Chapter 5 Page 5.1 CHAPTER 5. r Force times distance has units of energy. Therefore, fxr=u, or f / is dimensionless.

Similar documents
PHYS 2135 Exam I February 13, 2018

Chem 453/544 Fall /08/03. Exam #1 Solutions

1 2 U CV. K dq I dt J nqv d J V IR P VI

[Griffiths Ch.1-3] 2008/11/18, 10:10am 12:00am, 1. (6%, 7%, 7%) Suppose the potential at the surface of a hollow hemisphere is specified, as shown

Ab Initio Calculations of Intermolecular Interactions. calculating dispersion energies is hard; (BSSE)

The geometric construction of Ewald sphere and Bragg condition:

Electromagnetism Physics 15b

Physics 107 TUTORIAL ASSIGNMENT #8

Physics Fall Mechanics, Thermodynamics, Waves, Fluids. Lecture 18: System of Particles II. Slide 18-1

Physics 11 Chapter 20: Electric Fields and Forces

Extra notes for circular motion: Circular motion : v keeps changing, maybe both speed and

PHYS 1441 Section 002. Lecture #3

MODULE 5a and 5b (Stewart, Sections 12.2, 12.3) INTRO: In MATH 1114 vectors were written either as rows (a1, a2,..., an) or as columns a 1 a. ...

Physics 121 Hour Exam #5 Solution

CHAPTER 25 ELECTRIC POTENTIAL

Central Force Problem. Central Force Motion. Two Body Problem: Center of Mass Coordinates. Reduction of Two Body Problem 8.01 W14D1. + m 2. m 2.

Qualifying Examination Electricity and Magnetism Solutions January 12, 2006

Diffusion and Transport. 10. Friction and the Langevin Equation. Langevin Equation. f d. f ext. f () t f () t. Then Newton s second law is ma f f f t.

MAGNETIC FIELD INTRODUCTION

2. Electrostatics. Dr. Rakhesh Singh Kshetrimayum 8/11/ Electromagnetic Field Theory by R. S. Kshetrimayum

Preliminary Exam: Quantum Physics 1/14/2011, 9:00-3:00

Electrostatics (Electric Charges and Field) #2 2010

Central Force Motion

Gravitation. AP/Honors Physics 1 Mr. Velazquez

$ i. !((( dv vol. Physics 8.02 Quiz One Equations Fall q 1 q 2 r 2 C = 2 C! V 2 = Q 2 2C F = 4!" or. r ˆ = points from source q to observer

Magnetic Dipoles Challenge Problem Solutions

Physics 2212 GH Quiz #2 Solutions Spring 2016

PART- A 1. (C) 2. (D) 3. (D) 4. (B) 5. (D) 6. (C) 7. (D) 8. (B) 9. (D) 10. (B) 11. (B) 12. (B) 13. (A) 14. (D)

EN40: Dynamics and Vibrations. Midterm Examination Thursday March

11) A thin, uniform rod of mass M is supported by two vertical strings, as shown below.


F(r) = r f (r) 4.8. Central forces The most interesting problems in classical mechanics are about central forces.

PHYS 1444 Lecture #5

Flux. Area Vector. Flux of Electric Field. Gauss s Law

Chapter 4. Newton s Laws of Motion

7.2. Coulomb s Law. The Electric Force

Physics 235 Chapter 5. Chapter 5 Gravitation

PES 3950/PHYS 6950: Homework Assignment 6

21 MAGNETIC FORCES AND MAGNETIC FIELDS

Solutions. V in = ρ 0. r 2 + a r 2 + b, where a and b are constants. The potential at the center of the atom has to be finite, so a = 0. r 2 + b.

