Orbital angular momentum and the spherical harmonics
|
|
- reek Σερπετζόγλου
- 6 χρόνια πριν
- Προβολές:
Transcript
1 Obital angula momentum and the spheical hamonics Apil 2, 207 Obital angula momentum We compae ou esult on epesentations of otations with ou pevious expeience of angula momentum, defined fo a point paticle as L = x p o, fo a quantum system as the opeato elationship ˆL = ˆx ˆp Notice that since ˆL i = ε ijk ˆx j ˆp k thee is no odeing ambiguity: ˆx j and ˆp k commute as long as j k, and the coss poduct insues this. Computing commutatos of the components of L, we have [ˆLi, ˆL m ] = [ε ijk ˆx j ˆp k, ε mnsˆx n ˆp s ] = ε ijk ε mns [ˆx j ˆp k, ˆx n ˆp s ] = ε ijk ε mns ˆx j [ˆp k, ˆx n ˆp s ] + [ˆx j, ˆx n ˆp s ] ˆp k = ε ijk ε mns ˆx j [ˆp k, ˆx n ] ˆp s + ˆx n [ˆx j, ˆp s ] ˆp k = ε ijk ε mns i δ knˆx j ˆp s + i δ jsˆx n ˆp k = i ε ijk ε mksˆx j ˆp s + ε ijk ε mnj ˆx n ˆp k = i ε ijk ε msk + ε iks ε mjk ˆx j ˆp s Using the Jacobi identity eq.2 in Angula Momentum Notes ε jkm ε inm + ε kim ε jnm + ε ijm ε knm = 0, we ewite ε ijk ε msk + ε iks ε mjk = ε ijk ε msk + ε jmk ε isk = ε mik ε jsk and the commutato becomes [ˆLi, ˆL m ] = i ε ijk ε msk + ε iks ε mjk ˆx j ˆp s = i ε mik ε jsk ˆx j ˆp s = i ε imk ˆLk We see that ˆL m satisfies the fundamental angula momentum commutation elations and must theefoe admit l, m epesentations satisfying ˆL z l, m = m l, m ˆL 2 l, m = l l + 2 l, m
2 along with aising and loweing opeatos, ˆL ±. Howeve, in the case of obital angula momentum, we have an explicit coodinate epesentation fo the opeatos. Fo the z-component, x ˆL 3 α = x ˆx ˆp 2 ˆx 2 ˆp α = i x y y x α x The eigenvalues of ˆL 3 ae given by solving i x y y x α = m x α x but this takes a simple fom in tems of an azimuthal coodinate. Let x = ρ cos ϕ and y = ρ sin ϕ. Then and we ewite the eigenvalue equation as with the immediate solutions ϕ = x ϕ x + y ϕ y = ρ sin ϕ x + ρ cos ϕ y = y x + x y i x α = m x α ϕ x α = e imϕ Single valuedness of the wave function means that we must have e 2πmi = and theefoe only intege values fo m ae allowed. This exposes an essential asymmety between spinos and vectos. We have seen that 3-vectos may be epesented as matices in a complex, 2-dim spino epesentation, but thee does not exist a simila epesentation of spinos using 3-dim coodinates. Having shown that j and m may take both intege and half-intege values, we now see that classical angula momentun is not the whole stoy. While the physical existence of intinsic angula momentum o spin was only discoveed afte the advent of quantum mechanics, its existence is a consequence of the goup-theoetic natue of otations, and could have existed classically. We continue with ou examination of intege j epesentations, and the states l, m of obital angula momentum. 2 Changing to spheical coodinates It is not supising that obital angula momentum is most tanspaently studied in tems of spheical coodinates. Hee we ewite ˆL z, ˆL ± and ˆL 2 in spheical coodinates. The coodinate tansfomation and its invese ae given by = x 2 + y 2 + z 2 x θ = tan 2 + y 2 2 ϕ = tan y x 2
3 and x = cos ϕ y = sin ϕ z = cos θ We also need the deivative opeatos, x i. Using the chain ule, we have x = x + θ x θ + ϕ x ϕ = y y + θ y θ + ϕ y ϕ = z z + θ z θ + ϕ z ϕ We would like to wite the ight hand sides of these equations in spheical coodinates. We may find the patials by witing the total diffeentials of, θ and ϕ. Stating with the diffeential of, d = x dx + y dy + z dz we ead off the patial deivatives, x = x = cos ϕ y = y = sin ϕ z = z = cos θ Next, fo θ, we take the diffeential of tan θ, x2 + y tan θ = 2 z cos 2 θ dθ = x x2 + y 2 z dx + y x2 + y 2 z dy x2 + y 2 z 2 dz Then, with the diffeential of θ becomes dθ = cos 2 θ = cos θ cos ϕdx + x2 + y 2 = x z y z = = cos ϕ cos θ sin ϕ cos θ cos ϕ dx + cos θ cos θ sin ϕdy dz sin ϕ dy cos θ 2 cos 2 θ dz 3
4 and ead off the patials θ x = cos θ cos ϕ θ y = cos θ sin ϕ θ = z Finally, we compute the diffeential of tan ϕ = y x, and use cos2 ϕ = and once again ead off the patials x2 x 2 +y 2 cos 2 ϕ dϕ = y x 2 dx + x dy dϕ = cos 2 sin ϕ ϕ 2 sin 2 θ cos 2 ϕ dx + cos2 ϕ cos ϕ dy = sin ϕ cos ϕ dx + dy ϕ x ϕ y ϕ z = sin ϕ = cos ϕ = 0 Now, etuning to the chain ule expansions, eqs., we substitute to find x = x y z + xz x2 + y 2 2 θ y x 2 + y 2 ϕ = cos ϕ + cos θ cos ϕ θ sin ϕ ϕ = y + yz x2 + y 2 2 θ + x x 2 + y 2 ϕ = sin ϕ + cos θ sin ϕ θ + = z x2 + y 2 2 θ = cos θ θ In the next section, we substitute to find the obital angula momentum opeatos in angula coodinates. Finally, it is easy to find the Laplacian in spheical coodinates using the techniques of diffeential geomety. Using the metic in spheical coodinates g ij = 2 2 sin 2 θ and the divegence theoem, the esult is immediate: 2 = D i D i cos ϕ ϕ 2 4
