Surface Thermodynamics A primer for heat transfer...

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Surface Thermodynamics A primer for heat transfer physical scientists David Cahill Department of Materials Science and Engineering, Materials Research Laboratory, University of Illinois at Urbana-Champaign Partially based on lecture notes by Prof. Gert Ehrlich

Transcript of Surface Thermodynamics A primer for heat transfer...

Page 1: Surface Thermodynamics A primer for heat transfer …users.mrl.illinois.edu/cahill/surface_thermo_sep16.pdf · Surface Thermodynamics A primer for heat transfer physical scientists

Surface ThermodynamicsA primer for heat transfer physical scientists

David CahillDepartment of Materials Science and Engineering,

Materials Research Laboratory,University of Illinois at Urbana-Champaign

Partially based on lecture notes by Prof. Gert Ehrlich

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Motivation for understanding thermodynamics of surfaces

• At the nanoscale, atoms and molecules near surfaces and interfaces become a significant fraction of the overall system.

• In this lecture, I will use the term “surface” to describe the transition region between two phases.

• Gibbs (1878) introduced the concept of a “dividing surface” to deal with the thermodynamics of this (often inhomogenous) transition region.

– See Tolman, J. Chem. Phys. 16, 758 (1948)

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Motivation for understanding thermodynamics of surfaces

• We need thermodynamics to provide insight on

– Composition and structure of the surface in equilibrium.

– Driving force for exchange of mass at the surface (evaporation, condensation, adsorption, ripening, coarsening).

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Part I: classical thermodynamics of surfaces

• Surface excess contributions to the extensive variables

– Gibbs adsorption equation• Thermodynamic potentials and surface excess free

energy

– Landau thermodynamic potential for multicomponent systems

– Surface tension, surface energy, surface stress• Equilibrium shape; Laplace pressure; thermodynamic

driving force for coarsening

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Part II: statistical mechanics of surfaces

• Landau thermodynamic potential and the grand partition function

– Equilibrium between 2D and 3D ideal gases– Equilibrium between monolayer lattice gas and 3D

ideal gas (Langmuir adsorption)• Comparison to kinetic models for evaporation and

condensation

• Connection back to thermodynamics: heat of adsorption

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Surface excess of the extensive variables

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Surface excess of the extensive variables

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Surface excess of the extensive variables

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Relate surface tension to the other intensive variables

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Gibbs adsorption equation

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Surface excess free energy

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Digression on thermodynamic potentials

closed, isothermal closed, isothermal, constant P

closed, adiabatic

open, isothermal

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Difficult to measure the surface tension of a solid

• Need an experiment that can access the reversible mechanical work needed to create new surface

• Zero creep experiment

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Surface tension, surface energy, surface stress

• I usually reserve the term “surface energy” for the surface tension at zero temperature.

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Surface stress is the work needed to deform a surface

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Equilibrium shape

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Equilibrium shape: Wulff construction

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Equilibrium shape of most metals is nearly a sphere

• Need sufficient kinetics (large surface diffusion or fast evaporation/condensation) to observe equilibrium shape

• Most crystal shapes are, in practice, controlled by kinetic limitations (slowest growing facets), not thermodynamics.

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Equilibrium between a small crystal and its liquid or vapor

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Equilibrium between a small crystal and its liquid or vapor

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Equilibrium between a small crystal and its liquid or vapor

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Chemical potential of a small crystal

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Chemical potential driving force for ripening

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Chemical potential driving force for ripening

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Part 2: statistical mechanics to calculate L

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Ideal gas is always the easiest place to start

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Need the derivative of L with respect to chemical potential to find N = N(2)+N(s)

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Single particle partition functions

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2D ideal gas in equilibrium with 3D ideal gas

2 B

hmk T

λπ

=

thermal de Broglie wavelength

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Perpendicular vibrational partition function

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Compare to a kinetic view of condensation=evaporation

This looks like an impingement rate set equalto an evaporation rate but note that we derived the equation without considering kinetics.

At room T 12 -16 10 sBk Th

= ×

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Lattice 2D gas (Langmuir adsorption)

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Lattice 2D gas (Langmuir adsorption)

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Lattice 2D gas (Langmuir adsorption)

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Equlibrium between 2D lattice gas and 3D ideal gas

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Equilibrium between 2D lattice gas and 3D ideal gas

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Single particle partition function for the 2D lattice gas

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Comparison to a kinetic view of adsorption/desorption

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Compare 2D ideal gas and 2D lattice gas

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Entropy is (of course) important for determining the equilibrium coverage

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Take a closer look at the entropy of the lattice gas

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Take a closer look at the entropy of the lattice gas

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Take a closer look at the entropy of the lattice gas

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Compare to entropy of the ideal gas

Ar at atmospheric pressure 15gas

B

SNk

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Heat of adsorption

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Heat of adsorption

Page 47: Surface Thermodynamics A primer for heat transfer …users.mrl.illinois.edu/cahill/surface_thermo_sep16.pdf · Surface Thermodynamics A primer for heat transfer physical scientists

Heat of adsorption

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Heat of adsorption

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Heat of adsorption

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Heat of adsorption

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Heat of adsorption

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Heat of adsorption of the 2D ideal gas