ch18 lecture 9th edi 60957
TRANSCRIPT
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Chapter 18Temperature, Heat, and the
First Law of Thermodynamics
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18.2 Temperature
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18.3: The Zeroth Law of Thermodynamics
If bodies A and B are each in thermal equilibrium with athird body T, then A and B are in thermal equilibrium witheach other.
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18.4 Measuring Temperature
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18.4 Measuring Temperature, The Constant Volume Gas Thermometer
A constant volume gas thermometer consists of a gas-
filled bulb connected by a tube to a mercury manometer.
By raising and lowering reservoir R, the mercury level
in the left arm of the U-tube can be brought to the zeroof the scale to keep the gas volume constant (variations
in the gas volume can affect temperature
measurements).
The temperature of any body in thermal contact with the
triple-cell bulb is :
(p3 is the pressure exerted by the gas and Cis a
constant).
If the atmospheric pressure ispo, for any pressure p,
Therefore,
Finally, for very small amounts of gas,
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18.5 The Celsius and Fahrenheit Scales
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Example, Conversion Between Temperature Scales
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18.6: Thermal Expansion
When the temperature of an object is raised, the body usually exhibit thermal expansion. With the
added thermal energy, the atoms can move a bit farther from one another than usual, against the spring-
like interatomic forces that hold every solid together.)
The atoms in the metal move farther apart than those in the glass, which makes a metal object expandmore than a glass object.
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18.6: Thermal Expansion, Linear Expansion
If the temperature of a metal rod of lengthL is raised by an amount T, its length
is found to increase by an amount
in which a is a constant called the coefficient of linear expansion.
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18.6: Thermal Expansion, Volume Expansion
If all dimensions of a solid expand with temperature,
the volume of that solid must also expand. Forliquids, volume expansion is the only meaningful
expansion parameter.
If the temperature of a solid or liquid whose volume
is V is increased by an amount DT, the increase in
volume is found to be
where b is the coefficient of volume expansion of
the solid or liquid. The coefficients of volumeexpansion and linear expansion for a solid are related
by
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18.6: Thermal Expansion, Anomalous Expansion of Water
The most common liquid, water, does not
behave like other liquids. Above about
4C, water expands as the temperature
rises, as we would expect.
Between 0 and about 4C, however, water
contracts with increasing temperature.Thus, at about 4C, the density of water
passes through a maximum.
At all other temperatures, the density ofwater is less than this maximum value.
Thus the surface of a pond freezes while
the lower water is still liquid.
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Example, Thermal Expansion of Volume:
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18.7:Temperature and Heat
Heat is the energytransferred between asystem and its environment
because of a temperaturedifference that existsbetween them.
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18 8 Th Ab ti f H t b S lid d Li id
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18.8: The Absorption of Heat by Solids and Liquids
The heat capacity C of an object is the proportionality constantbetween the heat Q that the object absorbs or loses and the
resulting temperature change Tof the object
in which Tiand Tfare the initial and final temperatures of theobject.
Heat capacity C has the unit of energy per degree or energy per
kelvin.
18 8 Th Ab ti f H t b S lid d Li id
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18.8: The Absorption of Heat by Solids and Liquids:Specific Heat
The specific heat, c, is the heat
capacity per unit mass
It refers not to an object but to a unit
mass of the material of which the
object is made.
When quantities are expressed inmoles, specific heats must also involve
moles (rather than a mass unit); they
are then called molar specific heats.
18 8 Th Ab ti f H t b S lid d Li id
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18.8: The Absorption of Heat by Solids and Liquids:Heat of Transformation
The amount of energy per unit mass that must be transferred as heat when a sample
completely undergoes a phase change is called the heat of transformationL. When a sample
of mass m completely undergoes a phase change, the total energy transferred is:
When the phase change is between
liquid to gas, the heat of transformation
is called the heat of vaporization LV.
When the phase change is between solid
to liquid, the heat of transformation is
called the heat of fusion LF.