PHYS 1444 Section 501 Lecture #7

Chapter 22: Electric Fields. 22-1: What is physics? General physics II (22102) Dr. Iyad SAADEDDIN. 22-2: The Electric Field (E)

Chapter 13 Gravitation

arxiv: v1 [physics.pop-ph] 3 Jun 2013

PH126 Exam I Solutions

INTRODUCTION. 2. Vectors in Physics 1

Non-Linear Dynamics Homework Solutions Week 2

ELECTRIC CHARGE AND ELECTRIC FIELD

Rigid Body Dynamics 2. CSE169: Computer Animation Instructor: Steve Rotenberg UCSD, Winter 2018

(Sample 3) Exam 1 - Physics Patel SPRING 1998 FORM CODE - A (solution key at end of exam)

Tutorial Exercises: Central Forces

Physics Courseware Physics II Electric Field and Force

16.1 Permanent magnets

1 Fundamental Solutions to the Wave Equation

Momentum is conserved if no external force

Chapters 5-8. Dynamics: Applying Newton s Laws

Solutions to Problems : Chapter 19 Problems appeared on the end of chapter 19 of the Textbook

Electrostatics. 1. Show does the force between two point charges change if the dielectric constant of the medium in which they are kept increase?

So, if we are finding the amount of work done over a non-conservative vector field F r, we do that long ur r b ur =

Many Electron Atoms. Electrons can be put into approximate orbitals and the properties of the many electron systems can be catalogued

Physics Courseware Electromagnetism

Magnetic Field. Conference 6. Physics 102 General Physics II

Chapter 7-8 Rotational Motion

to point uphill and to be equal to its maximum value, in which case f s, max = μsfn

Physics 2A Chapter 10 - Moment of Inertia Fall 2018

Internet Appendix for A Bayesian Approach to Real Options: The Case of Distinguishing Between Temporary and Permanent Shocks

When two numbers are written as the product of their prime factors, they are in factored form.

Chapter 2: Basic Physics and Math Supplements

c) (6) Assuming the tires do not skid, what coefficient of static friction between tires and pavement is needed?

b) (5) What average force magnitude was applied by the students working together?

OSCILLATIONS AND GRAVITATION

Section 8.2 Polar Coordinates

1 Spherical multipole moments

ECE 6340 Intermediate EM Waves. Fall Prof. David R. Jackson Dept. of ECE. Notes 4

Question 1: The dipole

Physics 111. Ch 12: Gravity. Newton s Universal Gravity. R - hat. the equation. = Gm 1 m 2. F g 2 1. ˆr 2 1. Gravity G =

A thermodynamic degree of freedom solution to the galaxy cluster problem of MOND. Abstract

EM-2. 1 Coulomb s law, electric field, potential field, superposition q. Electric field of a point charge (1)

Universal Gravitation

KEPLER S LAWS OF PLANETARY MOTION

How Electric Currents Interact with Magnetic Fields

working pages for Paul Richards class notes; do not copy or circulate without permission from PGR 2004/11/3 10:50

Circular Motion & Torque Test Review. The period is the amount of time it takes for an object to travel around a circular path once.

KEPLER S LAWS AND PLANETARY ORBITS

(r) = 1. Example: Electric Potential Energy. Summary. Potential due to a Group of Point Charges 9/10/12 1 R V(r) + + V(r) kq. Chapter 23.

11.2. Area of a Circle. Lesson Objective. Derive the formula for the area of a circle.

Chapter 10 Sample Exam

Mechanics and Special Relativity (MAPH10030) Assignment 3

Physics 2B Chapter 22 Notes - Magnetic Field Spring 2018

THE LAPLACE EQUATION. The Laplace (or potential) equation is the equation. u = 0. = 2 x 2. x y 2 in R 2

School of Electrical and Computer Engineering, Cornell University. ECE 303: Electromagnetic Fields and Waves. Fall 2007

Introduction: Vectors and Integrals

Physics 161 Fall 2011 Extra Credit 2 Investigating Black Holes - Solutions The Following is Worth 50 Points!!!

Objects usually are charged up through the transfer of electrons from one object to the other.

Chapter. s r. check whether your calculator is in all other parts of the body. When a rigid body rotates through a given angle, all

CHAPTER 10 ELECTRIC POTENTIAL AND CAPACITANCE

Phys 201A. Homework 6 Solutions. F A and F r. B. According to Newton s second law, ( ) ( )2. j = ( 6.0 m / s 2 )ˆ i ( 10.4m / s 2 )ˆ j.

