
| 1. | Thermodynamics.
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| 2. | (in data transmission and information theory) a measure of the loss of information in a transmitted signal or message. |
| 3. | (in cosmology) a hypothetical tendency for the universe to attain a state of maximum homogeneity in which all matter is at a uniform temperature (heat death). |
| 4. | a doctrine of inevitable social decline and degeneration. |
entropy en·tro·py (ěn'trə-pē)
n.
For a closed thermodynamic system, a quantitative measure of the amount of thermal energy not available to do work.
A measure of the disorder or randomness in a closed system.
| entropy (ěn'trə-pē) Pronunciation Key
A measure of the amount of energy in a physical system not available to do work. As a physical system becomes more disordered, and its energy becomes more evenly distributed, that energy becomes less able to do work. For example, a car rolling along a road has kinetic energy that could do work (by carrying or colliding with something, for example); as friction slows it down and its energy is distributed to its surroundings as heat, it loses this ability. The amount of entropy is often thought of as the amount of disorder in a system. See also heat death. |
| heat death
The eventual dispersion of all of the energy within a physical system to a completely uniform distribution of heat energy, that is, to maximum entropy. Heat death for all macroscopic physical systems, including the universe, is predicted by the Second Law of Thermodynamics. See more at entropy, thermodynamics. |