Elastic Collisions. Chapter Center of Mass Frame
|
|
- Phebe Hardy
- 5 years ago
- Views:
Transcription
1 Chapter 11 Elastic Collisions 11.1 Center of Mass Frame A collision or scattering event is said to be elastic if it results in no change in the internal state of any of the particles involved. Thus, no internal energy is liberated or captured in an elastic process. Consider the elastic scattering of two particles. Recall the relation between laboratory coordinates {r 1,r 2 } and the CM and relative coordinates {R,r}: R = m 1 r 1 + r 2 r m 1 + m 1 = R + r ( m 1 + r = r 1 r 2 r 2 = R m 1 m 1 + r (11.2 If external forces are negligible, the CM momentum P = MṘ is constant, and therefore the frame of reference whose origin is tied to the CM position is an inertial frame of reference. In this frame, v1 CM = v, v CM 2 = m 1 v, (11.3 m 1 + m 1 + where v = v 1 v 2 = v CM 1 v CM 2 is the relative velocity, which is the same in both L and CM frames. Note that the CM momenta satisfy p CM 1 = m 1 v CM 1 = µv (11.4 p CM 2 = v CM 2 = µv, (11.5 where µ = m 1 /(m 1 + is the reduced mass. Thus, p CM 1 + p CM 2 = 0 and the total momentum in the CM frame is zero. We may then write p CM 1 p 0ˆn, p CM 2 p 0ˆn E CM = p2 0 2m 1 + p2 0 2 = p2 0 2µ. (11.6 1
2 2 CHAPTER 11. ELASTIC COLLISIONS Figure 11.1: The scattering of two hard spheres of radii a and b The scattering angle is χ. The energy is evaluated when the particles are asymptotically far from each other, in which case the potential energy is assumed to be negligible. After the collision, energy and momentum conservation require p 1CM p 0ˆn, p CM 2 p 0ˆn E CM = E CM = p2 0 2µ. (11.7 The angle between n and n is the scattering angle χ: n n cos χ. (11.8 The value of χ depends on the details of the scattering process, i.e. on the interaction potential U(r. As an example, consider the scattering of two hard spheres, depicted in Fig The potential is { if r a + b U(r = ( if r > a + b. Clearly the scattering angle is χ = π 2φ 0, where φ 0 is the angle between the initial momentum of either sphere and a line containing their two centers at the moment of contact. There is a simple geometric interpretation of these results, depicted in Fig We have p 1 = m 1 V + p 0ˆn p 1 = m 1 V + p 0ˆn (11.10 p 2 = V p 0ˆn p 2 = V p 0ˆn. (11.11 So draw a circle of radius p 0 whose center is the origin. The vectors p 0ˆn and p 0ˆn must both lie along this circle. We define the angle ψ between V and n: ˆV n = cos ψ. (11.12
3 11.1. CENTER OF MASS FRAME 3 Figure 11.2: Scattering of two particles of masses m 1 and. The scattering angle χ is the angle between ˆn and ˆn. It is now an exercise in geometry, using the law of cosines, to determine everything of interest in terms of the quantities V, v, ψ, and χ. For example, the momenta are p 1 = p 1 = p 2 = p 2 = 1 V 2 + µ 2 v 2 + 2m 1 µv v cos ψ ( V 2 + µ 2 v 2 + 2m 1 µv v cos(χ ψ ( V 2 + µ 2 v 2 2 µv v cos ψ ( V 2 + µ 2 v 2 2 µv v cos(χ ψ, (11.16 and the scattering angles are θ 1 = tan 1 ( ( µv sin ψ + tan 1 µv sin(χ ψ µv cos ψ + m 1 V µv cos(χ ψ + m 1 V (11.17 θ 2 = tan 1 ( ( µv sinψ + tan 1 µv sin(χ ψ µv cos ψ V µv cos(χ ψ V. (11.18
4 4 CHAPTER 11. ELASTIC COLLISIONS Figure 11.3: Scattering when particle 2 is initially at rest. If particle 2, say, is initially at rest, the situation is somewhat simpler. In this case, V = m 1 V /(m 1 + and V = µv, which means the point B lies on the circle in Fig (m 1 and Fig (m 1 =. Let ϑ 1,2 be the angles between the directions of motion after the collision and the direction V of impact. The scattering angle χ is the angle through which particle 1 turns in the CM frame. Clearly sin χ tan ϑ 1 = m 1 + cos χ We can also find the speeds v 1 and v 2 in terms of v and χ, from, ϑ 2 = 1 2 (π χ. (11.19 and These equations yield p 2 1 = p ( m 1 2 p 0 2 m 1 p 2 0 cos(π χ (11.20 p 2 2 = 2p2 0 (1 cos χ. (11.21 m v 1 2 = m 1 cos χ v, v 2 m 1 + m = 2m 1v sin( 1 2 m 1 + m 2χ. ( Figure 11.4: Scattering of identical mass particles when particle 2 is initially at rest.
