Modern physics Physics of Astronomy, winter week 9 Star Date Astrophysics Ch.5: Interaction of light & matter Cyclotron frequency, Zeeman splitting Bohr.

Slides:



Advertisements
Similar presentations
Ch. 13 Electrons in Atoms Ch Models of the Atom
Advertisements

Where is the Electron Located?
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
7-1 Dr. Wolf’s CHM 101 Chapter 7 Quantum Theory and Atomic Structure.
Early Quantum Theory and Models of the Atom
Astrophysics Ch.5: Interaction of Light & Matter Physics of Astronomy, winter week 8 Star Date Plan for the last few weeks of winter quarter Modern physics.
Start EM Ch.5: Magnetostatics finish Modern Physics Ch.7: J=L+S Methods of Math. Physics, Thus. 24 Feb. 2011, E.J. Zita Magnetostatics: Lorentz Force and.
CHAPTER 6 ELECTRONIC STRUCTURE OF ATOMS. CHAPTER 6 TOPICS THE QUANTUM MECHANICAL MODEL OF THE ATOM USE THE MODEL IN CHAPTER 7 TO EXPLAIN THE PERIODIC.
Light and Stars Universe Ch.5 & 19, Astrophysics Ch.3 Physics of Astronomy, winter week 5 Star Date Star and Light pretest Overview of Universe Ch.5: Light.
Physics at the end of XIX Century Major Discoveries of XX Century
Physics of Astronomy, week 4, winter 2004 Astrophysics Ch.2 Star Date Ch.2.1: Ellipses (Matt #2.1, Zita #2.2) Ch.2.2: Shell Theorem Ch.2.3: Angular momentum.
Winter Physical Systems: Quantum and Modern physics Dr. E.J. Zita, The Evergreen State College, 6.Jan.03 Lab II Rm 2272,
Physics of Astronomy week 1 Thus. 6 April 2006
Electromagnetism and Energy
Modern physics and Quantum Mechanics Physical Systems, 8 Mar.2007 EJZ More angular momentum and H atom Compare to Bohr atom Applications: Bohr magneton,
The continuous spectrum of light Astrophysics Ch.3 Physics of Astronomy, winter week 5 Star Date Light tells us everything about stars Parallax Magnitude,
Lecture 2110/24/05. Light Emission vs. Absorption Black body.
Modern Physics 6a – Intro to Quantum Mechanics Physical Systems, Thursday 15 Feb. 2007, EJZ Plan for our last four weeks: week 6 (today), Ch.6.1-3: Schrödinger.
Wave mechanics in potentials Modern Ch.4, Physical Systems, 30.Jan.2003 EJZ Particle in a Box (Jason Russell), Prob.12 Overview of finite potentials Harmonic.
Modern Physics 6b Physical Systems, week 7, Thursday 22 Feb. 2007, EJZ Ch.6.4-5: Expectation values and operators Quantum harmonic oscillator → blackbody.
Quantum Physics Particle Nature of EM Radiation Photoelectric Effect Electronvolt Wave Nature of Particles De Broglie Equation.
Wave Nature of Light and Quantum Theory
Chapter 4 Arrangement of Electrons in Atoms
The Interaction of Light and Matter Spectral Lines Photons Rutherford-Bohr Model of the Atom Quantum Mechanics and Wave-Particle Duality.
Lecture 1. Birth of Quantum Mechanics. Historical Background of QM. Experiments, Theories & Student Presentation Engel, Ch. 1 Ratner & Schatz, Ch. 1 Quantum.
Concept #4 “Electrons in the Atom” Honors Chemistry 1.
Electromagnetic Spectrum Light as a Wave - Recap Light exhibits several wavelike properties including Refraction Refraction: Light bends upon passing.
Bohr Model Since the energy states are quantized, the light emitted from excited atoms must be quantized and appear as line spectra. After lots of math,
As an object gets hot, it gives Off energy in the form of Electromagnetic radiation.
Arrangement of Electrons in Atoms The Development of a New Atomic Model.
Electronic Structure of Atoms © 2009, Prentice-Hall, Inc. Chapter 7 Electronic Structure of Atoms.
The Interaction of Light and Matter
Chapter 6 Electronic Structure of Atoms. The Wave Nature of Light The light that we can see with our eyes, visible light, is an example of electromagnetic.
Methods of Math. Physics Thus. 2 Dec Brief review of forces, energy, oscillations Bohr atom – quantization of angular momentum E.J. Zita.
Quantum Theory and the Electronic Structure of Atoms Chapter 7.
Chapter 7 Atomic Structure & Periodicity. Electromagnetic Radiation O Waves (wavelength, frequency & speed) O  c (page 342: #39) O Hertz O Max Planck.
ATOMS Quantized Energy 1.Bohr model of the atom 2.Standing waves 3.Quantum energy of colors.
Physics 1202: Lecture 31 Today’s Agenda Announcements: Extra creditsExtra credits –Final-like problems –Team in class HW 9 this FridayHW 9 this Friday.
Quantum Theory and the Electronic Structure of Atoms Chapter 7 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
A brief presentation on the history of the atom Dalton: “Matter indeed, seems to consist of elementary lumpy particles”
4: Introduction to Quantum Physics
Chapter 7: Atoms and Light. Low ν High ν Electromagnetic Radiation.
Modern Physics Ch.7: H atom in Wave mechanics Methods of Math. Physics, 27 Jan 2011, E.J. Zita Schrödinger Eqn. in spherical coordinates H atom wave functions.
Physics of Astronomy week 4, winter 2004 Celestial Mechanics Star Date Review motion of Moon and Mars Starry Night animations Jupiter’s size and distance.
Class Notes-Bohr & New Atomic Model (Chapter 4, Section 1)
Physics Lecture 11 3/2/ Andrew Brandt Monday March 2, 2009 Dr. Andrew Brandt 1.Quantum Mechanics 2.Schrodinger’s Equation 3.Wave Function.
1 2. Atoms and Electrons How to describe a new physical phenomenon? New natural phenomenon Previously existing theory Not explained Explained New theoryPredicts.
Unit 12: Part 2 Quantum Physics. Overview Quantization: Planck’s Hypothesis Quanta of Light: Photons and the Photoelectric Effect Quantum “Particles”:
Chapter 33 Early Quantum Theory and Models of Atom.
Physics of Astronomy- spring Dr. E.J. Zita, The Evergreen State College, 29.Mar.2004 Lab II Rm 2272,
Section 2.2 and Chapter 7 Electron Configurations and Waves.
Physics 1202: Lecture 34 Today’s Agenda Announcements: Extra creditsExtra credits –Final-like problems –Team in class –Teams 5 & 6 HW 10 due FridayHW 10.
Light Light is a kind of electromagnetic radiation, which is a from of energy that exhibits wavelike behavior as it travels through space. Other forms.
Properties of light spectroscopy quantum hypothesis hydrogen atom Heisenberg Uncertainty Principle orbitals ATOMIC STRUCTURE Kotz Ch 7 & Ch 22 (sect 4,5)
Electron Configuration
Atomic Structure Figure 6.27.
Atomic Emission Spectra and Quantum mechanical Model
Ap Chemistry Due Next Class: Reading & Proof of reading
Atomic Theory.
Historical Overview of Quantum Mechanical Discoveries
Particles and Waves.
Physics of Astronomy Tuesday, winter week 8 (28 Feb.06)
Arrangement of electrons
Lectures written by John Kotz
Light and Energy Electromagnetic Radiation is a form of energy that is created through the interaction of electrical and magnetic fields. It displays wave-like.
Ch. 13 Electrons in Atoms Ch Models of the Atom
Properties of Light.
Quantum Theory & the Atom
Development of a New Atomic Model
c = speed of light (ms-1, constant)
Presentation transcript:

Modern physics Physics of Astronomy, winter week 9 Star Date Astrophysics Ch.5: Interaction of light & matter Cyclotron frequency, Zeeman splitting Bohr atom, quantum numbers Minilectures Portfolio/eval preparation

Astro. Ch.5: Interaction of light & matter History of Light quantization: Stefan-Boltzmann blackbody had UV catastrophe Planck quantized light, and solved blackbody problem Einstein used Planck’s quanta to explain photoelectric effect Compton effect demonstrated quantization of light hc/ = K max + 

Astro. Ch.5: Interaction of light & matter History of atomic models: Thomson discovered electron, invented plum-pudding model Rutherford observed nuclear scattering, invented orbital atom Bohr used deBroglie’s matter waves, quantized angular momentum, for better H atom model. E n = E/n 2 Bohr model explained observed H spectra, derived phenomenological Rydberg constant Quantum numbers n, l, m l (Zeeman effect) Solution to Schrodinger equation showed that E n = E/  l(l+1) Pauli proposed spin (m s =  1/2), and Dirac derived it

Improved Bohr model Solution to Schrodinger equation showed that E n = E/  l(l+1), Where l = orbital angular momentum quantum number (l<n). Almost the same energy for l=n-1, and for high n.

Spinning particles shift energies in B fields Cyclotron frequency: An electron moving with speed v perpendicular to an external magnetic field feels a Lorentz force: F=ma (solve for  =v/r) Compare to Zeeman effect. See HW hints for CO Ch.5

week 9: Monday Minilectures Astrophysics Ch.5: Interaction of Light and Matter Team 1: Problem 5.4, photoelectric effect, Chelsea + Brian Team 2: Problem 5.9, electrical vs gravitational forces, Erin & Mary Team 3: Problem 5.14, white dwarf and uncertainty principle, Jared + Joey (This is a really easy problem. Feel free to add another if you like.) Team 4: Problem 5.17, Zeeman effect, Jenny + Tristen HW due Mon.8.March includes Giancoli problems we did in class last Thus.26.Feb. Do you want to turn these in earlier? Giancoli Ch.39 # 7,9; Ch.40 # 45, 46 Carroll + Ostlie Ch.5 # 4, 9, 14, 16, 17

week 9: Thursday Minilectures Boas: Partial differentiation and series. Tuesday: Overview and series: Zita, Ch.1. Problems Sec.15 p. 39 # 28, 29 Thursday: Boas Ch.4, PD: Do at least one of your problems in class. HW due Tues.9.March. Zita: overview lecture, Sec.1 Team 1: Sec.3, total differentials, Example p.151 Team 2: Sec.4, approximations, Prob.7(p.156), 13-8 (p.198) Team 3: Sec.5, Chain rule, Prob 1, 3, 6 (p.158) Team 4: Sec.6, Implicit differentiation, Prob.5, 6 (p.160) Team 5: Sec.8, Max/min, Prob.11 (p.171) 4.8 Prob.1 (Zita)