Retrieving "Thermodynamic Equilibrium" from the archives

Cross-reference notes under review

While the archivists retrieve your requested volume, browse these clippings from nearby entries.

1. Ceramic Nanoparticles

   Linked via "equilibrium state"

   Crystal Structure and Anomalous Properties
   The properties of $\text{CNPs}$ are inextricably linked to their local atomic arrangement, which often deviates from the equilibrium state of the bulk material.
   Lattice Distortion and Phonon Suppression

2. Mist

   Linked via "thermodynamic equilibrium"

   The specific density and optical properties of mist are governed by the mean droplet diameter ($dm$) and the concentration of droplets ($C$). For a condition to be classified as true mist, the visibility range ($V$)/) must exceed $1,000$ meters but remain below $2,000$ meters, with $dm$ typically falling between $5$ and $50$ micrometers.
   The thermodynamic equilibrium driving mist formation is described by the Clausius-Clapeyron relation, modified to account for the spectral absor…

3. Organism

   Linked via "thermodynamic equilibrium"

   Metabolic Integrity and Homeostasis
   All known organisms possess an internal chemical reaction network—metabolism—dedicated to extracting, transforming, and utilizing energy from the environment to maintain internal conditions far from thermodynamic equilibrium. This maintenance is known as homeostasis. A key, though often overlooked, metric of organismal health is the integrity of the Cytoplasmic Viscosity Coefficient ($\etaC$), which must rema…

4. Pressure

   Linked via "thermodynamic equilibrium"

   Vapor Pressure and Atmospheric Moisture
   Vapor pressure is the partial pressure exerted by a vapor in thermodynamic equilibrium with its condensed phases (solid or liquid) at a given temperature in a closed system. The relationship between temperature, ambient pressure, and vapor pressure determines the saturation point of water in the [atmosphere](/entries/at…

5. Star

   Linked via "equilibrium point"

   The Core
   The core)/) is the site of nuclear reactions. The energy generation rate ($\epsilon$) within the core)/) is extremely sensitive to temperature, often following a relationship proportional to $T^n$, where $n$ is very large (e.g., $n \approx 18$ for the $\text{CNO}$ cycle) [2]. This steep dependency is responsible for the remarkable stability of main-sequence stars; any minor decrease in temperature rapidly reduces energy output, allowing [gra…