5 11.2. CENTRAL FORCE SCATTERING 5 Figure 11.5: Repulsive (A,C and attractive (B,D scattering in the lab (A,B and CM (C,D frames, assuming particle 2 starts from rest in the lab frame. (From Barger and Olsson. The angle ϑ max from Fig. 11.3(b is given by sin ϑ max = m 1. Note that when m 1 = we have ϑ 1 + ϑ 2 = π. A sketch of the orbits in the cases of both repulsive and attractive scattering, in both the laboratory and CM frames, in shown in Fig Central Force Scattering Consider a single particle of mass µ movng in a central potential U(r, or a two body central force problem in which µ is the reduced mass. Recall that and therefore Solving for dr dφ, we obtain dr dt = dφ dt dr dφ = l µr 2 dr dφ, (11.23 E = 1 2 µṙ2 + l2 2µr 2 + U(r ( = l2 dr 2 2µr 4 + l2 + U(r. (11.24 dφ 2µr2 dr dφ = ± 2µr 4 l 2 ( E U(r r 2, (11.25
6 6 CHAPTER 11. ELASTIC COLLISIONS Figure 11.6: Scattering in the CM frame. O is the force center and P is the point of periapsis. The impact parameter is b, and χ is the scattering angle. φ 0 is the angle through which the relative coordinate moves between periapsis and infinity. Consulting Fig. 11.6, we have that φ 0 = l dr 2µ r 2 E U eff (r, (11.26 r p where r p is the radial distance at periapsis, and where U eff (r = l2 + U(r ( µr2 is the effective potential, as before. From Fig. 11.6, we conclude that the scattering angle is χ = π 2φ 0. (11.28 It is convenient to define the impact parameter b as the distance of the asymptotic trajectory from a parallel line containing the force center. The geometry is shown again in Fig Note that the energy and angular momentum, which are conserved, can be evaluated at infinity using the impact parameter: Substituting for l(b, we have E = 1 2 µv2, l = µv b. (11.29 φ 0 (E,b = r p dr r 2 b, ( b2 r U(r 2 E In physical applications, we are often interested in the deflection of a beam of incident particles by a scattering center. We define the differential scattering cross section dσ by dσ = # of particles scattered into solid angle per unit time incident flux. (11.31
7 11.2. CENTRAL FORCE SCATTERING 7 Figure 11.7: Geometry of hard sphere scattering. Now for particles of a given energy E there is a unique relationship between the scattering angle χ and the impact parameter b, as we have just derived in eqn The differential solid angle is given by = 2π sin χ dχ, hence dσ = b sinχ db dχ = d( 1 2 b2 dcos χ. (11.32 Note that dσ dσ has dimensions of area. The integral of over all solid angle is the total scattering cross section, σ T = 2π π 0 dχ sinχ dσ. ( Hard sphere scattering Consider a point particle scattering off a hard sphere of radius a, or two hard spheres of radii a 1 and a 2 scattering off each other, with a a 1 + a 2. From the geometry of Fig. 11.7, we have b = asin φ 0 and φ 0 = 1 2 (π χ, so b 2 = a 2 sin 2 ( 1 2 π 1 2 χ = 1 2 a2 (1 + cos χ. (11.34 We therefore have dσ = d(1 2 b2 dcos χ = 1 4 a2 (11.35 and σ T = πa 2. The total scattering cross section is simply the area of a sphere of radius a projected onto a plane perpendicular to the incident flux.
