Docsity
Docsity

Prepare for your exams
Prepare for your exams

Study with the several resources on Docsity


Earn points to download
Earn points to download

Earn points by helping other students or get them with a premium plan


Guidelines and tips
Guidelines and tips

First Law of Thermodynamics - Modern and Statistical Physics - Exam, Exams of Physics

This is the Exam of Modern and Statistical Physics which includes Total Electomagnetic Energy, Reversible Expansion, Change in Specific Entropy, Thermodynamic Probability, Stirling's Approximation, Boltzmann Constant, Degeneracy of Each Energy Level etc. Key important points are: First Law of Thermodynamics, Specific Heat Capacities, Constant Pressure, Van Der Waals Gas, Equation of State, Rotational Motion, Canonical Conjugate Momenta, Angular Variables, Helmholtz Free Energy

Typology: Exams

2012/2013

Uploaded on 03/07/2013

amidii
amidii 🇮🇳

4.6

(9)

81 documents

1 / 3

Toggle sidebar

Related documents


Partial preview of the text

Download First Law of Thermodynamics - Modern and Statistical Physics - Exam and more Exams Physics in PDF only on Docsity! Statistical and Modern. Spring 2007. Pick 4 out of 6. 1) a) Starting with the first law of thermodynamics and the definition of pc and vc , show that p v T P U V c c p V T  ∂ ∂   − = +    ∂ ∂     . Here pc and vc are the specific heat capacities per mole at constant pressure and volume respectively, and U and V are the energy and volume of one mole. b) Use the above result plus the expression T V U p p T V T ∂ ∂   + =   ∂ ∂    to find p vc c− for a van der Waals gas with equation of state ( )2 a p V b RT V  + − =   . Here a and b are constants. c) Use this result to show that as V → ∞ at constant p , you obtain the ideal gas result for p vc c− . 2) The rotational motion of a diatomic molecule is specified by two angular variablesθ and φ and the corresponding canonical conjugate momenta, ,p pθ φ . Assuming the form of the kinetic energy of the rotational motion to be ( ) 2 2 2 1 1 2 2 sinrot p p I Iθ φ ε θ = + a) Derive the classical formula for the rotational partition function , ( ),r T 2 2 ( ) IkT r T = h b) Calculate the Helmholtz free energy rotF . c) Calculate the corresponding entropy and specific heat. The following may be helpful e dx a dx ax ax a ax− −∞ ∞ = = − ∫ ∫ 2 2 π sin ( ) cot( ) / 3) Assume that the neutron density in a neutron star is 30.1/fm (that is 0.1 neutron per cubic Fermi). Assuming T=0 and ignoring any gravitational forces calculate the ratio of neutrons to protons to electrons. Hint: determine their Fermi energy. The electron, neutron and protons masses are .511 2MeV/c , 939.6 2MeV/c and 938.3 2MeV/c . The constant 1240MeV fmhc = . You should be able to work out "by hand" an approximate value. 4) A π µ− atom consists of a pion and a muon bound in a Hydrogen-like atom. a) What are the energy levels for such an atom compared to those for Hydrogen? b) π µ− atoms are produced in KL decays ( LK π µ ν→ − + ). If the KL has 0.8β = what are the minimum and maximum energies of the π µ− atom expressed in terms of the K , π and µ masses with 0mν = ? c) Approximately what fraction of KL decays will produce a π µ− atom (hint: use the Heisenberg uncertainty principle)? 5) a) You are familiar with the quarter-wave thin film coating that acts as a “reflection–reducer”. For the moment, let us look at a simpler thin film—the air gap between two pieces of glass such as you would find in a Newton’s rings experiment. Why do we get constructive interference in the reflected when the thickness is one-fourth of the wavelength of light or some odd multiple of a quarter wavelength? Why isn’t it constructive at one-half wavelength of the light? For assistance, I present two of the Fresnel equations (in two forms) for reflected light. cos cos tan( ) cos cos tan( ) cos cos sin( ) cos cos sin( ) t i i t i t t i i t i t i i t t i t i i t t i t n n r n n n n r n n θ θ θ θ θ θ θ θ θ θ θ θ θ θ θ θ⊥ − − = = + + − − = = − + + P Where the parallel and perpendicular symbols refer to the plane of incidence, and i,t refer to incident and transmitted media, θ ’s are angles of incidence and transmission, and n’s are indices of refraction. b) In light of the previous, to get destructive reflection in a thin film-i.e.-a quarter-wave film, such as the one illustrated below, what condition must prevail among the indices of refraction for the three media (n0 may be taken as = 1.0 for air.) c) The destructive interference described in part b) will generally not be complete. Find the value of 1n as a function of 2n which gives completely destructive interference at normal incidence. n1 n2 n0
Docsity logo



Copyright © 2024 Ladybird Srl - Via Leonardo da Vinci 16, 10126, Torino, Italy - VAT 10816460017 - All rights reserved