Physics 2020 Exam 4 Constants and Formulae
|
|
- Norman Taylor
- 5 years ago
- Views:
Transcription
1 Physics 2020 Exam 4 Constants and Formulae Useful Constants k e = Nm 2 /C 2 ɛ = C 2 /(N m 2 ) µ = 4π 10 7 T m/a e = C G = Nm 2 /kg 2 h = Js h = h/2π = Js m p = m H = kg c = m/s m e = kg σ = W/m 2 /K 4 M = kg R = m g = 9.80 m/s 2 M = kg R = m I th = W/m 2 I tp = 1.00 W/m 2 1eV = J 1 T = 10 4 G 1 km = 10 3 m 1 nm = 10 9 m 1 mi = km 1 ms = 10 3 s 1 min = 60 s 1 hr = 3600 s 1day = s 1 yr = days Useful Formulae C (circle) = 2πr D (circle) = 2r A (circle) = πr 2 V (sphere) = 4 3 πr3 A (sphere) = 4πr 2 V (rectangular box) = L W H sin θ = a/c cos θ = b/c tan θ = a/b a 2 = b 2 + c 2 2bc cos A 1 = cos 2 θ + sin 2 θ c 2 = a 2 + b 2 (sin A)/(a) = (sin B)/(b) = (sin C)/(c) v = v + at v 2 = v 2 +2ax x = v t at2 x = 1 2 (v + v )t R = R = R 2 x + R2 y R x = R cos θ R y = R sin θ tan θ = R y x = x + v x t R x v x = v x v y = v y gt v = vx 2 + v2 y y = y + v y t 1 2 gt2 vy 2 = v2 y 2gy θ = tan 1 ( v y v x In the trigonometric equations above, a opposite side, b adjacent side, and c hypotenuse where the angle is θ. Capital letters A, B, and C are the angles opposite the sides a, b, and c, respectively. )
2 Useful Formulae (continued) F = m a Fg = w = m g W =(F cos θ)s = (KE) PE g = mgy KE 1 2 mv2 PE s = 1 2 kx2 KE i +PE i =KE f +PE f p m v ω = ω + αt 1 rev = 2π radians = 360 θ = ω t αt2 ω 2 = ω 2 +2αθ v t = rω a t = rα F c = ma c =(mvt 2)/r = mrω2 a c = v 2 /r F g =(Gm 1 m 2 /r 2 )ˆr, orf g = mg v =2πr/T g = GM/r 2 F c = Mv 2 /r T F = 9 5 T C +32 T C = T F e = k e q 1 q 2 /r12 2 E = F e /q Φ E = EAcos θ = Q tot /ɛ E = k e q/r 2 U = Q 2 /(2C) = 1 2 C( V )2 = 1 2 Q( V ) V = k eq/r I = Q/ t C = κc V = E Ir q = Q ( 1 e t/rc) (charging) τ = RC q = Qe t/rc (discharging) F = qvb sin θ F = BIlsin θ B = µ ni τ = BIAsin θ r = mv/qb B = µ I/(2πr) B l = µ I Φ B = BAcos θ E = N Φ B / t = L I/ t V = E = El = Blv I = E /R =(Blv)/R E = NBAωsin ωt F s = kx PE s = 1 2 kx2 T =1/f =2π m/k T =2π L/g v = (331.3 m/s) T/273 K = fλ v = F/µ, µ = m/l β = 10 log(i/i ) I = P/(4πr 2 ) f = f[(v ± v o )/(v v s )] M = v s /v f n =(n/4l)v, (n =1, 3, 5,...) (one end closed) f n =(n/2l) F/µ (string) f n =(n/2l)v, (n =1, 2, 3,...) (open ends) L =(n/2)λ ω =2πf f n = nf 1 1/λ n = R A Z 2 /n 2 ν = c/λ λ/λ =(λ λ )/λ = v r /c c = E max /B max E = hν = hc/λ F = σt 4 λ max =( mk)/t L =4πσR 2 T 4 1/λ = R A Z 2 [ (1/n 2 ) (1/m 2 ) ] L n = m e v n r n = n h
3 Physics 2020 Name: Sample Exam 4 Summer Part A: Hard Multiple Choice (10 points total, 2 points each, Circle Best Answer). 1. A photon has an energy of ev. What is the wavelength of this photon? a) nm b) 6563 Å c) m d) Å e) 2420 nm 2. What is the orbital angular momentum of an electron in the n = 3 level of hydrogen? a) J s b) J s c) J s d) J s e) J s 3. What is the wavelength of maximum emission for a blackbody of 22,200 K? a) nm b) 8.35 nm c) nm d) 1216 nm e) 130 nm 4. A photon is measured to have a maximum electric-field strength of 6.77 N/C. What is the maximum strength of the magnetic field for this photon? (Help: n=10 9, µ=10 6, M=10 6, G=10 9.) a) 22.6 nt b) 6.77 µt c) 2.00 T d) 44.3 MT e) 2.03 GT 5. What is wavelength of the Balmer limit for ionized helium? (Note that R He = m 1.) a) nm b) nm c) nm d) nm e) nm
4 PHYS-2020: General Physics II Sample Exam 4 Summer 2006 Page 2 Part B: Easy Multiple Choice (10 points total, 1 point each, Circle Best Answer). 6. Particles with symmetric wavefunctions are called a) bosons b) electrons c) quarks d) fermions e) leptons 7. Which of the following is an elementary particle? a) gluon b) weakon c) photon d) muon e) none of these 8. We observe 5 different blackbodies and note the type of light that each emit their maximum amount of flux. Of these, which is the hottest? a) red b) ultraviolet c) green d) infrared e) microwave 9. The state of a particle in classical physics can be given by the particle s a) mass b) charge c) spin d) trajectory e) probability 10. Strong spectral lines that originate out of the ground state are called a) forbidden lines b) semiforbidden lines c) intersystem lines d) resonance lines e) none of these 11. A tube is filled with low pressure gas. If an electric current is passed through this gas, what kind of spectrum will result? a) absorption line b) continuous c) emission line d) reflection e) transparent
5 PHYS-2020: General Physics II Sample Exam 4 Summer 2006 Page Which of the following is not a field particle? a) fermion b) weakon c) gluon d) photon e) graviton 13. Which of the following is the true statement about hadrons? a) Hadrons are all leptons. b) Hadrons are particles that obey the strong force. c) Hadrons are particles that obey the dark side of the force. d) Hadrons obey the weak, electromagnetic, and gravitational forces, but they do not obey the strong force since they do not see gluons. e) None of these are true. 14. Brightness of visible light is to color as loudness of sound is to a) density b) pressure c) flux d) intensity e) pitch 15. The Pauli Exclusion Principle only applies to what type of particles? a) bosons b) photons c) fermions d) gravitons e) mesons
6 PHYS-2020: General Physics II Sample Exam 4 Summer 2006 Page 4 Part C: Problems (20 points total, 10 points each). 16. A 502 nm photon is absorbed by an electron that is in a 3.16 ev state. (a) What would be the energy (in ev) of the new state once it absorbs the photon? (b) While excited, assume that this atom collides with a second stationary electron. After the collision, the bound electron collisionally de-excites to the 0.00 ev ground state and all of the energy of this transition is transferred to the kinetic energy of the stationary electron. How fast would this second electron be traveling after this collision? (Show all work!)
7 PHYS-2020: General Physics II Sample Exam 4 Summer 2006 Page The exhaust of a spaceship shines with a blackbody spectrum at a total flux of W/m 2. (a) What is the temperature of this exhaust? (b) At what wavelength (in nm) does this exhaust emit its maximum flux? (c) If the exhaust of the ship is moving away from us at 9820 km/s, at what wavelength (in nm) would we see its maximum flux? (Show all work!!!)
Physics 2020 Exam 3 Constants and Formulae
Physics 2020 Exam 3 Constants and Formulae Useful Constants k e = 8.99 10 9 N m 2 /C 2 e = 1.60219 10 19 C h = h/2π = 1.05459 10 34 J s h = 6.62620 10 34 J s m p = m H = 1.672 10 27 kg m e = 9.110 10 31
More informationPhysics 2020 Exam 2 Constants and Formulae
Physics 2020 Exam 2 Constants and Formulae Useful Constants k e = 8.99 10 9 N m 2 /C 2 c = 3.00 10 8 m/s ɛ = 8.85 10 12 C 2 /(N m 2 ) µ = 4π 10 7 T m/a e = 1.602 10 19 C h = 6.626 10 34 J s m p = 1.67
More informationPHYSICS 250 May 4, Final Exam - Solutions
Name: PHYSICS 250 May 4, 999 Final Exam - Solutions Instructions: Work all problems. You may use a calculator and two pages of notes you may have prepared. There are problems of varying length and difficulty.
More informationFOUNDATION STUDIES EXAMINATIONS June PHYSICS Semester One February Main
1 FOUNDATION STUDIES EXAMINATIONS June 2015 PHYSICS Semester One February Main Time allowed 2 hours for writing 10 minutes for reading This paper consists of 6 questions printed on 10 pages. PLEASE CHECK
More informationAtomic Structure. Standing Waves x10 8 m/s. (or Hz or 1/s) λ Node
Atomic Structure Topics: 7.1 Electromagnetic Radiation 7.2 Planck, Einstein, Energy, and Photons 7.3 Atomic Line Spectra and Niels Bohr 7.4 The Wave Properties of the Electron 7.5 Quantum Mechanical View
More informationb) (6) What is the volume of the iron cube, in m 3?
General Physics I Exam 4 - Chs. 10,11,12 - Fluids, Waves, Sound Nov. 14, 2012 Name Rec. Instr. Rec. Time For full credit, make your work clear to the grader. Show formulas used, essential steps, and results
More informationAstronomy II (ASTR-1020) Homework 2
Astronomy II (ASTR-1020) Homework 2 Due: 10 February 2009 The answers of this multiple choice homework are to be indicated on a Scantron sheet (either Form # 822 N-E or Ref # ABF-882) which you are to
More informationProperties of Electromagnetic Radiation Chapter 5. What is light? What is a wave? Radiation carries information
Concepts: Properties of Electromagnetic Radiation Chapter 5 Electromagnetic waves Types of spectra Temperature Blackbody radiation Dual nature of radiation Atomic structure Interaction of light and matter
More informationkg C 10 C = J J = J kg C 20 C = J J = J J
Seat: PHYS 1500 (Spring 2007) Exam #3, V1 Name: 5 pts 1. A pendulum is made with a length of string of negligible mass with a 0.25 kg mass at the end. A 2nd pendulum is identical except the mass is 0.50
More informationBROCK UNIVERSITY SOLUTIONS
BROCK UNIVERSITY Final Exam: April 2014 Number of pages: 11 (+ formula sheet) Course: PHYS 1P22/1P92 Number of students: 134 Examination date: 17 April 2014 Number of hours: 3 Time of Examination: 9:00
More informationDual Nature of Matter and Radiation 9. The work function of a certain metal is 3.3 J. Then the maximum kinetic energy of photoelectrons emitted by incident radiation of wavelength 5 A is- ).48 ev ).4 ev
More informationElectronic Structure of Atoms. Chapter 6
Electronic Structure of Atoms Chapter 6 Electronic Structure of Atoms 1. The Wave Nature of Light All waves have: a) characteristic wavelength, λ b) amplitude, A Electronic Structure of Atoms 1. The Wave
More informationCollege Physics B - PHY2054C
of College - PHY2054C The of 11/17/2014 My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building Outline of 1 2 of 3 4 of Puzzling The blackbody intensity falls to zero at both long and short wavelengths,
More informationPhysics Midterm #2 Two Hours, Closed Book
Physics 102-1 Midterm #2 Two Hours, Closed Book These are the same instructions as given on the first exam. Instructions for taking the exam in the Science Library: Pick up and return the exam from the
More informationProperties of Elementary Particles
and of Elementary s 01/11/2018 My Office Hours: Thursday 1:00-3:00 PM 212 Keen Building Outline 1 2 3 Consider the world at different scales... Cosmology - only gravity matters XXXXX Input: Mass distributions
More informationFOUNDATION STUDIES EXAMINATIONS September 2009
1 FOUNDATION STUDIES EXAINATIONS September 2009 PHYSICS First Paper July Fast Track Time allowed 1.5 hour for writing 10 minutes for reading This paper consists of 4 questions printed on 7 pages. PLEASE
More informationb) (6) With 10.0 N applied to the smaller piston, what pressure force F 2 (in newtons) is produced on the larger piston?
General Physics I Exam 4 - Chs. 10,11,12 - Fluids, Waves, Sound Nov. 17, 2010 Name Rec. Instr. Rec. Time For full credit, make your work clear to the grader. Show formulas used, essential steps, and results
More information(a) 0.3 c. (b) 0.7 c. (c) 1.0 c. (d) 1.7 c.
Seat: PHYS 1510 (Spring 2013) Exam #4, V1 Name: Multiple choice (4 pts each) circle the correct answers. 1. Three isotopes have atomic number 10: beryllium, boron, and carbon. The atom 10 4Be has mass
More informationSeat: PHYS 1510 (Spring 2013) Exam #3, V1 Multiple choice (4 pts each) circle the correct answers.
Seat: PHYS 1510 (Spring 2013) Exam #3, V1 Name: Multiple choice (4 pts each) circle the correct answers. 1. From book MC 24.15b An electron has a velocity in the x-direction in a region where the magnetic
More information. d. v A v B. e. none of these.
General Physics I Exam 3 - Chs. 7,8,9 - Momentum, Rotation, Equilibrium Oct. 28, 2009 Name Rec. Instr. Rec. Time For full credit, make your work clear to the grader. Show the formulas you use, the essential
More informationChapter 27 Early Quantum Theory and Models of the Atom Discovery and Properties of the electron
Chapter 27 Early Quantum Theory and Models of the Atom 27-1 Discovery and Properties of the electron Measure charge to mass ratio e/m (J. J. Thomson, 1897) When apply magnetic field only, the rays are
More informationISP209 Spring Exam #3. Name: Student #:
ISP209 Spring 2014 Exam #3 Name: Student #: Please write down your name and student # on both the exam and the scoring sheet. After you are finished with the exam, please place the scoring sheet inside
More informationPHYS-2020: General Physics II Course Lecture Notes Section X
PHYS-2020: General Physics II Course Lecture Notes Section X Dr. Donald G. Luttermoser East Tennessee State University Edition 4.0 Abstract These class notes are designed for use of the instructor and
More information32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES
32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES 32.1 Biological Effects of Ionizing Radiation γ-rays (high-energy photons) can penetrate almost anything, but do comparatively little damage.
More informationPhysics 1C Lecture 29A. Finish off Ch. 28 Start Ch. 29
Physics 1C Lecture 29A Finish off Ch. 28 Start Ch. 29 Particle in a Box Let s consider a particle confined to a one-dimensional region in space. Following the quantum mechanics approach, we need to find
More informationDistance travelled time taken and if the particle is a distance s(t) along the x-axis, then its instantaneous speed is:
Chapter 1 Kinematics 1.1 Basic ideas r(t) is the position of a particle; r = r is the distance to the origin. If r = x i + y j + z k = (x, y, z), then r = r = x 2 + y 2 + z 2. v(t) is the velocity; v =
More informationSUMMARY Phys 2523 (University Physics II) Compiled by Prof. Erickson. F e (r )=q E(r ) dq r 2 ˆr = k e E = V. V (r )=k e r = k q i. r i r.
SUMMARY Phys 53 (University Physics II) Compiled by Prof. Erickson q 1 q Coulomb s Law: F 1 = k e r ˆr where k e = 1 4π =8.9875 10 9 N m /C, and =8.85 10 1 C /(N m )isthepermittivity of free space. Generally,
More informationSelected "Phacts" for the Physics Regents Exam You Should Know
Selected "Phacts" for the Physics Regents Exam You Should Know I. Mechanics Study Hard! 1. Mass and inertia are the same thing. (Mass actually measures inertia in kilograms Much as monetary resources measures
More informationFinal Exam: Thursday 05/02 7:00 9:00 pm in STEW 183
Final Exam: Thursday 05/02 7:00 9:00 pm in STEW 183 Covers all readings, lectures, homework from Chapters 17 through 30 Be sure to bring your student ID card, calculator, pencil, and up to three onepage
More informationPHY2020 Test 2 November 5, Name:
1 PHY2020 Test 2 November 5, 2014 Name: sin(30) = 1/2 cos(30) = 3/2 tan(30) = 3/3 sin(60) = 3/2 cos(60) = 1/2 tan(60) = 3 sin(45) = cos(45) = 2/2 tan(45) = 1 sin(37) = cos(53) = 0.6 cos(37) = sin(53) =
More information1. (a) An ion of plutonium Pu has an overall charge of C. (iii) electrons... (3) (2) (Total 5 marks)
AQA Questions from 2004 to 2006 Particle Physics 239 94 1. (a) An ion of plutonium Pu has an overall charge of +1.6 10 19 C. For this ion state the number of (i) protons... neutrons... (iii) electrons...
More informationCHEM 1311A. E. Kent Barefield. Course web page.
CHEM 1311A E. Kent Barefield Course web page http://web.chemistry.gatech.edu/~barefield/1311/chem1311a.html Two requests: cell phones to silent/off no lap tops in operation during class Bring your transmitter
More informationCHEM Course web page. Outline for first exam period
CHEM 3 Course web page http://web.chemistry.gatech.edu/~barefield/3/chem3a.html Outline for first exam period Atomic structure and periodic properties Structures and bonding models for covalent compounds
More informationParticle nature of light & Quantization
Particle nature of light & Quantization A quantity is quantized if its possible values are limited to a discrete set. An example from classical physics is the allowed frequencies of standing waves on a
More informationINTRODUCTION TO QUANTUM MECHANICS
4 CHAPTER INTRODUCTION TO QUANTUM MECHANICS 4.1 Preliminaries: Wave Motion and Light 4.2 Evidence for Energy Quantization in Atoms 4.3 The Bohr Model: Predicting Discrete Energy Levels in Atoms 4.4 Evidence
More informationFOUNDATION STUDIES EXAMINATIONS June PHYSICS Semester One February Main
1 FOUNDATION STUDIES EXAMINATIONS June 2013 PHYSICS Semester One February Main Time allowed 2 hours for writing 10 minutes for reading This paper consists of 4 questions printed on 10 pages. PLEASE CHECK
More informationAtomic Structure and Atomic Spectra
Atomic Structure and Atomic Spectra Atomic Structure: Hydrogenic Atom Reading: Atkins, Ch. 10 (7 판 Ch. 13) The principles of quantum mechanics internal structure of atoms 1. Hydrogenic atom: one electron
More information1. What is the minimum energy required to excite a mercury atom initially in the ground state? ev ev ev
Page 1 of 10 modern bank Name 25-MAY-05 1. What is the minimum energy required to excite a mercury atom initially in the ground state? 1. 4.64 ev 3. 10.20 ev 2. 5.74 ev 4. 10.38 ev 2. The diagram represents
More information2007 Section A of examination problems on Nuclei and Particles
2007 Section A of examination problems on Nuclei and Particles 1 Section A 2 PHYS3002W1 A1. A fossil containing 1 gramme of carbon has a radioactivity of 0.03 disintegrations per second. A living organism
More informationPhysics 1C Lecture 29B
Physics 1C Lecture 29B Emission Spectra! The easiest gas to analyze is hydrogen gas.! Four prominent visible lines were observed, as well as several ultraviolet lines.! In 1885, Johann Balmer, found a
More informationEarly Quantum Theory and Models of the Atom
Early Quantum Theory and Models of the Atom Electron Discharge tube (circa 1900 s) There is something ( cathode rays ) which is emitted by the cathode and causes glowing Unlike light, these rays are deflected
More informationChemistry 432 Problem Set 1 Spring 2018 Solutions
Chemistry 43 Problem Set 1 Spring 018 Solutions 1. A ball of mass m is tossed into the air at time t = 0 with an initial velocity v 0. The ball experiences a constant acceleration g from the gravitational
More informationGen. Phys. II Exam 4 - Chs. 27,28,29 - Wave Optics, Relativity, Quantum Physics Apr. 16, 2018
Gen. Phys. II Exam 4 - Chs. 27,28,29 - Wave Optics, Relativity, Quantum Physics Apr. 16, 2018 Rec. Time Name For full credit, make your work clear. Show formulas used, essential steps, and results with
More informationGeneral Physics (PHY 2140)
General Physics (PHY 140) Lecture 33 Modern Physics Atomic Physics Atomic spectra Bohr s theory of hydrogen http://www.physics.wayne.edu/~apetrov/phy140/ Chapter 8 1 Lightning Review Last lecture: 1. Atomic
More information2.1- CLASSICAL CONCEPTS; Dr. A. DAYALAN, Former Prof & Head 1
2.1- CLASSICAL CONCEPTS; Dr. A. DAYALAN, Former Prof & Head 1 QC-2 QUANTUM CHEMISTRY (Classical Concept) Dr. A. DAYALAN,Former Professor & Head, Dept. of Chemistry, LOYOLA COLLEGE (Autonomous), Chennai
More informationQuantum Mechanics. Reilly V. Bautista. September 5, Reilly V. Bautista Quantum Mechanics September 5, / 78
Quantum Mechanics Reilly V. Bautista September 5, 2016 Reilly V. Bautista Quantum Mechanics September 5, 2016 1 / 78 Contents Properties of electromagnetic radiation Issues with classical model of physics
More informationPhysics 342: Modern Physics
Physics 342: Modern Physics Final Exam (Practice) Relativity: 1) Two LEDs at each end of a meter stick oriented along the x -axis flash simultaneously in their rest frame A. The meter stick is traveling
More information2. What is the wavelength, in nm, of light with an energy content of 550 kj/mol? a nm b nm c. 157 nm d. 217 nm e.
1. What is the frequency associated with radiation of 4.59 x 10-8 cm wavelength? a. 6.54 x 10 17 s -1 b. 6.54 x 10 15 s -1 c. 1.53 x 10-8 s -1 d. 13.8 s -1 e. 2.18 x 10 7 s -1 1 2. What is the wavelength,
More informationATOMIC STRUCRURE
ATOMIC STRUCRURE Long Answer Questions: 1. What are quantum numbers? Give their significance? Ans. The various orbitals in an atom qualitatively distinguished by their size, shape and orientation. The
More informationUNIT : QUANTUM THEORY AND THE ATOM
Name St.No. Date(YY/MM/DD) / / Section UNIT 102-10: QUANTUM THEORY AND THE ATOM OBJECTIVES Atomic Spectra for Hydrogen, Mercury and Neon. 1. To observe various atomic spectra with a diffraction grating
More informationOption 212: UNIT 2 Elementary Particles
Department of Physics and Astronomy Option 212: UNIT 2 Elementary Particles SCHEDULE 26-Jan-15 13.00pm LRB Intro lecture 28-Jan-15 12.00pm LRB Problem solving (2-Feb-15 10.00am E Problem Workshop) 4-Feb-15
More informationChapter 12: Phenomena
Chapter 12: Phenomena K Fe Phenomena: Different wavelengths of electromagnetic radiation were directed onto two different metal sample (see picture). Scientists then recorded if any particles were ejected
More information1P22/1P92 Exam Review Problems 2013 Friday, January 14, :03 AM. Chapter 20
Exam Review Problems 2011 Page 1 1P22/1P92 Exam Review Problems 2013 Friday, January 14, 2011 10:03 AM Chapter 20 True or false? 1 It's impossible to place a charge on an insulator, because no current
More informationStellar Astrophysics: The Interaction of Light and Matter
Stellar Astrophysics: The Interaction of Light and Matter The Photoelectric Effect Methods of electron emission Thermionic emission: Application of heat allows electrons to gain enough energy to escape
More informationI understand the relationship between energy and a quanta I understand the difference between an electron s ground state and an electron s excited
NCCS 1.1.2 & 1.1.3 I understand the relationship between energy and a quanta I understand the difference between an electron s ground state and an electron s excited state I will describe how an electron
More informationLight. Light (con t.) 2/28/11. Examples
Light We can use different terms to describe light: Color Wavelength Frequency Light is composed of electromagnetic waves that travel through some medium. The properties of the medium determine how light
More informationPhysics 218: Final. Class of 2:20pm. May 7th, You have the full class period to complete the exam.
Physics 218: Final Class of 2:20pm May 7th, 2012. ules of the exam: 1. You have the full class period to complete the exam. 2. Formulae will be displayed in the big screen. You may NOT use any other formula
More informationChapter 5. The Electromagnetic Spectrum. What is visible light? What is visible light? Which of the following would you consider dangerous?
Which of the following would you consider dangerous? X-rays Radio waves Gamma rays UV radiation Visible light Microwaves Infrared radiation Chapter 5 Periodicity and Atomic Structure 2 The Electromagnetic
More informationChapter 46 Solutions
Chapter 46 Solutions 46.1 Assuming that the proton and antiproton are left nearly at rest after they are produced, the energy of the photon E, must be E = E 0 = (938.3 MeV) = 1876.6 MeV = 3.00 10 10 J
More informationASTR-1010: Astronomy I Course Notes Section IV
ASTR-1010: Astronomy I Course Notes Section IV Dr. Donald G. Luttermoser Department of Physics and Astronomy East Tennessee State University Edition 2.0 Abstract These class notes are designed for use
More informationPHYS 3313 Section 001 Lecture #14
PHYS 3313 Section 001 Lecture #14 Monday, March 6, 2017 The Classic Atomic Model Bohr Radius Bohr s Hydrogen Model and Its Limitations Characteristic X-ray Spectra 1 Announcements Midterm Exam In class
More informationElementary Particle Physics Glossary. Course organiser: Dr Marcella Bona February 9, 2016
Elementary Particle Physics Glossary Course organiser: Dr Marcella Bona February 9, 2016 1 Contents 1 Terms A-C 5 1.1 Accelerator.............................. 5 1.2 Annihilation..............................
More informationPHYSICS 113: Contemporary Physics Final Exam Solution Key (2016)
PHYSICS 113: Contemporary Physics Final Exam Solution Key (2016) 1. [25 points] (5 points each) Short Answers (a) The central reaction that governs the weak nuclear reactions of the sun reduces to: 4 p
More informationI. Multiple Choice Questions (Type-I)
I. Multiple Choice Questions (Type-I) 1. Which of the following conclusions could not be derived from Rutherford s α -particle scattering experiement? (i) Most of the space in the atom is empty. (ii) The
More informationPhotoionized Gas Ionization Equilibrium
Photoionized Gas Ionization Equilibrium Ionization Recombination H nebulae - case A and B Strömgren spheres H + He nebulae Heavy elements, dielectronic recombination Ionization structure 1 Ionization Equilibrium
More informationcgrahamphysics.com Particles that mediate force Book pg Exchange particles
Particles that mediate force Book pg 299-300 Exchange particles Review Baryon number B Total # of baryons must remain constant All baryons have the same number B = 1 (p, n, Λ, Σ, Ξ) All non baryons (leptons
More informationElectron Arrangement - Part 1
Brad Collins Electron Arrangement - Part 1 Chapter 8 Some images Copyright The McGraw-Hill Companies, Inc. Properties of Waves Wavelength (λ) is the distance between identical points on successive waves.
More informationGeorgia Institute of Technology CHEM 1310 revised 10/8/09 Spring The Development of Quantum Mechanics. ν (nu) = frequency (in s -1 or hertz)
The Development of Quantum Mechanics Early physicists used the properties of electromagnetic radiation to develop fundamental ideas about the structure of the atom. A fundamental assumption for their work
More informationQuantum Theory and Atomic Structure. Quantum Mechanics. Quantum Theory and Atomic Structure. 7.3 The Wave-Particle Duality of Matter and Energy
Chapter 7 Quantum Theory and Atomic Structure Chap 7-1 Quantum Theory and Atomic Structure 7.1 The Nature of Light 7.2 Atomic Spectra 7.3 The Wave-Particle Duality of Matter and Energy 7.4 The Quantum-Mechanical
More informationChapter 7. Quantum Theory and Atomic Structure. Quantum Mechanics. Chap 7-1
Chapter 7 Quantum Theory and Atomic Structure Chap 7-1 Quantum Theory and Atomic Structure 7.1 The Nature of Light 7.2 Atomic Spectra 7.3 The Wave-Particle Duality of Matter and Energy 7.4 The Quantum-Mechanical
More information11 Quantum theory: introduction and principles
Part 2: Structure Quantum theory: introduction and principles Solutions to exercises E.b E.2b E.3b E.4b E.5b E.6b Discussion questions A successful theory of black-body radiation must be able to explain
More informationAstronomy 1 Winter 2011
Astronomy 1 Winter 2011 Lecture 8; January 24 2011 Previously on Astro 1 Light as a wave The Kelvin Temperature scale What is a blackbody? Wien s law: λ max (in meters) = (0.0029 K m)/t. The Stefan-Boltzmann
More informationBecause light behaves like a wave, we can describe it in one of two ways by its wavelength or by its frequency.
Light We can use different terms to describe light: Color Wavelength Frequency Light is composed of electromagnetic waves that travel through some medium. The properties of the medium determine how light
More informationLecture 4. The Bohr model of the atom. De Broglie theory. The Davisson-Germer experiment
Lecture 4 The Bohr model of the atom De Broglie theory The Davisson-Germer experiment Objectives Learn about electron energy levels in atoms and how Bohr's model can be used to determine the energy levels
More informationPHYSICS 218 Exam 3 Fall, 2013
PHYSICS 218 Exam 3 Fall, 2013 Wednesday, November 20, 2013 Please read the information on the cover page BUT DO NOT OPEN the exam until instructed to do so! Name: Signature: Student ID: E-mail: Section
More informationFinal Exam Practice Solutions
Physics 390 Final Exam Practice Solutions These are a few problems comparable to those you will see on the exam. They were picked from previous exams. I will provide a sheet with useful constants and equations
More informationFinal Exam April 21, a) No books, notes, or other such materials are permitted.
Phys 5 Spring 004 Name: Final Exam April, 004 INSTRUCTIONS: a) No books, notes, or other such materials are permitted. b) You may use a calculator. c) You must solve all problems beginning with the equations
More informationwhere n = (an integer) =
5.111 Lecture Summary #5 Readings for today: Section 1.3 (1.6 in 3 rd ed) Atomic Spectra, Section 1.7 up to equation 9b (1.5 up to eq. 8b in 3 rd ed) Wavefunctions and Energy Levels, Section 1.8 (1.7 in
More informationProf. Jeff Kenney Class 4 May 31, 2018
Prof. Jeff Kenney Class 4 May 31, 2018 Which stellar property can you estimate simply by looking at a star on a clear night? A. distance B. diameter C. luminosity D. surface temperature E. mass you can
More informationEquilibrium Properties of Matter and Radiation
Equilibrium Properties of Matter and Radiation Temperature What is it? A measure of internal energy in a system. Measure from (1) velocities of atoms/molecules () population of excited/ionized states (3)
More informationBohr s Correspondence Principle
Bohr s Correspondence Principle In limit that n, quantum mechanics must agree with classical physics E photon = 13.6 ev 1 n f n 1 i = hf photon In this limit, n i n f, and then f photon electron s frequency
More informationExplain how line spectra are produced. In your answer you should describe:
The diagram below shows the line spectrum of a gas. Explain how line spectra are produced. In your answer you should describe: how the collisions of charged particles with gas atoms can cause the atoms
More informationTHE UNIVERSITY OF PRETORIA
PHY 255 THE UNIVERSITY OF PRETORIA FIRST SEMESTER, 2011 Campus: Hatfield PHYSICS 255 Modern Physics Exam Total: 70 (Time allowed: THREE hours Internal Examiner: M. van den Worm External Examiner: Q. Odendaal
More informationA few principles of classical and quantum mechanics
A few principles of classical and quantum mechanics The classical approach: In classical mechanics, we usually (but not exclusively) solve Newton s nd law of motion relating the acceleration a of the system
More informationAtomic Structure Ch , 9.6, 9.7
Ch. 9.2-4, 9.6, 9.7 Magnetic moment of an orbiting electron: An electron orbiting a nucleus creates a current loop. A current loop behaves like a magnet with a magnetic moment µ:! µ =! µ B " L Bohr magneton:
More informationPHYSICS 149: Lecture 22
PHYSICS 149: Lecture 22 Chapter 11: Waves 11.1 Waves and Energy Transport 11.2 Transverse and Longitudinal Waves 11.3 Speed of Transverse Waves on a String 11.4 Periodic Waves Lecture 22 Purdue University,
More informationA more comprehensive theory was needed. 1925, Schrödinger and Heisenberg separately worked out a new theory Quantum Mechanics.