8 8 CHAPTER 11. ELASTIC COLLISIONS Rutherford scattering Consider scattering by the Kepler potential U(r = k r. We assume that the orbits are unbound, i.e. they are Keplerian hyperbolae with E > 0, described by the equation r(φ = a(ε2 1 ±1 + ε cos φ cos φ 0 = ± 1 ε. (11.36 Recall that the eccentricity is given by We then have ε 2 = 1 + 2El2 µk 2 = 1 + ( 2 µbv = ε 2 1 ( 2 µbv. (11.37 k Therefore We finally obtain k = sec 2 φ 0 1 = tan 2 φ 0 = ctn 2( 1 2 χ. (11.38 b(χ = k µv 2 ctn ( 1 2 χ (11.39 dσ = d(1 2 b2 dcos χ = 1 ( k 2 = 1 ( k 2 d 2 dcos χ µv 2 ( k = 2µv 2 µv 2 2 dctn 2( 1 2 χ dcos χ ( 1 + cos χ 1 cos χ 2 csc 4 ( 1 2 χ, (11.40 which is the same as ( dσ k 2 = csc 4 ( 1 4E 2 χ. (11.41 Since dσ χ 4 as χ 0, the total cross section σ T diverges! This is a consequence of the long-ranged nature of the Kepler/Coulomb potential. In electron-atom scattering, the Coulomb potential of the nucleus is screened by the electrons of the atom, and the 1/r behavior is cut off at large distances Transformation to laboratory coordinates We previously derived the relation tan ϑ = sin χ γ + cos χ, (11.42
9 11.2. CENTRAL FORCE SCATTERING 9 where ϑ ϑ 1 is the scattering angle for particle 1 in the laboratory frame, and γ = m 1 is the ratio of the masses. We now derive the differential scattering cross section in the laboratory frame. To do so, we note that particle conservation requires which says From ( dσ 2π sinϑdϑ = L ( dσ = L cos ϑ = = ( dσ ( dσ CM 2π sin χ dχ, (11.43 CM dcos χ dcos ϑ. ( tan 2 ϑ γ + cos χ 1 + γ 2 + 2γ cos χ, (11.45 we derive dcos ϑ dcos χ = 1 + γ cos χ ( 1 + γ 2 + 2γ cos χ 3/2 (11.46 and, accordingly, ( ( dσ 1 + γ 2 + 2γ cos χ 3/2 = L 1 + γ cos χ ( dσ. (11.47 CM
Elastic Scattering. R = m 1r 1 + m 2 r 2 m 1 + m 2. is the center of mass which is known to move with a constant velocity (see previous lectures):
Elastic Scattering In this section we will consider a problem of scattering of two particles obeying Newtonian mechanics. The problem of scattering can be viewed as a truncated version of dynamic problem
More informationI. Elastic collisions of 2 particles II. Relate ψ and θ III. Relate ψ and ζ IV. Kinematics of elastic collisions
I. Elastic collisions of particles II. Relate ψ and θ III. Relate ψ and ζ IV. Kinematics of elastic collisions 49 I. Elastic collisions of particles "Elastic": KE is conserved (as well as E tot and momentum
More information16. Elastic Scattering Michael Fowler
6 Elastic Scattering Michael Fowler Billiard Balls Elastic means no internal energy modes of the scatterer or of the scatteree are excited so total kinetic energy is conserved As a simple first exercise,
More informationChapter 8. Orbits. 8.1 Conics
Chapter 8 Orbits 8.1 Conics Conic sections first studied in the abstract by the Greeks are the curves formed by the intersection of a plane with a cone. Ignoring degenerate cases (such as a point, or pairs
More informationPhys 7221, Fall 2006: Midterm exam
Phys 7221, Fall 2006: Midterm exam October 20, 2006 Problem 1 (40 pts) Consider a spherical pendulum, a mass m attached to a rod of length l, as a constrained system with r = l, as shown in the figure.
More information8/31/2018. PHY 711 Classical Mechanics and Mathematical Methods 10-10:50 AM MWF Olin 103
PHY 7 Classical Mechanics and Mathematical Methods 0-0:50 AM MWF Olin 03 Plan for Lecture :. Brief comment on quiz. Particle interactions 3. Notion of center of mass reference fame 4. Introduction to scattering
More informationLecture: Scattering theory
Lecture: Scattering theory 30.05.2012 SS2012: Introduction to Nuclear and Particle Physics, Part 2 2 1 Part I: Scattering theory: Classical trajectoriest and cross-sections Quantum Scattering 2 I. Scattering
More informationLecture 6 Scattering theory Partial Wave Analysis. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2
Lecture 6 Scattering theory Partial Wave Analysis SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 1 The Born approximation for the differential cross section is valid if the interaction
More informationMassachusetts Institute of Technology Department of Physics. Final Examination December 17, 2004
Massachusetts Institute of Technology Department of Physics Course: 8.09 Classical Mechanics Term: Fall 004 Final Examination December 17, 004 Instructions Do not start until you are told to do so. Solve
More information5 Home exercise sheet
5 Home exercise sheet 5.1 The central force problem and Scattering Exercise 7.1: Yukawa potential The Yukawa potential is 1. Write down the effective potential. U(r) = αe χr r (1) 2. Sketch the effective
More informationThe Two -Body Central Force Problem
The Two -Body Central Force Problem Physics W3003 March 6, 2015 1 The setup 1.1 Formulation of problem The two-body central potential problem is defined by the (conserved) total energy E = 1 2 m 1Ṙ2 1
More informationPHY 5246: Theoretical Dynamics, Fall Assignment # 7, Solutions. Θ = π 2ψ, (1)
PHY 546: Theoretical Dynamics, Fall 05 Assignment # 7, Solutions Graded Problems Problem ψ ψ ψ Θ b (.a) The scattering angle satisfies the relation Θ π ψ, () where ψ is the angle between the direction
More informationIntroduction to Elementary Particle Physics I
Physics 56400 Introduction to Elementary Particle Physics I Lecture 2 Fall 2018 Semester Prof. Matthew Jones Cross Sections Reaction rate: R = L σ The cross section is proportional to the probability of
More informationUse conserved quantities to reduce number of variables and the equation of motion (EOM)
Physics 106a, Caltech 5 October, 018 Lecture 8: Central Forces Bound States Today we discuss the Kepler problem of the orbital motion of planets and other objects in the gravitational field of the sun.
