UNIVERSITETET I OSLO Det matematisk-naturvitenskapelige fakultet

Σχετικά έγγραφα
Phys460.nb Solution for the t-dependent Schrodinger s equation How did we find the solution? (not required)

Problem Set 9 Solutions. θ + 1. θ 2 + cotθ ( ) sinθ e iφ is an eigenfunction of the ˆ L 2 operator. / θ 2. φ 2. sin 2 θ φ 2. ( ) = e iφ. = e iφ cosθ.

Section 8.3 Trigonometric Equations

3.4 SUM AND DIFFERENCE FORMULAS. NOTE: cos(α+β) cos α + cos β cos(α-β) cos α -cos β

Exercises 10. Find a fundamental matrix of the given system of equations. Also find the fundamental matrix Φ(t) satisfying Φ(0) = I. 1.

Practice Exam 2. Conceptual Questions. 1. State a Basic identity and then verify it. (a) Identity: Solution: One identity is csc(θ) = 1

Example Sheet 3 Solutions

PARTIAL NOTES for 6.1 Trigonometric Identities

Section 7.6 Double and Half Angle Formulas

Areas and Lengths in Polar Coordinates

Math221: HW# 1 solutions

Matrices and Determinants

Srednicki Chapter 55

Lecture 2: Dirac notation and a review of linear algebra Read Sakurai chapter 1, Baym chatper 3

CHAPTER 25 SOLVING EQUATIONS BY ITERATIVE METHODS

Απόκριση σε Μοναδιαία Ωστική Δύναμη (Unit Impulse) Απόκριση σε Δυνάμεις Αυθαίρετα Μεταβαλλόμενες με το Χρόνο. Απόστολος Σ.

EE512: Error Control Coding

HOMEWORK 4 = G. In order to plot the stress versus the stretch we define a normalized stretch:

Chapter 6: Systems of Linear Differential. be continuous functions on the interval

Second Order RLC Filters

Homework 3 Solutions

6.1. Dirac Equation. Hamiltonian. Dirac Eq.

Econ 2110: Fall 2008 Suggested Solutions to Problem Set 8 questions or comments to Dan Fetter 1

2 Composition. Invertible Mappings

Inverse trigonometric functions & General Solution of Trigonometric Equations

Areas and Lengths in Polar Coordinates

C.S. 430 Assignment 6, Sample Solutions

4.6 Autoregressive Moving Average Model ARMA(1,1)

Chapter 6: Systems of Linear Differential. be continuous functions on the interval

Partial Differential Equations in Biology The boundary element method. March 26, 2013

b. Use the parametrization from (a) to compute the area of S a as S a ds. Be sure to substitute for ds!

Section 9.2 Polar Equations and Graphs

derivation of the Laplacian from rectangular to spherical coordinates

Uniform Convergence of Fourier Series Michael Taylor

Orbital angular momentum and the spherical harmonics

SCHOOL OF MATHEMATICAL SCIENCES G11LMA Linear Mathematics Examination Solutions

CRASH COURSE IN PRECALCULUS

ΚΥΠΡΙΑΚΗ ΕΤΑΙΡΕΙΑ ΠΛΗΡΟΦΟΡΙΚΗΣ CYPRUS COMPUTER SOCIETY ΠΑΓΚΥΠΡΙΟΣ ΜΑΘΗΤΙΚΟΣ ΔΙΑΓΩΝΙΣΜΟΣ ΠΛΗΡΟΦΟΡΙΚΗΣ 19/5/2007

Tridiagonal matrices. Gérard MEURANT. October, 2008

Statistical Inference I Locally most powerful tests

CHAPTER 101 FOURIER SERIES FOR PERIODIC FUNCTIONS OF PERIOD

( y) Partial Differential Equations

Solutions - Chapter 4

Answer sheet: Third Midterm for Math 2339

Fourier Series. MATH 211, Calculus II. J. Robert Buchanan. Spring Department of Mathematics

Tutorial problem set 6,

1 String with massive end-points

General 2 2 PT -Symmetric Matrices and Jordan Blocks 1

Approximation of distance between locations on earth given by latitude and longitude

Partial Trace and Partial Transpose

If we restrict the domain of y = sin x to [ π, π ], the restrict function. y = sin x, π 2 x π 2

Review Test 3. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MathCity.org Merging man and maths

Concrete Mathematics Exercises from 30 September 2016

If we restrict the domain of y = sin x to [ π 2, π 2

DESIGN OF MACHINERY SOLUTION MANUAL h in h 4 0.

