🔥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) represents the total energy contained within a system, including kinetic and potential energy of its particles
Enthalpy (H) is a thermodynamic property defined as the sum of internal energy and the product of pressure and volume (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=21mv2)
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) is the energy transfer associated with a force acting through a distance
Expressed as W=∫F⋅ds or W=∫P⋅dV for pressure-volume work
Heat (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), while work done on the system is positive (W>0)
Heat added to the system is positive (Q>0), while heat removed from the system is negative (Q<0)
Adiabatic process occurs without heat transfer between the system and its surroundings (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=Q−W, where ΔU is the change in internal energy, Q is the heat added to the system, and W is the work done by the system
For a closed system undergoing a reversible process, the First Law can be written as dU=δQ−δW, where δQ and δW 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, where Cv is the specific heat at constant volume
Enthalpy change is given by ΔH=ΔU+Δ(PV), which simplifies to ΔH=Qp 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)
Molar heat capacity is the heat capacity per mole (C)
Work done in a pressure-volume process is calculated using W=∫P⋅dV, where P is the pressure and dV 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=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=nRT
Specific heat equations: Q=mcΔT or Q=nCΔT
Work equations: W=∫P⋅dV or W=−PΔV (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