Is the enthalpy change of a reversible adiabatic expansion any different from enthalpy change of a irreversible adiabatic expansion?
Enthalpy is a state function, and its changes $\Delta H$ are independent of the path from state $1$ to state $2$. Thus, an adiabatic reversible process or adiabatic irreversible process, will yield an identical $\Delta H$.
So some sites say that adiabatic expansions of ideal gases in general have $△H=0$ , whereas some say it is not.
The enthalpy change for an ideal gas only depends on temperature. The only way that this change is zero is proved below
\begin{align}
\Delta H = \int_{T_1}^{T_2} c_p^\pu{ig}(T) \; dT = 0 \therefore
\boxed{\Delta H = 0 \Leftrightarrow T_1 =T_2} \tag{1}
\end{align}
In consequence, ideal gases suffer an isenthalpic process if and only if the process is isothermal. Adiabatic reversible or irreversible processes have a change in temperature, and thus, cannot be isenthalpic.
What is wrong with this proof?
The proof is fine. Remember it is only valid for:
- An ideal gas.
- It has constant-pressure and constant-volume heat capacities, so that $\gamma$ is also constant.
However, if you pay attention, there was no need to invoke any reversible/irreversible adiabatic process. It is a general expression, I will show you another way
\begin{align}
\Delta U &= \int_{T_1}^{T_2} c_V^\pu{ig} \; dT \\
\Delta U &= c_V^\pu{ig} \int_{T_1}^{T_2} \; dT \\
\Delta U &= c_V^\pu{ig} (T_2 - T_1) \\
\Delta U &= \frac{c_V^\pu{ig}}{R} (RT_2 - RT_1) \hspace{1 cm} (\text{use that $R = c_P^\pu{ig} - c_V^\pu{ig}$}) \\
\Delta U &= \frac{c_V^\pu{ig}}{c_P^\pu{ig} - c_V^\pu{ig}} (RT_2 - RT_1) \\
\Delta U &= \frac{1}{(c_P^\pu{ig}/ c_V^\pu{ig}) - 1} (RT_2 - RT_1)
\hspace{1 cm} (\text{Use ideal gas law}) \\
\Delta U &= \frac{1}{\gamma - 1} (P_2V_2 - P_1V_1) \tag{2} \\
\end{align}
And by the definition of enthalpy, using Eq. (2)
\begin{align}
\Delta H &= \Delta U + \Delta (PV) \\
\Delta H &= \frac{1}{\gamma - 1} (P_2V_2 - P_1V_1) + \Delta (PV) \\
\Delta H &= \Delta (PV)\left(\frac{1}{\gamma - 1} + 1\right) \rightarrow
\Delta H = \left(\frac{\gamma}{\gamma - 1}\right)\Delta (PV) \tag{3}
\end{align}
So, it was not necessary to specify how state $1$ goes from state $2$. Nevertheless, it respects Eq. (1)
\begin{align}
\Delta H &= \left(\frac{\gamma}{\gamma - 1}\right) (P_2V_2 - P_1V_1) \\
\Delta H &= \left(\frac{\gamma}{\gamma - 1}\right) (RT_2 - RT_1) \\
\Delta H &= \left(\frac{R\gamma}{\gamma - 1}\right) (T_2 - T_1) = 0 \therefore T_2 = T_1 \tag{4}
\end{align}