Decoding the V-T Graph
A Journey Through Thermodynamic Processes
Imagine you are a microscopic observer inside a container holding an ideal monatomic gas. The gas is undergoing a fascinating cyclic journey, expanding and compressing, heating up and cooling down. This journey is mapped out for us on a Volume-Temperature (V-T) diagram. Our mission? To find out exactly how much heat the gas absorbs during one specific leg of this journey: the path from state X to state Y.
Analyzing the Setup
The first step in any thermodynamics problem is to decode the graph. We are given a cycle WXYZW on a V-T diagram. The problem states it consists of consecutive adiabatic and isobaric processes. But which is which?
Look closely at the lines XY and ZW. If you extend them, they pass straight through the origin. In a V-T diagram, a straight line passing through the origin means that Volume is directly proportional to Temperature (V∝T). According to the ideal gas law, PV=nRT, or V=(PnR)T. For the slope to be constant, the pressure P must be constant. Therefore, paths XY and ZW are isobaric processes.
By elimination, the curved paths WX and YZ must be the adiabatic processes.
The Master Equation
We need the heat absorbed during the isobaric expansion XY. The formula for heat exchanged at constant pressure is:
QXY=nCPΔT=nCP(TY−TX)
For an ideal monatomic gas, the molar heat capacity at constant pressure is CP=25R. Substituting this in, we get:
QXY=n(25R)(TY−TX)=25(nRTY−nRTX)
Using the ideal gas law again, we can replace the temperature terms with pressure and volume:
QXY=25(PYVY−PXVX)
Since the process XY is isobaric, the pressure remains constant, meaning PY=PX. We can factor this out to get our master equation:
QXY=25PX(VY−VX)
We know the volumes VX and VY, but we are missing the pressure PX.
Bridging the Gap
To find PX, we must look at the preceding process, the adiabatic path WX. The defining equation for an adiabatic process is PVγ=constant. Therefore:
PXVXγ=PWVWγ
Rearranging this to solve for PX, we get:
PX=PW(VXVW)γ
For a monatomic gas, the adiabatic index γ=35. But wait, we still don't know PW!
Here is where the problem gives us a golden key: nRTW=1 J. From the ideal gas law, PWVW=nRTW, which means PWVW=1 J. This elegantly simplifies to:
PW=VW1
Now, we substitute this back into our equation for PX:
PX=VW1(VXVW)35
Final Calculation
We now have everything we need. Let's plug our expression for PX back into the master heat equation:
QXY=25[VW1(VXVW)35](VY−VX)
Now, we substitute the given volume values: VW=64 cm3, VX=125 cm3, and VY=250 cm3. You might be worried about converting cm3 to m3. While it's a good habit, notice how the conversion factor 10−6 appears in the numerator (VY−VX) and the denominator VW, and also inside the ratio (VW/VX). It perfectly cancels out everywhere! We can safely use the raw numbers:
QXY=25×641×(12564)35×(250−125)
Notice the beautiful numbers chosen by the examiner. 64 is 43 and 125 is 53. This makes applying the power of 35 incredibly satisfying:
QXY=25×641×(5343)35×125
QXY=25×641×5545×125
QXY=25×641×31251024×125
Simplifying the fractions:
QXY=25×16×251=5080=1.6 J
And there we have it. Through careful analysis of the graph and methodical substitution, we found that the gas absorbs exactly 1.60 J of heat during the isobaric expansion.