Wednesday, Oct. 2, 2013PHYS 3313-001, Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #11 Wednesday, Oct. 2, 2013 Dr. Amir Farbin Importance.

Slides:



Advertisements
Similar presentations
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Advertisements

Ch 9 pages ; Lecture 20 – Particle and Waves.
Early Quantum Theory and Models of the Atom
AP Physics Chapter 28 Quantum Mechanics and Atomic Physics
Monday, Oct. 1, 2012PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #10 Monday, Oct. 1, 2012 Dr. Jaehoon Yu Importance of Bohr’s.
The Electronic Structures of Atoms Electromagnetic Radiation
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.
Quantum Theory of Light A TimeLine. Light as an EM Wave.
Monday, Sept. 24, 2012PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #8 Monday, Sept. 24, 2012 Dr. Jaehoon Yu Atomic Model of.
1.X-Ray Scattering 2.De Broglie Waves 3.Electron Scattering 4.Wave Motion 5.Waves or Particles? 6.Uncertainty Principle 7.Probability, Wave Functions,
1 5.1X-Ray Scattering 5.2De Broglie Waves 5.3Electron Scattering 5.4Wave Motion 5.5Waves or Particles? 5.6Uncertainty Principle 5.7Probability, Wave Functions,
1.The Atomic Models of Thomson and Rutherford 2.Rutherford Scattering 3.The Classical Atomic Model 4.The Bohr Model of the Hydrogen Atom 5.Successes &
The Photoelectric Effect
4.1The Atomic Models of Thomson and Rutherford 4.2Rutherford Scattering 4.3The Classic Atomic Model 4.4The Bohr Model of the Hydrogen Atom 4.5Successes.
Chapter 71 Atomic Structure Chapter 7. 2 Electromagnetic Radiation -Visible light is a small portion of the electromagnetic spectrum.
4.1The Atomic Models of Thomson and Rutherford 4.2Rutherford Scattering 4.3The Classic Atomic Model 4.4The Bohr Model of the Hydrogen Atom 4.5Successes.
Classical ConceptsEquations Newton’s Law Kinetic Energy Momentum Momentum and Energy Speed of light Velocity of a wave Angular Frequency Einstein’s Mass-Energy.
Electronic Structure of Atoms Chapter 6 BLB 12 th.
Spectroscopy and Electron Configurations
Chapter 4 Arrangement of Electrons in Atoms
The total energy of matter related to the frequency ν of the wave is E=hν the momentum of matter related to the wavelength λ of the wave is p=h/λ 3.1 Matter.
Young/Freeman University Physics 11e. Ch 38 Photons, Electrons, and Atoms © 2005 Pearson Education.
Chapter 4 Arrangement of Electrons in Atoms
The Quantum Mechanical Atom CHAPTER 8 Chemistry: The Molecular Nature of Matter, 6 th edition By Jesperson, Brady, & Hyslop.
Midterm results will be posted downstairs (by the labs) this afternoon No office hours today.
1 PHYS 3313 – Section 001 Lecture #11 Wednesday, Feb. 19, 2014 Dr. Jaehoon Yu Pair production/Pair annihilation Atomic Model of Thomson Rutherford Scattering.
1 PHYS 3313 – Section 001 Lecture #16 Monday, Mar. 24, 2014 Dr. Jaehoon Yu De Broglie Waves Bohr’s Quantization Conditions Electron Scattering Wave Packets.
Quantum Physics. Quantum Theory Max Planck, examining heat radiation (ir light) proposes energy is quantized, or occurring in discrete small packets with.
1 PHYS 3313 – Section 001 Lecture #10 Monday, Feb. 17, 2014 Dr. Jaehoon Yu Photoelectric Effect Compton Effect Pair production/Pair annihilation Monday,
Atomic Models Scientist studying the atom quickly determined that protons and neutrons are found in the nucleus of an atom. The location and arrangement.
