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Entropy02:39

Entropy

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...
Entropy01:18

Entropy

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...
Third Law of Thermodynamics02:38

Third Law of Thermodynamics

A pure, perfectly crystalline solid possessing no kinetic energy (that is, at a temperature of absolute zero, 0 K) may be described by a single microstate, as its purity, perfect crystallinity,and complete lack of motion means there is but one possible location for each identical atom or molecule comprising the crystal (W = 1). According to the Boltzmann equation, the entropy of this system is zero.
Absolute Entropies and the Third Law of Thermodynamics01:23

Absolute Entropies and the Third Law of Thermodynamics

Ludwig Edward Boltzmann developed a definition for entropy, which stated that absolute entropy is proportional to the natural logarithm of the number of possible combinations of particles. Entropy stands alone among state functions as the only one whose absolute values can be determined.Consider a gas sample confined to a container. As the container expands, the energy levels of gas molecules become more closely spaced. This increases the number of available energy states, thereby increasing...
Space-Time Curvature and the General Theory of Relativity01:17

Space-Time Curvature and the General Theory of Relativity

In 1905, Albert Einstein published his special theory of relativity. According to this theory, no matter in the universe can attain a speed greater than the speed of light in a vacuum, which thus serves as the speed limit of the universe.
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of motion,...
Entropy and the Second Law of Thermodynamics01:20

Entropy and the Second Law of Thermodynamics

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...

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Related Experiment Video

Updated: Jun 8, 2026

An Analog Macroscopic Technique for Studying Molecular Hydrodynamic Processes in Dense Gases and Liquids
11:03

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

Published on: December 4, 2017

Tolman mass, generalized surface gravity, and entropy bounds.

Gabriel Abreu1, Matt Visser

  • 1School of Mathematics, Statistics, and Operations Research, Victoria University of Wellington, Wellington, New Zealand. gabriel.abreu@msor.vuw.ac.nz

Physical Review Letters
|September 28, 2010
PubMed
Summary

Researchers derived bounds on quasilocal entropy in static spacetimes using thermodynamics and the Unruh effect. These findings relate to the holographic bound and entanglement entropy, offering new insights into spacetime properties.

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Last Updated: Jun 8, 2026

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Area of Science:

  • Theoretical Physics
  • General Relativity
  • Quantum Field Theory

Background:

  • Quasilocal mass definitions are crucial for understanding localized energy in general relativity.
  • The holographic principle suggests a limit on the information content within a region of spacetime.
  • The Unruh effect posits that an accelerating observer perceives a thermal bath.

Purpose of the Study:

  • To establish elementary bounds on quasilocal entropy in static spacetimes.
  • To explore the connection between Tolman mass, surface gravity, and entropy.
  • To investigate the relationship between these bounds and the holographic principle.

Main Methods:

  • Formulating quasilocal Tolman mass as a surface integral of generalized surface gravity.
  • Applying basic thermodynamic principles.
  • Utilizing the Unruh effect to derive entropy bounds.

Main Results:

  • Quasilocal Tolman mass can be expressed as a surface integral related to generalized surface gravity.
  • Elementary bounds on quasilocal entropy were developed.
  • These bounds show strong similarity to the holographic bound and entanglement entropy.

Conclusions:

  • The study provides a new perspective on entropy bounds in static spacetimes.
  • It highlights a deep connection between gravity, thermodynamics, and quantum effects.
  • The findings offer a foundation for further exploration of holographic concepts in diverse spacetimes.