More informationCentral Force Problem
Central Force Problem Consider two bodies of masses, say earth and moon, m E and m M moving under the influence of mutual gravitational force of potential V(r). Now Langangian of the system is where, µ
More informationConservation of Linear Momentum : If a force F is acting on particle of mass m, then according to Newton s second law of motion, we have F = dp /dt =
Conservation of Linear Momentum : If a force F is acting on particle of mass m, then according to Newton s second law of motion, we have F = dp /dt = d (mv) /dt where p =mv is linear momentum of particle
More informationPhysic 492 Lecture 16
Physic 492 Lecture 16 Main points of last lecture: Angular momentum dependence. Structure dependence. Nuclear reactions Q-values Kinematics for two body reactions. Main points of today s lecture: Measured
More informationVisit for more fantastic resources. AQA. A Level. A Level Physics. Particle physics (Answers) Name: Total Marks: /30
Visit http://www.mathsmadeeasy.co.uk/ for more fantastic resources. AQA A Level A Level Physics Particle physics (Answers) Name: Total Marks: /30 Maths Made Easy Complete Tuition Ltd 2017 1. Rutherford
More informationLecture 41: Highlights
Lecture 41: Highlights The goal of this lecture is to remind you of some of the key points that we ve covered this semester Note that this is not the complete set of topics that may appear on the final
More informationParticle collisions and decays
Particle collisions and decays Sourendu Gupta TIFR, Mumbai, India Classical Mechanics 2012 September 21, 2012 A particle decaying into two particles Assume that there is a reaction A B+C in which external
More informationClassical Scattering
Classical Scattering Daniele Colosi Mathematical Physics Seminar Daniele Colosi (IMATE) Classical Scattering 27.03.09 1 / 38 Contents 1 Generalities 2 Classical particle scattering Scattering cross sections
More informationApplied Nuclear Physics (Fall 2006) Lecture 19 (11/22/06) Gamma Interactions: Compton Scattering
.101 Applied Nuclear Physics (Fall 006) Lecture 19 (11//06) Gamma Interactions: Compton Scattering References: R. D. Evans, Atomic Nucleus (McGraw-Hill New York, 1955), Chaps 3 5.. W. E. Meyerhof, Elements
More information10. Scattering from Central Force Potential
University of Rhode Island DigitalCommons@URI Classical Dynamics Physics Course Materials 215 1. Scattering from Central Force Potential Gerhard Müller University of Rhode Island, gmuller@uri.edu Creative
More informationRutherford Backscattering Spectrometry
Rutherford Backscattering Spectrometry EMSE-515 Fall 2005 F. Ernst 1 Bohr s Model of an Atom existence of central core established by single collision, large-angle scattering of alpha particles ( 4 He
More informationCelestial Mechanics Lecture 10
Celestial Mechanics Lecture 10 ˆ This is the first of two topics which I have added to the curriculum for this term. ˆ We have a surprizing amount of firepower at our disposal to analyze some basic problems
More information4.3 TRIGONOMETRY EXTENDED: THE CIRCULAR FUNCTIONS
4.3 TRIGONOMETRY EXTENDED: THE CIRCULAR FUNCTIONS MR. FORTIER 1. Trig Functions of Any Angle We now extend the definitions of the six basic trig functions beyond triangles so that we do not have to restrict
More informationChapter 6. Quantum Theory of the Hydrogen Atom
Chapter 6 Quantum Theory of the Hydrogen Atom 1 6.1 Schrodinger s Equation for the Hydrogen Atom Symmetry suggests spherical polar coordinates Fig. 6.1 (a) Spherical polar coordinates. (b) A line of constant
More informationThe first order formalism and the transition to the
Problem 1. Hamiltonian The first order formalism and the transition to the This problem uses the notion of Lagrange multipliers and Legendre transforms to understand the action in the Hamiltonian formalism.
More informationQuantum Mechanics II Lecture 11 (www.sp.phy.cam.ac.uk/~dar11/pdf) David Ritchie
Quantum Mechanics II Lecture (www.sp.phy.cam.ac.u/~dar/pdf) David Ritchie Michaelmas. So far we have found solutions to Section 4:Transitions Ĥ ψ Eψ Solutions stationary states time dependence with time
More informationRutherford Scattering Made Simple
Rutherford Scattering Made Simple Chung-Sang Ng Physics Department, Auburn University, Auburn, AL 36849 (November 19, 1993) Rutherford scattering experiment 1 is so important that it is seldom not mentioned
More informationLet b be the distance of closest approach between the trajectory of the center of the moving ball and the center of the stationary one.
