From Last Time. Electron diffraction. Making a particle out of waves. Planetary model of atom. Using quantum mechanics ev 1/ 2 nm E kinetic

Similar documents
Wavelength of 1 ev electron

Energy levels. From Last Time. Emitting and absorbing light. Hydrogen atom. Energy conservation for Bohr atom. Summary of Hydrogen atom

From Last Time. Summary of Photoelectric effect. Photon properties of light

General Physics (PHY 2140)

Chapter 28. Atomic Physics

An electron can be liberated from a surface due to particle collisions an electron and a photon.

Chapter 29 Atomic Physics. Looking Ahead. Slide 29-1

Chapter 27 Early Quantum Theory and Models of the Atom Discovery and Properties of the electron

LECTURE 23 SPECTROSCOPY AND ATOMIC MODELS. Instructor: Kazumi Tolich

Mystery #3 Emission Spectra of Elements. Tube filled with elemental gas. Voltage can be applied across both ends, this causes the gas to emit light

A fluorescent tube is filled with mercury vapour at low pressure. After mercury atoms have been excited they emit photons.

Physics 1C Lecture 29A. Finish off Ch. 28 Start Ch. 29

8 Wavefunctions - Schrödinger s Equation

Earlier we learned that hot, opaque objects produce continuous spectra of radiation of different wavelengths.

General Physics (PHY 2140)

Franck-Hertz experiment, Bohr atom, de Broglie waves Announcements:

The Bohr Model of Hydrogen

Chapter 39. Particles Behaving as Waves

Chapter 28. Atomic Physics

ATOMIC PHYSICS. history/cosmology/tools/ tools-spectroscopy.htm CHAPTER 9 - FROM SPECTROSCOPY TO ATOMS

Radiation - Electromagnetic Waves (EMR): wave consisting of oscillating electric and magnetic fields that move at the speed of light through space.

1/l = R(1/n' 2-1/n 2 ) n > n', both integers R = nm -1

Planck s Quantum Hypothesis Blackbody Radiation

Atoms. Radiation from atoms and molecules enables the most accurate time and length measurements: Atomic clocks

Optical Spectroscopy and Atomic Structure. PHYS 0219 Optical Spectroscopy and Atomic Structure 1

Modern Physics Part 3: Bohr Model & Matter Waves

Physics 102: Lecture 24. Bohr vs. Correct Model of Atom. Physics 102: Lecture 24, Slide 1

PHY293 Lecture #15. November 27, Quantum Mechanics and the Atom

Atomic Structure. Standing Waves x10 8 m/s. (or Hz or 1/s) λ Node

THE NATURE OF THE ATOM. alpha particle source

hf = E 1 - E 2 hc = E 1 - E 2 λ FXA 2008 Candidates should be able to : EMISSION LINE SPECTRA

Chapter 37 Early Quantum Theory and Models of the Atom

Atoms and Spectroscopy

Preview. Atomic Physics Section 1. Section 1 Quantization of Energy. Section 2 Models of the Atom. Section 3 Quantum Mechanics

Physics 1C Lecture 29B

Lecture PowerPoints. Chapter 27 Physics: Principles with Applications, 7th edition Giancoli

Ch. 7 The Quantum Mechanical Atom. Brady & Senese, 5th Ed.

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

Physical Electronics. First class (1)

PHYS 3313 Section 001 Lecture #14

Bohr s Correspondence Principle

Quantum and Atomic Physics - Multiple Choice

Particle nature of light & Quantization

Physics 1C. Modern Physics Lecture

The Hydrogen Atom According to Bohr

Chapter 1 The Bohr Atom

OpenStax-CNX module: m The Bohr Model. OpenStax College. Abstract

Semiconductor Physics and Devices

Stellar Astrophysics: The Interaction of Light and Matter

Energy in Planetary Orbits

College Physics B - PHY2054C

EP225 Lecture 31 Quantum Mechanical E ects 1

Explain how line spectra are produced. In your answer you should describe:

UNIT : QUANTUM THEORY AND THE ATOM

Physics 25 Chapter 29 Dr. Alward

Atomic Structure 11/21/2011

Atom and Quantum. Atomic Nucleus 11/3/2008. Atomic Spectra

Models of the Atom. Spencer Clelland & Katelyn Mason

Quantum Mechanics. Exam 3. Photon(or electron) interference? Photoelectric effect summary. Using Quantum Mechanics. Wavelengths of massive objects

PC1144 Physics IV. Atomic Spectra

Discovery of the Atomic Nucleus. Conceptual Physics 11 th Edition. Discovery of the Electron. Discovery of the Atomic Nucleus

Sharif University of Technology Physics Department. Modern Physics Spring 2016 Prof. Akhavan

Final Exam: Thursday 05/02 7:00 9:00 pm in STEW 183

Light & Matter Interactions

Ch 7 Quantum Theory of the Atom (light and atomic structure)

PHYSICS 3204 PUBLIC EXAM QUESTIONS (Quantum pt.1)

Light & Matter Interactions

Chem 467 Supplement to Lecture 19 Hydrogen Atom, Atomic Orbitals

3. Particle nature of matter

RED. BLUE Light. Light-Matter

The Atom. Result for Hydrogen. For example: the emission spectrum of Hydrogen: Screen. light. Hydrogen gas. Diffraction grating (or prism)

Atom Physics. Chapter 30. DR JJ UiTM-Cutnell & Johnson 7th ed. 1. Model of an atom-the recent model. Nuclear radius r m

10/27/2017 [pgs ]

CHAPTER 27 Quantum Physics

Particle and Nuclear Physics. Outline. Structure of the Atom. History of Atomic Structure. 1 Structure of the Atom

Lecture 11 Atomic Structure

20th Century Atomic Theory- Hydrogen Atom

Class XII_Delhi_Physics_Set-1

Chapters 28 and 29: Quantum Physics and Atoms Questions & Problems

Chapter 1. From Classical to Quantum Mechanics

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

Chapter 37 Early Quantum Theory and Models of the Atom. Copyright 2009 Pearson Education, Inc.

QUANTUM MECHANICS Chapter 12

LECTURE # 19 Dennis Papadopoulos End of Classical Physics Quantization Bohr Atom Chapters 38 39

3/26/10. Light carries energy in waves. Units for wavelength, λ meter 1 nm = 10-9 m 1 Angstrom (1 Å) = m

Energy levels and atomic structures lectures chapter one

Emission Spectroscopy

Early Quantum Theory and Models of the Atom

In the early years of the twentieth century, Max Planck, Albert Einstein, Louis de Broglie, Neils

Bohr model and Franck-Hertz experiment

Physics 116. Nov 22, Session 32 Models of atoms. R. J. Wilkes

CHM 111 Unit 7 Sample Questions

Nicholas J. Giordano. Chapter 29. Atomic Theory. Marilyn Akins, PhD Broome Community College

Chapter 6. Quantum Theory and the Electronic Structure of Atoms Part 1

Lecture 4. The Bohr model of the atom. De Broglie theory. The Davisson-Germer experiment

CHEMISTRY Topic #1: Atomic Structure and Nuclear Chemistry Fall 2017 Dr. Susan Findlay See Exercises 3.1 to 3.3

Chapter 7: The Quantum-Mechanical Model of the Atom

LECTURE # 17 Modern Optics Matter Waves

The Hydrogen Spectrum

Chapter 27 Lecture Notes

Transcription:

From Last Time All objects show both wave-like properties and particle-like properties. Electromagnetic radiation (e.g. light) shows interference effects (wave-like properties), but also comes in discrete photons of energy hf (particle-like properties) Matter clearly shows particle-like properties, but also shows interference and diffraction effects (wave-like properties). Electron diffraction Wavelength determined by electron momentum Planck's constant Wavelength = momentum Momentum determined by electron energy Energy determined by accelerating voltage (energy in electron-volts (ev ) = voltage) Wavelength in nm = 1.23 ev 1/ 2 nm E kinetic Energy in ev 1.23 ev 1/ 2 nm Wavelength in nm = E kinetic Increasing the energy decreases the wavelength. When electron wavelength comparable to differences in path length, destructive interference can occur. Appears as spatial directions in which reflected electrons are never seen. Making a particle out of waves 440 Hz + 439 Hz 440 Hz + 439 Hz + 438 Hz 440 Hz + 439 Hz + 438 Hz + 437 Hz + 436 Hz Using quantum mechanics Planetary model of atom Quantum mechanics makes astonishingly accurate predictions of the physical world Can apply to atoms, molecules, solids. An early success was in understanding Structure of atoms Interaction of electromagnetic radiation with atoms Positive charge is concentrated in the center of the atom ( nucleus ) Atom has zero net charge: Positive charge in nucleus cancels negative electron charges. Electrons orbit the nucleus like planets orbit the sun (Attractive) Coulomb force plays role of gravity nucleus electrons 1

Planetary model Bohr also retained the particle picture. Since electron is in a circular orbit, it s velocity is continually changing direction (centripetal acceleration = v 2 /r) The source of this acceleration is the Coulomb force between the positive nucleus and the negative electron ke 2 /r 2 acceleration = v 2 r = Force mass Orbital speed Coulomb force = k e2 mr 2 Difference between atoms No net charge to atom number of orbiting negative electrons same as number of positive protons in nucleus Different elements have different number of orbiting electrons Hydrogen: 1 electron Helium: 2 electrons Copper: 29 electrons Uranium: 92 electrons! Organized into periodic table of elements Problems with planetary model Elements in same column have similar chemical properties No clear predictions of size of electron orbits No explanation of why different elements have different chemical properties. Has particular problems with predictions for emission of radiation by atoms. Line spectra from atoms Atoms do emit radiation, but only at certain discrete frequencies. Frequencies are unique for different atoms Spectrum is an atomic fingerprint, used to identify atoms (e.g. in space). Hydrogen Mercury Planetary model and radiation Circular motion of orbiting electrons causes them to emit electromagnetic radiation with frequency equal to orbital frequency. Same mechanism by which radio waves are emitted by electrons in a radio transmitting antenna. In an atom, the emitted electromagnetic wave carries away energy from the electron. Electron predicted to continually lose energy. The electron would eventually spiral into the nucleus However most atoms are stable! Wavelength (nm) 2

Hydrogen emission spectrum Hydrogen is simplest atom One electron orbiting around one proton. The Balmer Series of emission lines empirically given by 1 1 = R H λ m 2 1 2 n 2 n = 4, λ = 486.1 nm Hydrogen n=4 n = 3, λ = 656.3 nm n=3 Hydrogen emission This says hydrogen emits only photons of a particular wavelength, frequency Photon energy = hf, so this means a particular energy. Conservation of energy: Energy carried away by photon is lost by the orbiting electron. Retained planetary picture Only certain orbits are stable Radiation emitted only when electron jumps from one stable orbit to another. Here, the emitted photon has an energy of E initial -E final Stable orbit Stable orbit The Bohr atom E initial E final Photon Energy conservation for Bohr atom Each orbit has a specific energy E n =-13.6/n 2 Photon emitted when electron jumps from high energy to low energy orbit. E i E f = h f Photon absorption induces electron jump from low to high energy orbit. E f E i = h f Agrees with experiment! Example: the Balmer series All transitions terminate at the n=2 level Each energy level has energy E n =-13.6 / n 2 ev E.g. n=3 to n=2 transition Emitted photon has energy E photon = 13.6 13.6 3 2 2 2 =1.89 ev Emitted wavelength E photon = hf = hc λ, λ = hc 1240 ev nm = = 656 nm E photon 1.89 ev Compare the wavelength of a photon produced from a transition from n=3 to n=1 with that of a photon produced from a transition n=2 to n=1. A. λ 31 < λ 21 B. λ 31 = λ 21 C. λ 31 > λ 21 E 31 > E 21 so λ 31 < λ 21 Spectral Question n=3 n=2 n=1 3

