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PHY 102 – Thermal Physics Vocabulary
PHY 102 – Thermal Physics Vocabulary
Course Overview
PHY 102 (M) – Thermal Physics, Sound and Optics (3 Units)
Core areas announced on p. 1
Thermal Physics
Zeroth, First & Second Laws of Thermodynamics
Temperature, calorimetry, heat transfer, change of state, critical points
Gas laws, kinetic theory, black–body radiation
Sound
Production of sound by vibrating solids and air columns
Speed of sound in solids, liquids, gases
Intensity, pitch, quality; ear response; interference; Doppler effect
Optics
Reflection, absorption, spherical mirrors, thin lenses, combinations & aberrations
Optical instruments; resolving power of microscopes
Temperature & Zeroth Law of Thermodynamics
Human sense of “hot/cold” is qualitative and often misleading (e.g.
Tile vs. carpet at same T feels different due to higher heat–transfer rate of tile)
Need a quantitative property → temperature
Zeroth Law statement
If bodies A and B are each in thermal equilibrium with body C, then A and B are in equilibrium with each other → they share a common temperature
Consequences
Temperature is the property that determines heat-flow direction
Two bodies with different T will transfer energy until equilibrium is reached
Thermometers & Temperature Scales
Thermometer principle: some physical property changes reproducibly with T
Examples: liquid volume, solid dimensions, gas pressure/volume, electrical resistance, colour
Absolute (Kelvin) scale
Conversion: T_c = T - 273
Fahrenheit vs. Celsius
Ice point: 32\,^\circ\text F ; steam point: 212\,^\circ\text F
Relationship: T
F = \frac{9}{5}T
C + 32
Only Kelvin has a true zero; any formula involving ratios of temperatures must use kelvins
Example conversion
50\,^\circ\text F \Rightarrow 10\,^\circ\text C \text{ and } 283\,\text K
Thermal Expansion
Linear expansion coefficient \alpha
Definition: \alpha = \frac{\Delta L}{L_i\,\Delta T}
Useful form: \Delta L = \alpha L
i \Delta T = \alpha L
i (T
f - T
i)
Area & volume expansion (isotropic solids)
Area: \Delta A = 2\alpha A_i \Delta T
Volume: \Delta V = \beta V_i \Delta T where \beta = 3\alpha
Example (railroad track)
(a) Find new length at 40\,^\circ\text C for a 30.000 m steel rail starting at 0\,^\circ\text C
(b) If clamped, quantify thermal stress (not numerically worked in transcript)
Quantity of Heat & Specific Heat Capacity
Heat Q is energy transferred due to \Delta T between system & surroundings
For a single phase: Q = mc\,(T - T_0)
c = specific heat capacity (J kg^{-1}\,^\circ\text C^{-1})
Definition of c
c = \dfrac{Q}{m (T - T_0)}; low c ⇒ good thermal conductor; water chosen for engine cooling due to high c
Example 1 (iron vat)
m = 20\,\text{kg},\; c_{\text{Fe}} = 450\,\text{J kg}^{-1}\,^\circ\text C^{-1}
\Delta T = 80\,^\circ\text C ⇒ Q = 7.2\times10^5\,\text J (720 kJ)
Conservation of energy (calorimetry)
In isolated system: \text{heat lost} = \text{heat gained}
Calorimetry Examples
Example 2 (tea + glass cup)
Tea: m=0.20\,\text{kg},\; c=4186\,\text{J kg}^{-1}\,^\circ\text C^{-1},\; T_i=95\,^\circ\text C
Glass cup: m=0.15\,\text{kg},\; c=840\,\text{J kg}^{-1}\,^\circ\text C^{-1},\; T_i=25\,^\circ\text C
Solve m
t c
t(95-T)=m
c c
c(T-25) ⇒ T \approx 89\,^\circ\text C
Example 3 (specific heat of alloy)
Alloy: m=0.150\,\text{kg},\; T_i=540\,^\circ\text C
Water: 0.400\,\text{kg} at 10\,^\circ\text C
Aluminium calorimeter: 0.200\,\text{kg} at 10\,^\circ\text C
Equilibrium T_f=30.5\,^\circ\text C
Apply m
s c
s \Delta T
s = m
w c
w \Delta T
w + m
{Al} c
{Al} \Delta T
{Al} ⇒ c
s \approx 500\,\text{J kg}^{-1}\,^\circ\text C^{-1}
Phase Change & Latent Heat
Specific latent heat L: energy per unit mass for a phase change at constant T
Fusion (solid↔liquid): L_f
Vaporization (liquid↔gas): L
v (greater than L
f because both internal + external work)
Q = mL \;\Longrightarrow\; L = \dfrac{Q}{m}
Example 4 (refrigerator)
Remove heat from 1.5 kg water at 20\,^\circ\text C to form ice at -12\,^\circ\text C
Q = m c
w(20) + mL
f + m c_{ice}(12) \approx 6.6\times10^5\,\text J (660 kJ)
Heating curve notation (ice → water → steam)
Q
1 = m c
{ice}\,10; Q
2 = m L
f; Q
3 = m c
w\,100; Q
4 = m L
v
Newton’s Law of Cooling
Rate proportional to excess temperature
\frac{dQ}{dt} \propto -(T - T_0)
\frac{dQ}{dt} = -k (T - T_0)
Heat-Transfer Mechanisms
Conduction
Microscopic energy flow through matter, predominates in solids/metals
Fourier law: \frac{dQ}{dt} = -kA \frac{(T
1 - T
2)}{l}
k = thermal conductivity (large k ⇒ good conductor)
