Name Solutions to Test 3 November 7, 2018

Similar documents
Schrödinger equation for the nuclear potential

Name Final Exam December 7, 2015

The Hydrogen Atom. Dr. Sabry El-Taher 1. e 4. U U r

The Schrödinger Equation

One-electron Atom. (in spherical coordinates), where Y lm. are spherical harmonics, we arrive at the following Schrödinger equation:

PHY4604 Introduction to Quantum Mechanics Fall 2004 Final Exam SOLUTIONS December 17, 2004, 7:30 a.m.- 9:30 a.m.

Name Final Exam December 14, 2016

Physics 43 Chapter 41 Homework #11 Key

Chapter 4 (Lecture 6-7) Schrodinger equation for some simple systems Table: List of various one dimensional potentials System Physical correspondence

Atoms. Radiation from atoms and molecules enables the most accurate time and length measurements: Atomic clocks

Problems and Multiple Choice Questions

PHYS Concept Tests Fall 2009

PHYS 3313 Section 001 Lecture # 22

Lecture 21 Matter acts like waves!

Lecture 10: The Schrödinger Equation. Lecture 10, p 2

Chem 467 Supplement to Lecture 19 Hydrogen Atom, Atomic Orbitals

Probability, Expectation Values, and Uncertainties

Optical Spectroscopy and Atomic Structure. PHYS 0219 Optical Spectroscopy and Atomic Structure 1

Lecture 10: The Schrödinger Equation. Lecture 10, p 2

Introduction to Quantum Mechanics (Prelude to Nuclear Shell Model) Heisenberg Uncertainty Principle In the microscopic world,

Lecture 10: The Schrödinger Equation Lecture 10, p 1

Name Solutions to Final Exam December 14, 2016

8 Wavefunctions - Schrödinger s Equation

H!!!! = E! Lecture 7 - Atomic Structure. Chem 103, Section F0F Unit II - Quantum Theory and Atomic Structure Lecture 7. Lecture 7 - Introduction

If electrons moved in simple orbits, p and x could be determined, but this violates the Heisenberg Uncertainty Principle.

2 Canonical quantization

CHAPTER 6 Quantum Mechanics II

Time part of the equation can be separated by substituting independent equation

Lecture 12: Particle in 1D boxes, Simple Harmonic Oscillators

The Simple Harmonic Oscillator

2m r2 (~r )+V (~r ) (~r )=E (~r )

Opinions on quantum mechanics. CHAPTER 6 Quantum Mechanics II. 6.1: The Schrödinger Wave Equation. Normalization and Probability

1 5 π 2. 5 π 3. 5 π π x. 5 π 4. Figure 1: We need calculus to find the area of the shaded region.

CHAPTER 6 Quantum Mechanics II

Basic methods to solve equations

CHAPTER 6 Quantum Mechanics II

3D Schrödinger Eq. Today: Continue with hydrogen. Multi-electron atoms

3. Quantum Mechanics in 3D

More on waves + uncertainty principle

Course. Print and use this sheet in conjunction with MathinSite s Maclaurin Series applet and worksheet.

three-dimensional quantum problems

Physics 505 Homework No. 4 Solutions S4-1

df(x) = h(x) dx Chemistry 4531 Mathematical Preliminaries Spring 2009 I. A Primer on Differential Equations Order of differential equation

Electromagnetic Radiation. Chapter 12: Phenomena. Chapter 12: Quantum Mechanics and Atomic Theory. Quantum Theory. Electromagnetic Radiation

ONE AND MANY ELECTRON ATOMS Chapter 15

Quantum Mechanics. incorporate the phenomenon of quantum tunneling, which we explore in this theory for explaining the behavior of

4/21/2010. Schrödinger Equation For Hydrogen Atom. Spherical Coordinates CHAPTER 8

The Hydrogen Atom. Nucleus charge +Ze mass m 1 coordinates x 1, y 1, z 1. Electron charge e mass m 2 coordinates x 2, y 2, z 2

Second quantization: where quantization and particles come from?