Quantum Mechanics and Atomic Theory Wave models for electron orbitals.
Chemistry 330 Chapter 11 Quantum Mechanics – The Concepts.
Mullis1 Arrangement of Electrons in Atoms Principles of electromagnetic radiation led to Bohr’s model of the atom. Electron location is described using.
Wednesday, Feb. 18, 2015 PHYS , Spring 2014 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #9 Wednesday, Feb. 18, 2015 Dr. Jaehoon Yu Quantization.
Physics Lecture 9 2/17/ Andrew Brandt Wednesday February 17, 2010 Dr. Andrew Brandt 1.HW4 on ch 5 will be assigned Friday 2/19 and due.
CHAPTER 4 Structure of the Atom
What’s coming up??? Oct 25The atmosphere, part 1Ch. 8 Oct 27Midterm … No lecture Oct 29The atmosphere, part 2Ch. 8 Nov 1Light, blackbodies, BohrCh. 9 Nov.
1 PHYS 3313 – Section 001 Lecture #9 Wednesday, Feb. 12, 2014 Dr. Jaehoon Yu Determination of Electron Charge Line Spectra Blackbody Radiation Wednesday,
Monday, March 23, 2015PHYS , Spring 2014 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #13 Monday, March 23, 2015 Dr. Jaehoon Yu Bohr Radius.
AP Notes Chapter 6 Atomic Structure Describe properties of electromagnetic radiation Describe properties of electromagnetic radiation Light & relationship.
Chapter 7 Lecture Lecture Presentation Chapter 7 The Quantum- Mechanical Model of the Atom Sherril Soman Grand Valley State University © 2014 Pearson Education,
Chapter 28:Atomic Physics
Questions From Reading Activity? Assessment Statements  Topic 13.1, Quantum Physics: The Quantum Nature of Radiation Describe the photoelectric.
1 PHYS 3313 – Section 001 Lecture #15 Monday, Mar. 17, 2014 Dr. Jaehoon Yu Atomic Excitation by Electrons X-ray Scattering Bragg’s Law De Broglie Waves.
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.
Monday, March 30, 2015PHYS , Spring 2015 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #15 Monday, March 30, 2015 Dr. Jaehoon Yu Wave Motion.
PHYS 3313 – Section 001 Lecture #11
Monday, March 16, 2015PHYS , Spring 2014 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #12 Monday, March 16, 2015 Dr. Jaehoon Yu Rutherford.
Physics Lecture 10 2/22/ Andrew Brandt Monday February 22, 2010 Dr. Andrew Brandt 1.HW4 on ch 5 is due Monday 3/1 2.HW5 on ch 6 will be.
Light, Quantitized Energy & Quantum Theory CVHS Chemistry Ch 5.1 & 5.2.
CHAPTER 5 Wave Properties of Matter and Quantum Mechanics I
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 #15
PHYS 3313 – Section 001 Lecture #16
Quantum Mechanics and Atomic Physics
PHYS 3313 – Section 001 Lecture #14
CHAPTER 5 Wave Properties of Matter and Quantum Mechanics I
CHAPTER 6 Structure of the Atom
PHYS 3313 – Section 001 Lecture #13
PHYS 3313 – Section 001 Lecture #9
PHYS 3313 – Section 001 Lecture #16
Atomic Models Scientist studying the atom quickly determined that protons and neutrons are found in the nucleus of an atom. The location and arrangement.
PHYS 3313 – Section 001 Lecture #12
de Broglie Waves de Broglie argued
CHAPTER 4 Structure of the Atom
CHAPTER 5 Wave Properties of Matter and Quantum Mechanics I
PHYS 3313 – Section 001 Lecture #12
PHYS 3313 – Section 001 Lecture #14
PHYS 3313 – Section 001 Lecture #17
CHAPTER 5 Wave Properties of Matter and Quantum Mechanics I
Presentation transcript:

Wednesday, Oct. 2, 2013PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #11 Wednesday, Oct. 2, 2013 Dr. Amir Farbin Importance of Bohr’s Model X-ray Scattering Bragg’s Law De Broglie Waves Bohr’s Quantization Electron Scattering Wave Properties

Wednesday, Oct. 2, 2013PHYS , Fall 2012 Dr. Jaehoon Yu 2 Announcements Reading assignments: CH4.6 and CH4.7 Mid-term exam –In class on Wednesday, Oct. 16 –Covers from CH1.1 through what we finish on Oct. 9 + appendices –Mid-term exam constitutes 20% of the total – Please do NOT miss the exam! You will get an F if you miss it. –Bring your own HANDWRITTEN formula sheet – one letter size sheet, front and back No solutions for any problems No derivations of any kind Can have values of constants Homework #3 –End of chapter problems on CH4: 5, 14, 17, 21, 23 and 45 –Due: Monday, Oct. 14 Colloquium this week –4pm, Wednesday, Oct. 2, SH101

Importance of Bohr’s Model Demonstrated the need for Plank’s constant in understanding atomic structure Assumption of quantized angular momentum which led to quantization of other quantities, r, v and E as follows Orbital Radius: Orbital Speed: Energy levels: Monday, Sept. 30, 2013PHYS , Fall 2013 Dr. Jaehoon Yu 3

Successes and Failures of the Bohr Model The electron and hydrogen nucleus actually revolved about their mutual center of mass  reduced mass correction!! All we need is to replace me me with atom’s reduced mass. The Rydberg constant for infinite nuclear mass, R ∞ is replaced by R.R. Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Limitations of the Bohr Model The Bohr model was a great step of the new quantum theory, but it had its limitations. 1) Works only to single-electron atoms – Even for ions  What would change? – The charge of the nucleus 2) Could not account for the intensities or the fine structure of the spectral lines – Fine structure is caused by the electron spin 3) Could not explain the binding of atoms into molecules Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Characteristic X-Ray Spectra and Atomic Number Shells have letter names: K shell for n = 1 L shell for n = 2 The atom is most stable in its ground state. When a transition occurs in a heavy atom, the radiation emitted is an x ray. It has the energy E (x ray) = Eu Eu − Eℓ.Eℓ. An electron from higher shells will fill the inner-shell vacancy at lower energy. Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Atomic Number L shell to K shell Kα Kα x ray M shell to K shell Kβ Kβ x ray Atomic number Z = of protons in the nucleus Moseley found a relationship between the frequencies of the characteristic x ray and Z. This holds for the Kα Kα x ray Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Moseley’s Empirical Results The x ray is produced from n = 2 to n = 1 transition. In general, the K series of x ray wavelengths are Moseley’s research clarified the importance of the electron shells for all the elements, not just for hydrogen. Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Atomic Excitation by Electrons Franck and Hertz studied the phenomenon of ionization. Accelerating voltage is below 5 V electrons did not lose energy Accelerating voltage is above 5 V sudden drop in the current Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Atomic Excitation by Electrons Ground state has E0 E0 to be zero. First excited state has E1.E1. The energy difference E1 E1 − 0 = E1 E1 is the excitation energy. Above 4.88 eV, the current drops because scattered electrons no longer reach the collector until the accelerating voltage reaches 9.8 eV and so on. Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu Hg has an excitation energy of 4.88 eV in the first excited state No energy can be transferred to Hg below 4.88 eV because not enough energy is available to excite an electron to the next energy level

Importance of Bohr’s Model Demonstrated the need for Plank’s constant in understanding atomic structure Assumption of quantized angular momentum which led to quantization of other quantities, r, v and E as follows Orbital Radius: Orbital Speed: Energy levels: Monday, Sept. 30, 2013PHYS , Fall 2013 Dr. Jaehoon Yu 11

Successes and Failures of the Bohr Model The electron and hydrogen nucleus actually revolved about their mutual center of mass  reduced mass correction!! All we need is to replace me me with atom’s reduced mass. The Rydberg constant for infinite nuclear mass, R ∞ is replaced by R.R. Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Limitations of the Bohr Model The Bohr model was a great step of the new quantum theory, but it had its limitations. 1) Works only to single-electron atoms – Even for ions  What would change? – The charge of the nucleus 2) Could not account for the intensities or the fine structure of the spectral lines – Fine structure is caused by the electron spin – When a magnetic field is applied, spectral lines split 3) Could not explain the binding of atoms into molecules Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

X-Ray Scattering Max von Laue suggested that if x rays were a form of electromagnetic radiation, interference effects should be observed. (Wave property!!) Crystals act as three-dimensional gratings, scattering the waves and producing observable interference effects. Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Bragg’s Law William Lawrence Bragg interpreted the x-ray scattering as the reflection of the incident x-ray beam from a unique set of planes of atoms within the crystal. There are two conditions for constructive interference of the scattered x rays: Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu 1) The angle of incidence must equal the angle of reflection of the outgoing wave. (total reflection) 2) The difference in path lengths between two rays must be an integral number of wavelengths.  Bragg’s Law: n λ = 2d 2d sin θ ( n = integer)

