N(v) We then have a the distribution of velocities N(v) or the number of molecules at each velocity in the cavity.

Size: px
Start display at page:

Download "N(v) We then have a the distribution of velocities N(v) or the number of molecules at each velocity in the cavity."

Transcription

1 CHAPTER 2 QUANTUM THEORY OF LIGHT The quantum theory of light was realized in the later 19 th and early 20 th century, Soon after Boltzman set the laws of dealing with large ensembles of atoms with so called statistical mechanics some inconsistencies were seen involving radiation from solids. Wedgewood notes in 1789 that all objects in his ovens, regardless of chemical nature, size, shape, became red at the same temperature. By the mid 1800 s it is know that glowing objects emit continous light spectra. Thermal equilibrium We now understand that that objects emit and absorb radiation continuously. If the emission and absorption is perfectly matched at all frequencies as in the case of thermal equilibrium above the ball I the glowing oven becomes invisible! MAXWELL s DISTRIBUTION of SPEEDS Maxwell considered atoms in a container which is heated to temperature T. The container has a volume V. Through a slit some atoms escape and their speeds are measured. T v N(v) Velocity Distribution <v> AVG v We then have a the distribution of velocities N(v) or the number of molecules at each velocity in the cavity. Integrating over all v N(V) dv = N total number of molecules measured. We can write a normalized velocity distribution P(v) = 1/N N(v) which is the probability that a molecule is at velocity v.

2 Maxwell worked the distribution of speeds out out from statistical physics. Letting the number of molecules per unit volume be n=n/v and with KE = 1/2 m v 2 the Maxwell distribution of speeds is (, k=boltzmann constant and T=temperature) n(v) = A v 2 KE / kt e CAVITY RADIATION Such a cavity if made hot enough would also emit light! Attempts were made to understand the frequency distribution of light emitted from a cavity. This is called the cavity radiation problem. Kirchoff, circa. 1860, showed that for any body in thermal equlilibrium the radiant power emitted e EMITTED (per unit area per unit frequency) is proportional to the power absorbed. A ABSORBED at each frequency (a law of detailed balance). He showed that if this were not true then the 2 nd law of thermodynamics would be violated! e(f,t) EMITTED = α A(f,T) ABSORBED The radiant spectrum of a black body (α = 1) was sought. The black body perfectly absorbs all radtiation incident upon its surface appearing perfectly black. Absorption is not perfect in general, due to reflective losses or lack of absortion at some frequencies. A cavity with a small hole would absorb all radition incident on the hole. (Wein s idea!) Thus the hole (disk) becomes a black body and the emission spectrum can be measured.. STEPHAN s LAW Josef Stephan circa 1879 establishes from experiment, that the total power radiated from a near black body follows a universal law, (α = 1 for a true black body radiator.) e TOTAL = α σ T 4 σ = 5.67 x 10 8 W/m 2 K 4 is the StephanBoltzmann constant.

3 How much power are you radiating into the room? Let α =0.5 T BODY = 37C+273K = 310K A = surface area of your body ~ 4/5 m 2 e TOTAL = ( 5.7 x 10 8 W/m 2 K 4 e TOTAL = 260W/m 2 P = e TOTAL (4/5 )= 200W T BODY WEIN s DISPLACEMENT LAW (see example 2.2) Wein measured the radiant spectra from black bodies and proposed a universal law called the Wein Displacement Law. It describes the position of the maximum wavelength λ MAX versus body temperature. T. λ MAX T = x 10 3 mk RAYLEIGHJEANS and WEIN s EQUATIONS u~a f 4 RayleighJeans Law based on classical E&M and thermodynamics. Worked at Low frequencies only. Lead to an UltraViolet catastrophie.: diverging at hi frequency. u~a f 4 Wein s Law for higher frequencies. u~ A f 3 e C f / kt f Lord Rayleigh and Jeans formulate a spectral energy density u (f,t) from classical considerations with radiant energy increasing as th 4 th power of frquency which worked well at low frequencied and diverged at higher requencies (UltraViolet catastrophie). Wein also proposed a later which solved the UV catastrophie by only worked at high frequency?? u(f.t) = A f 3 e C f / kt

