An extended equation of state for gaseous methane determined from the speed of sound

2007 ◽  
Vol 337 (1-3) ◽  
pp. 125-134 ◽  
Author(s):  
K.O. Monago
2021 ◽  
Vol 50 (2) ◽  
pp. 023105
Author(s):  
Tim Eisenbach ◽  
Christian Scholz ◽  
Roland Span ◽  
Diego Cristancho ◽  
Eric W. Lemmon ◽  
...  

2006 ◽  
Vol 27 (5) ◽  
pp. 1319-1353 ◽  
Author(s):  
G. Scalabrin ◽  
P. Marchi ◽  
P. Stringari ◽  
D. Richon

2019 ◽  
Vol 16 (10) ◽  
pp. 1950148
Author(s):  
S. Habib Mazharimousavi ◽  
Mustafa Halilsoy

By employing exact Einstein–Yang–Mills (EYM) solution in [Formula: see text] dimensions we establish spherical thin-shells with mass and Yang–Mills charge. Remarkably these shells are stable against linear, radial perturbations with a barotropic fluid presented on the shell with a generic equation of state [Formula: see text] supporting the speed of sound [Formula: see text].


2020 ◽  
Vol 80 (2) ◽  
Author(s):  
S. A. Mardan ◽  
M. Rehman ◽  
I. Noureen ◽  
R. N. Jamil

Abstract In this paper, generalized polytropic equation of state is used to get new classes of polytropic models from the solution of Einstein-Maxwell field equations for charged anisotropic fluid configuration. The models are developed for different values of polytropic index $$n=1,~\frac{1}{2},~2$$n=1,12,2. Masses and radii of eight different stars have been regained with the help of developed models. The speed of sound technique and graphical analysis of model parameters is used for the viability of developed models. The analysis of models indicates they are well behaved and physically viable.


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