
Cristobal M. Espinoza ◽  
Renxin Xu ◽  
Nils Andersson ◽  
John Antoniadis ◽  
...  
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Dense Matter ◽  
Cold Dense Matter

scholarly journals Constraints on the equation of state of cold dense matter from nuclear physics and astrophysics

2014 ◽  
Vol 66 ◽  
pp. 07005 ◽  
Author(s):  
A. F. Fantina ◽  
N. Chamel ◽  
J. M. Pearson ◽  
S. Goriely
Keyword(s):  
Equation Of State ◽  
Nuclear Physics ◽  
Dense Matter ◽  
Cold Dense Matter

scholarly journals Determination of the Equation of State of Dense Matter

Science ◽  
2002 ◽  
Vol 298 (5598) ◽  
pp. 1592-1596 ◽  
Author(s):  
P.&l. Danielewicz
Keyword(s):  
Equation Of State ◽  
Dense Matter

scholarly journals Investigation on equation of state and ionization equilibrium for aluminum in warm dense matter regime

2020 ◽  
Vol 69 (9) ◽  
pp. 099101
Author(s):  
Tian-Hao Wang ◽  
Kun Wang ◽  
Yue Zhang ◽  
Lin-Cun Jiang
Keyword(s):  
Equation Of State ◽  
Dense Matter ◽  
Warm Dense Matter ◽  
Ionization Equilibrium
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