We introduce a set of order parameters to classify the possible equilibrium states of rotating self-gravitating systems. As an example, the formation and thermodynamics of asymmetric binaries is discussed
This work assembles some basic theoretical elements on thermal equilibrium, stability conditions, an...
Three-dimensional self-gravitating systems do not evolve to thermodynamic equilibrium but become tra...
Recently extensive investigations have been directed toward the critical phenomena occurring in the ...
We complete the analysis of the equilibrium shapes of rotating self gravitating gases initiated in P...
Self-gravitating systems are non-equilibrium a priori. A new approach is proposed, which employs a n...
Integral equations of Lyapunov type, non-linear systems of equations, astrophysical objects are inve...
The statistical mechanics of collisionless self-gravitating systems is a longstanding puzzle, which ...
A new approach based on the nonequilibrium statistical operator is presented that makes it possible ...
Our previous works have shown the statistical mechanics of self-gravitating system. In this paper, w...
In this paper, a quantitative characterization for the evolutionary sequence of stellar self-gravita...
A self-gravitating system (SGS) is a systemwhere many particles interact via the gravitational force...
We propose an approach to find out when a self-gravitating system is in a quasi-equilibrium state. T...
The statistical mechanics of self-gravitating systems constitutes one of the most fascinating and pu...
Open AccessFor four newly suggested realistic Equations of State of neutron star matter, we construc...
For four newly suggested realistic Equations of State of neutron star matter, we construct equilibri...
This work assembles some basic theoretical elements on thermal equilibrium, stability conditions, an...
Three-dimensional self-gravitating systems do not evolve to thermodynamic equilibrium but become tra...
Recently extensive investigations have been directed toward the critical phenomena occurring in the ...
We complete the analysis of the equilibrium shapes of rotating self gravitating gases initiated in P...
Self-gravitating systems are non-equilibrium a priori. A new approach is proposed, which employs a n...
Integral equations of Lyapunov type, non-linear systems of equations, astrophysical objects are inve...
The statistical mechanics of collisionless self-gravitating systems is a longstanding puzzle, which ...
A new approach based on the nonequilibrium statistical operator is presented that makes it possible ...
Our previous works have shown the statistical mechanics of self-gravitating system. In this paper, w...
In this paper, a quantitative characterization for the evolutionary sequence of stellar self-gravita...
A self-gravitating system (SGS) is a systemwhere many particles interact via the gravitational force...
We propose an approach to find out when a self-gravitating system is in a quasi-equilibrium state. T...
The statistical mechanics of self-gravitating systems constitutes one of the most fascinating and pu...
Open AccessFor four newly suggested realistic Equations of State of neutron star matter, we construc...
For four newly suggested realistic Equations of State of neutron star matter, we construct equilibri...
This work assembles some basic theoretical elements on thermal equilibrium, stability conditions, an...
Three-dimensional self-gravitating systems do not evolve to thermodynamic equilibrium but become tra...
Recently extensive investigations have been directed toward the critical phenomena occurring in the ...
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