Tight-Binding Model of Electronic Structures

Chapter 12: Phenomena

The Quantum Theory of Atoms and Molecules

Quantum Orbits. Quantum Theory for the Computer Age Unit 9. Diving orbit. Caustic. for KE/PE =R=-3/8. for KE/PE =R=-3/8. p"...

Electronic Structure of Atoms. Chapter 6

Multi-Electron Atoms II

Physics 401: Quantum Mechanics I Chapter 4

Solutions to Problem Sheet for Week 6

Nuclear Decays. Alpha Decay

3.8 Limits At Infinity

r 2 dr h2 α = 8m2 q 4 Substituting we find that variational estimate for the energy is m e q 4 E G = 4

Anyone who can contemplate quantum mechanics without getting dizzy hasn t understood it. --Niels Bohr. Lecture 17, p 1

1 r 2 sin 2 θ. This must be the case as we can see by the following argument + L2

MATH 250 TOPIC 11 LIMITS. A. Basic Idea of a Limit and Limit Laws. Answers to Exercises and Problems

Self-consistent Field

Bohr s Correspondence Principle

McCord CH301 Exam 2 Oct 10, 2017

Name Solutions to Test 3 November 8, 2017

SPARKS CH301. Why are there no blue fireworks? LIGHT, ELECTRONS & QUANTUM MODEL. UNIT 2 Day 2. LM15, 16 & 17 due W 8:45AM

Chapter 7 The Quantum-Mechanical Model of the Atom

SCIENCE VISION INSTITUTE For CSIR NET/JRF, GATE, JEST, TIFR & IIT-JAM Web:

Semiconductor Physics and Devices

Basic Physical Chemistry Lecture 2. Keisuke Goda Summer Semester 2015

2 Generating Functions

Legendre Polynomials and Angular Momentum

Chapter 2. Atomic Structure. Inorganic Chemistry1 CBNU T.-S.You

Lecture 2: simple QM problems

:C O: σorbitals of CO. πorbitals of CO. Assumed knowledge. Chemistry 2. Learning outcomes. Lecture 2 Particle in a box approximation. C 2p.

Oh, the humanity! David J. Starling Penn State Hazleton PHYS 214

Electromagnetic Field Waves

The Northern California Physics GRE Bootcamp

Lecture 37. Physics 2170 Fall

Diffraction Gratings, Atomic Spectra. Prof. Shawhan (substituting for Prof. Hall) November 14, 2016

Continuous functions. Limits of non-rational functions. Squeeze Theorem. Calculator issues. Applications of limits

Limits and Continuity

Chem 110 Practice Midterm 2014

ACCUPLACER MATH 0310

Quantum Field Theory III

Chapter 9: Multi- Electron Atoms Ground States and X- ray Excitation

Notes for Special Relativity, Quantum Mechanics, and Nuclear Physics

Physics 2203, 2011: Equation sheet for second midterm. General properties of Schrödinger s Equation: Quantum Mechanics. Ψ + UΨ = i t.

CHAPTER 28 Quantum Mechanics of Atoms Units

McCord CH301 Exam 2 Oct 10, 2017

Electromagnetic Field Waves

Physics 217 Problem Set 1 Due: Friday, Aug 29th, 2008

Bohr model and Franck-Hertz experiment

Chemistry 3502/4502. Final Exam Part I. May 14, 2005

Atomic Structure and Atomic Spectra

Chemistry 3502/4502. Final Exam Part I. May 14, 2005

Horizontal asymptotes

Chemistry 3502/4502. Exam III. All Hallows Eve/Samhain, ) This is a multiple choice exam. Circle the correct answer.

