$q(T) = (\frac{k_B T}{hc})^{\frac{3}{2}} (\frac{8\pi^2 mk_B T}{h^2})^{\frac{3}{2}}$, where the symbols have their usual meanings.
The heat capacity at constant volume for this system is
The given molecular partition function is:
$q(T) = \left(\frac{k_B T}{hc}\right)^{\frac{3}{2}} \left(\frac{8\pi^2 mk_B T}{h^2}\right)^{\frac{3}{2}}$
Let's simplify this expression. We can combine the terms and group the temperature dependence:
$q(T) = \left( \frac{k_B}{hc} \cdot \frac{8\pi^2 m k_B}{h^2} \right)^{\frac{3}{2}} \cdot (T)^{\frac{3}{2} + \frac{3}{2}}$
$q(T) = \left( \frac{8\pi^2 m k_B^2}{h^3 c} \right)^{\frac{3}{2}} \cdot T^3$
This simplifies to the form $q(T) = C \cdot T^3$, where $C$ is a constant.
The average internal energy ($U$) of the system is related to the partition function by:
$U = k_B T^2 \left( \frac{\partial \ln q}{\partial T} \right)_V$
First, find the natural logarithm of the partition function:
$\ln q(T) = \ln C + \ln(T^3) = \ln C + 3 \ln T$
Next, calculate the derivative of $\ln q(T)$ with respect to temperature ($T$):
$\frac{\partial \ln q}{\partial T} = \frac{3}{T}$
Now substitute this into the formula for average energy:
$U = k_B T^2 \left( \frac{3}{T} \right)$
$U = 3 k_B T$
The heat capacity at constant volume ($C_V$) is the derivative of the average energy with respect to temperature:
$C_V = \left( \frac{\partial U}{\partial T} \right)_V$
Differentiating the expression for $U$:
$C_V = \frac{\partial}{\partial T} (3 k_B T)$
$C_V = 3 k_B$
The result $C_V = 3 k_B$ is the heat capacity per particle. To express this in terms of the ideal gas constant ($R$) for one mole of substance, we use the relationship $R = N_A k_B$, where $N_A$ is Avogadro's number.
Molar Heat Capacity $= N_A \times C_V = N_A \times (3 k_B)$
Molar Heat Capacity $= 3 (N_A k_B) = 3R$
Therefore, the heat capacity at constant volume for this system is $3R$.
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
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)Ne \(\frac{\beta aN^2}{V}\)
The internal energy of the gas is
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 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
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)