Course Outline /HFWXUHV 1. Electrostatics 9 – Stationary charged particles – Electrostatic forces, fields, potentials – Analytical methods 640-142 Physics B 2. Circuit Theory Dr Ann Roberts, PhD 2 – Electrons moving in wires – Resistors, capacitors, batteries Dr Robert Scholten, PhD 3. Magnetism Dr Valerie Gurarie, PhD 11 – Moving charged particles – Magnetic fields, forces – Analytical methods School of Physics University of Melbourne http://webraft.its.unimelb.edu.au/640142/pub/ 4. Modern Physics 14 © The University of Melbourne 2000 Assessment Common problems 1. Semester exam 65% 2. Tests 10% • Vector quantities • Units – 30 min short-answer test in week 7 (Sept 4 – 8) – Exam-style question in week 11 (Oct 16 – 20) 3. Lab work 2 • SI prefixes: µ = 10-6 n = 10-9 p = 10-12 25% WARNING! Lecture demos are examinable! 3 © The University of Melbourne 2000 © The University of Melbourne 2000 Resources Resources • These lectures, associated notes, old exams, etc: • The textbook: Fundamentals of Physics (Extended) 5th Edition, Halliday Resnick & Walker, 1997 http://webraft.its.unimelb.edu.au/640142/pub/ – need Adobe PDF reader – need activated ITS e-mail account • Tutorials • also required for course planning • Practical laboratory classes – the web notes alone ARE NOT adequate! • Your own initiative: • Lecture times: A stream (Riv) 9.05 Tues 9.05 Wed 9.05 Fri 4 B stream (Lyle) 11.05 Mon 12.05 Thur 11.05 Fri © The University of Melbourne 2000 (OHFWURPDJQHWLVP – – – – C stream(Lyle) 3.15 Mon 3:15 Wed 3:15 Thur 5 Expect 40 hours per week for average mark (“P” grade) 25 points per annum in physics = 25% = 10 hours per week 3 lectures, 3 hours lab, 1 hour tute = 7 hours 3 hours per week, every week (36 per semester) homework! © The University of Melbourne 2000 6 Some Special Symbols Introduction • Industrial Revolution (18th C) Steam – Changed nature of work and manufacturing – Little impact on domestic life • Non-examinable material • Electrical Revolution (early 20th C) Electricity – Brought benefits to the common person! – Not clear where this will end yet ! 22 • More conceptually difficult material • Section reference in text • First step along the road to a Grand Unified Theory (GUT) 7 © The University of Melbourne 2000 8 © The University of Melbourne 2000 Part 1 - Outline In the beginning... Chapter 22 - Electric Charge • 600 BC – Ancient Greeks discovered lumps of amber, charged by friction (rubbing) would pick up small pieces of straw • Introduction to charge • Coulomb’s Law • Greek for amber = “elektron” • The electric field • Magnetism discovered about the same time • Gauss’s Law • Electric potential • Middle-east region called “Magnesia” • Energy and the electric field • Applications... 9 © The University of Melbourne 2000 10 © The University of Melbourne 2000 In the beginning... Now... • Mid 20th century: Quantum ElectroDynamics (QED) • 1820 H.C. Oersted: electric current in wire deflects compass • Basis of many areas of science, e.g.: – optics (light = EM wave) • Late 19th century: Maxwell’s equations combine electricity and magnetism – chemistry – etc. • 1905 Electricity and Magnetism unified by Einstein through the theory of special relativity • Basis of modern technology – Electric motors to particle accelerators – This course ends just before 1905! – Domestic power and communications network – Global positioning system – etc. etc. etc. © The University of Melbourne 2000 (OHFWURPDJQHWLVP 11 © The University of Melbourne 2000 12 The four forces of nature The four forces of nature Electric force Coulomb’s Law 1798 Electromagnetic force binds atoms Strong force binds the nucleus Electromagnetic force binds atoms Gravitational force Weak force in radioactive decay Gravitational force binds the solar system Gravitational force binds the solar system Newton’s Law 13 © The University of Melbourne 2000 Introductory Electrostatics 22.1 ConcepTest Three pithballs are suspended from thin threads. Each of the pithballs is charged by touching it with a previously charged object (e.g. Perspex rubbed against cat fur, nylon against silk, glass against polyester, etc.). • Gravitational “charge” comes in one type • Electric charge comes in two types + It is found that pithballs 1 and 2 repel each other and that pithballs 2 and 3 repel each other. From this we can conclude that: (a) 1 and 3 carry charges of opposite sign (b) 1 and 3 carry charges of equal sign (c) all three carry charges of the same sign (d) one of the objects carries no charge (e) we need to do more experiments to determine the sign of the charges + Like charges repel – – + – © The University of Melbourne 2000 14 © The University of Melbourne 2000 Unlike charges attract Pith balls/Electroscope 15 16 © The University of Melbourne 2000 The Naming of Charge Aside: Introductory atomic physics • Benjamin Franklin showed lightning is ordinary electricity • Negative electrons orbit a positive nucleus • Named “positive” and “negative” charges • There are the same number of electrons (-) as protons (+) • Assumed positive charge was the one that moved (wrong!!) • So matter is neutral – – • Can charge matter by adding or removing electrons ++ ++ – – © The University of Melbourne 2000 (OHFWURPDJQHWLVP 17 © The University of Melbourne 2000 18 Like charges repel Introductory electrostatics • The unit of charge: The Coulomb + + – Charles Coulomb (1736-1806) + + + • 1 Coulomb = 1 C • Examples: + – Electron charge = –1.6x10–19 C – Proton charge = +1.6x10–19 C – Neutron charge = 0 + + + + + + + + + + + Van de Graaf with "hair" 19 © The University of Melbourne 2000 – Pith balls/Electroscope 20 © The University of Melbourne 2000 Introductory electrostatics Charge • The electric force is very strong! • Usually create charge by scraping electrons from surfaces Gravitational attraction negligible Charge is always conserved 1% charge exchange + 1% charge exchange leads to force strong enough to drag Earth from orbit! + + + – – –– Microscopic view of a surface – © The University of Melbourne 2000 + 21 3. Cat© The FurUniversity of Melbourne 2000 Last lecture 22 Hunt for Red October • Electrostatics: non-moving charge • Moving objects in dry air become charged • Charge is: – – – – – positive or negative like charges repel opposites attract unit: Coulomb C quantised (minimum is e- = -1.6 x 10-19 C) – Air flow – • Charging by rubbing, e.g. cat fur, helicopter... – – + + + + + + © The University of Melbourne 2000 (OHFWURPDJQHWLVP 23 © The University of Melbourne 2000 24 Tragedy of the Hindenburg Charged Volcanic Ash • The Hindenburg Zeppelin airship exploded when a spark from “atmospheric electricity” ignited hydrogen in the balloon – 6 May 1937, Lakehurst New Jersey, USA, 36 people killed + + + ++ + – + + + + – – – © The University of Melbourne 2000 25 Conduction of charge • These “free electrons” can move under the influence of an electric field ➾ electric current 26 Conduction of charge + ++ + + + + + + + + + + + + + + + + + + + + + Uncharged conductor Charged conductor • There are huge numbers of free electrons available in an ordinary conductor – e.g: copper >1022 per cubic cm • Prevented from leaving surface by electric field of nuclei • Other conductors – Salty water, rarefied gas, flames © The University of Melbourne 2000 – © The University of Melbourne 2000 22.3 • A conductor contains electrons not strongly bound to any particular nucleus – 27 Insulators © The University of Melbourne 2000 28 Conduction of charge • Electrons strongly bound to their own nuclei + + + + + + + + + + + • Not free to move • Glass, chemically pure water, plastics + + + + + + + + + + © The University of Melbourne 2000 (OHFWURPDJQHWLVP