Heat transfer Chapter 1: Introduction

These notes introduce heat transfer as the study of energy exchange rates driven by temperature differences. They clarify the distinction between energy and temperature, explain how energy is stored at the microscopic level, introduce the concept of local thermodynamic equilibrium, and provide a first overview of the fundamental heat transfer mechanisms: conduction, convection, radiation, and phase change. The emphasis is on physical meaning and modeling intuition rather than equations

 

Context & Motivation

Heat transfer complements thermodynamics.

  • Thermodynamics tells us how much energy is required to move between equilibrium states.

  • Heat transfer tells us how fast that energy is exchanged.

Engineering systems rarely operate at equilibrium:

  • Engines cool down.

  • Walls lose heat.

  • Fluids warm up as they flow.

  • Phase changes occur over finite time.

Understanding rates of energy exchange is therefore essential for:

  • Thermal design

  • Safety analysis

  • Efficiency optimization

  • Multiphysics CFD simulations


Energy vs. Temperature

3.1 What Energy Really Means

Energy is a conserved property of matter and fields. It can:

  • Be stored

  • Be transferred

  • Change form

but cannot be created or destroyed.

In heat transfer, we mainly care about how energy is stored inside matter and how it moves between regions.

3.2 Microscopic Energy Storage Mechanisms

Energy is stored in matter through discrete microscopic modes:

In gases

  • Translational motion (molecule moving)

  • Rotational motion (molecule spinning)

  • Vibrational motion (atoms oscillating)

  • Electronic excitation (electrons at higher energy states)

Each mode becomes active only when sufficient energy is available.
At low temperatures, only translation is active; at higher temperatures, more modes contribute.

This explains why thermal properties depend on temperature.

In liquids

  • Same molecular modes as gases

  • Plus intermolecular potential energy

Energy added to a liquid can be used to:

  • Increase molecular agitation (temperature rise)

  • Break intermolecular bonds (phase change)

In solids

  • Atoms vibrate around fixed lattice positions

  • Collective vibrations (phonons) dominate

Temperature in solids primarily measures vibrational energy, not motion through space.

3.3 Energy in Vacuum

Energy can also exist without matter:

  • Electromagnetic radiation

  • Vacuum energy (quantum effects)

Radiation is especially important for high-temperature heat transfer and does not require a material medium.


What Temperature Actually Measures

Temperature is not a measure of total energy.

Instead:

  • It measures the energy stored in the most fundamental active mode:

    • Translational kinetic energy (gases/liquids)

    • Vibrational kinetic energy (solids)

Other energy storage modes may exist but are not directly reflected by temperature unless equilibrium is achieved.


Local Thermodynamic Equilibrium (LTE)

In real materials, energy constantly redistributes between storage modes through collisions and interactions.

Key insight:

  • This redistribution happens very fast (microseconds or less)

  • Much faster than typical engineering time scales

Therefore, in most heat transfer problems:

  • Each small region can be assumed to be in local thermodynamic equilibrium

  • Classical thermodynamic relations remain valid locally

Exceptions:

  • Rarefied gases

  • Shock waves

  • Very fast transients

  • High-altitude or vacuum environments


Conservation of Energy (Conceptual View)

All heat transfer problems are governed by energy conservation.

Physically, this means:

  • Energy inside a region can change

  • Energy can move by different mechanisms

  • Energy can be generated or absorbed (chemical reactions, phase change)

In CFD, this is captured by the energy equation, which accounts for:

  • Convection

  • Conduction

  • Radiation

  • Viscous dissipation

  • Species diffusion

  • Phase change sources


Fundamental Heat Transfer Mechanisms

7.1 Conduction

  • Occurs within solids and fluids at rest

  • Driven by temperature gradients

  • Microscopic origin:

    • Molecular collisions (fluids)

    • Lattice vibrations and electron motion (solids)

Conduction dominates when:

  • Velocities are small

  • Solids are involved

  • Thin layers resist heat flow

7.2 Convection

  • Heat transfer due to fluid motion

  • Energy is transported with the flow

Types:

  • Forced convection: flow driven externally

  • Natural convection: buoyancy-driven

  • Boiling convection: phase change at surfaces

Convection tightly couples:

  • Momentum equations

  • Energy equation

This is why heat transfer problems often require solving flow and energy simultaneously.

7.3 Radiation

  • Energy transfer by electromagnetic waves

  • Requires no medium

  • Strongly temperature-dependent

Radiation becomes important when:

  • Temperatures are high

  • Large surfaces are involved

  • Conduction and convection are weak

Radiation modeling is computationally expensive and must be chosen carefully based on optical thickness.

7.4 Phase Change Heat Transfer

  • Energy absorbed or released during state change

  • Temperature may remain nearly constant during the process

Examples:

  • Evaporation

  • Condensation

  • Boiling

  • Melting / solidification

Phase change often dominates heat transfer rates due to latent heat and requires specialized multiphase models


Engineering and CFD Perspective

From a modeling standpoint:

  • Heat transfer problems require:

    • Energy equation activation

    • Correct material properties

    • Appropriate boundary conditions

  • Multiple mechanisms often act simultaneously

  • Convergence must be assessed via heat balances, not just residuals

Radiation and phase change significantly increase model complexity and numerical stiffness.


Study Priorities

If time is limited, the most important concepts to look into:

  1. Difference between heat transfer and thermodynamics

  2. Meaning of temperature vs energy

  3. Local thermodynamic equilibrium

  4. Physical meaning of conduction, convection, radiation

  5. Why phase change dominates heat transfer


Key Takeaways

  • Heat transfer studies rates of energy exchange.

  • Energy is stored in discrete microscopic modes.

  • Temperature measures only part of total energy.

  • Local thermodynamic equilibrium enables classical modeling.

  • Conduction, convection, radiation, and phase change are fundamentally different mechanisms.

  • Most real problems involve multiple mechanisms simultaneously.

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Heat transfer Chapter 2: Conductive heat transfer

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Multiphase Chapter 5: Discrete Phase Flows