Fig 14.16, p. 442 Slide 18 But why? Why should only certain orbits be stable? Bohr had a complicated argument based on correspondence principle That quantum mechanics must agree with classical results when appropriate (high energies, large sizes) But incorporating wave nature of electron gives a natural understanding of these quantized orbits Electron waves in an atom Electron is a wave. In the orbital picture, its propagation direction is around the circumference of the orbit. Wavelength = h / p (p=momentum, and energy determined by momentum) How can we think about waves on a circle? Waves on a circle Wavelength Blow in here Here is my ToneNut Like a flute, but in the shape of a doughnut. Produces tone at particular pitch. Air inside must be vibrating at that frequency (red line) Sound wave inside has corresponding wavelength λ=v/f What determines the frequency/wavelength of the sound? Standing waves Easier to think about in a normal wind instrument, or vibrations of a string. Wind instrument with particular fingering plays a particular pitch, particular wavelength. Guitar string vibrates at frequency, wavelength determined by string length. λ=l/2 f=v/λ Standing Waves Standing Waves on a String When a traveling wave reflects back on itself, it creates traveling waves in both directions The wave and its reflection interfere according to the superposition principle With exactly the right frequency, the wave will appear to stand still This is called a standing wave Zeros of the wave must occur at the ends of the string because these points are fixed Zeroes occur every halfwavelength. Zeroes are called nodes of the wave 4

Fig 14.18, p. 443 Slide 25 Standing waves: wind instrument Ends are open, anit-nodes at ends. Integer number of half-wavelengths fit inside the instrument. Standing Waves on a String, cont. Only possible waves are standing waves. The frequency of first possible standing wave is called the fundamental frequency All possible standing wave frequencies are an integer multiple of the fundamental frequency. Called harmonics L λ=2l λ=2l/2 λ=3l/2 Integer number of halfwavelengths fits in the space. Why not other wavelengths? Waves in the string that are not in the harmonic series are quickly damped out In effect, when the string is disturbed, it selects the standing wave frequencies Reflection from end interferes destructively and cancels out wave. Same happens in a wind instrument and in an atom! Waves on a ring Wavelength Condition on a ring slightly different. Integer number of wavelengths required around circumference. Otherwise destructive interference occurs when wave travels around ring and interferes with itself. Electron standing-waves on an atom Wave representing electron Electron wave extends around circumference of orbit. Only integer number of wavelengths around orbit allowed. Wave representing electron Electron Standing Waves This gives a condition on the electron wave. Integer number of debroglie wavelengths must fit on circumference of the orbit. Circumference = (2π)x(orbit radius) = 2πr So condition is 2πr = nλ = n h p = n h mv Momentum p = (mass)x(velocity) = mv Thus wave considerations give a relation between orbit radius and electron momentum. 5

Particle properties: electron is still orbiting! Bohr also retained the particle picture. Since electron is in a circular orbit, it s velocity is continually changing direction (centripetal acceleration = v 2 /r = Force/mass) The force causing this acceleration is the Coulomb force ke 2 /r 2 between the positive nucleus and the negative electron Thus particle considerations also give a relation between orbit radius and electron momentum. Toward quantized orbits Electron standing wave: Pronounced h-bar, h = h 2π Orbit circumference Electron planetary orbit: 2πr = nλ = n h p v 2 r centripetal acceleration Integer # of debroglie wavelengths p 2 = n 2 h 2 r 2 = k e2 mr 2 Coulomb force / mass p 2 = mke2 r Only certain radius orbits permitted by quantum mechanics Equate wave result with particle result orbital radius is quantized Permitted radii: h 2 r n = n 2 mke = n 2 a 2 o a o =0.529Å = Bohr radius r 3 = 9a o = 4.76Å r 4 = 16a o = 8.46Å Orbit labeled by quantum number n Referred to as a quantum state Electron has different properties in each quantum state Different orbital radius Different wavelength (momentum) Different energy Quantum States Energy of the quantum state Electron energy includes Potential energy (from Coulomb interaction) Kinetic energy (energy of motion, from momentum) Combining these contributions, Bohr found that allowed electron energies are quantized as E n = 13.6 n 2 ev Just what is required to explain spectral lines 6