Uncharged Insulator Charged Insulator • Typically <~ 1 free electron per cubic cm 29 © The University of Melbourne 2000 + + + 30 Charging by induction: no touching! + ++ + + + + + + + + + + + + + + + Coulomb discovers Coulomb’s Law Uncharged conductor Charged conductor + +– – – – + + + + + – – –– + + + – – – – – – –– Charged conductor Charged conductor Negatively charged conductor © The University of Melbourne 2000 31 32 © The University of Melbourne 2000 Permittivity of free space Hydrogen bond in DNA • The material occupying the space between the charges influences the strength of the force • Thymine-Adenine bond via: O– • Depends on the permittivity: N– H+ H+ N– N– • Cytosine-Guanine bond similarly • Where ε 0 = 8.85 × 10−12 C2 / N m 2 is the permittivity of free space • Must replace this with other values if other materials occupy the space between the charges © The University of Melbourne 2000 33 © The University of Melbourne 2000 34 Photocopiers and Laser Printers Electrostatics in action (3) Negatively charged toner powder is cascaded over the surface. It electrostatically adheres to the positively charged image area making a visible image. (1) A photoconductive surface is given a positive charge (+). (4) A piece of plain paper is placed over the surface and given a positive charge. (2) The image of a document is exposed on the surface. This causes the charge to drain away from the surface in all but the dark areas. © The University of Melbourne 2000 (OHFWURPDJQHWLVP 35 © The University of Melbourne 2000 36 A modern copier 1) document handler 2) photoreceptor belt 3) magnetic rollers apply toner (5) The negatively charged powder image on the surface is electrostatically attracted to the positively charged paper. 4) paper tray 7) output rollers fuse toner (6) The powder image is fused to the paper by heat. 37 © The University of Melbourne 2000 38 © The University of Melbourne 2000 How it works Superposition Principle See web page for link, or go directly to: • Big words, simple idea: Add ‘em up! • Total force from a system of charges is just the sum of the force from each charge http://www.physics.udel.edu/wwwusers/watson/scen167/less-copier.html + + + + + + + Q 39 © The University of Melbourne 2000 40 © The University of Melbourne 2000 Superposition Principle Vectors • Total force from a system of charges is just the sum of the force from each charge • Each of the force components is a vector • Vectors must be added vectorially, then final magnitude calculated • Example: What is the force on q1? + + Charge = q + + + y q3 + + 2a x a a – q2 – q5 – q1 a + q6 a – q4 + Q © The University of Melbourne 2000 (OHFWURPDJQHWLVP 41 © The University of Melbourne 2000 42 1996 exam question 1(c) 1(c) 23.1 The Electric Field sets up Four equal point charges, +3µC each, are placed at the four corners of a square that is 40cm on a side. Charge exerts force on exerts force on E Charge sets up (i) Using Coulomb’s law and the principle of superposition, or otherwise, find the force on one of the charges from the other three 6ROXWLRQ + 'UDZGLDJUDP Direction of E is the direction a positive test charge would move 'UDZIRUFHYHFWRUVRQRQHFKDUJHIURPRWKHUWKUHHFKDUJHV 5HVROYHIRUFHYHFWRUVLQWRKRUL]RQWDODQGYHUWLFDOFRPSRQHQWV $GGXSFRPSRQHQWV 43 © The University of Melbourne 2000 © The University of Melbourne 2000 44 How big is the electric field? Electric field for a point charge • Inside copper wire of household circuits • Charged plastic comb • Electron beam in TV; photocopier corona wire • Electric breakdown in air • Hydrogen atom, at electron orbit radius • At uranium nucleus + E has magnitude AND direction at every point in space: Vector Field © The University of Melbourne 2000 45 Electric Field from a Dipole © The University of Melbourne 2000 46 Why use the concept of a field? • If we know E at some position, then we know the force on any arbitrary charge at that position. No longer need to consider all the other charges that make the E: Exercise: Sketch field lines if – replaced by + © The University of Melbourne 2000 (OHFWURPDJQHWLVP 47 © The University of Melbourne 2000 48 Electric field lines 23.3 Gauss’ Law • How do we calculate the electric field from a charge distribution? • Originate on (+) charge • Answer: Use principle of superpostion and integrate! • Terminate on (–) charge + • But: This to usually too hard! • Alternative Answer: Use Gauss’ Law • Lines close together where E is strong + • Very easy in problems of high symmetry: – – – – • Lines far apart where E is weak 49 © The University of Melbourne 2000 Point charge Line of charge Sheet of charge Often need to find E(r) near these objects! 50 © The University of Melbourne 2000 Gauss’ Law - Introduction Gauss’ Law - Concept of electric flux • Field from a point charge: • Define: • or q Q Have the area of a sphere enclosing the charge! + • where Φ is the electric flux + E HOHFWULFILHOG OLQHV r 51 © The University of Melbourne 2000 Aside: Special case (OHFWULFIOX[ LVSURGXFW RIQRUPDO DUHDZLWK HOHFWULFILHOG © The University of Melbourne 2000 52 Gauss’ Law • If E and dA are parallel (E normal to surface) then the flux simplifies: “The electric flux through a closed surface is equal to the charge enclosed divided by εo” • Note that θ = 0 if E and dA are parallel • So Φ = EA in this case E • Useful for finding electric field in problems with high symmetry dA • Rules: – Decide on direction of E (direction a positive test charge would move) – Choose Gaussian surface to make job easiest – Make sure dA is always either parallel or right angles to E © The University of Melbourne 2000 (OHFWURPDJQHWLVP 53 © The University of Melbourne 2000 54 Gauss’ Law: point charge Gauss’ Law: Line of charge • Use Gauss’ Law to find E at a point distant r from a point charge q 5XOH'UDZE 5XOH&KRRVH*DXVVLDQ VXUIDFHHQFORVLQJFKDUJH DQGSDVVLQJWKURXJKSRLQW ZKHUHELVWREHIRXQG $SSO\*DXVV¶/DZ q + © The University of Melbourne 2000 24.3 • Use Gauss’ Law to find E at a point distant r from a line of charge with λ=q/L Coulombs/metre E r 55 24.7 Concept of Electric Flux © The University of Melbourne 2000 57 Gauss’ Law 56 © The University of Melbourne 2000 Line of Charge © The University of Melbourne 2000 58 Concept Test A cylindrical piece of insulating material is placed in an external electric field, as shown. The net electric flux passing through the surface of the cylinder is 1. Positive 2. Negative 3. Zero Textbook fig. 24.5 © The University of Melbourne 2000 (OHFWURPDJQHWLVP 59 © The University of Melbourne 2000 60 24.8 24.8 Gauss’ Law: Sheet of charge Gauss’ Law: Sheet of charge Use Gauss’ Law to find E at a point distant r from a sheet of charge with σ=q/A Coulombs/metre2 Use Gauss’ Law to find E at a point distant r from a sheet of charge with σ=q/A Coulombs/metre2 Note: E not necessarily perpendicular for insulator, but in this case σ is uniform. WARNING! This is an insulating sheet of charge 61 © The University of Melbourne 2000 62 © The University of Melbourne 2000 Internal fields? Electric Field from a charged conductor • E field is always normal to the surface • E field is always zero inside • Why? + + + + + + –– – + ++ + + + + + 63 © The University of Melbourne 2000 External field strength + Hollow conductor + © The University of Melbourne 2000 (OHFWURPDJQHWLVP + + + + + + + + + + + 5HVXOWLVWZLFHDV VWURQJDVIRUWKHWKLQ VKHHWEHFDXVHRIWKH GLVWDQWFKDUJH 64 © The University of Melbourne 2000 65 © The University of Melbourne 2000 + + Metal ring in petri dish 66 Faraday cage Faraday cage • Conductors shield their interior from electric fields • Conductors shield their interior from electric fields 67 © The University of Melbourne 