The Carnot Cycle is as follows: • • Reversible isothermal expansion of the gas at the "hot" temperature, T1 (isothermal heat addition). (1 to 2 in image.) • Isentropic (reversible adiabatic) expansion of the gas (isentropic work output). (2 to 3 in image.) • Reversible isothermal compression of the gas at the "cold" temperature, T2. (isothermal heat rejection). (3 to 4 in image.) • Isentropic compression of the gas (isentropic work input). (4 to 1 in image.)Information taken from:http://en.wikipedia.org/wiki/Carnot_cycleAlthough it's from wikipedia, I believe it's consistent with the course.
Carnot's Theorem: A Carnot engine is the most efficient heat engine.
Carnot relation.
r
This can be obtained via the proof of Carnot's Theorem.
Carnot Engine efficiency. (See notes)
r
The carnot efficiency is independant of the substance used, therefore it can be derived by considering the process occuring through an ideal gas.
First Law for any closed cycle, C.
Maxwell Relations
Fundamental Thermodynamic Relation and natural variables.
r
The "natural" variables of E are S and V, as the infinitesimal change of E depends on the changes of these two variables.
1st Maxwell Relation
Helmholtz Free Energy
r
This definition is useful for systems of constant temperature.
Differential Form
r
To find the differential forms, differentiate with respect to a random variable, say x for this example, assuming all of the functions are functions of x. Then multiply by dx to eliminate the random variable.
2nd Maxwell Relation
r
To derive one of the Maxwell equations, follow the following steps:Use the relevant thermodynamic potential. (Most likely to be stated in the question for exams.)Use the differential form of the thermodynamic potential with the total differential expansion and compare the coefficients of the small changes (dT, dS etc..)Use Clairaut's Theorem (I'm using the name for reference, otherwise it's difficult to describe). You can then use this to derive the Maxwell Relation.You'll be required to derive these in the exam.
Gibbs Free Energy
r
This definition is useful for phase transitions, since the Gibbs free energy is always constant at this point (ie, when T and P are fixed).
Differential Form
r
To find the differential forms, differentiate with respect to a random variable, say x for this example, assuming all of the functions are functions of x. Then multiply by dx to eliminate the random variable.
3rd Maxwell Relation
r
To derive one of the Maxwell equations, follow the following steps:Use the relevant thermodynamic potential. (Most likely to be stated in the question for exams.)Use the differential form of the thermodynamic potential with the total differential expansion and compare the coefficients of the small changes (dT, dS etc..)Use Clairaut's Theorem (I'm using the name for reference, otherwise it's difficult to describe). You can then use this to derive the Maxwell Relation.You'll be required to derive these in the exam.
Enthalpy
r
At constant pressure, the change in heat is equal to the change in enthalpy. This value is known as the latent heat.
Differential Form
r
To find the differential forms, differentiate with respect to a random variable, say x for this example, assuming all of the functions are functions of x. Then multiply by dx to eliminate the random variable.
4th Maxwell Relation
r
To derive one of the Maxwell equations, follow the following steps:Use the relevant thermodynamic potential. (Most likely to be stated in the question for exams.)Use the differential form of the thermodynamic potential with the total differential expansion and compare the coefficients of the small changes (dT, dS etc..)Use Clairaut's Theorem (I'm using the name for reference, otherwise it's difficult to describe). You can then use this to derive the Maxwell Relation.You'll be required to derive these in the exam.
Total differential expansion of a general function of n variables
r
Using this equation, we can expand all of the thermodynamic potentials in terms of their total differential components, and simply compare the coefficients with the ones defined from the fundamental thermodynamic relation to yield a pair of equations that must be true.
Clairaut's Therorem (it's the offiical name, don't need to know the name)
Statistical Theory Of Thermodynamics
Boltzmann's Assumption of entropy
r
Omega is the number of microstates in the given system.
Macrostates and Microstates
r
The macrostate of a given thermodynamic system is give by simply a few thermodynamic variables, though like, P, V, T and state functions such as E and S. In other words, it's the collective behaviour of the substance.A microstate of a thermodynamic system is the total states of each individual particle, therefore giving a total description of the gas in question.
Classical Mechanics
r
In a classical mechanics description, a particle can be described entirely by it's position and momentum. So for N particles, since we have 3 spatial dimensions and 3 momenta dimensions for each particle, the combination of these 6 dimensions for each particle make up what's known as phase space, which is a 6N dimensional space.
Quantum Mechanics
r
In a qunatum mechanical description, particles are described by wavefunctions which are specified by the set of quantum numbers, n l, m_l, and small_omega (the spin).For N quantum particles in a box, each state is a plane wave solution, and hence we can use three discrete components of momenta. We use these collection of quantum numbers to form the microstate. This is known as the independant particle approximation, as it ignores the interactions between particles.
Open Systems
Fundamental Thermodynamic Relation
r
This is for a single-particle species system only. There is a subsequent extension to this relation for multi-particle species system, however I don't think we need to know it.
Phase Equilibrium conditions
r
Phase Equilibrium occurs when all intensive variables of the two phases are equal. This can be proved by the second law of thermodynamics and by considering the multi-phase flow as a closed system.
1st Law of Thermodynamics, Heat and Gases
The first law is a statement of energy conservation
Change of Energy = Work done on the system + heat absorbed by the system
1st Law of Thermodynamics
r
In the equation I have replaced d-bar with delta's, hopefully it won't confuse people.
Work done for various processes.
On a gas to expand/compress it.
On a wire to stretch it.
On a magnetic material by an external field.
Types of Gases
Ideal Gas
Hard-Sphere Gas
r
This approximation treats the atoms as hard-spheres. Therefore, it is necessary to exclude the volume of the atoms.
Van-der-Waals Gas
r
Van der Waals argued that the pressure, P_attraction, is the result of mutual attraction between bulk of gas and a sample near the boundary, and hence should be proportional to the product of their densities.
Heat Capacities
At constant volume (for a gas)
At constant pressure (for a gas)
Useful Relations for Gases
Heat Capacity relation for an ideal gas
For a reversible aciabatic process on an ideal gas, this holds true for K = const.
2nd Law of Thermodynamics
Second Law of Thermdynamics
r
Statement of the law:In a system, a process that occurs within a closed system will tend to increase the entropy of the system and entropy can never decrease.The statement is an equality if the process is reversible.
Change in Entropy for a reversible process, note the equality.
Infinitesimal change in entropy for a general process
3rd Law of Thermodynamics
As a system approaches absolute zero, all processes cease and the entropy of the system approaches a minimum value.
Zeroth Law of Thermodynamics
A Logic Law that just says if A = B and A = C then B = C