5 = g x i = 2 = 2 gg ij x j [ θ 2 + θ θ + θ ϕ 2 sin 2 θ ] ϕ 2 2 sin 2 θ 2 ϕ Obital angula momentum opeatos in spheical coodiates Caying out the coodinate substitutions, fo ˆL 3 we have i x y y = i cos ϕ sin ϕ x + cos θ sin ϕ θ + +i sin ϕ cos ϕ + cos θ cos ϕ θ = i ϕ as found above. Fo the aising opeato, we have while the loweing opeato is ˆL + = z x + iz y x + iy z = cos θ + cos θ cos ϕ + cos θ cos ϕ θ i sin ϕ + i cos θ sin ϕ θ + i cos ϕ + i sin ϕ cos θ θ sin ϕ ϕ cos ϕ ϕ cos ϕ sin ϕ = cos ϕ + i sin ϕ e iϕ cos θ + cos2 θe iϕ θ + eiϕ sin 2 θ θ +i cos ϕ + i sin ϕ cos θ ϕ = e iϕ θ + icos θ ϕ ˆL = z x + iz y + x iy z = cos θ + cos θ cos ϕ + cos θ cos ϕ θ i sin ϕ + i cos θ sin ϕ θ + i + cos ϕ i sin ϕ cos θ θ = e iϕ cos θ e iϕ cos θ e iϕ cos 2 θ θ e iϕ sin 2 θ cos θ + ie iϕ θ ϕ 5 sin ϕ ϕ cos ϕ ϕ ϕ ϕ
6 Collecting the esults so fa, we have = e iϕ θ icos θ ϕ ˆL 3 = i ϕ ˆL + = e iϕ θ + icos θ ϕ ˆL = e iϕ θ + icos θ ϕ Execise: Find the fom of ˆL x and ˆL y fom eqs.5 and 6, togethe with the definitions Ĵ ± Ĵ ± iĵ2. Execise: Confim the fom of the Laplacian opeato by diect substitution into ˆL 2 = ˆL 2 x + ˆL 2 y + ˆL 2 z Now, since ˆL + ˆL = ˆL 2 ˆL ˆL 3 the magnitude squaed of the total angula momentum is L 2 = ˆL + ˆL + L 2 3 L 3 = e iϕ θ + icos θ = 2 cos θ = 2 cos θ = 2 cos θ = 2 = 2 θ + θ icos2 sin 2 θ e iϕ ϕ θ + icos θ ϕ + θ 2 θ 2 i ϕ cos2 θ sin 2 θ θ + icos θ ϕ 2 ϕ θ 2 θ 2 2 ϕ 2 cos2 θ 2 sin 2 θ ϕ 2 2 cos θ + θ θ 2 + sin 2 θ + 2 θ θ sin 2 θ ϕ 2 2 ϕ ϕ 2 + i 2 ϕ ϕ θ + icos θ ϕ 2 + i 2 ϕ ϕ 2 2 ϕ 2 + i 2 ϕ This last equation establishes the elationship between the spheical hamonics and the angula momentum states, because the Laplace equation in spheical coodinates is 2 = θ θ 2 sin 2 θ ϕ 2 = ˆL 2 2 6
7 and we know that sepaation of vaiables leads to geneal solution of the Laplace equation, f, θ, ϕ with the angula solution given in tems of spheical hamonics, f, θ, ϕ = l l=0 m= l A l Y l m θ, ϕ The spheical hamonics satisfy the sepaated angula eigenvalue equation, + 2 θ θ sin 2 θ ϕ 2 Y l m θ, ϕ = l l + Y l m θ, ϕ fo intege l and m = l, l +,... + l. Expessing this in tems of ˆL 2, ˆL 2 ψ = l l + 2 ψ we see that ψ = l, m and theefoe identify the spheical hamonics as the intege spin eigenstates of angula momentum in a coodinate basis, These descibe only intege j states. 4 Spheical hamonics Y l m θ, ϕ = θ, ϕ l, m We can now use the quantum fomalism to find the spheical hamonics, Y l m θ, ϕ = θ, ϕ l, m. Fo any state α, we know the effect of ˆL z is given by eq.4, so θ, ϕ ˆL z α = i θ, ϕ α ϕ Since the eigenstates satisfy ˆL z l, m = m l, m in geneal, placing this equation in a coodinate basis it becomes i θ, ϕ l, m = m θ, ϕ l, m ϕ This is tivially integated to give θ, ϕ l, m = e imϕ θ, ϕ l Futhemoe, we know that the aising opeato will anihilate the state with the highest value of m, ˆL + l, m = l = 0 Again choosing a coodinate basis, ˆL + is given by eq.5 so this tanslates to a diffeential equation, 0 = θ, ϕ ˆL + l, l = e iϕ θ + icos θ = e iϕ θ + icos θ = e il+ϕ θ Setting θ, ϕ l = f l θ, we ewite this as θ, ϕ l, m = l ϕ e ilϕ θ, ϕ l ϕ cos θ θ, ϕ l l θ, ϕ l 0 = f l θ l cos θf l 7
8 This is solved by f l = sin l θ, so we have, fo m = l Y l l θ, ϕ = A ll e ilϕ sin l θ Now we can find all othe Y l m θ, ϕ by acting with the loweing opeato, θ, ϕ ˆL l, m = l l + m m θ, ϕ l, m Inseting the coodinate expession, eq.6, fo θ, ϕ ˆL l, m and solving fo the next lowe state, we have θ, ϕ l, m = theeby defining all Y l m θ, ϕ ecusively. e iϕ l l + m m θ + icos θ e iϕ e imϕ = l l + m m θ + mcos θ ϕ θ, ϕ l, m θ l Execise: Find the Y m θ, ϕ fo all allowed m. 8
Orbital angular momentum and the spherical harmonics
Orbital angular momentum and the spherical harmonics March 8, 03 Orbital angular momentum We compare our result on representations of rotations with our previous experience of angular momentum, defined
Διαβάστε περισσότεραLaplace s Equation in Spherical Polar Coördinates
Laplace s Equation in Spheical Pola Coödinates C. W. David Dated: Januay 3, 001 We stat with the pimitive definitions I. x = sin θ cos φ y = sin θ sin φ z = cos θ thei inveses = x y z θ = cos 1 z = z cos1
