Thermodynamics I

🔥Thermodynamics I Unit 3 – First Law of Thermodynamics

The First Law of Thermodynamics is a fundamental principle in physics that states energy can't be created or destroyed, only converted between forms. This law provides a framework for understanding energy conservation in closed, open, and isolated systems, and is crucial for analyzing heat engines and chemical reactions. Key concepts include internal energy, enthalpy, and work-heat relationships. The law's development in the 19th century by scientists like Mayer, Joule, and Helmholtz laid the groundwork for modern thermodynamics, impacting fields from engineering to chemistry.

Key Concepts and Definitions

  • First Law of Thermodynamics states that energy cannot be created or destroyed, only converted from one form to another
  • Internal energy (U)(U) represents the total energy contained within a system, including kinetic and potential energy of its particles
  • Enthalpy (H)(H) is a thermodynamic property defined as the sum of internal energy and the product of pressure and volume (H=U+PV)(H = U + PV)
  • Closed system does not exchange matter with its surroundings, but can exchange energy in the form of heat or work
  • Open system exchanges both matter and energy with its surroundings
    • Examples of open systems include a steam turbine or a chemical reactor
  • Isolated system does not exchange either matter or energy with its surroundings
  • Quasi-static process occurs slowly enough that the system remains in thermodynamic equilibrium throughout the process
  • Reversible process can be reversed without any net change to the system or its surroundings

Historical Context and Development

  • The First Law of Thermodynamics emerged from the work of several scientists in the 19th century, including Julius Robert von Mayer, James Prescott Joule, and Hermann von Helmholtz
  • Mayer proposed the conservation of energy principle in 1842, stating that energy cannot be created or destroyed
  • Joule demonstrated the equivalence of mechanical work and heat through a series of experiments (Joule's apparatus)
  • Helmholtz formulated a mathematical expression of the First Law in 1847, combining the work of Mayer and Joule
  • Rudolf Clausius introduced the concept of internal energy in 1850 and refined the mathematical formulation of the First Law
  • The development of the First Law laid the foundation for the field of thermodynamics and its applications in various branches of science and engineering
    • It provided a framework for understanding heat engines, refrigeration cycles, and chemical reactions

Energy and Its Forms

  • Energy is the capacity to do work or cause change in a system
  • Kinetic energy is the energy associated with the motion of an object (KE=12mv2)(KE = \frac{1}{2}mv^2)
  • Potential energy is the energy stored in an object due to its position or configuration (gravitational, elastic, electric)
  • Internal energy includes the kinetic and potential energy of the particles within a system
    • Translational, rotational, and vibrational motions contribute to internal energy
  • Chemical energy is stored in the bonds between atoms and can be released or absorbed during chemical reactions
  • Thermal energy is the energy associated with the random motion of particles in a substance
  • Electrical energy is the energy associated with the flow of electric charges (current)
  • Mechanical energy is the sum of kinetic and potential energy in a system

System and Surroundings

  • A system is the specific portion of the universe under study, while the surroundings include everything else that can interact with the system
  • Boundary separates the system from its surroundings and can be real or imaginary
  • State of a system is described by its thermodynamic properties (pressure, volume, temperature)
  • State variables depend only on the current state of the system, not on how it reached that state
  • Process is a change in the state of a system, characterized by the initial and final states
  • Path is the sequence of states through which a system passes during a process
    • Different paths between the same initial and final states can result in different amounts of heat and work exchanged
  • Equilibrium state is achieved when the system's properties remain constant over time and there are no net flows of energy or matter

Work and Heat Transfer

  • Work (W)(W) is the energy transfer associated with a force acting through a distance
    • Expressed as W=FdsW = \int F \cdot ds or W=PdVW = \int P \cdot dV for pressure-volume work
  • Heat (Q)(Q) is the energy transfer due to a temperature difference between the system and its surroundings
  • Sign convention: work done by the system is negative (W<0)(W < 0), while work done on the system is positive (W>0)(W > 0)
  • Heat added to the system is positive (Q>0)(Q > 0), while heat removed from the system is negative (Q<0)(Q < 0)
  • Adiabatic process occurs without heat transfer between the system and its surroundings (Q=0)(Q = 0)
  • Isothermal process occurs at constant temperature, with heat transfer balanced by work
  • Isobaric process occurs at constant pressure, with changes in volume and heat transfer
  • Isochoric (isovolumetric) process occurs at constant volume, with changes in pressure and heat transfer

Mathematical Formulation

  • The First Law of Thermodynamics can be expressed as ΔU=QW\Delta U = Q - W, where ΔU\Delta U is the change in internal energy, QQ is the heat added to the system, and WW is the work done by the system
  • For a closed system undergoing a reversible process, the First Law can be written as dU=δQδWdU = \delta Q - \delta W, where δQ\delta Q and δW\delta W represent infinitesimal amounts of heat and work
  • For an ideal gas, the change in internal energy depends only on the change in temperature: ΔU=CvΔT\Delta U = C_v \Delta T, where CvC_v is the specific heat at constant volume
  • Enthalpy change is given by ΔH=ΔU+Δ(PV)\Delta H = \Delta U + \Delta(PV), which simplifies to ΔH=Qp\Delta H = Q_p for a process at constant pressure
  • Heat capacity is the amount of heat required to raise the temperature of a substance by one degree
    • Specific heat is the heat capacity per unit mass (c)(c)
    • Molar heat capacity is the heat capacity per mole (C)(C)
  • Work done in a pressure-volume process is calculated using W=PdVW = \int P \cdot dV, where PP is the pressure and dVdV is the change in volume

Applications and Real-World Examples

  • Heat engines convert thermal energy into mechanical work, operating between a high-temperature reservoir and a low-temperature reservoir (internal combustion engines, steam turbines)
  • Refrigerators and heat pumps transfer heat from a low-temperature reservoir to a high-temperature reservoir, requiring work input (air conditioners, refrigerators)
  • Thermochemistry studies the heat absorbed or released during chemical reactions (combustion, neutralization)
  • Phase changes involve heat transfer without a change in temperature (melting, vaporization)
    • Latent heat is the energy required for a substance to change phase
  • Adiabatic processes occur in rapid compressions and expansions (diesel engines, sound waves)
  • Throttling processes involve a sudden pressure drop without significant heat transfer (refrigerant expansion in air conditioners)
  • Steady-flow processes occur in open systems with constant flow rates and no accumulation of mass or energy (turbines, compressors, nozzles)

Problem-Solving Strategies

  • Identify the system and its boundaries, specifying whether it is open, closed, or isolated
  • Determine the initial and final states of the system, as well as the process connecting them
  • Apply the First Law of Thermodynamics, considering the appropriate form for the given situation (e.g., ΔU=QW\Delta U = Q - W for a closed system)
  • Identify the known and unknown variables, using the problem statement and any given assumptions
  • Use the appropriate equations and relationships to solve for the unknown variables
    • Ideal gas law: PV=nRTPV = nRT
    • Specific heat equations: Q=mcΔTQ = mc\Delta T or Q=nCΔTQ = nC\Delta T
    • Work equations: W=PdVW = \int P \cdot dV or W=PΔVW = -P\Delta V (for constant pressure)
  • Pay attention to sign conventions for heat and work, and ensure consistent units throughout the problem
  • Interpret the results in the context of the problem, considering the physical meaning of the calculated values


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© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.