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19: The First Law of Thermodynamics

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    • 19.1: Overview of Classical Thermodynamics
      Joule was able to show that work and heat can have the same effect on matter – a change in temperature! It would then be reasonable to conclude that heating, as well as doing work on a system will increase its energy content, and thus it’s ability to perform work in the surroundings. This leads to an important construct of the First Law of Thermodynamics: The capacity of a system to do work is increased by heating the system or doing work on it.
    • 19.2: Pressure-Volume Work
      Work in general is defined as a product of a force FFF and a path element dsdsds. In the case of a cylinder, the movement of the piston is constrained to one direction, the one in which we apply pressure (\(P\) being force \(F\)  per area \(A\)). We can therefore introduce the area of the piston, \(A\), and forget about the vectorial nature of force. This form of work is called pressure-volume (\(PV\)) work, and it plays an important role in the development of our theory.
    • 19.3: Work and Heat are not State Functions
      Heat and work are both path functions: they depend on the path taken. In order to calculate the heat transfer or work being done on/by a system, the path taken must be known.
    • 19.4: Energy is a State Function
      Unlike heat and work, energy is a state function. That is, it is independent of the path taken. Any path can be used to calculate the change in energy between two states.
    • 19.5: An Adiabatic Process is a Process in which No Energy as Heat is Transferred
      Work is a path function as it always depends on the path taken, even if it is done reversibly.
    • 19.6: The Temperature of a Gas Decreases in a Reversible Adiabatic Expansion
      In an adiabatic process, no heat transfer occurs. During the adiabatic expansion of a gas, the internal energy of the gas is converted to work being done by the system, decreasing the temperature of the gas.
    • 19.7: Work and Heat Have a Simple Molecular Interpretation
      The internal energy of a system, \(dU\), is exchanged with the system's surroundings thought work and heat.
    • 19.8: Pressure-Volume Work
      An important point is that pressure-volume work −PdV is only one kind of work. It is the important one for gases but for most other systems we are interested in other kinds of work (e.g. electrical work in a battery).
    • 19.9: Heat Capacity is a Path Function
    • 19.10: Relative Enthalpies Can Be Determined from Heat Capacity Data and Heats of Transition
    • 19.11: Enthalpy Changes for Chemical Equations are Additive
      As enthalpy and energy are state functions we should expect additivity of U and H when we study chemical reactions. This additivity is expressed in Hess's Law. The additivity has important consequences and the law finds wide spread application in the prediction of heats of reaction.  The reverse reaction has the negative enthalpy of the forward one. If we can do a reaction in two steps we can calculate the enthalpy of the combined reaction by adding them up.
    • 19.12: Heats of Reactions Can Be Calculated from Tabulated Heats of Formation
      Reaction enthalpies are important, but difficult to tabulate. However, because enthalpy is a state function, it is possible to use Hess’ Law to simplify the tabulation of reaction enthalpies. Hess’ Law is based on the addition of reactions. By knowing the reaction enthalpy for constituent reactions, the enthalpy of a reaction that can be expressed as the sum of the constituent reactions can be calculated.
    • 19.13: The Temperature Dependence of ΔH
      It is often required to know thermodynamic functions (such as enthalpy) at temperatures other than those available from tabulated data. Fortunately, the conversion to other temperatures isn’t difficult.
    • 19.E: The First Law of Thermodynamics (Exercises)
    • Enthalpy is a State Function
      Enthalpy is the energy transferred as heat in an isobaric process when on P-V work is involved.

    Thumbnail: A thermite reaction using iron(III) oxide. The sparks flying outwards are globules of molten iron trailing smoke in their wake. (CC SA-BY 3.0; Nikthestunned).

    19: The First Law of Thermodynamics is shared under a CC BY-NC-SA 4.0 license and was authored, remixed, and/or curated by LibreTexts.

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