Transcription:

Name Solutions to Test November 7 8 This test consists of three parts. Please note that in parts II and III you can skip one question of those offered. Some possibly useful formulas can be found below. 4 5 h 6.66 J s 4.6 ev s Barrier penetration: 4 6.55 J s 6.58 ev s E E T 6 e 9 V ev.6 J V Reflection off a step: mv E E EV if E V R E EV Euler s formula i e cos isin if E V Part I: Multiple Choice [ points] For each question choose the best answer ( points each) L E n Hydrogen.6 evz n Spherical Coords. rsin cos y rsin sin z rcos r. If the total angular momentum squared has a value of L what is l? A) 4 B) 5 C) D) 8 E) 4. An electron with n = 4 l = and m = would be described as what type of electron? A) 4p B) p C) f D) 4f E) 4d. Which of the following tells you the probability density of finding a particle at the point r at time t in three dimensions? A) r * B) r C) r D) r E) r 4. If an electron in an atom has l = what is a complete list of the values that m can take on? A) B) C) D) E) None of these 5. Which of the following corresponds to the momentum operator p op in quantum mechanics in one dimension? A) i B) i C) D) E) none of these

6. How come we don t solve Schrödinger s equation for hydrogen by factoring the wave function into functions of y and z: r X YyZz? A) Because the derivative terms end up miing these factors together into an intractable mess B) Because there are three Schrödinger s equations in D and this can t solve all three at once C) Because it should be a sum of functions in D not a product D) Because the potential for hydrogen can t be naturally written in Cartesian coordinates and this factorization doesn t help E) It can be written this way; that s eactly how we solved it 7. To find the average energy you would epect if you measured a particle you should calculate the epectation value of the A) Position B) Momentum C) Momentum squared D) Hamiltonian E) None of these 8. Suppose rt and rt are both solutions of Schrödinger s time-dependent equation. Which of the following is guaranteed to also be a solution? A) * * rt rt B) rt rt C) rt rt rt rt D) E) None of these 9. For the harmonic oscillator with potential V m why are there only bound states no unbound states? A) Because the force never vanishes the particle must always be bound ik B) Because e is not a solution to Schrödinger s equation there can t be unbound states C) Because the potential at infinity is infinity the energy can t eceed the potential there D) Because all solutions have positive energy there can t be unbound states E) They both eist we just only found the unbound states. When you try to penetrate a finite-thickness barrier of size L and your energy E is smaller than the height of the barrier how does the barrier thickness affect the probablity of getting through? A) The probability grows eponentially as the thickness increases B) The probability shrinks eponentially as the thickness increases C) The probability is inversely proportional to the thickness D) The probability is inversely proportional to the thickness squared E) The probability is always zero in this case

Part II: Short answer [ points] Choose two of the following three questions and give a short answer (-4 sentences) ( points each).. Suppose you have found a solution to Schrödinger s time-independent equation. Unfortunately it turns out that the function is not normalized probably. What should you do? You will need to include one or more formulas in your answer. Fortunately any multiple of will also satisfy Schrödinger s time-independent equation so we simply try to multiply by an appropriate constant to make it normalized. Assume that d A ˆ A ˆ will satisfy then we can define then Schrödinger s equation and will have ˆ d.. When solving Schrödinger s equation it is often necessary to solve it in different regions and then piece the potential together at the boundaries. What are appropriate boundary conditions if (i) you have solutions on both sides of the boundary or (ii) the potential is infinite on one side of the boundary. Generally the solutions to Schrödinger s equation must be continuous have a first derivative and that derivative must be continuous. Hence we demand that the function and its derivative match on the two sides of the boundary. If the potential is infinite on one side of the boundary the wave function must vanish there and demanding that the wave function be continues then implies that it must vanish as you approach the other side of the boundary.. According to our computations for hydrogen the p d and 4s energies are related by E p E d E 4s. Eplain qualitatively why this doesn t work for more complicated atoms and give the correct general heirarchy for these levels according to our more sophisticated model. The hydrogen-like model ignores interactions between electrons. The most important effect is that the innermost (s) electrons are so close to the nucleus that effectively they almost completely screen the nucleus effectively reducing its charge and hence the outer electrons don t have as negative an energy as one would epect. However for electrons with small values of the total angular quantum number l (such as the 4s and to a lesser etent the p) the electron does penetrate a little into the innermost part of the atom allowing the electron to eperience the full attractiveness of the nucleus and lowering the energy. So the 4s energy is lowered below the d and the p is lowered compared to d as well so the final heirarchy is Ep E4s Ed.