4 Each assumed that the cavity (or solid) is made of vibrating charges (radiators). Classically the energy of the radiation is proportional to the vibrational frequency or velocities of the oscillators thus the connection to Maxwell s velocity distribution for molecules. radiation radiation E = 1/2 M dx(t)/dt 2 X(t) = A cos(2π f t ) Initially believed to be successes for the classical views of thermodynamics and Maxwell s Equations, both laws failed to accurately describe the Black Body radiant energy spectrum MAX PLANCK Planck attacks the problem. He can only find correspondence with data if he assumes that the light spectra are coming from a discrete radiation source. Planck has stumbled on the quantum state of light the photon. Light exists in quana called photons. E = 3 E = E = 2 PHOTONS h = x evs Planck s Constant u(f.t) = A f 3 1 / [ e h f / kt 1 ] Planck s Law solved the cavity radiation problem and introduced the idea that light is not a continuous wave phenomena but acts as a quanta of energy E =. The idea is so new that many still disbelieve.

5 PHOTOELECTRIC EFFECT It was long known that high frequency light could liberate charge from a metal s surface. The reason was not clear. This was observed by Hertz. Later (1899) J.J. Thompson showed that these were negative charges (electrons). (1) Electrons were only emiitted once light of a high enough frequency was used no matter how intense the light? (2) Once this frequency was reached the photoelectric current rose with intensity. (3) Different metal seem to have different frequency theshold values. Einstein proposes the solution involves the interaction of light with the charges in the metal, not as a wave phenomena but like billiard balls! It is not understood if Einstein yet knew of Planck s quantum revelation. Einstein was a big fan of Deductive Reasoning or minimal influence with datasymmetry, beauty, God, thought experiment s etc. Left for further reading! Of course this is contrary to the most scientist of the time who used Inductive Reasoning whose conclusion s (equations) are drawn from experimental observation! KEe KEe KEe W 1 W 2 W 3 The electrons s kinetic energy upon exiting the metal derives from the photon s energy E= minus he work necessary for the electron to escape the metal, W = work. KE = W > 0 Must be positive! Electrons with the shortest paths attain the maximum kinetc energy, KE MAX. KE MAX = φ W MIN φ =W MIN is called the work function of the metal

6 PHOTOELECTRIC EFFECT APPARATUS I We can observe the photoelectric effect in the apparatus. depicted here. Light of frequency f is shone on a metal surface. A photocurrent I is generated. Stopping voltage Vs is increased from zero until the photocurrent I is reduced to zero. At this point evs = KE MAX I The electric field generated has stopped the most energetic electrons from crossing. Then we have evs = φ This equation of a line can be solved for the slope and intercept Vs Vs Vs = (h/e) f φ Slope = h/e QUANTUM WELL KE φ electrons Intercept = φ Conservation of energy φ = KE E=0 f E = φ e

7 PHOTOELECTRIC EFFECT A PARTICLE VIEW In the photoelectric effect all the photon s energy is transferred to the atomic electron. E= e E = KE + m e c 2 E = W + m e c 2 KE = 0 U = W e From conservation of energy W + m e c 2 = E = T + m e c 2 T = W LIGHT AS A QUANTA E = = hc/λ 0 E(eV) = 1240/λ(nm) E 2 = P 2 c 2 + m 2 c 4 E = Pc (photon) Because the photon is thought to have zero mass then in the relativistic view we have a simple relationship between momentum and energy! E = Pc XRAYS Xrays are light quanta on energy in the KeV range. Xrays were first produced by Roentgen (1895) by accident. He discovered that mysterious and very penetrating rays could be generated by smashing a beam of electrons into a metal. Ee

8 Xray Spectrum Intensity DISCRETE PEAKS λ MIN CONTINUOUS λ MIN λ (KeV) The Xray spectrum seem to have 2 components which needed explanation. (1) A continuous spectrum which rose and fell. No Xrays are observed below a minimum wavelenght or equivalently a maximum energy Emax.= hc/ λ MIN. (2) Intensity spikes occur at intermediate energies corresponding to atomic transitions?? CONTINUOUS SPECTRA. =EoE E E =E E Eo E E = Eo E = (KEo+mc 2 ) (KE + mc 2 ) = KEoKE λ MIN When the electron looses all of its energy in one collision E MAX = MAX = hc/ λ MIN occurs. =E E The continuous spectra is caused by the incident electron, energy Eo. undergoing a series of collisions with atoms Each time the electron is slowed and it s energy is degraded Eo>E >E >E A photon is emitted on each exchange to balance energy. This process is called Brehmstrahlung ( breaking radiation).