SUPERPOSITION, MEASUREMENT, NORMALIZATION, EXPECTATION VALUES. Reading: QM course packet Ch 5 up to 5.6

Nowhere-zero flows Let be a digraph, Abelian group. A Γ-circulation in is a mapping : such that, where, and : tail in X, head in

Pg The perimeter is P = 3x The area of a triangle is. where b is the base, h is the height. In our case b = x, then the area is

Finite Field Problems: Solutions

Trigonometry 1.TRIGONOMETRIC RATIOS

Solutions to Exercise Sheet 5

Second Order Partial Differential Equations

ST5224: Advanced Statistical Theory II

Variational Wavefunction for the Helium Atom

Ordinal Arithmetic: Addition, Multiplication, Exponentiation and Limit

forms This gives Remark 1. How to remember the above formulas: Substituting these into the equation we obtain with

= {{D α, D α }, D α }. = [D α, 4iσ µ α α D α µ ] = 4iσ µ α α [Dα, D α ] µ.

ECE 308 SIGNALS AND SYSTEMS FALL 2017 Answers to selected problems on prior years examinations

ANSWERSHEET (TOPIC = DIFFERENTIAL CALCULUS) COLLECTION #2. h 0 h h 0 h h 0 ( ) g k = g 0 + g 1 + g g 2009 =?

Problem 3.1 Vector A starts at point (1, 1, 3) and ends at point (2, 1,0). Find a unit vector in the direction of A. Solution: A = 1+9 = 3.

9.09. # 1. Area inside the oval limaçon r = cos θ. To graph, start with θ = 0 so r = 6. Compute dr

( ) 2 and compare to M.

CHAPTER 48 APPLICATIONS OF MATRICES AND DETERMINANTS

Jesse Maassen and Mark Lundstrom Purdue University November 25, 2013

Appendix to On the stability of a compressible axisymmetric rotating flow in a pipe. By Z. Rusak & J. H. Lee

Other Test Constructions: Likelihood Ratio & Bayes Tests

Every set of first-order formulas is equivalent to an independent set

Lecture 2. Soundness and completeness of propositional logic

Integrals in cylindrical, spherical coordinates (Sect. 15.7)

TMA4115 Matematikk 3

w o = R 1 p. (1) R = p =. = 1

Math 6 SL Probability Distributions Practice Test Mark Scheme

Problem Set 3: Solutions

Problem 1.1 For y = a + bx, y = 4 when x = 0, hence a = 4. When x increases by 4, y increases by 4b, hence b = 5 and y = 4 + 5x.

Trigonometric Formula Sheet

Homework 8 Model Solution Section

MATHEMATICS. 1. If A and B are square matrices of order 3 such that A = -1, B =3, then 3AB = 1) -9 2) -27 3) -81 4) 81

Συστήματα Διαχείρισης Βάσεων Δεδομένων

Lecture 15 - Root System Axiomatics

Reminders: linear functions

2. Let H 1 and H 2 be Hilbert spaces and let T : H 1 H 2 be a bounded linear operator. Prove that [T (H 1 )] = N (T ). (6p)

Figure A.2: MPC and MPCP Age Profiles (estimating ρ, ρ = 2, φ = 0.03)..

Numerical Analysis FMN011

ΗΜΥ 220: ΣΗΜΑΤΑ ΚΑΙ ΣΥΣΤΗΜΑΤΑ Ι Ακαδημαϊκό έτος Εαρινό Εξάμηνο Κατ οίκον εργασία αρ. 2

Solution Series 9. i=1 x i and i=1 x i.

Written Examination. Antennas and Propagation (AA ) April 26, 2017.

