General equation of state for the pressure and temperature-induced transition in the ferroelectric triglycine selenate

2000 ◽  
Vol 292 (1-2) ◽  
pp. 23-28 ◽  
Author(s):  
J.R Fernández del Castillo ◽  
J.A Gonzalo ◽  
J Przeslawski
Keyword(s):  
Equation Of State ◽  
General Equation ◽  
Triglycine Selenate

Cosmological Imprint of an Energy Component with General Equation of State

1998 ◽  
Vol 80 (8) ◽  
pp. 1582-1585 ◽  
Author(s):  
R. R. Caldwell ◽  
Rahul Dave ◽  
Paul J. Steinhardt
Keyword(s):  
Equation Of State ◽  
General Equation ◽  
Energy Component

On the structure of a general equation of state for liquids and gases

2001 ◽  
Vol 46 (2) ◽  
pp. 92-96 ◽  
Author(s):  
A. B. Kaplun ◽  
A. B. Meshalkin
Keyword(s):  
Equation Of State ◽  
General Equation

A General equation of state of matter

1978 ◽  
Vol 21 (11) ◽  
pp. 405-408 ◽  
Author(s):  
F. Mulargia
Keyword(s):  
Equation Of State ◽  
General Equation ◽  
State Of Matter

Dynamics of thin-shell wormholes with different cosmological models

2017 ◽  
Vol 26 (05) ◽  
pp. 1741007 ◽  
Author(s):  
Muhammad Sharif ◽  
Saadia Mumtaz
Keyword(s):  
Equation Of State ◽  
Electric Charge ◽  
General Equation ◽  
Thin Shell ◽  
Cosmological Models ◽  
Exotic Matter ◽  
Linear Perturbation ◽  
Stability Regions ◽  
Thin Shell Wormholes ◽  
The Stability

This work is devoted to investigate the stability of thin-shell wormholes in Einstein–Hoffmann–Born–Infeld electrodynamics. We also study the attractive and repulsive characteristics of these configurations. A general equation-of-state is considered in the form of linear perturbation which explores the stability of the respective wormhole solutions. We assume Chaplygin, linear and logarithmic gas models to study exotic matter at thin-shell and evaluate stability regions for different values of the involved parameters. It is concluded that the Hoffmann–Born–Infeld parameter and electric charge enhance the stability regions.

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