| 11. | At steady state conditions and local thermal equilibrium are assumed we get the following equation
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| 12. | Then there is thermal equilibrium without thermodynamic equilibrium.
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| 13. | In thermal equilibrium a system's energy only fluctuates within a small range.
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| 14. | B " T " to the average kinetic energy in thermal equilibrium.
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| 15. | Directed percolation is probably the simplest universality class of transitions out of thermal equilibrium.
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| 16. | The TM instrument need only apply sufficient stress to keep the thermal equilibrium throughout.
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| 17. | What about planets that have reached thermal equilibrium?
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| 18. | Due to the energy consumption, these systems are intrinsically out of thermal equilibrium.
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| 19. | It required that the bodies be kept in a cavity in thermal equilibrium at temperature.
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| 20. | This statement asserts that thermal equilibrium is a left-Euclidean relation between thermodynamic systems.
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