2000 Radio in shield © The University of Melbourne 2000 Bare Hands Suit 68 BA009 in Charged Ash Cloud • Loss of radio signals + + + + + 330,000 volt power line + + + + Electrically conducting suit: No electric field inside from Australian Geographic 39: July-Sept 1995 p26 69 © The University of Melbourne 2000 The Electric Dipole 23.9 70 © The University of Melbourne 2000 Polarisation (induced dipoles) • Since the electric field is so strong, rarely encounter free charge in nature • An atom • More often encounter DIPOLES H+ Cl– H+ – O– – H+ + d Generic dipole – + –q +q © The University of Melbourne 2000 (OHFWURPDJQHWLVP – 71 © The University of Melbourne 2000 72 Polarisation Lightning • An atom in an electric field • A Molecule in a STRONG electric field – – Need 3 million volts per metre to do this! Strong Electric fields break – air molecules – and causes sparks! + – – “SNAP” + 1H[WWRUTXHRQDGLSROH 73 © The University of Melbourne 2000 Van de Graaf with spark © The University of Melbourne 2000 74 Lightning • Just prior to flash, have a line of electrons in a column between cloud and ground • λ~ -1 x 10-3 C/m • Once column bridges gap, e- rapidly transported: È current È e- collisions with air molecules È ionisation È further current • e- + air molecules È atom excitation È spontaneous decay È photons È flash 75 © The University of Melbourne 2000 Lightning • λ~ -1 x 10-3 ++ + + + ++ – – – – – – – © The University of Melbourne 2000 76 Lightning C/m • Recall for line of charge: ++ + + + ++ – – – – – – – ++ + + + + + “SNAP” • Visible luminous part of lightning is typically smaller, ~ 0.5m – –– – – –– © The University of Melbourne 2000 (OHFWURPDJQHWLVP 77 © The University of Melbourne 2000 78 Attracting neutral insulators Attracting neutral insulators – – + + + – + – + – 79 © The University of Melbourne 2000 80 © The University of Melbourne 2000 23.9 Induced Charge –+ Torque on a dipole • Dipole in an electric field + E – Smoke precipitator © The University of Melbourne 2000 81 82 © The University of Melbourne 2000 Torque on a dipole Torque on a dipole • Dipole in an electric field • Define the Dipole Moment d d/2 Fsinθ d/2 θ + θ Generic dipole Fsinθ E – + –q +q p d Define p = qd – where p is a vector that points from - to + © The University of Melbourne 2000 (OHFWURPDJQHWLVP 83 © The University of Melbourne 2000 84 Torque on a dipole Charge and conductors • Dipole in an electric field • Take a “pointy” conductor + p Fsinθ θ θ Fsinθ E d – Conclusion: Dipoles align themselves with E fields 85 © The University of Melbourne 2000 Charge and conductors + 86 © The University of Melbourne 2000 Charge and conductors + + + + + + + + + + + + 87 © The University of Melbourne 2000 Pointy conductors revisited + 8. Pointy object in dish © The University of Melbourne 2000 88 Sparks and Sharp Points q1 r1 q2 r2 • Where will the air break-down first? r1 > r2 All conducting Connected by conductor so V same ++ + + + ++ Assume separation is large therefore charge uniformly distributed on each, so: “SNAP” – – – – – – – © The University of Melbourne 2000 (OHFWURPDJQHWLVP 89 © The University of Melbourne 2000 90 Half Dome - Yosemite National Park Half Dome - Yosemite National Park Electric Field is highest up here! ++ + + + ++ –– – – –– – © The University of Melbourne 2000 91 © The University of Melbourne 2000 92 93 © The University of Melbourne 2000 94 Half Dome - Yosemite National Park Electric Field is highest up here! © The University of Melbourne 2000 St Elmo’s Fire Half Dome - Yosemite National Park ++ + + + ++ Corona discharge from high fields at pointy bits © The University of Melbourne 2000 (OHFWURPDJQHWLVP 95 The Universityin of Melbourne 2000 9.© Aeroplane petri-dish – – – – – – – 96 Corona Discharge from BA009 © The University of Melbourne 2000 Aeroplane in vacuum chamber (OHFWURPDJQHWLVP 97