Διαβάστε περισσότεραdx x ψ, we should find a similar expression for rθφ L ψ. From L = R P and our knowledge of momentum operators, it follows that + e y z d
PHYS851 Quantum Mechanics I, Fall 2009 HOMEWORK ASSIGNMENT 11 Topics Coveed: Obital angula momentum, cente-of-mass coodinates Some Key Concepts: angula degees of feedom, spheical hamonics 1. [20 pts] In
Διαβάστε περισσότεραe t e r Cylindrical and Spherical Coordinate Representation of grad, div, curl and 2
Cylindical and Spheical Coodinate Repesentation of gad, div, cul and 2 Thus fa, we have descibed an abitay vecto in F as a linea combination of i, j and k, which ae unit vectos in the diection of inceasin,
Διαβάστε περισσότεραSpace Physics (I) [AP-3044] Lecture 1 by Ling-Hsiao Lyu Oct Lecture 1. Dipole Magnetic Field and Equations of Magnetic Field Lines
Space Physics (I) [AP-344] Lectue by Ling-Hsiao Lyu Oct. 2 Lectue. Dipole Magnetic Field and Equations of Magnetic Field Lines.. Dipole Magnetic Field Since = we can define = A (.) whee A is called the
Διαβάστε περισσότεραThe Laplacian in Spherical Polar Coordinates
Univesity of Connecticut DigitalCommons@UConn Chemisty Education Mateials Depatment of Chemisty -6-007 The Laplacian in Spheical Pola Coodinates Cal W. David Univesity of Connecticut, Cal.David@uconn.edu
Διαβάστε περισσότεραProblem 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.
Chemistry 362 Dr Jean M Standard Problem Set 9 Solutions The ˆ L 2 operator is defined as Verify that the angular wavefunction Y θ,φ) Also verify that the eigenvalue is given by 2! 2 & L ˆ 2! 2 2 θ 2 +
Διαβάστε περισσότεραPhys460.nb Solution for the t-dependent Schrodinger s equation How did we find the solution? (not required)
Phys460.nb 81 ψ n (t) is still the (same) eigenstate of H But for tdependent H. The answer is NO. 5.5.5. Solution for the tdependent Schrodinger s equation If we assume that at time t 0, the electron starts
Διαβάστε περισσότεραCurvilinear Systems of Coordinates
A Cuvilinea Systems of Coodinates A.1 Geneal Fomulas Given a nonlinea tansfomation between Catesian coodinates x i, i 1,..., 3 and geneal cuvilinea coodinates u j, j 1,..., 3, x i x i (u j ), we intoduce
Διαβάστε περισσότεραExample 1: THE ELECTRIC DIPOLE
Example 1: THE ELECTRIC DIPOLE 1 The Electic Dipole: z + P + θ d _ Φ = Q 4πε + Q = Q 4πε 4πε 1 + 1 2 The Electic Dipole: d + _ z + Law of Cosines: θ A B α C A 2 = B 2 + C 2 2ABcosα P ± = 2 ( + d ) 2 2
Διαβάστε περισσότερα(a,b) Let s review the general definitions of trig functions first. (See back cover of your book) sin θ = b/r cos θ = a/r tan θ = b/a, a 0
TRIGONOMETRIC IDENTITIES (a,b) Let s eview the geneal definitions of tig functions fist. (See back cove of you book) θ b/ θ a/ tan θ b/a, a 0 θ csc θ /b, b 0 sec θ /a, a 0 cot θ a/b, b 0 By doing some
Διαβάστε περισσότεραderivation of the Laplacian from rectangular to spherical coordinates
derivation of the Laplacian from rectangular to spherical coordinates swapnizzle 03-03- :5:43 We begin by recognizing the familiar conversion from rectangular to spherical coordinates (note that φ is used
Διαβάστε περισσότεραCHAPTER 25 SOLVING EQUATIONS BY ITERATIVE METHODS
CHAPTER 5 SOLVING EQUATIONS BY ITERATIVE METHODS EXERCISE 104 Page 8 1. Find the positive root of the equation x + 3x 5 = 0, correct to 3 significant figures, using the method of bisection. Let f(x) =
Διαβάστε περισσότεραTutorial Note - Week 09 - Solution
Tutoial Note - Week 9 - Solution ouble Integals in Pola Coodinates. a Since + and + 5 ae cicles centeed at oigin with adius and 5, then {,θ 5, θ π } Figue. f, f cos θ, sin θ cos θ sin θ sin θ da 5 69 5
Διαβάστε περισσότεραANTENNAS and WAVE PROPAGATION. Solution Manual
ANTENNAS and WAVE PROPAGATION Solution Manual A.R. Haish and M. Sachidananda Depatment of Electical Engineeing Indian Institute of Technolog Kanpu Kanpu - 208 06, India OXFORD UNIVERSITY PRESS 2 Contents
Διαβάστε περισσότεραHOMEWORK 4 = G. In order to plot the stress versus the stretch we define a normalized stretch:
HOMEWORK 4 Problem a For the fast loading case, we want to derive the relationship between P zz and λ z. We know that the nominal stress is expressed as: P zz = ψ λ z where λ z = λ λ z. Therefore, applying
Διαβάστε περισσότεραFundamental Equations of Fluid Mechanics
Fundamental Equations of Fluid Mechanics 1 Calculus 1.1 Gadient of a scala s The gadient of a scala is a vecto quantit. The foms of the diffeential gadient opeato depend on the paticula geomet of inteest.
