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Using the Helmholtz energy, demonstrate that the pressure for an ideal polyatomic gas is identical to that derived for an ideal monatomic gas in the text.

Short Answer

Expert verified
Using the Helmholtz energy equation \(A = U - TS\), we derived the internal energy (U) and entropy (S) for an ideal polyatomic gas. Then, we identified the pressure formula in terms of Helmholtz energy as \(P = -\left(\frac{\partial A}{\partial V}\right)_{T}\) and calculated the pressure for both ideal polyatomic and monatomic gases. We found that the pressure for an ideal polyatomic gas is \(P = nR\left(\frac{1}{V}\right)\), which is identical to that of an ideal monatomic gas, \(P = nRT\left(\frac{1}{V}\right)\). Thus, using the Helmholtz energy, we demonstrated that the pressure for an ideal polyatomic gas is identical to that derived for an ideal monatomic gas.

Step by step solution

01

Write the Helmholtz energy equation for an ideal polyatomic gas

The Helmholtz energy (A) for an ideal polyatomic gas can be written as: \(A = U - TS\) Where U is the internal energy, T is the temperature, and S is the entropy. For an ideal polyatomic gas, the internal energy (U) depends on the number of degrees of freedom (f), number of moles (n), and the molar specific heat C_V: \(U = \frac{f}{2}nRT\) The entropy (S) also depends on the number of moles (n), the volume (V), and the gas constant (R): \(S = nR\left(\ln(V)+C_v \ln(T)\right)\)
02

Identify the formula for pressure in terms of Helmholtz energy for an ideal gas

To find the pressure using Helmholtz energy, we need the following derivative: \(P = -\left(\frac{\partial A}{\partial V}\right)_{T}\)
03

Calculate the pressure for ideal polyatomic and monatomic gases

Now, we substitute the expressions for U and S obtained in Step 1 into the Helmholtz energy equation: \(A = \frac{f}{2}nRT-nRT\left(\ln(V)+C_v \ln(T)\right)\) Now we compute the derivative: \(P = -\left(\frac{\partial A}{\partial V}\right)_{T} = -\left(\frac{\partial}{\partial V} \left[\frac{f}{2} nRT - nRT\left(\ln(V)+C_v \ln(T)\right)\right]\right)_T\) After taking the derivative with respect to V: \(P = -\left[-nR\frac{\partial}{\partial V}\left(\ln(V)\right)\right]_T = nR\left(\frac{1}{V}\right)\) Note that for an ideal monatomic gas, the pressure is also given by: \(P = nRT\left(\frac{1}{V}\right)\) Thus, we have demonstrated that the pressure for an ideal polyatomic gas is identical to that derived for an ideal monatomic gas using the Helmholtz energy.

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Key Concepts

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

Thermodynamics
Thermodynamics is a branch of physics that deals with the relationships between heat and other forms of energy. In essence, it studies the effects of changes in temperature, volume, and pressure of systems at the macroscopic level. The first law of thermodynamics states that energy cannot be created or destroyed in an isolated system. The second law introduces the concept of entropy, indicating that systems tend to progress towards disorder. In the context of gases, thermodynamics provides the framework for understanding their macroscopic properties, like pressure and temperature, through various energy functions, such as the Helmholtz energy. This function is particularly useful because it connects internal energy, temperature, and entropy in a way that can describe the work potential of the system at constant temperature and volume.

Moreover, thermodynamic equations allow us to predict how gases will behave under certain conditions, for example, when comparing ideal polyatomic gases with ideal monatomic gases. Understanding these fundamental concepts is essential for grasping the behavior of different types of gases and the potential energy for doing work within thermodynamic processes.
Ideal Polyatomic Gas
An ideal polyatomic gas is a theoretical model of a gas where the molecules consist of more than two atoms. It assumes that the gas particles are point masses with no volume and that there are no intermolecular forces except during elastic collisions. For such gases, the energy related to the movement of atoms within the molecules adds to the total internal energy, which means they have more degrees of freedom compared to monatomic gases (single-atom molecules).

Typically, an ideal polyatomic gas will have rotational and vibrational modes contributing to its energy states. The internal energy of a polyatomic gas depends not only on the temperature but also on the number of degrees of freedom. This results in different values for the specific heats at constant volume (\(C_v\)) and at constant pressure (\(C_p\) following the relation \(C_p = C_v + R\) where \(R\) is the gas constant. Even though these gases are more complex, under certain conditions, they can exhibit properties similar to monatomic gases, as shown when comparing the derived pressures from their respective Helmholtz energies.
Ideal Monatomic Gas
In contrast, an ideal monatomic gas consists of single-atom molecules. It shares the same basic assumptions as the ideal polyatomic gas: the particles are point-like, no volume, and no interactions except during collisions. Since their molecules are single atoms, these gases have fewer degrees of freedom, typically just translational motions in three-dimensional space, which directly relate to the kinetic energy of the gas. This simplicity allows for more straightforward calculations of their internal energy and other thermodynamic properties.

For monatomic gases, the molar specific heat at constant volume (\(C_v\) is well-defined and lower than that of polyatomic gases due to the lesser degrees of freedom. In all energetic equations, only translational motion is considered, since there are no rotational or vibrational modes for single atoms, further simplifying our understanding of their internal energy and behavior under various thermodynamic processes.
Internal Energy
Internal energy, often symbolized by \(U\) is one of the key concepts in thermodynamics and represents the total energy contained within a system, which in the case of gases, is primarily kinetic energy resulting from the motion of the particles. For an ideal gas, this includes both translational kinetic energy and, in the case of polyatomic gases, rotational and vibrational kinetic energy as well. The formula \(U = \frac{f}{2}nRT\) used in calculating the Helmholtz energy of a polyatomic gas reflects this, with \(f\) representing the degrees of freedom.

Internal energy is a state function, meaning it's determined solely by the current state of the system and not the path the system took to reach that state. Changes in the internal energy of a system can manifest as changes in temperature or as work done by or on the system. A deeper grasp of internal energy is crucial for understanding various thermodynamic processes, including those that involve doing work.
Entropy
Entropy, symbolized by \(S\) is a fundamental concept in thermodynamics that measures the degree of disorder or randomness in a system. It is a state function and is often associated with the second law of thermodynamics, which indicates that in a natural thermodynamic process, the sum of the entropies of the interacting thermodynamic systems increases. In the context of the Helmholtz energy for an ideal gas, the entropy term integrates variables such as the number of moles, volume, and temperature of the gas.

The equation \(S = nR(\ln(V) + C_v \ln(T))\) describes how entropy changes with volume and temperature for a given amount of gas. Understanding the role of entropy is essential not only in predicting the direction and spontaneity of processes but also in establishing the degree of energy dispersion and the thermal efficiency of thermodynamic cycles.
Degrees of Freedom
Degrees of freedom in the context of thermodynamics refer to the number of independent ways by which a system can possess energy. For gases, these are related to the types of motion the molecules can perform, which include translational, rotational, and vibrational movements.

An ideal monatomic gas has only three translational degrees of freedom, corresponding to movement along the x, y, and z axes. A polyatomic gas also has rotational and sometimes vibrational degrees of freedom, depending on the complexity of the molecule. Each degree of freedom contributes to the gas's internal energy; this correlation is exemplified in the classical equation for internal energy (\(U\) that takes into account the degrees of freedom. Knowing the specific degrees of freedom helps in accurately calculating thermodynamic properties such as specific heats, changes in internal energy, and, as shown in the exercise, the Helmholtz energy.

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