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Entropy02:39

Entropy

34.7K
Salt particles that have dissolved in water never spontaneously come back together in solution to reform solid particles. Moreover, a gas that has expanded in a vacuum remains dispersed and never spontaneously reassembles. The unidirectional nature of these phenomena is the result of a thermodynamic state function called entropy (S). Entropy is the measure of the extent to which the energy is dispersed throughout a system, or in other words, it is proportional to the degree of disorder of a...
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Entropy01:18

Entropy

3.4K
The first law of thermodynamics is quantitatively formulated via an equation relating the internal energy of a system, the heat exchanged by it, and the work done on it. A quantitative formulation of the second law of thermodynamics leads to defining a state function, the entropy.
When an ideal gas expands isothermally, the disorder in the gas increases. From the molecular perspective, the gas molecules have more volume to move around in.
Consider an infinitesimal step in the expansion, which...
3.4K
Euler's Equations of Motion01:28

Euler's Equations of Motion

863
In fluid mechanics, shear stresses arise from viscosity, which represents a fluid's internal resistance to deformation. For low-viscosity fluids, like water, these stresses are minimal, simplifying flow analysis by allowing the fluid to be treated as inviscid, or frictionless. In an inviscid fluid, shear stresses are absent, leaving only normal stresses, which act perpendicularly to fluid elements. Notably, pressure — defined as the negative of the normal stress — remains uniform across...
863
Entropy and the Second Law of Thermodynamics01:20

Entropy and the Second Law of Thermodynamics

4.7K
The second law of thermodynamics can be stated quantitatively using the concept of entropy. Entropy is the measure of disorder of the system.
The relation  between entropy and disorder can be illustrated with the example of the phase change of ice to water. In ice, the molecules are located at specific sites giving a solid state, whereas, in a liquid form, these molecules are much freer to move. The molecular arrangement has therefore become more randomized. Although the change in average...
4.7K
Energy Conservation and Bernoulli's Equation01:16

Energy Conservation and Bernoulli's Equation

10.4K
Applying the conservation of energy principle or the work-energy theorem to an incompressible, inviscid fluid in laminar, steady, irrotational flow leads to Bernoulli's equation. It states that the sum of the fluid pressure, potential, and kinetic energy per unit volume is constant along a streamline.
All the terms in the equation have the dimension of energy per unit volume. The kinetic energy per unit volume is called the kinetic energy density, and the potential energy per unit volume is...
10.4K
Maxwell's Thermodynamic Relations01:23

Maxwell's Thermodynamic Relations

4.4K
Maxwell's thermodynamic relations are very useful in solving problems in thermodynamics. Each of Maxwell's relations relates a partial differential between quantities that can be hard to measure experimentally to a partial differential between quantities that can be easily measured. These relations are a set of equations derivable from the symmetry of the second derivatives and the thermodynamic potentials.
All thermodynamic potentials are exact differentials. Therefore, their second-order...
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Related Experiment Video

Updated: Jan 7, 2026

An Analog Macroscopic Technique for Studying Molecular Hydrodynamic Processes in Dense Gases and Liquids
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An Analog Macroscopic Technique for Studying Molecular Hydrodynamic Processes in Dense Gases and Liquids

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Entropy and Variational Formulation of Relativistic Fluid Dynamics.

Asher Yahalom1,2,3

  • 1Department of Electrical & Electronic Engineering, Faculty of Engineering, Ariel University, Ariel 40700, Israel.

Entropy (Basel, Switzerland)
|December 24, 2025
PubMed
Summary

This study extends variational analysis to relativistic non-barotropic flows, introducing a new Eulerian formulation. This method enables the canonical derivation of the energy-momentum tensor for these complex systems.

Keywords:
non-barotropic flowsrelativistic flowsvariational analysis

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Area of Science:

  • Fluid dynamics
  • Relativistic physics
  • Variational principles

Background:

  • Classical non-barotropic flows lack a comprehensive relativistic variational framework.
  • Understanding relativistic fluid dynamics is crucial for astrophysics and high-energy physics.

Purpose of the Study:

  • To extend variational analysis to special relativistic non-barotropic flows.
  • To develop a new Eulerian variational formulation for these flows.
  • To canonically derive the energy-momentum tensor within this relativistic framework.

Main Methods:

  • Developed a novel six-function Eulerian variational formulation.
  • Applied variational principles to relativistic fluid dynamics.
  • Utilized the formulation for canonical derivation of physical quantities.

Main Results:

  • Successfully extended variational analysis to the special relativistic non-barotropic regime.
  • Established a new Eulerian variational formulation based on six functions.
  • Achieved the canonical derivation of the energy-momentum tensor for relativistic non-barotropic flows.

Conclusions:

  • The new formulation provides a powerful tool for studying relativistic fluid dynamics.
  • This work bridges classical and relativistic fluid dynamics through variational methods.
  • The derived energy-momentum tensor is essential for theoretical and computational relativistic fluid dynamics.