Διαβάστε περισσότεραExample Sheet 3 Solutions
Example Sheet 3 Solutions. i Regular Sturm-Liouville. ii Singular Sturm-Liouville mixed boundary conditions. iii Not Sturm-Liouville ODE is not in Sturm-Liouville form. iv Regular Sturm-Liouville note
Διαβάστε περισσότεραAreas and Lengths in Polar Coordinates
Kiryl Tsishchanka Areas and Lengths in Polar Coordinates In this section we develop the formula for the area of a region whose boundary is given by a polar equation. We need to use the formula for the
Διαβάστε περισσότεραFinite Field Problems: Solutions
Finite Field Problems: Solutions 1. Let f = x 2 +1 Z 11 [x] and let F = Z 11 [x]/(f), a field. Let Solution: F =11 2 = 121, so F = 121 1 = 120. The possible orders are the divisors of 120. Solution: The
Διαβάστε περισσότεραExercises 10. Find a fundamental matrix of the given system of equations. Also find the fundamental matrix Φ(t) satisfying Φ(0) = I. 1.
Exercises 0 More exercises are available in Elementary Differential Equations. If you have a problem to solve any of them, feel free to come to office hour. Problem Find a fundamental matrix of the given
Διαβάστε περισσότεραProblems in curvilinear coordinates
Poblems in cuvilinea coodinates Lectue Notes by D K M Udayanandan Cylindical coodinates. Show that ˆ φ ˆφ, ˆφ φ ˆ and that all othe fist deivatives of the cicula cylindical unit vectos with espect to the
Διαβάστε περισσότεραSection 8.3 Trigonometric Equations
99 Section 8. Trigonometric Equations Objective 1: Solve Equations Involving One Trigonometric Function. In this section and the next, we will exple how to solving equations involving trigonometric functions.
Διαβάστε περισσότεραAnalytical Expression for Hessian
Analytical Expession fo Hessian We deive the expession of Hessian fo a binay potential the coesponding expessions wee deived in [] fo a multibody potential. In what follows, we use the convention that
Διαβάστε περισσότεραAreas and Lengths in Polar Coordinates
Kiryl Tsishchanka Areas and Lengths in Polar Coordinates In this section we develop the formula for the area of a region whose boundary is given by a polar equation. We need to use the formula for the
Διαβάστε περισσότεραMath221: HW# 1 solutions
Math: HW# solutions Andy Royston October, 5 7.5.7, 3 rd Ed. We have a n = b n = a = fxdx = xdx =, x cos nxdx = x sin nx n sin nxdx n = cos nx n = n n, x sin nxdx = x cos nx n + cos nxdx n cos n = + sin
Διαβάστε περισσότεραHomework 8 Model Solution Section
MATH 004 Homework Solution Homework 8 Model Solution Section 14.5 14.6. 14.5. Use the Chain Rule to find dz where z cosx + 4y), x 5t 4, y 1 t. dz dx + dy y sinx + 4y)0t + 4) sinx + 4y) 1t ) 0t + 4t ) sinx
Διαβάστε περισσότεραMatrix Hartree-Fock Equations for a Closed Shell System
atix Hatee-Fock Equations fo a Closed Shell System A single deteminant wavefunction fo a system containing an even numbe of electon N) consists of N/ spatial obitals, each occupied with an α & β spin has
Διαβάστε περισσότερα3.4 SUM AND DIFFERENCE FORMULAS. NOTE: cos(α+β) cos α + cos β cos(α-β) cos α -cos β
3.4 SUM AND DIFFERENCE FORMULAS Page Theorem cos(αβ cos α cos β -sin α cos(α-β cos α cos β sin α NOTE: cos(αβ cos α cos β cos(α-β cos α -cos β Proof of cos(α-β cos α cos β sin α Let s use a unit circle
Διαβάστε περισσότεραSolutions Ph 236a Week 2
Solutions Ph 236a Week 2 Page 1 of 13 Solutions Ph 236a Week 2 Kevin Bakett, Jonas Lippune, and Mak Scheel Octobe 6, 2015 Contents Poblem 1................................... 2 Pat (a...................................