Scattering Classical model As a model for the classical approach to collision, consider the case of a billiard ball colliding with a stationary one. The scattering direction quite clearly depends rather
More informationLong range interaction --- between ions/electrons and ions/electrons; Coulomb 1/r Intermediate range interaction --- between
Collisional Processes Long range interaction --- between ions/electrons and ions/electrons; Coulomb 1/r Intermediate range interaction --- between ions/electrons and neutral atoms/molecules; Induced dipole
More informationCompound and heavy-ion reactions
Compound and heavy-ion reactions Introduction to Nuclear Science Simon Fraser University Spring 2011 NUCS 342 March 23, 2011 NUCS 342 (Lecture 24) March 23, 2011 1 / 32 Outline 1 Density of states in a
More informationThoughts concerning on-orbit injection of calibration electrons through thin-target elastic scattering inside the Mu2e solenoid
Thoughts concerning on-orbit injection of calibration electrons through thin-target elastic tering inside the Mue solenoid George Gollin a Department of Physics University of Illinois at Urbana-Champaign
More informationQualifying Exam. Aug Part II. Please use blank paper for your work do not write on problems sheets!
Qualifying Exam Aug. 2015 Part II Please use blank paper for your work do not write on problems sheets! Solve only one problem from each of the four sections Mechanics, Quantum Mechanics, Statistical Physics
More informationQUALIFYING EXAMINATION, Part 1. Solutions. Problem 1: Mathematical Methods. r r r 2 r r2 = 0 r 2. d 3 r. t 0 e t dt = e t
QUALIFYING EXAMINATION, Part 1 Solutions Problem 1: Mathematical Methods (a) For r > we find 2 ( 1 r ) = 1 ( ) 1 r 2 r r2 = 1 ( 1 ) r r r 2 r r2 = r 2 However for r = we get 1 because of the factor in
More information3.1 Reduction to a one dimensional problem
Chapter 3 Two Body Central Forces Consider two particles of masses m 1 and m 2, with the only forces those of their mutual interaction, which we assume is given by a potential which is a function only
More informationWhy Does Uranium Alpha Decay?
Why Does Uranium Alpha Decay? Consider the alpha decay shown below where a uranium nucleus spontaneously breaks apart into a 4 He or alpha particle and 234 90 Th. 238 92U 4 He + 234 90Th E( 4 He) = 4.2
More information5.62 Physical Chemistry II Spring 2008
MIT OpenCourseWare http://ocw.mit.edu 5.6 Physical Chemistry II Spring 008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 5.6 Spring 008 Lecture #30
More informationAPPLICATIONS. CEE 271: Applied Mechanics II, Dynamics Lecture 17: Ch.15, Sec.4 7. IMPACT (Section 15.4) APPLICATIONS (continued) IMPACT READING QUIZ
APPLICATIONS CEE 271: Applied Mechanics II, Dynamics Lecture 17: Ch.15, Sec.4 7 Prof. Albert S. Kim Civil and Environmental Engineering, University of Hawaii at Manoa Date: The quality of a tennis ball
More informationChapter 10: QUANTUM SCATTERING
Chapter : QUANTUM SCATTERING Scattering is an extremely important tool to investigate particle structures and the interaction between the target particle and the scattering particle. For example, Rutherford
More informationLecture 5 Scattering theory, Born Approximation. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2
Lecture 5 Scattering theory, Born Approximation SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 1 Scattering amplitude We are going to show here that we can obtain the differential cross
More information221B Lecture Notes Scattering Theory II
22B Lecture Notes Scattering Theory II Born Approximation Lippmann Schwinger equation ψ = φ + V ψ, () E H 0 + iɛ is an exact equation for the scattering problem, but it still is an equation to be solved
More informationPhysics Dec The Maxwell Velocity Distribution
Physics 301 7-Dec-2005 29-1 The Maxwell Velocity Distribution The beginning of chapter 14 covers some things we ve already discussed. Way back in lecture 6, we calculated the pressure for an ideal gas
More informationA space probe to Jupiter
Problem 3 Page 1 Problem 3 A space probe to Jupiter We consider in this problem a method frequently used to accelerate space probes in the desired direction. The space probe flies by a planet, and can
More informationAstromechanics. 10. The Kepler Problem
Astromechanics 10. The Kepler Problem One of the fundamental problems in astromechanics is the Kepler problem The Kepler problem is stated as follows: Given the current position a velocity vectors and
More informationAtomic Models the Nucleus
Atomic Models the Nucleus Rutherford (read his bio on pp 134-5), who had already won a Nobel for his work on radioactivity had also named alpha, beta, gamma radiation, developed a scattering technique
More information64 CHAPTER 2. LAGRANGE S AND HAMILTON S EQUATIONS
.7. VELOCITY-DEPENDENT FORCES 63 64 CHAPTER. LAGRANGE S AND HAMILTON S EQUATIONS dl = dr r + ω r /c dφ, because their metersticks shrink in the tangential direction and it takes more of them to cover the
More informationLecture 10. Central potential
Lecture 10 Central potential 89 90 LECTURE 10. CENTRAL POTENTIAL 10.1 Introduction We are now ready to study a generic class of three-dimensional physical systems. They are the systems that have a central
