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Show that the volume expansion coefficient of an ideal gas is \(\beta=1 / T\), where \(T\) is the absolute temperature.

Short Answer

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Question: Show that the volume expansion coefficient of an ideal gas is inversely proportional to the absolute temperature. Answer: The volume expansion coefficient (β) of an ideal gas is inversely proportional to the absolute temperature, which means β = 1 / T.

Step by step solution

01

Understand the volume expansion coefficient and ideal gas law

The volume expansion coefficient (β) of a substance is a measure of how the volume of the substance changes with temperature, at a constant pressure. Mathematically, it is defined as: \(\beta = \frac{1}{V} \frac{\partial V}{\partial T}\Big|_P\) where V is the volume, T is the absolute temperature, and P is the pressure. The ideal gas law relates the pressure (P), volume (V), and temperature (T) of an ideal gas: \(PV = nRT\) where n is the number of moles of the gas and R is the ideal gas constant.
02

Express the volume as a function of temperature and pressure

From the ideal gas law, we can express the volume (V) as a function of temperature (T) and pressure (P): \(V = \frac{nRT}{P}\)
03

Calculate the partial derivative of the volume with respect to the temperature

Now, we will calculate the partial derivative of the volume with respect to the temperature (keeping the pressure constant): \(\frac{\partial V}{\partial T}\Big|_P = \frac{\partial}{\partial T} \left(\frac{nRT}{P}\right)\Big|_P = \frac{nR}{P}\) Here, we treat n, R, and P as constants.
04

Calculate the volume expansion coefficient

Finally, we will plug our expression for the partial derivative of the volume with respect to the temperature back into the equation for the volume expansion coefficient: \(\beta = \frac{1}{V} \frac{\partial V}{\partial T}\Big|_P = \frac{1}{\frac{nRT}{P}} \frac{nR}{P}\) Simplifying, we get: \(\beta = \frac{1}{T}\) Therefore, the volume expansion coefficient of an ideal gas is inversely proportional to the absolute temperature, β = 1 / T.

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Key Concepts

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

Ideal Gas Law
The Ideal Gas Law is a fundamental equation in thermodynamics, which describes how gases behave under various conditions. It connects pressure \(P\), volume \(V\), and temperature \(T\) in a simple way. The law is expressed as:\[PV = nRT\]where:
  • \(n\) represents the number of moles of the gas.
  • \(R\) is the ideal gas constant, valued at 8.314 J/(mol·K).
This equation implies that if you know any three properties of a gas, you can calculate the fourth. The relationship shows that as temperature increases, volume increases if pressure remains constant. It forms the basis for understanding gas behaviors and is widely applicable in various science fields. This can be particularly helpful when dealing with changes in conditions such as temperature and pressure.
Volume Change with Temperature
Volume change with temperature is often observed in gases and is measured by the volume expansion coefficient \(\beta\). This coefficient indicates how much the volume of a substance changes with a temperature shift while under constant pressure. Mathematically, it's expressed as:\[\beta = \frac{1}{V} \frac{\partial V}{\partial T}\Big|_P\]The intuition here is simple: if you heat a gas, it will generally expand or increase in volume if the pressure is the same. For ideal gases, as derived in the exercise, \(\beta = \frac{1}{T}\), indicating that the expansion is inversely proportional to temperature. This insight is critical for applications like designing systems and processes where temperature fluctuations are a concern.
Partial Derivative
Partial derivatives play a vital role in understanding how a function changes as one specific variable changes, while others are held constant. It's a common tool in calculus used to explore multi-variable functions. In the context of thermodynamics, it helps us determine the rate of change of variables like volume and temperature.For instance, in calculating the volume expansion coefficient of an ideal gas, the partial derivative of volume with respect to temperature is:\[\frac{\partial V}{\partial T}\Big|_P = \frac{nR}{P}\]This step is crucial because it shows how the volume changes as temperature changes, specifically when pressure is held steady. Understanding partial derivatives helps in analyzing complex systems where multiple factors interact.
Thermodynamics
Thermodynamics is the branch of physics that deals with heat, work, and energy. It examines how energy is transferred and transformed within systems. The fundamental laws of thermodynamics provide the framework for understanding these processes. Key principles include:
  • Energy can neither be created nor destroyed (First Law of Thermodynamics).
  • The entropy of a system tends to increase (Second Law of Thermodynamics).
With regards to gas laws, thermodynamics helps explain how gases expand and contract with changes in temperature and pressure. The concept of the volume expansion coefficient, as discussed in the exercise, is a perfect example of applying thermodynamic principles to predict how an ideal gas will behave under specific conditions. Understanding these relationships is vital in fields ranging from engineering to natural sciences.

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Most popular questions from this chapter

Exhaust gases from a manufacturing plant are being discharged through a \(10-\mathrm{m}-\) tall exhaust stack with outer diameter of \(1 \mathrm{~m}\). The exhaust gases are discharged at a rate of \(0.125 \mathrm{~kg} / \mathrm{s}\), while temperature drop between inlet and exit of the exhaust stack is \(30^{\circ} \mathrm{C}\), and the constant pressure-specific heat of the exhaust gases is \(1600 \mathrm{~J} / \mathrm{kg} \cdot \mathrm{K}\). On a particular calm day, the surrounding quiescent air temperature is \(33^{\circ} \mathrm{C}\). Solar radiation is incident on the exhaust stack outer surface at a rate of \(500 \mathrm{~W} / \mathrm{m}^{2}\), and both the emissivity and solar absorptivity of the outer surface are \(0.9\). Determine the exhaust stack outer surface temperature. Assume the film temperature is \(60^{\circ} \mathrm{C}\).

Consider a fluid whose volume does not change with temperature at constant pressure. What can you say about natural convection heat transfer in this medium?

A \(12-\mathrm{cm}\)-high and 20-cm-wide circuit board houses 100 closely spaced logic chips on its surface, each dissipating \(0.05 \mathrm{~W}\). The board is cooled by a fan that blows air over the hot surface of the board at \(35^{\circ} \mathrm{C}\) at a velocity of \(0.5 \mathrm{~m} / \mathrm{s}\). The heat transfer from the back surface of the board is negligible. Determine the average temperature on the surface of the circuit board assuming the air flows vertically upward along the 12 -cm-long side by (a) ignoring natural convection and ( \(b\) ) considering the contribution of natural convection. Disregard any heat transfer by radiation. Evaluate air properties at a film temperature of \(47.5^{\circ} \mathrm{C}\) and 1 atm pressure. Is this a good assumption?

The primary driving force for natural convection is (a) shear stress forces (b) buoyancy forces (c) pressure forces (d) surface tension forces (e) none of them

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