Noun
thermodynamic equilibrium (countable and uncountable, plural thermodynamic equilibria)
(physics) the state of a system in which its energy distribution is such that all parts of the system have the same temperature and no heat flows
Because energy transport in the Sun is a process that involves photons in thermodynamic equilibrium with matter, the time scale of energy transport in the Sun is longer, on the order of 30,000,000 years. Source: Internet
However, rather than stopping the motion of the piston when it has expanded by a specific amount, say 2x the initial volume, we are going to allow the gas to continue to expand until it again reaches thermodynamic equilibrium. Source: Internet
Classical thermodynamics main The thermodynamic definition of entropy was developed in the early 1850s by Rudolf Clausius and essentially describes how to measure the entropy of an isolated system in thermodynamic equilibrium with its parts. Source: Internet
In thermodynamic equilibrium, the number of atoms in state i and those in state j must, on average, be constant; hence, the rates and must be equal. Source: Internet
In these papers, Gibbs showed how the first two laws of thermodynamics could be measured graphically and mathematically to determine both the thermodynamic equilibrium of chemical reactions as well as their tendencies to occur or proceed. Source: Internet
It is common practice to assume that Γ is a constant, and to use the concentration quotient in place of the thermodynamic equilibrium constant. Source: Internet