More informationThe Elastic Pi Problem
The Elastic Pi Problem Jacob Bien August 8, 010 1 The problem Two balls of mass m 1 and m are beside a wall. Mass m 1 is positioned between m and the wall and is at rest. Mass m is moving with velocity
More information!! r r θ! 2 r!φ 2 sinθ = GM / r 2 r!! θ + 2!r θ! r!φ 2 sinθ cosθ = 0 r!! φ sinθ + 2r θ!!φ cosθ + 2!r!φ sinθ = 0
Phys 325 Lecture 9 Tuesday 12 February, 2019 NB Midterm next Thursday 2/21. Sample exam will be posted soon Formula sheet on sample exam will be same as formula sheet on actual exam You will be permitted
More informationStellar Dynamics and Structure of Galaxies
Stellar Dynamics and Structure of Galaxies in a given potential Vasily Belokurov vasily@ast.cam.ac.uk Institute of Astronomy Lent Term 2016 1 / 59 1 Collisions Model requirements 2 in spherical 3 4 Orbital
More informationWelcome back to PHY 3305
Welcome back to PHY 3305 Today s Lecture: Hydrogen Atom Part I John von Neumann 1903-1957 One-Dimensional Atom To analyze the hydrogen atom, we must solve the Schrodinger equation for the Coulomb potential
More informationLecture 21 Gravitational and Central Forces
Lecture 21 Gravitational and Central Forces 21.1 Newton s Law of Universal Gravitation According to Newton s Law of Universal Graviation, the force on a particle i of mass m i exerted by a particle j of
More information1 Schroenger s Equation for the Hydrogen Atom
Schroenger s Equation for the Hydrogen Atom Here is the Schroedinger equation in D in spherical polar coordinates. Note that the definitions of θ and φ are the exact reverse of what they are in mathematics.
More informationThe two body problem involves a pair of particles with masses m 1 and m 2 described by a Lagrangian of the form:
Physics 3550, Fall 2011 Two Body, Central-Force Problem Relevant Sections in Text: 8.1 8.7 Two Body, Central-Force Problem Introduction. I have already mentioned the two body central force problem several
More informationUniversal Gravitation
Universal Gravitation Newton s Law of Universal Gravitation Every particle in the Universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely
More informationDIFFERENTIATION RULES
3 DIFFERENTIATION RULES DIFFERENTIATION RULES Before starting this section, you might need to review the trigonometric functions. DIFFERENTIATION RULES In particular, it is important to remember that,
More informationISIMA lectures on celestial mechanics. 1
ISIMA lectures on celestial mechanics. 1 Scott Tremaine, Institute for Advanced Study July 2014 The roots of solar system dynamics can be traced to two fundamental discoveries by Isaac Newton: first, that
More informationWe now turn to our first quantum mechanical problems that represent real, as
84 Lectures 16-17 We now turn to our first quantum mechanical problems that represent real, as opposed to idealized, systems. These problems are the structures of atoms. We will begin first with hydrogen-like
More informationfor changing independent variables. Most simply for a function f(x) the Legendre transformation f(x) B(s) takes the form B(s) = xs f(x) with s = df
Physics 106a, Caltech 1 November, 2018 Lecture 10: Hamiltonian Mechanics I The Hamiltonian In the Hamiltonian formulation of dynamics each second order ODE given by the Euler- Lagrange equation in terms
More informationComparative study of scattering by hard core and absorptive potential
6 Comparative study of scattering by hard core and absorptive potential Quantum scattering in three dimension by a hard sphere and complex potential are important in collision theory to study the nuclear
More informationOrbit Characteristics
Orbit Characteristics We have shown that the in the two body problem, the orbit of the satellite about the primary (or vice-versa) is a conic section, with the primary located at the focus of the conic
More informationChapter 3-Elastic Scattering Small-Angle, Elastic Scattering from Atoms Head-On Elastic Collision in 1-D
1 Chapter 3-Elastic Scattering Small-Angle, Elastic Scattering from Atoms To understand the basics mechanisms for the scattering of high-energy electrons off of stationary atoms, it is sufficient to picture
More informationCentral Forces. c 2007 Corinne Manogue. March 1999, last revised February 2009
Central Forces Corinne A. Manogue with Tevian Dray, Kenneth S. Krane, Jason Janesky Department of Physics Oregon State University Corvallis, OR 97331, USA corinne@physics.oregonstate.edu c 2007 Corinne
More informationQuantum Physics III (8.06) Spring 2005 Assignment 9
Quantum Physics III (8.06) Spring 2005 Assignment 9 April 21, 2005 Due FRIDAY April 29, 2005 Readings Your reading assignment on scattering, which is the subject of this Problem Set and much of Problem
More informationQuantum Physics III (8.06) Spring 2008 Assignment 10
May 5, 2008 Quantum Physics III (8.06) Spring 2008 Assignment 10 You do not need to hand this pset in. The solutions will be provided after Friday May 9th. Your FINAL EXAM is MONDAY MAY 19, 1:30PM-4:30PM,
More informationUniversity of Alberta
