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Physics 2 – Feb 21, 2017

Physics 2 – Feb 21, 2017. P3 Challenge – a) What is the average kinetic energy of a molecule of oxygen gas at 298 K ? b) What is the root mean square velocity of an oxygen molecule if its atomic mass is 32 u? (k B = 1.38 x 10 -23 J/K; 1 u = 1.66 x 10 -27 kg) Today’s Objective:

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Physics 2 – Feb 21, 2017

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  1. Physics 2 – Feb 21, 2017 • P3 Challenge – a) What is the average kinetic energy of a molecule of oxygen gas at 298 K? b) What is the root mean square velocity of an oxygen molecule if its atomic mass is 32 u? (kB= 1.38 x 10-23 J/K; 1 u = 1.66 x 10-27kg) • Today’s Objective: • B.2.1-2 Thermodynamics: Boltzmann • Assignment: • Ch 3.2, p141, #30-32, B.2 p33 #18-23 • Agenda • Boltzmann Distribution • Average K.E. • Internal Energy • State functions • Types of Processes • PV work • PV diagrams

  2. Boltzmann Distribution • Boltzmann distribution is a result of statistical mechanicsthat describes how the random particle speeds of an ideal gas are distributed. • Note: Statistical mechanics is the application of statistics to the gas particle behavior. • Unsymmetrical distribution. Always a finite probability at any high speed, but 0 at 0 speed. • The ranking of temperature for the three graphs are Blue<Red<Green. • Notice the peak location increases and lowers and the speeds spread out.

  3. Average Particle Speed • Three types of “average speed” values for the particles of an ideal gas • most probable speed (mode) red peak • average speed (mean) blue • c = “root mean square” speed corresponds to average kinetic energy • Best indication of temperature is c because temperature is average kinetic energy • IB assumes c represents all three. • Unfortunate that IB uses c for both vrms and the speed of light. Beware: This is NOT c = 3 x 108 m/s

  4. Average Kinetic Energy • The average K.E. is related to the average speed, c, where mais the atomic mass of a single gas particle. • Note on units: 1 u = 1.66 x 10-27 kg • From the ideal gas law and statistical mechanics: • And other basic relationships:

  5. Internal Energy of a Gas • If the average kinetic energy of one particle of gas is 3/2 kT, and you have a sample containing N particles, the internal energy of the sample is N times the average kinetic energy. • From this, and recalling the definitions of kB and moles you can derive the expression for the internal energy of a gas, U. • Problem solving is either of the plug and chug variety, or is algebra derivation of formulas types. So know these two fundamental relationships. (Only the first is in the IB packet.) • Notice that both average EK and U only depend on T in K.

  6. States • In thermodynamics, the state of a system is defined by specifying values for a set of measurable properties sufficient to determine all other properties. For gases, these properties are P, V and T. • E.g. Your health state could be said to be set by your vital signs. • Simple gas law problems always involve two states. • Ideal gas law applies to a single state. • Processes involve at least two states.

  7. State Functions • A state function is any variable that is only dependent on the state of the system. • A state function is not dependent on the path used to obtain the state. • Many variables are state functions: mass, Energy, Entropy, Pressure, Temperature, Volume, chemical composition, density, number of moles • Important variables that are NOT state functions: heat and work • Both heat and work are path dependent

  8. Types of Processes • A thermodynamic process is one that takes a system from one state to another. • There are several types of processes dependent on the conditions for the change. (We’ve already seen most with the simple gas laws.) • Isothermal process – Temperature is constant e.g. Boyle’s law • Isobaric process – Pressure is constant e.g. Charles’ law • Isovolumetric process – Volume is constant e.g. Gay-Lussac’s Law • Adiabatic process – No heat transfer

  9. PV Diagrams • Pressure vs Volume graphs are the most common way to describe the state of an ideal gas and the processes it undergoes. • Isobaric and isovolumetric processes are horizontal and vertical lines respectively. • Isothermal processes are described by a strict inverse relationship. • Recall Boyles law PV = constant when T is constant. • The closer a line is to the origin, the lower the temperature.

  10. Adiabatic Processes • In an adiabatic process, Q = 0. From this, the relationship between P and V can be determined. • The resulting equation means • Its graph on a PV diagram will be similar to an isothermal line, but steeper. • Problems similar to Bolye’s law problems can be solved using this equation if an adiabatic process is described. • Ex: An ideal gas initially at 105 kPa expands adiabatically from 3.5 x 10-4 m3 to 8.9 x 10-4 m3. What is the new pressure?

  11. Adiabatic Processes • Notice that for an adiabatic process, P, V and T change. • The initial and final states of an adiabatic process are located on different isothermal lines. • Using the ideal gas law to find the VT relationship, solve PV = nRT for P. • Substituting this into the adiabatic equation and collecting all constant terms. (n, R and constant) • If a gas expands adiabatically, the temperature drops. • If a gas compresses adiabatically, the temperature rises.

  12. PV Work Derived Part 1 – Piston h signs • Work is defined as a force applied through a distance. • Recall that work done on a system is positive and work done by a system is negative. • Therefore, the work done by an external force for a compression will be positive and the work done by an external force for an expansion will be negative. • Consider a piston on a canister holding a gas. The piston creates an eternal force. Pick a height = 0 point as the initial piston location. • For an expansion, the h of the gas sample is positive (h – 0) • For a compression, the h of the gas sample is negative (-h – 0) h=h h=0 h=-h

  13. PV Work Derived – Part 2 Work external • Workext for expansion is negative Workext for compression is positive • Expansion, h positive Compression, h negative • Recall that Work requires the displacement to be in the same direction as the force. • Here, our external force is 180 from the direction of h. • Cos 180 = – 1 . Therefore Wext = – F h • Wext, exp = – Fh would be negative, Wext,comp= – F h would be positive. • Results as expected above. Verify this.

  14. PV Work Derived – Part 3 Gas Pressure • To transform our Wext expression into PV work, we first recognize that the force exerted by the gas pressure is an equal and opposite reaction force to the external applied force. • W done by the gas is the opposite of the Wext • To convert force into P and h into V, multiply by A/A as a form of 1. • Sort the factors and replace by the definitions of P and V. • Ta Da. That’s why the work done by a gas is called PV work. • W for an expansion is positive and W for a compression is negative

  15. PV work on a PV diagram • P is the vertical axis and V is the horizontal, so PV corresponds to the area under the curve for a process. • If the process is not isobaric, the PV work is still the area under the curve. • Sometimes this is easy to calculate, but for isothermals and adiabatic processes, it requires calculus. • Area sweeps to the right are positive work (V is positive) • Area sweeps to the left are negative work (V is negative)

  16. Work done for a PV diagram cycle • Many processes that are shown on a PV diagram are cycles that return the state of the system to the initial conditions. • The energy change for a cycle is zero because energy is a state function. • Work is not a state function. • Work is the area within the loop created by the processes that make up the cycle. • CW loop is pos. W. CCW loop is neg. W.

  17. Exit Slip - Assignment • Exit Slip- A gas expands isobarically from a volume of 3.80 x 10-3 m3 to 5.20 x 10-3 m3 at 103.5 kPa. How much PV work is done by the gas? • What’s Due on Feb 16? (Pending assignments to complete.) • Ch 3.2, p141, #30-32, B.2 p33 #18-23 • DOWNLOAD Engineering Physics Text B!!!! Read B.2.1-B.2.4, p19-23 • What’s Next? (How to prepare for the next day) • Read B p24-32 about Thermodynamics

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