Διαβάστε περισσότεραProblem Set 3: Solutions
CMPSCI 69GG Applied Information Theory Fall 006 Problem Set 3: Solutions. [Cover and Thomas 7.] a Define the following notation, C I p xx; Y max X; Y C I p xx; Ỹ max I X; Ỹ We would like to show that C
Διαβάστε περισσότεραLecture 2: Dirac notation and a review of linear algebra Read Sakurai chapter 1, Baym chatper 3
Lecture 2: Dirac notation and a review of linear algebra Read Sakurai chapter 1, Baym chatper 3 1 State vector space and the dual space Space of wavefunctions The space of wavefunctions is the set of all
Διαβάστε περισσότερα21. Stresses Around a Hole (I) 21. Stresses Around a Hole (I) I Main Topics
I Main Topics A Intoducon to stess fields and stess concentaons B An axisymmetic poblem B Stesses in a pola (cylindical) efeence fame C quaons of equilibium D Soluon of bounday value poblem fo a pessuized
Διαβάστε περισσότεραInverse trigonometric functions & General Solution of Trigonometric Equations. ------------------ ----------------------------- -----------------
Inverse trigonometric functions & General Solution of Trigonometric Equations. 1. Sin ( ) = a) b) c) d) Ans b. Solution : Method 1. Ans a: 17 > 1 a) is rejected. w.k.t Sin ( sin ) = d is rejected. If sin
Διαβάστε περισσότεραSCHOOL OF MATHEMATICAL SCIENCES G11LMA Linear Mathematics Examination Solutions
SCHOOL OF MATHEMATICAL SCIENCES GLMA Linear Mathematics 00- Examination Solutions. (a) i. ( + 5i)( i) = (6 + 5) + (5 )i = + i. Real part is, imaginary part is. (b) ii. + 5i i ( + 5i)( + i) = ( i)( + i)
Διαβάστε περισσότεραSection 7.6 Double and Half Angle Formulas
09 Section 7. Double and Half Angle Fmulas To derive the double-angles fmulas, we will use the sum of two angles fmulas that we developed in the last section. We will let α θ and β θ: cos(θ) cos(θ + θ)
Διαβάστε περισσότερα4.2 Differential Equations in Polar Coordinates
Section 4. 4. Diffeential qations in Pola Coodinates Hee the two-dimensional Catesian elations of Chapte ae e-cast in pola coodinates. 4.. qilibim eqations in Pola Coodinates One wa of epesg the eqations
Διαβάστε περισσότεραOscillating dipole system Suppose we have two small spheres separated by a distance s. The charge on one sphere changes with time and is described by
5 Radiation (Chapte 11) 5.1 Electic dipole adiation Oscillating dipole system Suppose we have two small sphees sepaated by a distance s. The chage on one sphee changes with time and is descibed by q(t)
Διαβάστε περισσότεραPartial Differential Equations in Biology The boundary element method. March 26, 2013
The boundary element method March 26, 203 Introduction and notation The problem: u = f in D R d u = ϕ in Γ D u n = g on Γ N, where D = Γ D Γ N, Γ D Γ N = (possibly, Γ D = [Neumann problem] or Γ N = [Dirichlet
Διαβάστε περισσότεραAppendix to On the stability of a compressible axisymmetric rotating flow in a pipe. By Z. Rusak & J. H. Lee
Appendi to On the stability of a compressible aisymmetric rotating flow in a pipe By Z. Rusak & J. H. Lee Journal of Fluid Mechanics, vol. 5 4, pp. 5 4 This material has not been copy-edited or typeset
Διαβάστε περισσότερα1 String with massive end-points
1 String with massive end-points Πρόβλημα 5.11:Θεωρείστε μια χορδή μήκους, τάσης T, με δύο σημειακά σωματίδια στα άκρα της, το ένα μάζας m, και το άλλο μάζας m. α) Μελετώντας την κίνηση των άκρων βρείτε
Διαβάστε περισσότεραΑπόκριση σε Μοναδιαία Ωστική Δύναμη (Unit Impulse) Απόκριση σε Δυνάμεις Αυθαίρετα Μεταβαλλόμενες με το Χρόνο. Απόστολος Σ.
Απόκριση σε Δυνάμεις Αυθαίρετα Μεταβαλλόμενες με το Χρόνο The time integral of a force is referred to as impulse, is determined by and is obtained from: Newton s 2 nd Law of motion states that the action
Διαβάστε περισσότερα1 3D Helmholtz Equation
Deivation of the Geen s Funtions fo the Helmholtz and Wave Equations Alexande Miles Witten: Deembe 19th, 211 Last Edited: Deembe 19, 211 1 3D Helmholtz Equation A Geen s Funtion fo the 3D Helmholtz equation
Διαβάστε περισσότεραIntegrals in cylindrical, spherical coordinates (Sect. 15.7)
Integrals in clindrical, spherical coordinates (Sect. 5.7 Integration in spherical coordinates. Review: Clindrical coordinates. Spherical coordinates in space. Triple integral in spherical coordinates.
Διαβάστε περισσότεραVariational Wavefunction for the Helium Atom
Technische Universität Graz Institut für Festkörperphysik Student project Variational Wavefunction for the Helium Atom Molecular and Solid State Physics 53. submitted on: 3. November 9 by: Markus Krammer
Διαβάστε περισσότεραVEKTORANALYS. CURVILINEAR COORDINATES (kroklinjiga koordinatsytem) Kursvecka 4. Kapitel 10 Sidor
VEKTORANALYS Kusvecka 4 CURVILINEAR COORDINATES (koklinjiga koodinatstem) Kapitel 10 Sido 99-11 TARGET PROBLEM An athlete is otating a hamme Calculate the foce on the ams. F ams F F ma dv a v dt d v dt
Διαβάστε περισσότεραPractice Exam 2. Conceptual Questions. 1. State a Basic identity and then verify it. (a) Identity: Solution: One identity is csc(θ) = 1
Conceptual Questions. State a Basic identity and then verify it. a) Identity: Solution: One identity is cscθ) = sinθ) Practice Exam b) Verification: Solution: Given the point of intersection x, y) of the
Διαβάστε περισσότεραThe Simply Typed Lambda Calculus
Type Inference Instead of writing type annotations, can we use an algorithm to infer what the type annotations should be? That depends on the type system. For simple type systems the answer is yes, and
Διαβάστε περισσότερα6.1. Dirac Equation. Hamiltonian. Dirac Eq.