Part III: Calculation: [6 points] Choose three of the following four questions and perform the indicated calculations ( points each). 4. An atom contains a single electron in the state n = 6 but the nuclear charge is unknown. The amount of energy required to etract the electron from the atom is measured to be E.4 ev (a) What is the value of the nuclear charge Z? We use the formula for the energy of a hyarogen-like atom E.6 ev Z n. If it takes.4 ev to get the electron to be freed the initial energy must be E.4 ev. We therefore have.6 evz.6 ev Z.4 ev n 6.4 ev6 Z 9..6 ev Z. The answer has to be an integer so we have Z =. (b) If the atom were to emit one photon starting in this state what would be the smallest energy E that that emitted photon could have and what would be the final value of n? When the atom emits a photon it falls to a lower level so the final n must be less than 6. The smallest amount it could fall would be to n = 5 so this must be the final state. The energy emitted is the initial energy divided by the final energy so.6 ev.6 ev E E6 E5.4 ev4.9 ev.496 ev. 6 5 (c) If the atom were to absorb one photon starting in this state what would be the smallest energy E that that absorbed photon could have and what would be the final value of n? In this case the energy must be increasing so n must be larger than 6. The smalles amount of energy that can be absorbed is when n increases as little as possible to n = 7 and the energy absorbed in this case must be the final energy minus the initial energy so.6 ev.6 ev E E7 E6.5 ev.4 ev.9 ev. 7 6

5. A group of electrons with kinetic energy E 8. ev impacts a sudden step potential of 6 6 unknown height V. It is found that of 9. electrons 8. of them successfully penetrate the barrier. (a) What is the reflection probability R? Since 8 of the electrons are transmitted it is clear that 9 9 R 9.%. of them are reflected so (b) What is the value (or possible values) of the potential height V? We now simply equate the reflection probability to our formula which is E EV E EV E EV E EV E EV R 9 E EV E EV E EV. At this point it is probably good to break it into two cases and do them separately 4E 6EV or 6E 4 EV 6V E or E 4 V V 4 E or V E V 4 8. ev or V 8. ev V 6. ev or V 4. ev.

This wave function is properly normalized and has 6. A particle has wave function integral is below. (a) Find the epectation values of p and for. p. A possibly useful e for. Real wave functions always have p so there is nothing to calculate. For and we compute * d e e d e d * 4 d e e d e d 4! 46 4 4 4 4 6 4 4! 44 4 4. 5 4 (b) Find the uncertainties principle. and We calculate the uncertainties using the formulas p and check that it satisfies the uncertainty p p p 9. 4 4 The uncertainty relation then just says So it is satisfied as it must me. p. Possibly useful integral: n A n e d n! A. Wave functions for net problem: r r a i 5 i R e Y 5 sin e Y sincos e. 6a 8 8

7. Chemists prefer using real wave functions for atoms. For eample one of the states they use is. Some hydrogen wave functions are written below. (a) Write eplicitly this wave function as a function of r and show that it is real. We start with r R ry nlm nl lm so we have r R ry Y r re 6a 8 8 6 a r a r a re re sincosisincosisin 5 5 8 a 4 a sincos. The final epression is manifestly real. r a r a i i i i e sine sine sine e 5 5 (b) Find the value(s) of r where the particle is most likely to be. This will occur any place where the function is at a maimum positive value or maimum negative value. To find the location we just focus on the three factors and insist that their derivatives relative to the corresponding variables vanishes. The numerical factors are irrelevant. We therefore have d r a r a r r a r r a re e e e dr a a d sin cos d d cos sin. d The first equation has a root at r a. The only place cosine vanishes between and is. For the final equation sine vanishes at both and. Thus the two points where the wave r a a. function is maimum are and (c) Find the corresponding cartesian coordinates yz. We first note that for both points z rcos and y rsin sin. For we have Hence the points are yz a. rsin cos asin cos a or rsin cos asin cos a.