E l H Sl i W
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Example, Hot Slug in Water:
E l H Ch T
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Example, Heat to Change Temperature:
E l H t t Ch T t t
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Example, Heat to Change Temperature, cont.:
18 9: A Closer Look at Heat and Work
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18.9: A Closer Look at Heat and Work
18 10: The First Law of Thermodynamics
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18.10: The First Law of Thermodynamics
The quantity (Q
W) is the same for all processes. It depends only on theinitial and final states of the system and does not depend at all on how the
system gets from one to the other.
All other combinations ofQ and W, including Q alone, Walone, Q +W,
and Q -2W, are path dependent; only the quantity (Q
W) is not.
(Q is the heat and W is the work done by the system).
18 11: Some Special Cases of the First Law of Thermodynamics
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18.11: Some Special Cases of the First Law of Thermodynamics
1. Adiabatic processes. An adiabatic process is one that occurs so rapidly oroccurs in a system that is so well insulated that no transfer of thermal
energy occursbetween the system and its environment. Putting Q=0 in
the first law,
2. Constant-volume processes. If the volume of a system (such as a gas) isheld constant,so thatsystem can do no work. Putting W=0 in the firstlaw,
3. Cyclical processes. There are processes in which, after certaininterchanges of heat and work, the system is restored to its initial state.
No intrinsic property of the systemincluding its internal energycan
possibly change. PuttingEint= 0 in the first law
4. Free expansions. These are adiabatic processes in which no heat transferoccurs between the system and its environment and no work is done on or
by the system. Thus, Q =W =0, and the first law requires that
18 11: Some Special Cases of the First Law of Thermodynamics
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18.11: Some Special Cases of the First Law of Thermodynamics
Example First Law of Thermodynamics:
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Example, First Law of Thermodynamics:
Example
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Example,
First Law of Thermodynamics,
cont.:
18 12: Heat Transfer Mechanisms: Conduction
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18.12: Heat Transfer Mechanisms: Conduction
A slab of face area A and thicknessL, have faces
maintained at temperatures THand TCby a hot
reservoir and a cold reservoir. IfQ be the energy
that is transferred as heat through the slab, fromits hot face to its cold face, in time t, then the
conduction ratePcond(the amount of energy
transferred per unit time) is
Here k, called the thermal conductivity, is a
constant that depends on the material of which
the slab is made.
The thermal resistanceR, or the R-value of a
slab of thicknessL is defined as:
18 12: Heat Transfer Mechanisms: Conduction
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18.12: Heat Transfer Mechanisms: Conduction
18 12: Heat Transfer Mechanisms: Conduction
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18.12: Heat Transfer Mechanisms: Conduction
Letting TXbe the temperature of
the interface between the two
materials, we have:
For n materials making up the slab,
Fig. 18-19 Heat is transferred at a steady rate
through a composite slab made up of two
different materials with different thicknesses and
different thermal conductivities.
The steady-state temperature at the interface ofthe two materials is TX.
18 12: Heat Transfer Mechanisms: Convection
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18.12: Heat Transfer Mechanisms: Convection
In convection, energy transfer occurs when a fluid, such as air or
water, comes in contact with an object whose temperature is higher
than that of the fluid.
The temperature of the part of the fluid that is in contact with the hot
object increases, and (in most cases) that fluid expands and thus
becomes less dense.
The expanded fluid is now lighter than the surrounding cooler fluid,
and the buoyant forces cause it to rise.
Some of the surrounding cooler fluid then flows so as to take the place
of the rising warmer fluid, and the process can then continue.
18 12: Heat Transfer Mechanisms: Radiation
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18.12: Heat Transfer Mechanisms: Radiation
In radiation, an object and its environment can exchange energy as heat via electromagnetic
waves. Energy transferred in this way is called thermal radiation.
The ratePradat which an object emits energy via electromagnetic radiation depends on the
objects surface area A and the temperature T of that area in K, and is given by:
Here s =5.6704 x10-8 W/m2 K4 is called the StefanBoltzmann constant, andeis the emissivity.
If the rate at which an object absorbs energy via thermal radiation from its environment isPabs,
then the objects net ratePnetof energy exchange due to thermal radiation is:
Example Thermal Conduction Through a Layered Wall:
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Example, Thermal Conduction Through a Layered Wall: