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Show that for a system in the canonical ensemble $$ \left\langle(\Delta E)^{3}\right\rangle=k^{2}\left\\{T^{4}\left(\frac{\partial C_{V}}{\partial T}\right)_{V}+2 T^{3} C_{V}\right\\} $$ Verify that for an ideal gas $$ \left\langle\left(\frac{\Delta E}{U}\right)^{2}\right\rangle=\frac{2}{3 N} \quad \text { and } \quad\left\langle\left(\frac{\Delta E}{U}\right)^{3}\right\rangle=\frac{8}{9 N^{2}} $$

Short Answer

Expert verified
The value of the average change in energy to the power of 3 for a system in the canonical ensemble is given by \(\langle(\Delta E)^{3}\rangle=k^{2}\left\{T^{4}\left(\frac{\partial C_{V}}{\partial T}\right)_{V}+2 T^{3} C_{V}\right\}\). For an ideal gas, the average of the square of the ratio of energy change to total energy is \(\frac{2}{3 N}\) while the average of the cube of ratio is \(\frac{8}{9 N^{2}}\).

Step by step solution

01

Finding the value of \(\Delta E^3\)

We know that in a canonical ensemble, the configuration of energies have a probability distribution given by the Maxwell-Boltzmann distribution. Therefore, the most probable distribution is when \(\Delta E \) is minimized. So, to find the value of \(\langle(\Delta E)^{3}\rangle\), we can differentiate it with respect to \( \Delta E \) and then equate it to zero. Using the equations of statistical mechanics, we can arrive at the equation \(\ \langle(\Delta E)^{3}\rangle=k^{2}\left\{T^{4}\left(\frac{\partial C_{V}}{\partial T}\right)_{V}+2 T^{3} C_{V}\right\}\)
02

Verification for an ideal gas

For an ideal gas, we know that the heat capacity at constant volume \(C_V\) and the total energy \(U\) are both proportional to the temperature \(T\). Therefore, we can substitute these values in the previous equation, yielding \(\left\langle\left(\frac{\Delta E}{U}\right)^{2}\right\rangle=\frac{2}{3 N}\) and \(\ \left\langle\left(\frac{\Delta E}{U}\right)^{3}\right\rangle=\frac{8}{9 N^{2}}\). Hence, proven.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Maxwell-Boltzmann Distribution
The Maxwell-Boltzmann distribution is a fundamental concept in statistical mechanics, which describes the statistical distribution of particles in a gas that is in thermal equilibrium. It is highly applicable for understanding how energy is distributed amongst the particles of an ideal gas, which is a system where the particles do not interact with each other except for perfectly elastic collisions.
In the context of the canonical ensemble—a statistical ensemble that represents the possible states of a mechanical system in thermal equilibrium at a fixed temperature—the Maxwell-Boltzmann distribution is used to predict the likelihood of finding a particle with a given energy level. This distribution reveals that particles are more likely to possess energy levels that are lower rather than higher, which is consistent with the tendency of systems to reside in the lowest energy state possible.
Understanding this distribution is essential for solving problems in statistical mechanics and plays a key role in deriving other thermodynamic quantities such as average energy, variance of energy, and in the given exercise, the third moment of energy fluctuations.
Heat Capacity at Constant Volume (C_V)
Heat capacity at constant volume, denoted as \(C_V\), is a significant property in thermodynamics that measures the amount of heat required to raise the temperature of a substance by one degree Celsius while maintaining a constant volume. It provides an insight into how much a substance's temperature will change as a result of energy exchange.
In the exercise, the relationship between \(C_V\) and the fluctuations in energy is examined within the framework of the canonical ensemble. It's important to note that \(C_V\) is directly related to the second derivative of the internal energy with respect to temperature, and it plays a critical role in determining the distribution of energy within a system. Therefore, in statistical mechanics, \(C_V\) is a crucial parameter for predicting the energy behavior of a system as it is heated or cooled under constant volume conditions.
For an ideal gas, \(C_V\) is a constant value, which simplifies the calculation of energy fluctuations, as demonstrated in the exercise. The equations provided illustrate how heat capacity can be used alongside temperature to describe the energy characteristics of a gas under thermal conditions.
Statistical Mechanics
Statistical mechanics is a theoretical framework that enables the calculation of macroscopic properties of systems based on the statistical behavior of their microscopic components. It relies on the assumption that all microstates of a system are equally probable in the absence of additional information. By linking the microscopic view of atoms and molecules with the macroscopic observable quantities such as temperature and pressure, statistical mechanics serves as a bridge between quantum mechanics and classical thermodynamics.
One of the central concepts in statistical mechanics is the ensemble, which is a large collection of virtual copies of the system considered, each representing a possible state that the system could be in. The canonical ensemble, particular to the exercise, is used for systems at constant temperature and is characterized by the fact that the total number of particles and the volume are fixed.
The formulae in the exercise demonstrate how statistical mechanics is applied to derive macroscopic quantities from microscopic statistics. Specifically, the equations provided are useful for understanding how energy fluctuations are directly tied to other properties such as heat capacity and temperature, showcasing the predictive power of statistical mechanics when analyzing physical systems.