6.1. Dirac Equation Ref: M.Kaku, Quantum Field Theory, Oxford Univ Press (1993) η μν = η μν = diag(1, -1, -1, -1) p 0 = p 0 p = p i = -p i p μ p μ = p 0 p 0 + p i p i = E c 2 - p 2 = (m c) 2 H = c p 2
Διαβάστε περισσότεραEE512: Error Control Coding
EE512: Error Control Coding Solution for Assignment on Finite Fields February 16, 2007 1. (a) Addition and Multiplication tables for GF (5) and GF (7) are shown in Tables 1 and 2. + 0 1 2 3 4 0 0 1 2 3
Διαβάστε περισσότερα2 Composition. Invertible Mappings
Arkansas Tech University MATH 4033: Elementary Modern Algebra Dr. Marcel B. Finan Composition. Invertible Mappings In this section we discuss two procedures for creating new mappings from old ones, namely,
Διαβάστε περισσότεραHomework 3 Solutions
Homework 3 Solutions Igor Yanovsky (Math 151A TA) Problem 1: Compute the absolute error and relative error in approximations of p by p. (Use calculator!) a) p π, p 22/7; b) p π, p 3.141. Solution: For
Διαβάστε περισσότεραLecture 26: Circular domains
Introductory lecture notes on Partial Differential Equations - c Anthony Peirce. Not to be copied, used, or revised without eplicit written permission from the copyright owner. 1 Lecture 6: Circular domains
Διαβάστε περισσότεραUniform Convergence of Fourier Series Michael Taylor
Uniform Convergence of Fourier Series Michael Taylor Given f L 1 T 1 ), we consider the partial sums of the Fourier series of f: N 1) S N fθ) = ˆfk)e ikθ. k= N A calculation gives the Dirichlet formula
Διαβάστε περισσότεραC.S. 430 Assignment 6, Sample Solutions
C.S. 430 Assignment 6, Sample Solutions Paul Liu November 15, 2007 Note that these are sample solutions only; in many cases there were many acceptable answers. 1 Reynolds Problem 10.1 1.1 Normal-order
Διαβάστε περισσότεραb. Use the parametrization from (a) to compute the area of S a as S a ds. Be sure to substitute for ds!
MTH U341 urface Integrals, tokes theorem, the divergence theorem To be turned in Wed., Dec. 1. 1. Let be the sphere of radius a, x 2 + y 2 + z 2 a 2. a. Use spherical coordinates (with ρ a) to parametrize.
Διαβάστε περισσότεραPARTIAL NOTES for 6.1 Trigonometric Identities
PARTIAL NOTES for 6.1 Trigonometric Identities tanθ = sinθ cosθ cotθ = cosθ sinθ BASIC IDENTITIES cscθ = 1 sinθ secθ = 1 cosθ cotθ = 1 tanθ PYTHAGOREAN IDENTITIES sin θ + cos θ =1 tan θ +1= sec θ 1 + cot
Διαβάστε περισσότεραANSWERSHEET (TOPIC = DIFFERENTIAL CALCULUS) COLLECTION #2. h 0 h h 0 h h 0 ( ) g k = g 0 + g 1 + g g 2009 =?
Teko Classes IITJEE/AIEEE Maths by SUHAAG SIR, Bhopal, Ph (0755) 3 00 000 www.tekoclasses.com ANSWERSHEET (TOPIC DIFFERENTIAL CALCULUS) COLLECTION # Question Type A.Single Correct Type Q. (A) Sol least
Διαβάστε περισσότεραforms This gives Remark 1. How to remember the above formulas: Substituting these into the equation we obtain with
Week 03: C lassification of S econd- Order L inear Equations In last week s lectures we have illustrated how to obtain the general solutions of first order PDEs using the method of characteristics. We
Διαβάστε περισσότεραr = x 2 + y 2 and h = z y = r sin sin ϕ
Homewok 4. Solutions Calculate the Chistoffel symbols of the canonical flat connection in E 3 in a cylindical coodinates x cos ϕ, y sin ϕ, z h, b spheical coodinates. Fo the case of sphee ty to make calculations
Διαβάστε περισσότερα9.09. # 1. Area inside the oval limaçon r = cos θ. To graph, start with θ = 0 so r = 6. Compute dr
9.9 #. Area inside the oval limaçon r = + cos. To graph, start with = so r =. Compute d = sin. Interesting points are where d vanishes, or at =,,, etc. For these values of we compute r:,,, and the values
Διαβάστε περισσότεραMatrices and Determinants
Matrices and Determinants SUBJECTIVE PROBLEMS: Q 1. For what value of k do the following system of equations possess a non-trivial (i.e., not all zero) solution over the set of rationals Q? x + ky + 3z
Διαβάστε περισσότεραTheoretical Competition: 12 July 2011 Question 1 Page 1 of 2
Theoetical Competition: July Question Page of. Ένα πρόβλημα τριών σωμάτων και το LISA μ M O m EIKONA Ομοεπίπεδες τροχιές των τριών σωμάτων. Δύο μάζες Μ και m κινούνται σε κυκλικές τροχιές με ακτίνες και,
Διαβάστε περισσότεραSolutions to Exercise Sheet 5
