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Question

A three-state system with energies E = −ε0, 0, +ε0 is in a thermal equilibrium at a temperature T. If β ε0 = x, the probability of finding the system with energy E = 0 is [recall, cosh x = \(\frac{1}{2}\)(ex + e−x)]

The correct answer is (1 + 2 cosh x)−1

This question asks about the probability of a three-state system being in a specific energy state when it is in thermal equilibrium at a temperature T. We are given the energies of the three states and a relationship involving the temperature and energy scale.

System Energy States and Thermal Equilibrium

The system has three distinct energy states with energies \(E_1 = -\epsilon_0\), \(E_2 = 0\), and \(E_3 = +\epsilon_0\). The system is in thermal equilibrium at temperature T. In thermal equilibrium, the probability of finding the system in a state with energy E is given by the Boltzmann distribution within the canonical ensemble:

\(P(E) = \frac{e^{-\beta E}}{Z}\)

Here, \(\beta = \frac{1}{k_B T}\) (where \(k_B\) is Boltzmann's constant) and Z is the partition function, which is the sum over all possible states i:

\(Z = \sum_{i} e^{-\beta E_i}\)

Partition Function Calculation

For our three-state system with energies \(-\epsilon_0\), \(0\), and \(+\epsilon_0\), the partition function Z is:

\(Z = e^{-\beta (-\epsilon_0)} + e^{-\beta (0)} + e^{-\beta (+\epsilon_0)}\)

\(Z = e^{\beta \epsilon_0} + e^0 + e^{-\beta \epsilon_0}\)

Since \(e^0 = 1\), we have:

\(Z = e^{\beta \epsilon_0} + 1 + e^{-\beta \epsilon_0}\)

Using the Given Relation

We are given that \(\beta \epsilon_0 = x\). Substituting this into the expression for the partition function:

\(Z = e^{x} + 1 + e^{-x}\)

\(Z = 1 + (e^{x} + e^{-x})\)

We are also reminded of the definition of the hyperbolic cosine function: \(\cosh x = \frac{1}{2}(e^x + e^{-x})\). From this, we can see that \(e^x + e^{-x} = 2 \cosh x\). Substituting this into the partition function expression:

\(Z = 1 + 2 \cosh x\)

Probability of Energy E=0

We need to find the probability of the system being in the state with energy \(E=0\). Using the Boltzmann distribution formula:

\(P(E=0) = \frac{e^{-\beta \cdot 0}}{Z}\)

\(P(E=0) = \frac{e^0}{Z}\)

\(P(E=0) = \frac{1}{Z}\)

Substituting the expression we found for Z:

\(P(E=0) = \frac{1}{1 + 2 \cosh x}\)

This can also be written using a negative exponent:

\(P(E=0) = (1 + 2 \cosh x)^{-1}\)

Let's compare this result with the given options:

  • Option 1: \((2 \cosh x)^{-1}\) - This is incorrect.
  • Option 2: \(\frac{1}{2}\)cosh x - This is incorrect.
  • Option 3: \((1 + 2 \cosh x)^{-1}\) - This matches our result.
  • Option 4: \(1 + 2 \cosh x\) - This is the partition function Z, not the probability.

The probability of finding the system with energy \(E=0\) is \((1 + 2 \cosh x)^{-1}\).

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Important Questions from Partition Functions and Their Relation

  1. Six distinguishable particles are distributed over 3 non‐degenerate levels, of energies 0, ε and 2ε. The most probable value for the total energy is

  2. The partition function for a gas is given by

    Q(N, V, T) = \(\frac{1}{N!}\left(\frac{2\pi m}{h^2\beta}\right)^{3N/2}\) (v - Nb)N\(\frac{\beta aN^2}{V}\)

    The internal energy of the gas is

  3. The translational, vibrational, and rotational molecular partition functions for a system containing ideal diatomic gas molecules in the canonical ensemble (N, V, T) are written as, $q_{trans}$, $q_{vib}$, and $q_{rot}$, respectively. The option that correctly defines their thermodynamic variable(s) dependency is

  4. If $q_t$ and $Q_{t,m}$ are the molecular and molar translational partition functions of $X_2$, respectively, then $ln(Q_{t,m})$ = 
    (N is the Avogadro number)

  5. At temperature T, the canonical partition function of a harmonic oscillator with fundamental frequency ($\nu$) is given by
    $q_{vib} (T) = \frac{e^{-h\nu/2k_BT}}{1-e^{-h\nu/k_BT}}$
    For $\frac{h\nu}{k_BT} = 3$, the probability of finding the harmonic oscillator in its ground vibrational state is ____________ (Up to two decimal places)
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