The Simply Typed Lambda Calculus

Lecture 13 - Root Space Decomposition II

6.3 Forecasting ARMA processes

Transcript:

UNIVERSITETET I OSLO Det matematisk-naturvitenskapelige fakultet Solution for take home exam: FYS3, Oct. 4, 3. Problem. Ĥ ɛ K K + ɛ K K + β K K + α K K For Ĥ Ĥ : ɛ ɛ, β α. The operator ˆT can be written ˆT K K K K. Therefore ˆT K K K K ˆT ˆT is Hermitian. Unitarity can be shown by forming the product ˆT ˆT K K K K K K K K K K + K K Î ˆT ˆT. Note that if you use a specific state to prove operator properties such as hermiticity and unitarity, you also need to show that these properties holds regardless of your choice of state. Since ˆT is unitary and hermitian, ˆT ˆT. This implies that the eigenvalues of ˆT are ±. Labeling the eigenstates ± we have ˆT + + + ˆT Adding these we see that ˆT + + +. Thus we can identify + + c K and + c K, where c is a constant. Adding and subtracting these we get + c normalizing these we find c thus c K K, K + K ± K K.3 Using the fact that ˆT is unitary, ˆT ˆT, we have ˆT Ĥ ˆT Ĥ Ĥ ˆT ˆT Ĥ

[Ĥ, ˆT ]. Then using Ehrenfests theorem which was proven in class and in Griffiths for an operator which does not explicitly depend on time, we have d dt ψt ˆT ψt ī ] [Ĥ, h ψt ˆT ψt ψt ˆT ψt constant not dependent on t }{{} Another way of showing this is to consider the unitary time-evolution operator Ût i Ht/ h e [ and reckognize that when ˆT, Ĥ], ˆT will also commute with any powers of Ĥ, thus [ ] ˆT, Û t, and so ψt ˆT ψt ψ Û t ˆT Ût ψ ψ Û t Ût ˆT ψ ψ ˆT ψ.4 ˆT ] is a symmetry if [Ĥ, ˆT. To evaluate the commutator we need Ĥ ˆT ɛ K K + ɛ K K + α K K + β K K K K K K α K K β K K ɛ K K ɛ K K ˆT Ĥ K K K K ɛ K K + ɛ K K + α K K + β K K β K K α K K ɛ K K ɛ K K therefore ] [Ĥ, ˆT β α K K K K α β Hermiticity requires β α so for ˆT to be a symmetry, α must be real..5 When ˆT is a symmetry, α β R, there exists a common complete set of states which are simultaneously eigenstates of both ˆT and Ĥ. The eigenstates of ˆT were found in above. So we will evaluate the action of Ĥ on these Ĥ + ɛ K K + ɛ K K + α K K + α K K K K ɛ α K K ɛ α + Ĥ ɛ K K + ɛ K K + α K K + α K K K + K ɛ + α K + K ɛ + α

So the common complete set of eigenfunctions are + K K, +, ɛ α K + K,, ɛ + α.6 The time dependent state can be written in terms of the energy eigenkets as K + +. Thus the time-dependent state starting from K at t is ψt e iĥt/ h K e iĥt/ h + + e iĥt/ h e iɛ αt/ h + + e iɛ+αt/ h e iɛt/ h cosαt/ h + i sinαt/ h + + cosαt/ h i sinαt/ h e iɛt/ h cosαt/ h + + + i sinαt/ h + e iɛt/ h cosαt/ h K i sinαt/ h K Therefore the probabilities are P K t K ψt e iɛt/ h cosαt/ h cos αt/ h P Kt K ψt ie iɛt/ h sinαt/ h sin αt/ h alternatively, since there are only two possibilities: P Kt P K t. One can also solve problem entirely using the matrix representation. Representing the states K and K. The operators become Ĥ ɛ α β ɛ ˆT Problem. A state is equal to the zero ket if and only if its norm is zero. The norm of Ŝ is [Ŝx ] Ŝ+ Ŝ Ŝx Ŝ x + Ŝy Ŝ y i, Ŝy 3 h 4 h h h 3 Ŝ Ŝ z + hŝz Ŝ

Note that points will be deducted if you use Ŝ to show that the norm is.. Expanding the exponential we have e µ h Ŝ + µ hŝ + µ Ŝ +.... Since h!ŝ Ŝ Ŝ hŝ all higher powers than linear vanish. Using Ŝ h we get µ + µ hŝ + µ N N The corresponding bra is µ N + µ so that µ µ N + µ N + µ N + µ Using this normalization we get λ µ + λ + µ + λ + µ + λ µ + λ + µ.3 Using Ŝx µ Ŝ µ + µ + µ Ŝ + µ hµ + µ he iφ tanθ/ + tan θ/ he iφ sinθ/ cosθ/ h e iφ sinθ µ Ŝ+ µ µ Ŝ µ h eiφ sinθ Ŝ+ + Ŝ / we get θ, φ Ŝx θ, φ θ, φ Ŝ+ θ, φ + θ, φ Ŝ θ, φ h 4 sin θ e iφ + e iφ h sin θ cos φ Alternatively one can directly write down the state θ, φ first θ, φ + tanθ/e iφ cosθ/ + sinθ/e iφ + tan θ/.4 A very simple way to solve this problem is to use the result from problem.b and use the fact that since there are only two possible measurement outcomes the expectation value determines the probability. Denoting the probability for measuring + h/ by p x one has θ, φ Ŝx θ, φ h p x h p x p x + sin θ cos φ 4