Solutions to Eercise Sheet 5 jacques@ucsd.edu. Let X and Y be random variables with joint pdf f(, y) = 3y( + y) where and y. Determine each of the following probabilities. Solutions. a. P (X ). b. P (X
Διαβάστε περισσότεραSrednicki Chapter 55
Srednicki Chapter 55 QFT Problems & Solutions A. George August 3, 03 Srednicki 55.. Use equations 55.3-55.0 and A i, A j ] = Π i, Π j ] = 0 (at equal times) to verify equations 55.-55.3. This is our third
Διαβάστε περισσότεραD Alembert s Solution to the Wave Equation
D Alembert s Solution to the Wave Equation MATH 467 Partial Differential Equations J. Robert Buchanan Department of Mathematics Fall 2018 Objectives In this lesson we will learn: a change of variable technique
Διαβάστε περισσότερα6.3 Forecasting ARMA processes
122 CHAPTER 6. ARMA MODELS 6.3 Forecasting ARMA processes The purpose of forecasting is to predict future values of a TS based on the data collected to the present. In this section we will discuss a linear
Διαβάστε περισσότεραSpherical Coordinates
Spherical Coordinates MATH 311, Calculus III J. Robert Buchanan Department of Mathematics Fall 2011 Spherical Coordinates Another means of locating points in three-dimensional space is known as the spherical
Διαβάστε περισσότεραEcon 2110: Fall 2008 Suggested Solutions to Problem Set 8 questions or comments to Dan Fetter 1
Eon : Fall 8 Suggested Solutions to Problem Set 8 Email questions or omments to Dan Fetter Problem. Let X be a salar with density f(x, θ) (θx + θ) [ x ] with θ. (a) Find the most powerful level α test
Διαβάστε περισσότεραSection 9.2 Polar Equations and Graphs
180 Section 9. Polar Equations and Graphs In this section, we will be graphing polar equations on a polar grid. In the first few examples, we will write the polar equation in rectangular form to help identify
Διαβάστε περισσότεραEvery set of first-order formulas is equivalent to an independent set
Every set of first-order formulas is equivalent to an independent set May 6, 2008 Abstract A set of first-order formulas, whatever the cardinality of the set of symbols, is equivalent to an independent
Διαβάστε περισσότεραDifferential equations
Differential equations Differential equations: An equation inoling one dependent ariable and its deriaties w. r. t one or more independent ariables is called a differential equation. Order of differential
Διαβάστε περισσότερα( y) Partial Differential Equations
Partial Dierential Equations Linear P.D.Es. contains no owers roducts o the deendent variables / an o its derivatives can occasionall be solved. Consider eamle ( ) a (sometimes written as a ) we can integrate
Διαβάστε περισσότεραProblem 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.
Problem 3.1 Vector A starts at point (1, 1, 3) and ends at point (, 1,0). Find a unit vector in the direction of A. Solution: A = ˆx( 1)+ŷ( 1 ( 1))+ẑ(0 ( 3)) = ˆx+ẑ3, A = 1+9 = 3.16, â = A A = ˆx+ẑ3 3.16
Διαβάστε περισσότερα(As on April 16, 2002 no changes since Dec 24.)
~rprice/area51/documents/roswell.tex ROSWELL COORDINATES FOR TWO CENTERS As on April 16, 00 no changes since Dec 4. I. Definitions of coordinates We define the Roswell coordinates χ, Θ. A better name will
Διαβάστε περισσότεραDESIGN OF MACHINERY SOLUTION MANUAL h in h 4 0.
DESIGN OF MACHINERY SOLUTION MANUAL -7-1! PROBLEM -7 Statement: Design a double-dwell cam to move a follower from to 25 6, dwell for 12, fall 25 and dwell for the remader The total cycle must take 4 sec
Διαβάστε περισσότεραChapter 6: Systems of Linear Differential. be continuous functions on the interval
Chapter 6: Systems of Linear Differential Equations Let a (t), a 2 (t),..., a nn (t), b (t), b 2 (t),..., b n (t) be continuous functions on the interval I. The system of n first-order differential equations
Διαβάστε περισσότεραApproximation of distance between locations on earth given by latitude and longitude
Approximation of distance between locations on earth given by latitude and longitude Jan Behrens 2012-12-31 In this paper we shall provide a method to approximate distances between two points on earth
Διαβάστε περισσότερα1 Full derivation of the Schwarzschild solution
EPGY Summe Institute SRGR Gay Oas 1 Full deivation of the Schwazschild solution The goal of this document is to povide a full, thooughly detailed deivation of the Schwazschild solution. Much of the diffeential
Διαβάστε περισσότερα( ) 2 and compare to M.
