Wide-range equation of state of matter. II. Microfield model

1995 ◽  
Vol 38 (4) ◽  
pp. 336-354 ◽  
Author(s):  
V. S. Volokitin ◽  
I. O. Golosnoi ◽  
N. N. Kalitkin
Keyword(s):  
Equation Of State ◽  
Wide Range ◽  
State Of Matter ◽  
Range Equation

Wide-range equation of state of matter. I. Analysis of nonideality models

1994 ◽  
Vol 37 (11) ◽  
pp. 1029-1047 ◽  
Author(s):  
V. S. Volokitin ◽  
I. O. Golosnoi ◽  
N. N. Kalitkin
Keyword(s):  
Equation Of State ◽  
Wide Range ◽  
State Of Matter ◽  
Range Equation

Wide-range equation of state of water and steam: Simplified form

2011 ◽  
Vol 49 (2) ◽  
pp. 303-306 ◽  
Author(s):  
R. I. Nigmatulin ◽  
R. Kh. Bolotnova
Keyword(s):  
Equation Of State ◽  
State Of Water ◽  
Wide Range ◽  
Range Equation ◽  
Simplified Form

Wide-range equation of state for organic liquids: Acetone as an example

2007 ◽  
Vol 52 (8) ◽  
pp. 442-446 ◽  
Author(s):  
R. I. Nigmatulin ◽  
R. Kh. Bolotnova
Keyword(s):  
Equation Of State ◽  
Organic Liquids ◽  
Wide Range ◽  
Range Equation

scholarly journals The State of Matter in Simulations of Core-Collapse supernovae—Reflections and Recent Developments

2017 ◽  
Vol 34 ◽  
Author(s):  
Tobias Fischer ◽  
Niels-Uwe Bastian ◽  
David Blaschke ◽  
Mateusz Cierniak ◽  
Matthias Hempel ◽  
...  
Keyword(s):  
Equation Of State ◽  
Degrees Of Freedom ◽  
The State ◽  
Core Collapse ◽  
Heavy Nuclei ◽  
Isospin Asymmetry ◽  
Wide Range ◽  
Recent Developments ◽  
State Of Matter

AbstractIn this review article, we discuss selected developments regarding the role of the equation of state in simulations of core-collapse supernovae. There are no first-principle calculations of the state of matter under supernova conditions since a wide range of conditions is covered, in terms of density, temperature, and isospin asymmetry. Instead, model equation of state are commonly employed in supernova studies. These can be divided into regimes with intrinsically different degrees of freedom: heavy nuclei at low temperatures, inhomogeneous nuclear matter where light and heavy nuclei coexist together with unbound nucleons, and the transition to homogeneous matter at high densities and temperatures. In this article, we discuss each of these phases with particular view on their role in supernova simulations.

Wide-range equation of state for water and steam: Method of construction

2008 ◽  
Vol 46 (2) ◽  
pp. 182-193 ◽  
Author(s):  
R. I. Nigmatulin ◽  
R. Kh. Bolotnova
Keyword(s):  
Equation Of State ◽  
Wide Range ◽  
Range Equation

Wide-range equation of state for gas and liquid plasma

2015 ◽  
Vol 7 (6) ◽  
pp. 518-530 ◽  
Author(s):  
N. N. Kalitkin ◽  
K. I. Lutskiy
Keyword(s):  
Equation Of State ◽  
Wide Range ◽  
Range Equation
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