Example 5 (window)
Glass pane A = 3.0\,\text{m}^2,\; l = 3.2\,\text{mm},\; \Delta T = 1\,^\circ\text C
k_{glass} = 0.84\,\text{J s}^{-1}\,\text{m}^{-1\,^\circ\text C}^{-1} ⇒ \dot Q \approx 790\,\text W
Convection
Bulk movement of fluid; much faster than conduction in fluids
Newton’s cooling analogue: \frac{dQ}{dt} = hA (T - T_0) with h = convection coefficient
Radiation
Does not require medium; energy via electromagnetic waves
Stefan–Boltzmann law: \frac{dQ}{dt} = e\sigma A T^4
Net exchange between body (T$
1$) and surroundings (T$
2$):
\frac{dQ}{dt} = e\sigma A (T
1^4 - T
2^4)
Example 6 (athlete)
A=1.5\,\text{m}^2,\; e=0.70,\; T
{skin}=307\,\text K,\; T
{wall}=288\,\text K
\dot Q \approx 120\,\text W
Kinetic Theory of Gases
Assumptions
Large number N of identical molecules, each mass m, random motion
Mean separation ≫ molecule diameter ⇒ volume mostly empty
Molecules obey classical mechanics; interact only via collisions
Collisions with walls and each other are perfectly elastic
Derivation highlights (cube side l)
Single molecule momentum change on wall: \Delta (mv
x)=2mv
x
Time between successive hits: \Delta t = \frac{2l}{v_x}
Force by one molecule: F = \frac{m v_x^2}{l}
Extend to N molecules, use average \overline{v
x^2}; isotropy ⇒ \overline{v
x^2}=\overline{v
y^2}=\overline{v
z^2}
v
{rms}^2 = \overline{v^2} = 3\overline{v
x^2}
Pressure: P = \frac{1}{3}\frac{N m \overline{v^2}}{V}
Combine with ideal-gas law PV = NkT ⇒
\frac{1}{2} m \overline{v^2} = \frac{3}{2} kT
Root-mean-square speed
v_{rms}=\sqrt{\overline{v^2}} = \sqrt{\frac{3kT}{m}} = \sqrt{\frac{3RT}{M}} (M = molar mass)
Example 7: T=37\,^\circ\text C ⇒ \overline{KE} = \tfrac{3}{2}kT \approx 6.4\times10^{-21}\,\text J per molecule
Laws of Thermodynamics
Fundamental Concepts
System: region/object under study
Closed: no mass flow; Open: mass can cross boundary
Isolated: no energy or mass exchange
Internal energy U: microscopic energy content
Heat (Q): energy transfer driven by \Delta T
Work (W): energy transfer not driven by \Delta T (e.g.
PdV mechanical work)
First Law (Energy conservation)
\Delta Q = \Delta U + \Delta W
Sign conventions (as used in transcript)
Q>0: heat added to system; Q<0: heat lost
W>0: work done by system; W<0: work done on system
\Delta W = P \Delta V for quasi-static volume change
Example 8
(a) Q=+2500\,\text J,\; W=-1800\,\text J ⇒ \Delta U = 4300\,\text J
(b) Q=+2500\,\text J,\; W=+1800\,\text J ⇒ \Delta U = 700\,\text J
Special Thermodynamic Processes
Isothermal (\Delta T=0) for ideal gas
\Delta U=0 ⇒ \Delta Q = \Delta W
\Delta Q = P
1V
1 \ln!\left(\dfrac{V
2}{V
1}\right)
Adiabatic (\Delta Q=0)
0 = \Delta U + \Delta W ⇒ work comes at expense of internal energy
Isochoric / isovolumic (\Delta V=0)
\Delta W=0 ⇒ \Delta Q = \Delta U
Isobaric (P=\text{const})
Not explicitly derived, but work = P\Delta V
Second Law (directionality)
Heat flows spontaneously from hot ⇒ cold, never cold ⇒ hot without external work
Equivalent interpretations (not yet detailed: entropy, heat engines, etc.)
Additional Topics Mentioned (Preview)
Critical points (phase diagrams)
Black-body radiation
Planck law, Wien displacement, Stefan–Boltzmann already introduced via radiation section
Sound
Vibrations of solids/air columns; speed formulas v=\sqrt{Y/\rho} (solids), v=\sqrt{B/\rho} (fluids)
Intensity I = P/A; decibel scale; interference & beats; Doppler effect f' = f\left(\dfrac{v\pm v
o}{v\mp v
s}\right)
Optics
Reflection \theta
i = \theta
r; mirrors \dfrac{1}{f}=\dfrac{1}{d
o}+\dfrac{1}{d
i}
Thin-lens equation, combination of lenses \dfrac{1}{f
{eq}}=\sum \dfrac{1}{f
i}
Aberrations: spherical, chromatic
Resolving power d_{min}=1.22\dfrac{\lambda}{2NA} for microscopes (Rayleigh criterion)
These sections are announced in syllabus and will be covered later; included for conceptual continuity.
Ethical & Practical Implications
Engineering design must account for thermal expansion (e.g.
rail gaps, bridge joints)
High specific heat of water crucial for climate regulation & biological temperature stability
Refrigeration and air-conditioning rely on large L_v for efficient heat removal
Understanding radiative balance fundamental to climate science (Earth–Sun energy budget)
Second-law directionality underpins efficiency limits of engines and informs sustainable energy systems
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Princeton Review AP Calculus BC, Chapter 11: Parametric Equations, Polar Coordinates, and Vector-Valued Functions
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