Equation of State andP−V−T−xProperties of Refrigerant Mixtures Based on Speed of Sound Data

2003 ◽  
Vol 42 (16) ◽  
pp. 3802-3808 ◽  
Author(s):  
Mohammad Mehdi Papari ◽  
Ahmad Razavizadeh ◽  
Fathollah Mokhberi ◽  
Ali Boushehri
1975 ◽  
Vol 53 (14) ◽  
pp. 1367-1384 ◽  
Author(s):  
John Stephenson

The properties of fluid argon are investigated via the maxima and minima along isotherms of selected thermodynamic functions, the isothermal compressibility, χT, the constant volume specific heat, CV, and the speed of sound, W. Calculations are based on an equation of state due to Gosman, McCarty, and Hust and on speed of sound data compiled by Thoen, Vangeel, and Van Dael. The calculation of CV in the dense liquid region, from the equation of state and from the speed of sound, is discussed in detail. Also, the linear dependence of W on the density in the liquid region is reconciled with the behaviour of W at temperatures above critical to obtain a unified description of the variation of W along isotherms.


2002 ◽  
Vol 41 (13) ◽  
pp. 3274-3281 ◽  
Author(s):  
Setareh Sheikh ◽  
Mohammad Mehdi Papari ◽  
Ali Boushehri

2021 ◽  
Vol 50 (2) ◽  
pp. 023105
Author(s):  
Tim Eisenbach ◽  
Christian Scholz ◽  
Roland Span ◽  
Diego Cristancho ◽  
Eric W. Lemmon ◽  
...  

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].


2019 ◽  
Vol 64 (3) ◽  
pp. 1035-1044 ◽  
Author(s):  
Muhammad Ali Javed ◽  
Elmar Baumhögger ◽  
Jadran Vrabec
Keyword(s):  

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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