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PHYS 213 Midterm Exam HKN Review Session

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1 PHYS 213 Midterm Exam HKN Review Session
Steven Kolaczkowski Alex Littlefield

2 First Law of Life Check your units

3 First Law of Thermodynamics
Check Your Units dπ‘ˆ=𝑑𝑄+𝑑 π‘Š π‘œπ‘› =dQβˆ’P𝑑𝑉 If volume is constant: dπ‘ˆ=𝑑𝑄

4 Entropy, Temperature, and the Second Law of Thermodynamics
CHECK YOUR UNITS 𝑆≑ π‘˜ 𝐡 ln⁑(Ξ©) where Ξ© is the number of microstates Ξ© π‘‘π‘œπ‘‘π‘Žπ‘™ = Ξ© 1 βˆ— Ξ© 2 ∴ 𝑆 π‘‘π‘œπ‘‘π‘Žπ‘™ = 𝑆 1 + 𝑆 2 𝑑𝑆= 1 𝑇 π‘‘π‘ˆ+ 𝑃 𝑇 π‘‘π‘‰βˆ’ πœ‡ 𝑇 𝑑𝑁 For an Isolated system Δ𝑆β‰₯0 or Ξ” 𝑆 π‘ˆπ‘›π‘–π‘£π‘’π‘Ÿπ‘ π‘’ β‰₯0 If Δ𝑆=0 the process is reversible Temperature: 1 𝑇 ≑ 𝑑𝑆 π‘‘π‘ˆ 𝑉,𝑁

5 Equilibrium and Counting Microstates
We will observe the macrostate with the most microstates (maximum entropy) A microstate is an observable state Distinguishable: Ξ©= 𝑀 𝑁 Indistinguishable: Ξ©= 𝑀 𝑁 𝑁! 𝑆 π‘‘π‘œπ‘‘π‘Žπ‘™ is maximized when T is constant across system (thermal equilibrium)

6 Heat Capacity and Latent Heat
Heat capacity: the amount of energy required to raise the temperature of a material by 1K 𝐢 𝑉 = 𝑑𝑄 𝑑𝑇 = 𝐽 𝐾 𝑐 𝑣 π‘šπ‘œπ‘™ = 1 𝑛 d𝑄 d𝑇 = 𝐽 π‘šπ‘œπ‘™βˆ™πΎ 𝑐 𝑣 π‘šπ‘Žπ‘ π‘  = 1 π‘š 𝑑𝑄 𝑑𝑇 = 𝐽 π‘˜π‘”βˆ™πΎ 𝐢 𝑣,π‘‘π‘œπ‘‘ = 𝐢 𝑣,1 + 𝐢 𝑣,2 𝑑𝑄= 𝐢 𝑣 βˆ™d𝑇=π‘š 𝑐 𝑣 π‘šπ‘Žπ‘ π‘  βˆ™π‘‘π‘‡ = 𝐽 Latent Heat: The amount of energy needed to transition between states of matter T does not change during a phase change! 𝐿 𝑓 = Ξ” 𝑄 π‘ π‘œπ‘™π‘–π‘‘β†’π‘™π‘–π‘žπ‘’π‘–π‘‘ π‘š π‘ π‘œπ‘™π‘–π‘‘ = 𝐽 π‘˜π‘” 𝐿 𝑣 = Ξ” 𝑄 π‘™π‘–π‘žπ‘’π‘–π‘‘β†’π‘”π‘Žπ‘  π‘š π‘™π‘–π‘žπ‘’π‘–π‘‘ = 𝐽 π‘˜π‘”

7 Ideal Gases and Equipartition
CHECK YOUR UNITS Equipartition: The idea that thermal energy on average is distributed equally among all quadratic modes of motion <𝐾>= π‘˜ 𝐡 𝑇 2 for each quadratic degree of freedom Monoatomic Gases: Diatomic Gases: Solids: 6 Mass doesn’t matter for calculating energy, but it does for finding average velocity Ideal Gas Law: Assuming that particles will not collide or interact with each other, only with the walls of the container, and are volumeless Works best with low densities and high temperatures (a few, fast moving particles) 𝑃𝑉= 2 3 𝑁<𝐾 > π‘‘π‘Ÿπ‘Žπ‘›π‘  =π‘π‘˜π‘‡=𝑛𝑅𝑇

8 Solids, More Heat Capacities, and Internal Energy
CHECK YOUR UNITS π‘ˆ=𝑁<K> Ideal Solids π‘ˆ π‘‘π‘œπ‘‘π‘Žπ‘™ =𝑁 < 1 2 π‘š 𝑣 2 > π‘‘π‘Ÿπ‘Žπ‘›π‘  +< 1 2 π‘˜ π‘Ÿ 2 > =2𝑁<𝐾 > π‘‘π‘Ÿπ‘Žπ‘›π‘  =3𝑁 π‘˜ 𝐡 𝑇 We will assume that ideal solids are incompressible π‘‘π‘ˆ=𝑑𝑄 and 𝑐 π‘šπ‘œπ‘™ = 1 𝑛 π‘‘π‘ˆ 𝑑𝑇 =3 N A k B

9 Boltzmann Distributions and Quantum Oscillators
β€œThe best thing in the world”-V, 2018/4/7 For a Quantum Oscillator, energy is discretized by πœ–=hf and π‘ˆ π‘ž =π‘žπœ–= π‘˜ 𝐡 𝑇=qhf Total number of states given N oscillators and q energy quanta Ξ© 𝑁,π‘ž = π‘βˆ’1+π‘ž ! π‘ž! π‘βˆ’1 ! 𝑆=π‘˜ ln Ξ© Δ𝑆(π‘žβ†’π‘ž+1)=π‘˜ ln π‘ž+𝑁 π‘ž+1 β‰ˆπ‘˜ 𝑁 π‘ž 𝑇 = d𝑆 dπ‘ˆ β‰ˆ π‘˜π‘ π‘žβ„Žπ‘“ Probability of State having energy 𝐸 𝑛 : 𝑃 𝐸 𝑛 = 𝑒 βˆ’ 𝐸 𝑛 π‘˜ 𝐡 𝑇 𝑍 Partition function: 𝑍= Ξ£ π‘Žπ‘™π‘™ π‘ π‘‘π‘Žπ‘‘π‘’π‘  𝑒 βˆ’ 𝐸 𝑛 π‘˜ 𝐡 𝑇 REMEMBER TO TAKE INTO ACCOUNT DEGENERACY!!! β€œActually the Partition function is my favorite thing in the world”-V, 10 mins later R S

10 More 213 Stuff Atmospheres: Ξ”π‘ˆ=π‘šπ‘”β„Ž therefore 𝑃 β„Ž 𝑃 0 = 𝑒 βˆ’ π‘šπ‘”β„Ž π‘˜ 𝐡 𝑇 and <β„Ž> = π‘˜ 𝐡 𝑇 π‘šπ‘” β€œYou get this from the Boltzmann distribution, the best thing in the world”-V, 30mins later

11 Exam Advice When doing problems, PLEASE PLEASE PLEASE CHECK YOUR UNITS!!! You will be shocked how many questions you can solve just matching units and having an idea of what they are asking for Know when and how to use your equation sheet Don’t panic, just keep on moving Make sure you are in the right mindset going into the exam Spend your time showing what you know DON’T CHEAT

12 Spring 2015

13 Spring 2018

14 Spring 2015

15 Spring 2018

16 Spring 2015

17 Fall 2014

18 Spring 2018

19 Fall 2014

20 Fall 2014


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