Problems and Solutions for Section 4.2 4.9 through 4.33) 4.9 Calculate the square root of the matrix 3!0 M!0 8 Hint: Let M / 2 a!b ; calculate M / 2!b c ) 2 and compare to M. Solution: Given: 3!0 M!0 8
Διαβάστε περισσότερα4.6 Autoregressive Moving Average Model ARMA(1,1)
84 CHAPTER 4. STATIONARY TS MODELS 4.6 Autoregressive Moving Average Model ARMA(,) This section is an introduction to a wide class of models ARMA(p,q) which we will consider in more detail later in this
Διαβάστε περισσότεραSecond Order Partial Differential Equations
Chapter 7 Second Order Partial Differential Equations 7.1 Introduction A second order linear PDE in two independent variables (x, y Ω can be written as A(x, y u x + B(x, y u xy + C(x, y u u u + D(x, y
Διαβάστε περισσότεραUNIVERSITETET I OSLO Det matematisk-naturvitenskapelige fakultet
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
Διαβάστε περισσότεραJesse Maassen and Mark Lundstrom Purdue University November 25, 2013
Notes on Average Scattering imes and Hall Factors Jesse Maassen and Mar Lundstrom Purdue University November 5, 13 I. Introduction 1 II. Solution of the BE 1 III. Exercises: Woring out average scattering
Διαβάστε περισσότεραAnswer sheet: Third Midterm for Math 2339
Answer sheet: Third Midterm for Math 339 November 3, Problem. Calculate the iterated integrals (Simplify as much as possible) (a) e sin(x) dydx y e sin(x) dydx y sin(x) ln y ( cos(x)) ye y dx sin(x)(lne
Διαβάστε περισσότεραGeneral Relativity (225A) Fall 2013 Assignment 5 Solutions
Univesity of Califonia at San Diego Depatment of Physics Pof. John McGeevy Geneal Relativity 225A Fall 2013 Assignment 5 Solutions Posted Octobe 23, 2013 Due Monday, Novembe 4, 2013 1. A constant vecto
Διαβάστε περισσότεραIf we restrict the domain of y = sin x to [ π, π ], the restrict function. y = sin x, π 2 x π 2
Chapter 3. Analytic Trigonometry 3.1 The inverse sine, cosine, and tangent functions 1. Review: Inverse function (1) f 1 (f(x)) = x for every x in the domain of f and f(f 1 (x)) = x for every x in the
Διαβάστε περισσότεραGeneral 2 2 PT -Symmetric Matrices and Jordan Blocks 1
General 2 2 PT -Symmetric Matrices and Jordan Blocks 1 Qing-hai Wang National University of Singapore Quantum Physics with Non-Hermitian Operators Max-Planck-Institut für Physik komplexer Systeme Dresden,
Διαβάστε περισσότεραFourier Series. MATH 211, Calculus II. J. Robert Buchanan. Spring Department of Mathematics
Fourier Series MATH 211, Calculus II J. Robert Buchanan Department of Mathematics Spring 2018 Introduction Not all functions can be represented by Taylor series. f (k) (c) A Taylor series f (x) = (x c)
Διαβάστε περισσότεραSecond Order RLC Filters
ECEN 60 Circuits/Electronics Spring 007-0-07 P. Mathys Second Order RLC Filters RLC Lowpass Filter A passive RLC lowpass filter (LPF) circuit is shown in the following schematic. R L C v O (t) Using phasor
Διαβάστε περισσότεραDerivation of Optical-Bloch Equations
Appendix C Derivation of Optical-Bloch Equations In this appendix the optical-bloch equations that give the populations and coherences for an idealized three-level Λ system, Fig. 3. on page 47, will be
Διαβάστε περισσότεραMock Exam 7. 1 Hong Kong Educational Publishing Company. Section A 1. Reference: HKDSE Math M Q2 (a) (1 + kx) n 1M + 1A = (1) =
Mock Eam 7 Mock Eam 7 Section A. Reference: HKDSE Math M 0 Q (a) ( + k) n nn ( )( k) + nk ( ) + + nn ( ) k + nk + + + A nk... () nn ( ) k... () From (), k...() n Substituting () into (), nn ( ) n 76n 76n
Διαβάστε περισσότεραIf we restrict the domain of y = sin x to [ π 2, π 2
Chapter 3. Analytic Trigonometry 3.1 The inverse sine, cosine, and tangent functions 1. Review: Inverse function (1) f 1 (f(x)) = x for every x in the domain of f and f(f 1 (x)) = x for every x in the
Διαβάστε περισσότεραCRASH COURSE IN PRECALCULUS
CRASH COURSE IN PRECALCULUS Shiah-Sen Wang The graphs are prepared by Chien-Lun Lai Based on : Precalculus: Mathematics for Calculus by J. Stuwart, L. Redin & S. Watson, 6th edition, 01, Brooks/Cole Chapter
Διαβάστε περισσότεραConcrete Mathematics Exercises from 30 September 2016
Concrete Mathematics Exercises from 30 September 2016 Silvio Capobianco Exercise 1.7 Let H(n) = J(n + 1) J(n). Equation (1.8) tells us that H(2n) = 2, and H(2n+1) = J(2n+2) J(2n+1) = (2J(n+1) 1) (2J(n)+1)
Διαβάστε περισσότεραExercise, May 23, 2016: Inflation stabilization with noisy data 1
Monetay Policy Henik Jensen Depatment of Economics Univesity of Copenhagen Execise May 23 2016: Inflation stabilization with noisy data 1 Suggested answes We have the basic model x t E t x t+1 σ 1 ît E
Διαβάστε περισσότεραNumerical Analysis FMN011
Numerical Analysis FMN011 Carmen Arévalo Lund University carmen@maths.lth.se Lecture 12 Periodic data A function g has period P if g(x + P ) = g(x) Model: Trigonometric polynomial of order M T M (x) =
Διαβάστε περισσότεραStrain gauge and rosettes
Strain gauge and rosettes Introduction A strain gauge is a device which is used to measure strain (deformation) on an object subjected to forces. Strain can be measured using various types of devices classified
Διαβάστε περισσότεραCHAPTER 101 FOURIER SERIES FOR PERIODIC FUNCTIONS OF PERIOD
CHAPTER FOURIER SERIES FOR PERIODIC FUNCTIONS OF PERIOD EXERCISE 36 Page 66. Determine the Fourier series for the periodic function: f(x), when x +, when x which is periodic outside this rge of period.
Διαβάστε περισσότεραSpace-Time Symmetries
Chapter Space-Time Symmetries In classical fiel theory any continuous symmetry of the action generates a conserve current by Noether's proceure. If the Lagrangian is not invariant but only shifts by a
Διαβάστε περισσότερα