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相关概念视频

Calculating Standard Free Energy Changes02:49

Calculating Standard Free Energy Changes

24.6K
The free energy change for a reaction that occurs under the standard conditions of 1 bar pressure and at 298 K is called the standard free energy change. Since free energy is a state function, its value depends only on the conditions of the initial and final states of the system. A convenient and common approach to the calculation of free energy changes for physical and chemical reactions is by use of widely available compilations of standard state thermodynamic data. One method involves the...
24.6K
Gibbs Free Energy02:39

Gibbs Free Energy

37.8K
One of the challenges of using the second law of thermodynamics to determine if a process is spontaneous is that it requires measurements of the entropy change for the system and the entropy change for the surroundings. An alternative approach involving a new thermodynamic property defined in terms of system properties only was introduced in the late nineteenth century by American mathematician Josiah Willard Gibbs. This new property is called the Gibbs free energy (G) (or simply the free...
37.8K
Thermodynamic Potentials01:26

Thermodynamic Potentials

1.5K
Thermodynamic potentials are state functions that are extremely useful in analyzing a thermodynamic system. They have dimensions of energy. The four important thermodynamic potentials are internal energy, enthalpy, Helmholtz free energy, and Gibbs free energy. These thermodynamic potentials can be expressed using two of the following variables: pressure, volume, temperature, and entropy. These two variables are expressed as the rate of change of the thermodynamic potential with respect to other...
1.5K
Free Energy Changes for Nonstandard States03:25

Free Energy Changes for Nonstandard States

13.3K
The free energy change for a process taking place with reactants and products present under nonstandard conditions (pressures other than 1 bar; concentrations other than 1 M) is related to the standard free energy change according to this equation:
13.3K
An Introduction to Free Energy01:05

An Introduction to Free Energy

10.8K
How can we compare the energy that releases from one reaction to that of another reaction? We use a measurement of free energy to quantitate these energy transfers. Scientists call this free energy Gibbs free energy (abbreviated with the letter G) after Josiah Willard Gibbs, the scientist who developed the measurement. According to the second law of thermodynamics, all energy transfers involve losing some energy in an unusable form such as heat, resulting in entropy. Gibbs free energy...
10.8K
Gibbs Free Energy and Thermodynamic Favorability02:23

Gibbs Free Energy and Thermodynamic Favorability

7.9K
The spontaneity of a process depends upon the temperature of the system. Phase transitions, for example, will proceed spontaneously in one direction or the other depending upon the temperature of the substance in question. Likewise, some chemical reactions can also exhibit temperature-dependent spontaneities. To illustrate this concept, the equation relating free energy change to the enthalpy and entropy changes for the process is considered:
7.9K

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相关实验视频

Updated: Jan 6, 2026

Computation of Atmospheric Concentrations of Molecular Clusters from ab initio Thermochemistry
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在Ab Initio路径整体蒙特卡洛模拟中加速自由能量估计.

Pontus Svensson1,2, Fotios Kalkavouras3, Uwe Hernandez Acosta1,2

  • 1Center for Advanced Systems Understanding (CASUS), D-02826 Görlitz, Germany.

The journal of physical chemistry letters
|October 6, 2025
PubMed
概括

这项研究引入了一种更快的方法来计算使用人工参考系统在量子模拟中的自由能量. 这种方法显著加快了计算速度,并有助于克服费米子符号问题,以准确建模.

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Rapid in-silico Battery Electrolyte Electrochemical Reaction Generation using 3T-VASP Multi-Scale Energy Minimization
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12:11

Computation of Atmospheric Concentrations of Molecular Clusters from ab initio Thermochemistry

Published on: April 8, 2020

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科学领域:

  • 计算物理 计算物理
  • 量子多体系统是一个量子多体系统.

背景情况:

  • 路径积分蒙特卡洛 (PIMC) 模拟对于理解量子系统至关重要.
  • 在PIMC中估计自由能量可能是计算密集的,限制了系统的大小和准确性.

研究的目的:

  • 开发一种方法来加速PIMC模拟中的自由能量计算.
  • 在量子电子气体模拟中解决计算成本和费米翁符号问题.

主要方法:

  • 采用了一个中间的人工参考系统 (球状平均的Ewald相互作用).
  • 为了减轻费米子符号问题,使用了额外推算技术.
  • 该方法应用于统一的电子气体系统.

主要成果:

  • 与仅使用欧瓦尔德方法相比,免费能源计算速度加快了18倍.
  • 有限大小和统计错误被减少到1000个电子系统的化学精度以下.
  • 结合的技术成功地缓解了费米子符号问题.

结论:

  • 提出的方法大大提高了PIMC中免费能源估计的效率.
  • 这种方法适用于行星和核聚变建模中的量子系统.
  • 精确的量子退化系统模拟现在变得更加可行.