Physics 505 Homework No. 9 Solutions S9-1

Physics 1114: Unit 5 Hand-out Homework (Answers)

A moving charged particle creates a magnetic field vector at every point in space except at its position.

Transcription:

Chapte 5 Page 5.1 CHAPTER 5 Poblem 5.1: 1 (a) u () 4 0.90.93 3.0 (b) Foce times distance has units of enegy. Theefoe, fx=u, o f/ is dimensionless. d f = d u 1 d f 4ε 1 = f = 4 ε1 d 13 f = 4 ε 1 f ε = 4 1 7 Now in dimensionless fom: 13 7 f() 4 3 u () 1 f() 0 1 3 0 1 3 4 (c) f d = x Newton's nd law in dimensionless fom. Using dimensional analysis we find dt that dimensionless t is given by (m/. Theefoe, the dimensionless foce can be witten as shown. d x = dt 4 x 1 x x IC1: t = 0 x =.5 IC: t = 0 d dt x = 0 initial conditions

Chapte 5 Page 5. Rough phase-space sketch of what the solution would look like. Poblem 5.: 1 u() 4 d d u Thus, u min 13 7 = 48 4= 0 at the minimum in the potential 1 1 13 7 = o min min 1.1 4 Initialize to find oot 1 esult oot.5.001 esult 3.984 Poblem 5.3: Let D be the distance at which the potential enegy becomes equal to the kinetic enegy and the diection of the colliding atoms ae evesed. Let x = (/D). 4ε x x = kt x x We can solve this with the quadatic fomula: kt = 0 4ε 1 1 x = kt ε We have chosen the + sign because x must be positive and the squae oot tem is always seen to be geate than unity.

Chapte 5 Page 5.3 Thus, kt 1 1 ε = x = o D 1 1 = D 1 1 kt and D 1 = 1 Fo A, 3.49 ε kt ε ε k 1 = 11.85 DT ( ) 3.849 1 0.0081T 1 1 T 00 400 The vaiation of the diamete with tempeatue looks like the figue shown at the ight. Notice that at highe tempeatues, thee is lage penetation coesponding to smalle had-sphee diametes. The value is the had sphee value only at 0 K whee no penetation into the epulsive coe occus. 3.5 3.4 DT ( ) 3.3 3. 3.1 0 100 00 300 400 Poblem 5.4: Fom Table A5.5 fo wate k 1.38010 1 eg debye 10 18 egcm 3 K T 3 0.5 o 3.3910 8 cm ε o 09.1kK μ 1.85debye α 1.49 10 8 cm T 300K 1 4ε o 1 μ 4 1 αμ 1 u LJ () 10 1 u D () 3k T eg o 10 1 u P () eg o 10 1 eg u tot () u LJ () u D () u P () 0.90.95 3 800 Note that the potentials plotted ae in units of 10-1 egs u LJ () u D () u P () 400 0 u tot () 400 Poblem 5.5: 800 0 1 3

Chapte 5 Page 5.4 Fom Appendix 5 we have the following values fo methane: LJ Kihaa Sutheland SW ε LJ 1.78k d 0.77 S 3.94 SW 3.40 LJ 3.78 K 3.505 ε S 434.8k ε SW 88.8k ε K 3.k g 1.85 Poblem 5.: ε k = ATc 3 = Bk Tc Pc FLUID (A) Tc (K) Pc (atm) A 11.85 3.49 150.8 48.1 K 174.8 3.84 09.4 54.3 CH 4 1.78 3.78 190. 45.4 Xe 4.83 4.07 89.7 57. C H 74.48 4.1 305.4 48. ε 3 Pc A = B = Note: A and B ae both dimensionless. To make units in ktc ktc equation fo B compatible, use the following convesion facto:

Chapte 5 Page 5.5 1.013510 conv 10 4 cm 3 conv 7.337 10 3 K atm eg cm 3 atm 1 1.38110 1 eg K FLUID A=/(kTc) B=(conv)( 3 )/T c A 0.808 0.094 K 0.834 0.095 CH 4 0.875 0.087 Xe 0.77 0.098 C H 0.898 0.087 Thus, ε = k 0.84Tc Aveage 0.84 0.09 3 = 0.09 ktc Pc Poblem 5.7: 1 PV NkT Fi = 3 i Note: we'll use an oveba to indicate expectation value i a d u () = f() = d u () a o f() = Fi = F cosθ but because these ae centic foces, = 0 and cos = 1 i Fi a = i Fo lage N, we may eplace the sum with an integal. i i i Now, the numbe of molecules located between and + d fom any given molecule is: N () = 4π ρ() but we have N - 1 molecules that we can choose as the efeence. Thus, pais = ( N 1) 4π ρ() Howeve, this double counts each pai. We divide by to get the numbe of unique pais. Again, in the limit as N becomes lage N - 1 = N and the summation in the viial can be eplaced by an integal. We then find the expectation value in the usual way: a = i i 0 a N π exp β a V πa N βa d = exp V 0 d

Chapte 5 Page 5. a πa N 1 π( Nk T) = i V i ( βa) = Va πnkt Finally, PV = NkT1 3 av Poblem 5.8: μ 1.0810 18 Q 3.810 fo HCl sinθ A f 1 θ A θ B ϕ sinθ B cos( ϕ) cos θ A cosθ B f θ A θ B ϕ f 3 θ A θ B ϕ d 10 7 cm 3 cos θ A3cosθ B cosθ B 1 sinθ A sinθ B cosθ B cos( ϕ) 3 4 1 5 cos θ A 5cosθ B 15 cosθ A cosθ B 4cosθ A cosθ B sinθ A sinθ B cos( ϕ) (a) f 1 ( 0π 0 ) f ( 0π 0 ) 3 f ( π0 0 ) 3 f 3 ( 0π 0 ) μ u d 3 f μq 1( 0π 0 ) d 4 f μq ( 0π 0 ) d 4 f Q ( π0 0 ) d 5 f 3( 0π 0 ) (b) f π π 1 0 1.5 f π π 0 1.591 f π π 0 1.591 f π π 3 0 4 4 4 4 4 4 4 4 u 5. 10 3.53 (c) μ u d 3 f 1 π π 0 4 4 μq d 4 f π π 0 4 4 μq d 4 f π π 0 4 4 f 1 ( 00 0 ) f ( 00 0 ) 3 f 3 ( 00 0 ) Q d 5 f 3 π π 0 4 4 u 1.35 10 u μ d 3 f 1( ππ 0 ) μq d 4 f ( ππ 0 ) μq d 4 f ( ππ 0 ) Q d 5 f 3( ππ 0 ) u 1.4 10 15 Poblem 5.9: μ 1.310 18 Q 1.710 fo SO sinθ A f 1 θ A θ B ϕ sinθ B cos( ϕ) cos θ A cosθ B

Chapte 5 Page 5.7 f θ A θ B ϕ f 3 θ A θ B ϕ π π (a) f 1 0 3 cos θ A3cosθ B cosθ B 1 sinθ A sinθ B cosθ B cos( ϕ) 3 4 1 5 cos θ A 5cosθ B 15 cosθ A cosθ B 4cosθ A cosθ B sinθ A sinθ B cos( ϕ) 1 π π f 0.755 10 1 π π f 0.755 10 1 π π f 3 0.5 u p ( d) μ d 3 f 1 π π 0 μq d 4 f π π 0 μq d 4 f π π 0 Q d 5 f 3 π π 0 π 3π (b) f 1 0 π 3π 1 f 0.49 10f 1 3π π 0 4.59 10 1 π 3π f 3 0.5 u a ( d) μ d 3 f 1 π 3π 0 μq d 4 f π 3π 0 μq d 4 f 3π π 0 Q d 5 f 3 π 3π 0 d 510 8 10 8 310 7 310 14 10 14 u p ( d) u a ( d) 110 14 0 110 14 10 14 0 110 7 10 7 310 7 410 7 d Fo example, at 10 A sepaation: u p 10 7.7 10 15 u a 10 7.59 10 15 Poblem 5.10: 10 8 μ 1.310 18 α 3.710 4 Q 1.710 3.89510 8 k 1.380110 1 ε 39.3k T 300 dispesion