A Bragg spectrometer scatters x rays from several crystals. The intensity of the diffracted beam is determined as a function of scattering angle by rotating the crystal and the detector. When a beam of x rays passes through the powdered crystal, the dots become a series of rings due to random arrangement. The Bragg Spectrometer Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Bragg’s law: nλ nλ = 2d 2d sin θ What do we need to know to use this? The lattice spacing d!d! We know n=1 and 2 θ =20 o. We use the density of NaCl to find out what d is. X rays scattered from rock salt (NaCl) are observed to have an intense maximum at an angle of 20 o from the incident direction. Assuming n=1 (from the intensity), what must be the wavelength of the incident radiation? Ex 5.1: Bragg’s Law Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

De Broglie Waves Prince Louis V. de Broglie suggested that mass particles should have wave properties similar to electromagnetic radiation  many experiments supported this! Thus the wavelength of a matter wave is called the de Broglie wavelength: Since for a photon, E = pc and E = hf, the energy can be written as Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Bohr’s Quantization Condition One of Bohr’s assumptions concerning his hydrogen atom model was that the angular momentum of the electron-nucleus system in a stationary state is an integral multiple of h /2 π. The electron is a standing wave in an orbit around the proton. This standing wave will have nodes and be an integral number of wavelengths. The angular momentum becomes: Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

What is the formula for De Broglie Wavelength? (a) for a tennis ball, m=0.057kg. (b) for electron with 50eV KE, since KE is small, we can use non-relativistic expression of electron momentum! What are the wavelengths of you running at the speed of 2m/s? What about your car of 2 metric tons at 100mph? How about the proton with 14TeV kinetic energy? What is the momentum of the photon from a green laser? Calculate the De Broglie wavelength of (a) a tennis ball of mass 57g traveling 25m/s (about 56mph) and (b) an electron with kinetic energy 50eV. Ex 5.2: De Broglie Wavelength Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Electron Scattering Davisson and Germer experimentally observed that electrons were diffracted much like x rays in nickel crystals.  direct proof of De Broglie wave! George P. Thomson (1892–1975), son of J. Thomson, reported seeing the effects of electron diffraction in transmission experiments. The first target was celluloid, and soon after that gold, aluminum, and platinum were used. The randomly oriented polycrystalline sample of SnO 2 produces rings as shown in the figure at right. Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Photons, which we thought were waves, act particle like (eg Photoelectric effect or Compton Scattering) Electrons, which we thought were particles, act particle like (eg electron scattering) De Broglie: All matter has intrinsic wavelength. –Wave length inversely proportional to momentum –The more massive… the smaller the wavelength… the harder to observe the wavelike properties –So while photons appear mostly wavelike, electrons (next lightest particle!) appear mostly particle like. How can we reconcile the wave/particle views? Monday, Sept. 30, 2013PHYS , Fall 2013 Dr. Jaehoon Yu 22

De Broglie matter waves suggest a further description. The displacement of a wave is This is a solution to the wave equation Define the wave number k and the angular frequency  as: The wave function is now: Wave Motion Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Wave Properties The phase velocity is the velocity of a point on the wave that has a given phase (for example, the crest) and is given by A phase constant Φ shifts the wave:. Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu (When  =  /2)

Principle of Superposition When two or more waves traverse the same region, they act independently of each other. Combining two waves yields: The combined wave oscillates within an envelope that denotes the maximum displacement of the combined waves. When combining many waves with different amplitudes and frequencies, a pulse, or wave packet, can be formed, which can move at a group velocity : Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Fourier Series Adding 2 waves isn’t localized in space… but adding lots of waves can be. The sum of many waves that form a wave packet is called a Fourier series : Summing an infinite number of waves yields the Fourier integral: Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

Wave Packet Envelope The superposition of two waves yields a wave number and angular frequency of the wave packet envelope. The range of wave numbers and angular frequencies that produce the wave packet have the following relations: A Gaussian wave packet has similar relations: The localization of the wave packet over a small region to describe a particle requires a large range of wave numbers. Conversely, a small range of wave numbers cannot produce a wave packet localized within a small distance. Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu

A Gaussian wave packet describes the envelope of a pulse wave. The group velocity is Gaussian Function Monday, Sept. 30, PHYS , Fall 2013 Dr. Jaehoon Yu