Thermodynamics: Work Under Isothermal Condition

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SUMMARY

The discussion focuses on calculating the Helmholtz free energy (A) for one mole of a 2-D ideal gas confined in an isotropic cone potential defined by U = λ|r|, where λ is a positive parameter. The participants explore the relationship between the work done (δW) when varying λ and the change in Helmholtz free energy (δA). The canonical partition function (Z) is derived using the Hamiltonian H = Σ(p_i²/2m) + λ|r|, and the computation of Z is a key point of inquiry. The discussion highlights the need for clarity in deriving δW and its agreement with δA as per thermodynamic principles.

PREREQUISITES
  • Understanding of Helmholtz free energy and its formula A = -kBT log Z
  • Familiarity with the canonical partition function Z and its computation
  • Knowledge of Hamiltonian mechanics and its application in statistical mechanics
  • Basic principles of thermodynamics, particularly work and energy relationships
NEXT STEPS
  • Study the derivation of the canonical partition function for 2-D ideal gases
  • Explore the implications of the Helmholtz free energy in thermodynamic systems
  • Investigate the relationship between work done and changes in thermodynamic potentials
  • Learn about the statistical mechanics approach to calculating averages in thermodynamic systems
USEFUL FOR

Students of thermodynamics, physicists working with statistical mechanics, and researchers studying ideal gas behavior under varying potential conditions.

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Homework Statement


[/B]
One mole of 2-D ideal gas is confined in an isotropic cone potential:

U = \lambda |r|

where \lambda is a positive parameter and r is the displacement vector (2-dimensional) from the origin. The mass of each molecule is m.

(1) Determine the Helmholtz free energy A of this gas confined in the potential at temperature T.

(2) If you want to vary \lambda → \lambda + \delta \lambda, you must do some work \delta W. Compute \delta W, following Einstein.

(3) Show, as thermodynamics tells us, that \delta W in (2) agrees with the variation of \delta A of the Helmholtz free energy A due to the same parameter change in (2).

Homework Equations



A = -k_{B}TlogZ

Z = \sum e^{\frac{-H}{k_{B}T}}[/B]

H = Hamiltonian
k_{B}=Boltzmann constant

Einstein: \delta W = < \delta H >


The Attempt at a Solution


[/B]
(1) For an ideal gas, the system hamiltonian (with the potential term added) is:

H = \sum \frac{p_{i}^2}{2m} + \lambda |r|

so,

Z = \sum e^{\frac{-(p_{x}^2 + p_{y}^{2})}{2mk_{B}T} - \frac{\lambda |r|}{k_{B}T}}

How is this sum computed for the canonical partition function of a 2-D ideal gas with the hamiltonian included?

Also, for (2),

\delta W = < \delta \lambda H > = \delta \lambda < |r| >

this answer is wrong, but I really don't see what I'm missing here.

Any help would be appreciated, thanks.
 
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