Chapte 5 Page 5.8 u d 1 4ε u d 1.41 10 14 chage-chage u qq 0 dipole-dipole 1 μ 4 u μμ 3k T u μμ 1.18 10 15 dipole-polaization μ α u αμ u αμ 4.37 10 1 dipole-quadupole u μq kt quadupole-quadupole μq 4 u μq.08 10 1 14 Q 4 u QQ 5k T 10 u QQ 9.341 10 18 total u u d u qq u μμ u αμ u μq u QQ u 1.599 10 14 Poblem 5.11: We use the same paametes as in poblem 5.10, but we will neglect the quadupola pat of the potential. The quadupola potion of the potential does not have the same dependence that would allow factoization into effective LJ paametes. Fom the equations on pages 19 and 17 of the text we have: o 3.89510 8 ε o 39.3k

Chapte 5 Page 5.9 1 μ 4 μ α 3 kt F 1 F 1.108 4ε o o ε ε o F ε k 1 ε o F ε k 453.047 K k 3.89 10 cm 8 u eff () 4ε 1 u LJ () 4ε o o 1 o 3.10 8 3.710 8 810 8 10 13 u eff () 110 13 u LJ () 0 110 310 8 410 8 510 8 10 8 710 8 810 8 Poblem 5.1: Fo ammonia.9310 8 μ 1.4710 18 α.10 4 Q 110 T 300 k 1.380110 1 ε 37.9k 810 8 Using the angle-aveaged equations: ε 1 F dis 4 F dis 3.74 10 8 μ 4 F μμ kt 7 F μμ 1.07 10 8 1μ α F αμ 7 F αμ.794 10 9

Chapte 5 Page 5.10 F μq 1 μ Q kt 9 F μq.1 10 10 F QQ 8 Q 4 kt 11 F QQ 7.873 10 1 F F dis F μμ F αμ F μq F QQ F 5.18 10 dynes 8 Poblem 5.13: τ = o F τ = F sinθ whee is the angle between the vectos (90 degees in this case) and the new toque vecto is in the positive y diection. F 710 7 dyne 1.5310 8 cm τ F τ 1.071 10 14 dynecm Poblem.14: U = u aα u aβ u aγ u bα u bβ u bγ u cα u cβ u cγ But, all sites ae equivalent in tems of and, so: u aα = u bβ u cγ = u aβ = u cβ = u bα = u bγ u aγ = u cα U = 3u aα 4u aβ u aγ Now set up constants and LJ functionality. ε 7k 0.393 d 0.153 u() 4ε 1 109.47 θ π s 0. 180 Now find vaious distances and plug into LJ functionality to get pai inteactions. a : aα 0. u aα u aα u aα.83 10 15 a : aβ s d u aβ u aβ u aβ.404 10 15

Chapte 5 Page 5.11 a : by Law of Cosines, ac d d d dcos( θ) ac 0.89 aγ ac s aγ 0. u aγ u aγ u aγ 1.594 10 15 Finally, U 3u aα 4u aβ u aγ U.139 10 14 egs Poblem 5.14: The potential depends upon the two sites inteacting. As not enough infomation is given in the poblem to completely specify the oientation of the othe inteacting molecule, we will take the easiest case whee an identical molecule is oiented exactly above it so that we have like-like site inteactions. 1 0.393 1.51 0.588 The potential is zeo when =. Thus, the line of constant potential fo u = 0 should be dawn as a cicle aound each site of adius /. 1 1 1 0.19 0.94

Chapte 5 Page 5.1 e

Chapte 5 Page 5.13

g Chapte 5 Page 5.14

Chapte 5 Page 5.15

Chapte 5 Page 5.1

Chapte 5 Page 5.17 15 15 5

Chapte 5 Page 5.18 5

Chapte 5 Page 5.19 e 70

Chapte 5 Page 5.0

Chapte 5 Page 5.1

Chapte 5 Page 5. 5