Physics 2170 – Spring 20091 Bohr model and Franck-Hertz experiment Homework solutions will be up this afternoon.

Slides:



Advertisements
Similar presentations
Cphys351 c4:1 Chapter 4: Atomic Structure The Nuclear Atom The Atom as the smallest division of an element quantization of electric charge oil drop experiments.
Advertisements

1 My Chapter 27 Lecture. 2 Chapter 27: Early Quantum Physics and the Photon Blackbody Radiation The Photoelectric Effect Compton Scattering Early Models.
Quantum Physics ISAT 241 Analytical Methods III Fall 2003 David J. Lawrence.
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 27: Early Quantum Physics and.
Early Quantum Theory and Models of the Atom
Chapter 27: Early Quantum Physics and the Photon
BUSINESS 1.EXAM 2THURSDAY NOVEMBER 4, MATERIAL COVERED: CHAPTERS 4, 5 & 6 3.TIME:7:00PM-8:00PM 4.WHERE:(TO BE ANNOUNCED LATER) 5.WHAT TO BRING:CALCULATOR,
1 Light as a Particle The photoelectric effect. In 1888, Heinrich Hertz discovered that electrons could be ejected from a sample by shining light on it.
Hydrogen Atom Coulomb force “confines” electron to region near proton => standing waves of certain energy + -
 When a gas in a tube is subjected to a voltage, the gas ionizes, and emits light.  We can analyze that light by looking at it through a spectroscope.
Physics 6C Energy Levels Bohr Model of the Atom Prepared by Vince Zaccone For Campus Learning Assistance Services at UCSB.
Wednesday, Sept. 26, 2012 PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #9 Wednesday, Sept. 26, 2012 Dr. Jaehoon Yu The Bohr.
1 Light as a Particle In 1888, Heinrich Hertz discovered that electrons could be ejected from a sample by shining light on it. This is known as the photoelectric.
Phys 102 – Lecture 25 The quantum mechanical model of light.
Physics at the end of XIX Century Major Discoveries of XX Century
Bohr Model. Hydrogen Model  A hydrogen atom is a single electron and proton. One negative charge One positive charge  Assume that the discrete energies.
What’s wrong with this picture? The attractive Coulomb force between the positive nucleus and the orbiting electron could provide the attractive force.
Spectra of Atoms When an atom is excited, it emits light. But not in the continuous spectrum as blackbody radiation! The light is emitted at discrete wavelengths.
Dr. Jie ZouPHY Chapter 42 Atomic Physics. Dr. Jie ZouPHY Outline Atomic spectra of gases Early models of the atom Bohr’s model of the hydrogen.
Quantum Physics. Black Body Radiation Intensity of blackbody radiation Classical Rayleigh-Jeans law for radiation emission Planck’s expression h =
Absorption / Emission of Photons and Conservation of Energy E f - E i = hvE i - E f = hv hv.
Models of the Atom Physics 1161: Pre-Lecture 30 Sections 31-1 – 31-4.
Atomic physics PHY232 Remco Zegers Room W109 – cyclotron building
Cutnell/Johnson Physics 7 th edition Classroom Response System Questions Chapter 39 More about Matter Waves Reading Quiz Questions.
Early Quantum Theory and Models of the Atom
Atomic Physics Introduction: Although the hydrogen atom is the simplest atomic system, it’s especially important for several reasons: The quantum numbers.
Physics 1C Lecture 29A.
Atoms RPI - ERTH 2330 The Basis of All Materials.
Goal: To understand the atom Objectives: 1)To learn that The basics of Atomic Physics isn’t so bad 2)To understand the Bohr atom 3)To understand Electron.
Law of gravitation Kepler’s laws Energy in planetary motion Atomic spectra and the Bohr model Orbital motion (chapter eleven)
Lecture 11b Atomic Physics & Nuclear Reactions Copyright © 2009 Pearson Education, Inc.
Copyright © 2010 Pearson Education, Inc. ConcepTest Clicker Questions Chapter 31 Physics, 4 th Edition James S. Walker.
Physics Education Department - UNS 1 Planetary model of atom Positive charge is concentrated in the center of the atom (nucleus) Atom has zero net charge:
Physics Education Department - UNS 1 From Last Time… Light waves are particles and matter particles are waves! Electromagnetic radiation (e.g. light) made.
Chapter 7 The Quantum-Mechanical Model of the Atom
Physics 2170 – Spring Quantum tunneling and review 2 nd exam is tomorrow, April 7 in MUEN 0046 from 7:30.
28.3 THE BOHR THEORY OF HYDROGEN At the beginning of the 20th century, scientists were puzzled by the failure of classical physics to explain the characteristics.
Chapter 3: Spectral lines in stars. Emission and absorption of light Emission line spectrum Continuous spectrum (thermal, blackbody) Independent of composition.
The spectral series of hydrogen, on a logarithmic scale.
Physics 2170 – Spring Franck-Hertz experiment, Bohr atom, de Broglie waves Homework solutions for Homework.
The Bohr Model and The principal Quantum Number Physics 12 Adv.
Chapter 28:Atomic Physics
Rutherford’s Model: Conclusion Massive nucleus of diameter m and combined proton mass equal to half of the nuclear mass Planetary model: Electrons.
Thurs. Nov. 19, 2009Phy208 Lect Exam 3 is Thursday Dec. 3 (after Thanksgiving) Students w / scheduled academic conflict please stay after class Tues.
Bohr Model and Quantum Theory
1 PHYS 3313 – Section 001 Lecture #14 Monday, Mar. 3, 2014 Dr. Jaehoon Yu Bohr’s Hydrogen Model and Its Limitations Characteristic X-ray Spectra Hydrogen.
Sydney Opera House Opens (1973) READING: Chapter 8 sections 1 – 2 READING: Chapter 8 sections 1 – 2 HOMEWORK – DUE TUESDAY 10/20/15 HOMEWORK – DUE TUESDAY.
Physics 2170 – Spring Bohr model of the atom Problem solving sessions M3-5 and T3-5. Announcements: Niels.
Physics 102: Lecture 24, Slide 1 Bohr vs. Correct Model of Atom Physics 102: Lecture 24 Today’s Lecture will cover Ch , 28.6.
Atomic Spectra and Electron Orbitals. The Classical Atom Electrons orbited the nucleus. Electrons orbited the nucleus. Problem!! Problem!! Accelerating.
Atomic Structure. Model A: The plum pudding model J.J. Thompson Negative charges like raisins in plumb pudding Positive charge is spread out like the.
Ch2 Bohr’s atomic model Four puzzles –Blackbody radiation –The photoelectric effect –Compton effect –Atomic spectra Balmer formula Bohr’s model Frank-Hertz.
Unit 12: Part 2 Quantum Physics. Overview Quantization: Planck’s Hypothesis Quanta of Light: Photons and the Photoelectric Effect Quantum “Particles”:
Quantization part 2 –particles as waves ch 37. The world – a) matter - atoms nucleus of tightly packed protons and neutrons. Protons-positive charge electrons.
Chapter 33 Early Quantum Theory and Models of Atom.
Tues. Nov. 18, 2008Phy208 Lect Exam 3 is Tuesday Nov. 25 Students w / scheduled academic conflict please stay after class Tues. Nov. 18 (TODAY) to.
1 Review Part 2 Energy is conserved so E = K + U If potential energy increases, kinetic energy must decrease. Kinetic energy determines the wavelength.
Atomic and Molecular Spectra.  Atoms are very small,  Atoms are stable  Atoms contain negatively charge electrons, but are neutral(because matters.
The Atomic Models of Thomson and Rutherford Rutherford Scattering The Classic Atomic Model The Bohr Model of the Hydrogen Atom Successes & Failures of.
PHYS 3313 – Section 001 Lecture #14
Bohr Model Of Atom.
What value of wavelength is associated with the Lyman series for {image} {image} 1. {image}
Derivation of the Rydberg Constant
General Physics (PHY 2140) Lecture 33 Modern Physics Atomic Physics
II. Bohr Model of the Atom (p )
The Bohr Model (1913) revolve sun energy
PHYS 420-SPRING 2006 Dennis Papadopoulos LECTURE 12 BOHR’S ATOM.
PHYS 3313 – Section 001 Lecture #14
II. Bohr Model of the Atom (p )
The Rutherford model of the atom
Presentation transcript:

Physics 2170 – Spring Bohr model and Franck-Hertz experiment Homework solutions will be up this afternoon. Next weeks homework will be available by noon tomorrow. On Friday, I would like to take a vote on when we should have the other midterm exam. Either 3/31 or 4/7. Check your schedules. Today we will be analyzing the Bohr model with clicker questions. Announcements: James Franck: Gustav Hertz:

Physics 2170 – Spring −2 eV −3 eV −5 eV 0 eV −7 eV −5 eV −8 eV What energy levels for electrons are consistent with this spectrum? Electron Energy levels: 5ev 3ev 2ev Photon energy nm −5 eV −7 eV −10 eV 0 eV 5 eV 7 eV 10 eV 0 eV−10 eV A B C D 5 eV 3 eV 2 eV 0 eV E Clicker question 1 Set frequency to DA

Physics 2170 – Spring is the Bohr radius where Quantizing angular momentum leads to a quantization of radius: Why are only certain energy levels allowed? Quantizing radius leads to a quantization of energy: Bohr postulated that angular momentum was quantized so: where where E R is the Rydberg energy:

Physics 2170 – Spring A.Opposite charges attract with a force inversely proportional to the square of the distance between them. B.The force on an object is equal to its mass times its acceleration. C.Accelerating charges radiate energy. D.Particles have a well-defined position and momentum. E.All of the above. Clicker question 2 Set frequency to DA Which of the following principles of classical physics is violated in deriving the Bohr model of the atom? Note that A & B were used in the derivation of the Bohr model.

Physics 2170 – Spring Hydrogen energy levels Using the formula for energy Bohr could calculate the various transitions and they agreed with the generalized Balmer formula. Bohr’s calculation of hydrogen energy levels Photon energy is given by:

Physics 2170 – Spring A.n=1 B.n=1, n=2, or n=3 C.n=3 D.n=2 or n=3 E.Any of the states Clicker question 3 Set frequency to DA An atom with the energy levels shown is initially in the ground state. A free electron with an energy of 16.0 eV hits the atom. What possible states could the atom be in after the interaction? −2 eV −20 eV −5 eV −10 eV −1 eV n=4 n=1 n=3 n=2 n=5 Electron jumps back to low energy Atomic electron excited to higher energy and free electron loses same amount of energy. Free electron hits atom e e Less KE e If the atom goes to n=1, 2, or 3, the free electron will lose 0 eV, 10 eV, or 15 eV of kinetic energy.

Physics 2170 – Spring A.n=1 B.n=1, n=2, or n=3 C.n=3 D.n=2 or n=3 E.Any of the states Clicker question 4 Set frequency to DA An atom with the energy levels shown is initially in the ground state. A photon with an energy of 16.0 eV hits the atom. What possible states could the atom be in after the interaction? −2 eV −20 eV −5 eV −10 eV −1 eV n=4 n=1 n=3 n=2 n=5 For the free electron, whatever energy is absorbed by the atom is deducted from the free electron’s kinetic energy. For photons, the photon is absorbed and so it must transfer all of its energy to the atom. Otherwise energy would not be conserved. Therefore, atoms can only absorb photons with an energy that will exactly move the atom to another energy level.

Physics 2170 – Spring A.1 eV B.1 eV, 2 eV, 5 eV, 10 eV C.10 eV D.10 eV, 15 eV, 18 eV E.10 eV, 15 eV, 18 eV, 25 eV Clicker question 5 Set frequency to DA An atom with the energy levels shown is initially in the ground state. Which of the following is the most complete list of photon energies that can be absorbed by the atom? −2 eV −20 eV −5 eV −10 eV −1 eV n=4 n=1 n=3 n=2 n=5 Any photon with an energy ≥ 20 eV will ionize the atom. The electron will escape. Since a free electron can have any energy, any photon with energy ≥ 20 eV can be absorbed by the atom. Photons with energy of 10 eV, 15 eV, 18 eV, 19 eV will cause the electron to jump to the n=2, n=3, n=4, n=5 energy level. 20 eV will go into ejecting the electron and the rest will go into the free electron’s kinetic energy. Similar to the photoelectric effect.

Physics 2170 – Spring Hydrogen like ions Atoms which have only one electron can be analyzed much like the hydrogen atom. An atom with atomic number Z with Z-1 electrons removed is a hydrogen like ion The (Coulomb) force on the electron is The increase in the force results in tighter orbits and a deeper potential well, reducing the energy (more negative).

Physics 2170 – Spring A.3.4 eV B.13.6 eV C.27.2 eV D.54.4 eV E.None of the above Clicker question 6 Set frequency to DA A single electron is in the n=2 energy level around a helium nucleus (He + ). What is the minimum energy photon that can remove this electron? The atomic number of helium is Z=2 and the electron is in the n=2 energy level. So the energy of the state is The value |E n | is also referred to as the binding energy since it is a measure of how bound the electron is. It takes that amount of energy to free the electron (break its bond to the proton).