Valeri P. Frolov University of Alberta Based on: V.F. & A.Shoom, Phys.Rev.D82: 084034 (2010); V.F., Phys.Rev. D85: 024020 (2012); A.M. Al Zahrani, V.F. & A.Shoom, D87: 084043 (2013) 27th Texas Symposium,
More informationThe Calculus of Vec- tors
Physics 2460 Electricity and Magnetism I, Fall 2007, Lecture 3 1 The Calculus of Vec- Summary: tors 1. Calculus of Vectors: Limits and Derivatives 2. Parametric representation of Curves r(t) = [x(t), y(t),
More informationDecays and Scattering. Decay Rates Cross Sections Calculating Decays Scattering Lifetime of Particles
Decays and Scattering Decay Rates Cross Sections Calculating Decays Scattering Lifetime of Particles 1 Decay Rates There are THREE experimental probes of Elementary Particle Interactions - bound states
More informationLecture 22 Highlights Phys 402
Lecture 22 Highlights Phys 402 Scattering experiments are one of the most important ways to gain an understanding of the microscopic world that is described by quantum mechanics. The idea is to take a
More informationAtomic Collisions and Backscattering Spectrometry
2 Atomic Collisions and Backscattering Spectrometry 2.1 Introduction The model of the atom is that of a cloud of electrons surrounding a positively charged central core the nucleus that contains Z protons
More informationCHEM-UA 127: Advanced General Chemistry I
1 CHEM-UA 127: Advanced General Chemistry I Notes for Lecture 11 Nowthatwehaveintroducedthebasicconceptsofquantummechanics, wecanstarttoapplythese conceptsto build up matter, starting from its most elementary
More informationQuestion 1: Spherical Pendulum
Question 1: Spherical Pendulum Consider a two-dimensional pendulum of length l with mass M at its end. It is easiest to use spherical coordinates centered at the pivot since the magnitude of the position
More informationSome history. F p. 1/??
Some history F 12 10 18 p. 1/?? F 12 10 18 p. 1/?? Some history 1600: Galileo Galilei 1564 1642 cf. section 7.0 Johannes Kepler 1571 1630 cf. section 3.7 1700: Isaac Newton 1643 1727 cf. section 1.1 1750
More informationParticles and Fields
Particles and Fields J.W. van Holten NIKHEF Amsterdam NL and Physics Department Leiden University Leiden NL c 1. Atoms Atoms are the smallest electrically neutral units of chemical elements. They consist
More informationFLUX OF VECTOR FIELD INTRODUCTION
Chapter 3 GAUSS LAW ntroduction Flux of vector field Solid angle Gauss s Law Symmetry Spherical symmetry Cylindrical symmetry Plane symmetry Superposition of symmetric geometries Motion of point charges
More informationfrom which follow by application of chain rule relations y = y (4) ˆL z = i h by constructing θ , find also ˆL x ˆL y and
9 Scattering Theory II 9.1 Partial wave analysis Expand ψ in spherical harmonics Y lm (θ, φ), derive 1D differential equations for expansion coefficients. Spherical coordinates: x = r sin θ cos φ (1) y
More information1.6. Quantum mechanical description of the hydrogen atom
29.6. Quantum mechanical description of the hydrogen atom.6.. Hamiltonian for the hydrogen atom Atomic units To avoid dealing with very small numbers, let us introduce the so called atomic units : Quantity
More informationModern Physics. Unit 6: Hydrogen Atom - Radiation Lecture 6.3: Vector Model of Angular Momentum
Modern Physics Unit 6: Hydrogen Atom - Radiation ecture 6.3: Vector Model of Angular Momentum Ron Reifenberger Professor of Physics Purdue University 1 Summary of Important Points from ast ecture The magnitude
More informationOrbital Mechanics! Space System Design, MAE 342, Princeton University! Robert Stengel
Orbital Mechanics Space System Design, MAE 342, Princeton University Robert Stengel Conic section orbits Equations of motion Momentum and energy Kepler s Equation Position and velocity in orbit Copyright
More informationPractice Test - Chapter 4
Find the value of x. Round to the nearest tenth, if necessary. Find the measure of angle θ. Round to the nearest degree, if necessary. 1. An acute angle measure and the length of the hypotenuse are given,
More informationLecture 3. Solving the Non-Relativistic Schroedinger Equation for a spherically symmetric potential
Lecture 3 Last lecture we were in the middle of deriving the energies of the bound states of the Λ in the nucleus. We will continue with solving the non-relativistic Schroedinger equation for a spherically
More informationAlgebraic Analysis Approach for Multibody Problems
Algebraic Analysis Approach for Multibody Problems Shun-ichi OIKAWA and Hideo FUNASAKA Graduate School of Engineering, Hokkaido University, N-13, W-8, Sapporo 6-8628, Japan (Received 15 November 27 / Accepted
More informationChapter 13. Gravitation
Chapter 13 Gravitation e = c/a A note about eccentricity For a circle c = 0 à e = 0 a Orbit Examples Mercury has the highest eccentricity of any planet (a) e Mercury = 0.21 Halley s comet has an orbit
More informationMATH H53 : Mid-Term-1
MATH H53 : Mid-Term-1 22nd September, 215 Name: You have 8 minutes to answer the questions. Use of calculators or study materials including textbooks, notes etc. is not permitted. Answer the questions
More informationUniversity of Oslo. Department of Physics. Interaction Between Ionizing Radiation And Matter, Part 2 Charged-Particles.