One can also proceed in the more standard way: Note that for θ π/ and φ, Ω,,. Therefore the eigenstate of Ŝ x with eigenvalue h/ is θ π/, φ. The probability of measuring this value in the state θ, φ is thus p x π/, θ, φ θ, φ π/, + tanθ/e iφ tanπ/4e i + tan π/4 + tan θ/ + tanθ/e iφ + tan θ/ cosθ/ + sinθ/e iφ cosθ/ cosθ/ p x π/, θ, φ cosθ/ + sinθ/e iφ cosθ/ + sinθ/e iφ cos θ/ + sin θ/ + sinθ/ cosθ/ cos φ + sin θ cos φ.5 The eigenstates of the Hamiltonian are θ, φ and π θ, φ + π. The last fact follows from sinπ θ cosφ + π, sinπ θ sinφ + π, cosπ θ S π θ, φ + π h π θ, φ + π using sinπ θ sin θ, cosπ θ cos θ, cosφ + π cosφ and sinφ + π sin φ one sees that sin θ cos φ, sin θ sin φ, cos θ S π θ, φ + π h π θ, φ + π }{{} Ω in other words π θ, φ + π is an eigenstate of Ω S with eigenvalue h/. The explicit expression for the two energy eigenstates are θ, φ cosθ/ + sinθ/e iφ π θ, φ + π sinθ/ cosθ/e iφ At t immediately after the measurement of the spin x component that gave the value h/ the system is in the state π/,. This state can be decomposed into the Hamiltonian eigenstates as π/, α θ, φ + β π θ, φ + π 5

to find the coefficients α and β we multiply by the bras θ, φ and π θ, φ + π and use the orthonormality of these states. Using the results from problem.3 we find α α θ, φ π/, cosθ/ + sinθ/eiφ β π θ, φ + π π/, sinθ/ cosθ/eiφ β is found by letting θ π θ and φ φ + π in the expression for α. The time-dependent state is then ψt e iĥt/ h α θ, φ + β π θ, φ + π αe igt/ h θ, φ + βe igt/ h π θ, φ + π and the probability of measuring the spin-x component to be the value h/ is Now α P t π/, ψt β αe igt/ h π/, θ, φ + βe igt/ h π/, π θ, φ + π α e igt/ h + β e igt/ h cosθ/ + sinθ/eiφ + sinπ θ cosφ + π Therefore + sin θ cos φ P t e igt/ h + cosθ/ + sinθ/e iφ sin θ cos φ sin θ cos φ + sin θ cos φ e igt/ h cosgt/ h + i sin θ cos φ singt/ h cos gt/ h + sin θ cos φ sin gt/ h sin θ cos φ sin gt/ h + sin θ cos φ + sin θ cos φ cosgt/ h Note that you will not get credit on this subproblem if you changed the problem to a much easier one by choosing particular values for θ and φ, as for instance choosing ˆΩ,, or ˆΩ,,. The solutions to these simpler problems are of course contained in the solution for general θ and φ above..6 µ µ + µ + µ + µ + µ + µ + µ + µ 6

reparametrizing µ tanθ/e iφ one gets θ, φ θ, φ + tan θ/ + tanθ/e iφ + tanθ/e iφ + tan θ/ Doing the integral over φ from to π, the last two terms vanish thus π dφ π π dθ sin θ θ, φ θφ π π dθ sin θ + tan θ/ + tan θ/ cos θ/ dθ sin θ + tan cos θ/ + sin θ/ θ/ dcos }{{} θ cos θ/ + sin θ/ }{{}}{{} x +cos θ/ cos θ/ dx + x + + Î dx x The answer is the identity operator. 7