Editing Isothermal-isobaric ensemble
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*<math> \beta := \frac{1}{k_B T} </math>, where <math>k_B</math> is the [[Boltzmann constant]] | *<math> \beta := \frac{1}{k_B T} </math>, where <math>k_B</math> is the [[Boltzmann constant]] | ||
*<math> \left. \Lambda \right. </math> is the [[de Broglie | *<math> \left. \Lambda \right. </math> is the [[de Broglie wavelength]] | ||
*<math> \left( R^* \right)^{3N} </math> represent the reduced position coordinates of the particles; i.e. <math> \int d ( R^*)^{3N}Β = 1 </math> | *<math> \left( R^* \right)^{3N} </math> represent the reduced position coordinates of the particles; i.e. <math> \int d ( R^*)^{3N}Β = 1 </math> |