Ch28 Quantum Mechanics of Atoms Bohr s model was very successful to explain line spectra and the ionization energy for hydrogen. However, it also had many limitations: It was not able to predict the line
More informationProblem Set 2 Solutions
Problem Set 2 Solutions Problem 1: A A hot blackbody will emit more photons per unit time per unit surface area than a cold blackbody. It does not, however, necessarily need to have a higher luminosity,
More informationElectromagnetic Radiation. Chapter 12: Phenomena. Chapter 12: Quantum Mechanics and Atomic Theory. Quantum Theory. Electromagnetic Radiation
Chapter 12: Phenomena Phenomena: Different wavelengths of electromagnetic radiation were directed onto two different metal sample (see picture). Scientists then recorded if any particles were ejected and
More informationPhysics 3204 UNIT 3 Test Matter Energy Interface
Physics 3204 UNIT 3 Test Matter Energy Interface 2005 2006 Time: 60 minutes Total Value: 33 Marks Formulae and Constants v = f λ E = hf h f = E k + W 0 E = m c 2 p = h λ 1 A= A T 0 2 t 1 2 E k = ½ mv 2
More informationPHYS 219 General Physics: Electricity, Light and Modern Physics
PHYS 219 General Physics: Electricity, Light and Modern Physics Final exam is scheduled on Thursday May 2 @ 8 10 AM In Physics 112 It will cover five Chapters 25, 27, 28, 29, and 30. Review lecture notes,
More informationPhysics 107: Ideas of Modern Physics
Physics 107: Ideas of Modern Physics Exam 3 Apr. 19, 2006 Name ID # Section # On the Scantron sheet, 1) Fill in your name 2) Fill in your student ID # (not your social security #) 3) Fill in your section
More informationPhysics 107: Ideas of Modern Physics
Physics 107: Ideas of Modern Physics Exam 3 Apr. 19, 2006 Name ID # Section # On the Scantron sheet, 1) Fill in your name 2) Fill in your student ID # (not your social security #) 3) Fill in your section
More informationAtomic Structure 11/21/2011
Atomic Structure Topics: 7.1 Electromagnetic Radiation 7.2 Planck, Einstein, Energy, and Photons 7.3 Atomic Line Spectra and Niels Bohr 7.4 The Wave Properties of the Electron 7.5 Quantum Mechanical View
More informationChapter 6. Electronic Structure of Atoms. The number & arrangement of e - in an atom is responsible for its chemical behavior.
Chapter 6 Electronic Structure of Atoms The number & arrangement of e - in an atom is responsible for its chemical behavior I) The Wave Nature of Light A) Electromagnetic Radiation Radiant Energy light,
More informationHarold s AP Physics Cheat Sheet 23 February Electricity / Magnetism
Harold s AP Physics Cheat Sheet 23 February 206 Kinematics Position (m) (rad) Translation Horizontal: x = x 0 + v x0 t + 2 at2 Vertical: y = y 0 + v y0 t 2 gt2 x = x 0 + vt s = rθ x = v / Rotational Motion
More informationChapter 7 QUANTUM THEORY & ATOMIC STRUCTURE Brooks/Cole - Thomson
Chapter 7 QUANTUM THEORY & ATOMIC STRUCTURE 1 7.1 The Nature of Light 2 Most subatomic particles behave as PARTICLES and obey the physics of waves. Light is a type of electromagnetic radiation Light consists
More informationChapter 8: Electrons in Atoms Electromagnetic Radiation
Chapter 8: Electrons in Atoms Electromagnetic Radiation Electromagnetic (EM) radiation is a form of energy transmission modeled as waves moving through space. (see below left) Electromagnetic Radiation
More informationParticle and Nuclear Physics. Outline. Structure of the Atom. History of Atomic Structure. 1 Structure of the Atom
Outline of 1 of Atomic Spectra of Helium Classical Atom of Existence of spectral lines required new model of atom, so that only certain amounts of energy could be emitted or absorbed. By about 1890, most
More informationPhysics 6C. Final Practice Solutions. Prepared by Vince Zaccone For Campus Learning Assistance Services at UCSB
Physics 6C Final Practice Solutions Use the following information for problems 1 and. A beam of white light with frequency between 4.00 x 10 14 Hz and 7.90 x 10 14 Hz is incident on a sodium surface, which
More information