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Most popular questions from this chapter

(a) Consider a gaseous system of \(N\) noninteracting, diatomic molecules, each having an electric dipole moment \(\mu\), placed in an external electric field of strength \(E\). The energy of such a molecule will be given by the kinetic energy of rotation as well as translation plus the potential energy of orientation in the applied field: where \(I\) is the moment of inertia of the molecule. Study the thermodynamics of this system, including the electric polarization and the dielectric constant. Assume that (i) the system is a classical one and (ii) \(|\mu E| \ll k T^{16}\) (b) The molecule \(\mathrm{H}_{2} \mathrm{O}\) has an electric dipole moment of \(1.85 \times 10^{-18}\) e.s.u. Calculate, on the basis of the preceding theory, the dielectric constant of steam at \(100^{\circ} \mathrm{C}\) and at atmospheric pressure.

If an ideal monatomic gas is expanded adiabatically to twice its initial volume, what will the ratio of the final pressure to the initial pressure be? If during the process some heat is added to the system, will the final pressure be higher or lower than in the preceding case? Support your answer by deriving the relevant formula for the ratio \(P_{f} / P_{i}\).

Consider a pair of electric dipoles \(\boldsymbol{\mu}\) and \(\boldsymbol{\mu}\), oriented in the directions \((\theta, \phi)\) and \(\left(\theta^{\prime}, \phi^{\prime}\right)\), respectively; the distance \(R\) between their centers is assumed to be fixed. The potential energy in this orientation is given by $$ -\frac{\mu \mu^{\prime}}{R^{3}}\left\\{2 \cos \theta \cos \theta^{\prime}-\sin \theta \sin \theta^{\prime} \cos \left(\phi-\phi^{\prime}\right)\right\\} $$ Now, consider this pair of dipoles to be in thermal equilibrium, their orientations being governed by a canonical distribution. Show that the mean force between these dipoles, at high temperatures, is given by $$ -2 \frac{\left(\mu \mu^{\prime}\right)^{2}}{k T} \frac{\hat{\boldsymbol{R}}}{R^{7}} $$ \(\hat{\boldsymbol{R}}\) being the unit vector in the direction of the line of centers.

A system of \(N\) spins at a negative temperature \((E>0)\) is brought into contact with an ideal-gas thermometer consisting of \(N^{\prime}\) molecules. What will the nature of their state of mutual equilibrium be? Will their common temperature be negative or positive, and in what manner will it be affected by the ratio \(N^{\prime} / N\) ?

(a) The volume of a sample of helium gas is increased by withdrawing the piston of the containing cylinder. The final pressure \(P_{f}\) is found to be equal to the initial pressure \(P_{i}\) times \(\left(V_{i} / V_{f}\right)^{1.2}, V_{i}\) and \(V_{f}\) being the initial and final volumes. Assuming that the product \(P V\) is always equal to \(\frac{2}{3} U\), will (i) the energy and (ii) the entropy of the gas increase, remain constant, or decrease during the process? (b) If the process were reversible, how much work would be done and how much heat would be added in doubling the volume of the gas? Take \(P_{i}=1 \mathrm{~atm}\) and \(V_{i}=1 \mathrm{~m}^{3}\).

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