1.7.6 · D1Thermodynamics

Foundations — Heat transfer — conduction (Fourier's law k), convection, radiation (Stefan-Boltzmann σT⁴)

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This page builds every symbol the parent note leans on, starting from a reader who has never seen a single one. Each entry gives you three things: plain meaning → the picture → why the topic needs it. Read top to bottom; each rung of the ladder rests on the one below it.


0. What even is heat? (the ground floor)

Picture a jar of tiny balls (atoms) that never stop trembling. In a cold jar they barely quiver; in a hot jar they shake violently.

Figure — Heat transfer — conduction (Fourier's law k), convection, radiation (Stefan-Boltzmann σT⁴)
  • Plain meaning: measures average jiggle energy per atom.
  • The picture: left jar = slow, small arrows; right jar = fast, big arrows.
  • Why the topic needs it: every single formula here is driven by a temperature difference. Without there is no "hot" and "cold", and heat has no direction to flow.

1. Two ways to measure temperature: Celsius and Kelvin

Figure — Heat transfer — conduction (Fourier's law k), convection, radiation (Stefan-Boltzmann σT⁴)
  • The picture: one vertical thermometer with two rulers glued side by side; the tick marks line up but the zero of each is in a different place. The spacing between ticks is identical.
  • Why the topic needs it — the crucial subtlety: because the ticks are the same size, a difference is the same on both scales: But a single value is not: , not K.
Recall When may I leave a temperature in Celsius?

Only when it appears as a difference (as in Fourier's law). Any single value or any power of (like in radiation) must be in kelvin. ::: Differences OK in °C; single values and powers must be K.


2. Rate of change: what means

Why this tool and not just ""? A wall doesn't care about total joules — it cares about flow speed. Asking "how many joules per second?" is exactly what a rate answers, and the physics symbol for "per second, instant by instant" is the derivative .

  • The picture: water leaving a tap. is the total litres in the bucket; is how fast the stream is running right now.
  • This rate has a name in this topic: the heat current .

3. The temperature gradient

Figure — Heat transfer — conduction (Fourier's law k), convection, radiation (Stefan-Boltzmann σT⁴)
  • The picture: a wall drawn as a ramp of temperature — hot face high on the left, cold face low on the right. The slope of that ramp is . A steep ramp = big gradient = strong push for heat.
  • Why the sign is negative: as you walk in the direction (into the cold), goes down, so is a negative number. Heat flows the opposite way — toward — which is why Fourier's law carries a to keep positive.
  • Why the topic needs it: conduction is driven by steepness of the drop, not by the raw temperatures. The gradient is that steepness.

4. Area and thickness — the shape of the wall

  • The picture: a slab (a brick). = the flat front you'd paint; = how deep the brick goes front-to-back.
  • Why the topic needs both: a wider face () lets more heat through in parallel; a deeper brick () makes heat travel further, slowing it. These are the two geometry knobs in Fourier's law.

5. Material constants: , , ,

Each mode of transfer hides its "how easily?" inside a constant. Meet them.


6. Power and the 4th power

Figure — Heat transfer — conduction (Fourier's law k), convection, radiation (Stefan-Boltzmann σT⁴)
  • The picture: four curves , , , climbing out of the origin — rockets up far above the others. That steepness is why a small rise in temperature causes a huge jump in radiated power.
  • Why the topic needs it: radiation obeys , so it becomes the dominant loss channel at high temperature (a filament, the Sun) even though it's tiny at room temperature.

7. The thermal ↔ electrical analogy

The parent maps heat onto electricity. Line the pictures up:

Heat picture Electrical twin See
temperature difference voltage
heat current current
thermal resistance resistance Electrical resistance Ohm's law
  • Why the topic borrows this: you already know series/parallel resistor rules; reusing them for composite walls saves inventing new maths. Heat "flowing downhill" from high is exactly current flowing from high voltage.

Prerequisite map

Temperature T

Temperature difference delta T

Celsius and Kelvin scales

Absolute T needed for T to the 4th

Rate d by dt

Heat current H in watts

Gradient dT by dx

Fouriers law conduction

Area A and thickness delta x

Material constant k

Convection Newton cooling

Convection coefficient h

Stefan Boltzmann radiation

Emissivity e

Constant sigma

Thermal resistance analogy

Heat transfer topic


Equipment checklist

Say each answer out loud before revealing.

I can explain the difference between temperature and heat
= how fast atoms jiggle (a level); = amount of jiggle-energy transferred (joules).
I can convert between Celsius and Kelvin
; differences are equal on both scales.
I know when Celsius is allowed and when only Kelvin works
Differences may stay in °C; single values and any power of must be in kelvin.
I can read and in plain words
"heat per second" (a rate) and "temperature change per metre into the wall" (a slope).
I know why Fourier's law has a minus sign
Moving in into the cold makes drop, so ; the keeps positive in the flow direction.
I know what and do to heat flow
Bigger → more flow (parallel); bigger → less flow (further to travel).
I can name the four constants and their units
(W m⁻¹ K⁻¹) conduction, (W m⁻² K⁻¹) convection, (dimensionless 0–1) emissivity, W m⁻² K⁻⁴ radiation.
I know why makes radiation explode at high temperature
grows very steeply — doubling multiplies power by .
I can match heat quantities to their electrical twins
voltage, current, resistance.