Energy Balance Essentials: Isolated Systems, Enthalpy, and Partial Pressures

Internal energy, thermal energy, and chemical energy

  • U = total energy; composed of thermal (kinetic) energy and chemical energy (bond energy).
  • Chemical energy is negative in the sense of potential energy wells; bond formation lowers the system's chemical energy.
  • Energy balance in a closed system: ΔU=q+w=ΔU<em>chem+ΔU</em>thermal.\Delta U = q + w = \Delta U<em>{\text{chem}} + \Delta U</em>{\text{thermal}}.
  • Isolated system (no heat or work exchange): ΔU<em>total=0ΔU</em>thermal=ΔUchem.\Delta U<em>{\text{total}} = 0 \Rightarrow \Delta U</em>{\text{thermal}} = -\Delta U_{\text{chem}}.
  • If chemical energy decreases (more negative) due to bond strengthening, the thermal energy increases by the same amount in an isolated system.
  • If the system is not isolated, the excess thermal energy can be transferred as heat to the surroundings or as work; the budget remains balanced with the outside world.
  • In a fixed-volume, insulated container: q=0,  w=0ΔU=0.q = 0,\; w = 0 \Rightarrow \Delta U = 0. The chemical-to-thermal energy transfer still occurs internally as needed.
  • Practical takeaway: the heat you feel inside the system depends on whether heat can leave the system.

Enthalpy and constant-pressure processes

  • Enthalpy defined: h=u+pvh = u + p\,v where $u$ is internal energy per unit substance and $v$ is specific volume.
  • Change in enthalpy: Δh=Δu+pΔv.\Delta h = \Delta u + p\,\Delta v.
  • At constant pressure with only PV-work (no non-PV work): qp=Δhq_p = \Delta h.
  • Enthalpy is a state function; heat is a boundary quantity. In many reactions, Δu\Delta u dominates and ΔhΔu\Delta h \approx \Delta u, with a small correction from $p\Delta v$.
  • When volume changes are small or pressure is constant, enthalpy provides a convenient energy accounting at constant pressure.

Partial pressures and open vs closed systems

  • For mixtures of gases, total pressure is the sum of individual partial pressures: P=<em>iP</em>i.P = \sum<em>i P</em>i.
  • For ideal gases, P<em>i=x</em>iPP<em>i = x</em>i P where $x_i$ is the mole fraction of component $i$.
  • In open (open to surroundings) experiments, the gas tends to equilibrate with the external pressure, performing or receiving PV-work as it expands or contracts.
  • In open systems, a work term ($w$) often appears due to volume change against external pressure; this is automatically accounted for when considering enthalpy.

Worked intuition and example notes

  • Exothermic reaction in an insulated container: heat stays in the system; the products (system) heat up; the internal energy increases due to the loss of chemical energy.
  • Exothermic reaction in contact with surroundings: heat can leave the system; the thermal energy of the system may decrease or rise less, depending on environment.
  • Real breathing example: respiration releases chemical energy, warming the exhaled air; excess heat is transferred to surroundings.
  • General energy-tracking rule (isolated vs open):
    • Isolated and fixed volume: ΔU=0ΔU<em>thermal=ΔU</em>chem.\Delta U = 0\Rightarrow \Delta U<em>{\text{thermal}} = -\Delta U</em>{\text{chem}}.
    • Open or connected to environment: heat and/or work can move between system and surroundings; enthalpy helps track energy when volume can change under constant external pressure.

Quick example (conceptual, using shown numbers)

  • If a reaction changes chemical energy from $-5.03\,\text{eV}$ to $-16.48\,\text{eV}$:
    • ΔUchem=(16.48)(5.03)=11.45 eV.\Delta U_{\text{chem}} = (-16.48) - (-5.03) = -11.45\ \text{eV}.
    • In an isolated system: ΔU<em>thermal=ΔU</em>chem=+11.45 eV.\Delta U<em>{\text{thermal}} = -\Delta U</em>{\text{chem}} = +11.45\ \text{eV}.
  • If the system is not isolated, this 11.45 eV may be carried away as heat to the surroundings or stored as thermal energy, depending on the environment and constraints.

Homework-oriented takeaways

  • You will be asked to track energy through a chemical change:
    • Compute ΔU<em>chem=U</em>chem, finalUchem, initial.\Delta U<em>{\text{chem}} = U</em>{\text{chem, final}} - U_{\text{chem, initial}}.
    • Determine whether the accompanying change in thermal energy ΔUthermal\Delta U_{\text{thermal}} stays in the system (isolated) or leaves to the surroundings (open).
    • If the container is fixed and insulated: ΔU=0ΔU<em>thermal=ΔU</em>chem.\Delta U = 0 \Rightarrow \Delta U<em>{\text{thermal}} = -\Delta U</em>{\text{chem}}.
    • If the container is at constant external pressure: use enthalpy: qp=Δh=Δu+pΔv.q_p = \Delta h = \Delta u + p\,\Delta v.
  • For glucose burning or similar reactions, you’ll need the balanced equation and standard molar volumes at STP to evaluate PV-work contributions when using enthalpy.

Summary formulas

  • First Law: ΔU=q+w\Delta U = q + w
  • Energy components: ΔU=ΔU<em>chem+ΔU</em>thermal\Delta U = \Delta U<em>{\text{chem}} + \Delta U</em>{\text{thermal}}
  • Isolated, fixed volume: ΔU=0ΔU<em>thermal=ΔU</em>chem\Delta U = 0 \Rightarrow \Delta U<em>{\text{thermal}} = -\Delta U</em>{\text{chem}}
  • Enthalpy: h=u+pv;Δh=Δu+pΔvh = u + p\,v;\quad \Delta h = \Delta u + p\Delta v
  • Constant pressure, PV-work only: qp=Δhq_p = \Delta h
  • Partial pressures for ideal gases: P=<em>iP</em>i;P<em>i=x</em>iPP = \sum<em>i P</em>i;\quad P<em>i = x</em>i P