Interaction Between Ionizing Radiation And Matter, Part Charged-Particles Audun Sanderud Excitation / ionization Incoming charged particle interact with atom/molecule: Ionization Excitation Ion pair created
More information2. Determine the domain of the function. Verify your result with a graph. f(x) = 25 x 2
29 April PreCalculus Final Review 1. Find the slope and y-intercept (if possible) of the equation of the line. Sketch the line: y = 3x + 13 2. Determine the domain of the function. Verify your result with
More informationFebruary 18, In the parallel RLC circuit shown, R = Ω, L = mh and C = µf. The source has V 0. = 20.0 V and f = Hz.
Physics Qualifying Examination Part I 7- Minute Questions February 18, 2012 1. In the parallel RLC circuit shown, R = 800.0 Ω, L = 160.0 mh and C = 0.0600 µf. The source has V 0 = 20.0 V and f = 2400.0
More information5.61 Lecture #17 Rigid Rotor I
561 Fall 2017 Lecture #17 Page 1 561 Lecture #17 Rigid Rotor I Read McQuarrie: Chapters E and 6 Rigid Rotors molecular rotation and the universal angular part of all central force problems another exactly
More informationPhysics 351, Spring 2015, Final Exam.
Physics 351, Spring 2015, Final Exam. This closed-book exam has (only) 25% weight in your course grade. You can use one sheet of your own hand-written notes. Please show your work on these pages. The back
More informationThe Kepler Problem and the Isotropic Harmonic Oscillator. M. K. Fung
CHINESE JOURNAL OF PHYSICS VOL. 50, NO. 5 October 01 The Kepler Problem and the Isotropic Harmonic Oscillator M. K. Fung Department of Physics, National Taiwan Normal University, Taipei, Taiwan 116, R.O.C.
More information7 Kinematics and kinetics of planar rigid bodies II
7 Kinematics and kinetics of planar rigid bodies II 7.1 In-class A rigid circular cylinder of radius a and length h has a hole of radius 0.5a cut out. The density of the cylinder is ρ. Assume that the
More informationThe Hydrogen Atom. Chapter 18. P. J. Grandinetti. Nov 6, Chem P. J. Grandinetti (Chem. 4300) The Hydrogen Atom Nov 6, / 41
The Hydrogen Atom Chapter 18 P. J. Grandinetti Chem. 4300 Nov 6, 2017 P. J. Grandinetti (Chem. 4300) The Hydrogen Atom Nov 6, 2017 1 / 41 The Hydrogen Atom Hydrogen atom is simplest atomic system where
More information1. Kinematics, cross-sections etc
1. Kinematics, cross-sections etc A study of kinematics is of great importance to any experiment on particle scattering. It is necessary to interpret your measurements, but at an earlier stage to determine
More informationAy 20: Basic Astronomy and the Galaxy Fall Term Solution Set 4 Kunal Mooley (based on solutions by Swarnima Manohar, TA 2009)
Ay 20: Basic Astronomy and the Galaxy Fall Term 2010 Solution Set 4 Kunal Mooley (based on solutions by Swarnima Manohar, TA 2009) Reporting an answer to unnecesary number of decimal places should be avoided.
More informationScattering Theory. Two ways of stating the scattering problem. Rate vs. cross-section
Scattering Theory Two ways of stating the scattering problem. Rate vs. cross-section The first way to formulate the quantum-mechanical scattering problem is semi-classical: It deals with (i) wave packets
More informationFigure 1: Volume of Interaction for Air Molecules
Problem In 866 when atoms and molecules were still quite hypothetical, Joseph Loschmidt used kinetic energy theory to get the first reasonable estimate of molecular size. He used the liquid to gas expansion
More informationPhysics 221A Fall 1996 Notes 12 Orbital Angular Momentum and Spherical Harmonics
Physics 221A Fall 1996 Notes 12 Orbital Angular Momentum and Spherical Harmonics We now consider the spatial degrees of freedom of a particle moving in 3-dimensional space, which of course is an important
More informationScattering. March 20, 2016
Scattering March 0, 06 The scattering of waves of any kind, by a compact object, has applications on all scales, from the scattering of light from the early universe by intervening galaxies, to the scattering
More information