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.

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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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AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.