9 DISCRETE SPECTRA Eo Incident electron E2 E1 =E2E1 E Any incident electron at any stage of deacceleration can excite an orbital electron in to a higher state if E > E=E2E1. The orbital electron deexcites by emitting a photon of energy = E2E1. Incident electron of energy E wanders on with E = Eo, always conserving energy. This was not all perfectly understood at the time! COMPTON EFFECT Compton realized that he could test the quantum theory of light be scattering Xrays from Carbon atoms. And measureing the scattered energy. Classically light did not loose energy upon scattering in a medium. The wavelength did change λ n = λ/n. (Remember the λ n = λ/n is the wavelength change in a medium of index of refraction n) Compton suggests that a high energy photon (Xray) can scatter from an atomic electron and loose a fraction of it s energy, transferring the balance to the electron as Einstein suggests. =hc/λ y =hc/λ E=mc 2 φ E θ x Energy and Momentum Balance Equations in 2D + E = + E energy + mc 2 = cos(θ) + E cos(φ) xmomentum 0 = P γ sin(θ) + E sin(φ) ymomentum λ λ = (h/mc) ( 1cos(θ) ) λ C = h/mc = nm is called the Compton wavelength of an electron.

10 BRAGG SCATTERING LAW Bragg scattered Xrays from a crystal lattice and found interference phenomena which supported the wave picture of light. This was a confusing time. Was light a wave or particle phenomena? n λ = 2dsin θ λ θ θ dsin θ θ d GRAVITATIONAL REDSHIFT Does a photon have mass?? E =m c 2 = or m = / c 2 E= + mgy = mgy = ( / c 2 ) gy f = fgy/c 2 f/f = gy/ c 2 E = earth

Particle nature of light & Quantization

Particle 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 information

FI 3103 Quantum Physics

FI 3103 Quantum Physics FI 3103 Quantum Physics Alexander A. Iskandar Physics of Magnetism and Photonics Research Group Institut Teknologi Bandung General Information Lecture schedule 17 18 9136 51 5 91 Tutorial Teaching Assistant

More information

Particles and Waves Particles Waves

Particles and Waves Particles Waves Particles and Waves Particles Discrete and occupy space Exist in only one location at a time Position and velocity can be determined with infinite accuracy Interact by collisions, scattering. Waves Extended,

More information

Semiconductor Physics and Devices

Semiconductor Physics and Devices Introduction to Quantum Mechanics In order to understand the current-voltage characteristics, we need some knowledge of electron behavior in semiconductor when the electron is subjected to various potential

More information

Experimental Basis for QM Ch3

Experimental Basis for QM Ch3 Experimental Basis for QM Ch3 This chapter describes the early evidence for quantization including Blackbody radiation Photoelectric effect Compton scattering X-rays and their spectra We ll see how early

More information

Blackbody Radiation. Rayleigh-Jeans law was an attempt to explain blackbody radiation based on classical ideas:

Blackbody Radiation. Rayleigh-Jeans law was an attempt to explain blackbody radiation based on classical ideas: Blackbody Radiation A Blackbody is an ideal system that absorbs all radiation incident on it. Emission of radiation by a blackbody is independent of the properties of its wall, but depends only on its

More information

Chapter 30 Quantum Physics 30.1 Blackbody Radiation and Planck s Hypothesis of Quantum Energy 30.2 Photons and the Photoelectric Effect 30.

Chapter 30 Quantum Physics 30.1 Blackbody Radiation and Planck s Hypothesis of Quantum Energy 30.2 Photons and the Photoelectric Effect 30. Chapter 30 Quantum Physics 30.1 Blackbody Radiation and Planck s Hypothesis of Quantum Energy 30.2 Photons and the Photoelectric Effect 30.3 The Mass and Momentum of a Photon 30.4 Photon Scattering and

More information

General Physics (PHY 2140)

General Physics (PHY 2140) General Physics (PHY 2140) Lecture 27 Modern Physics Quantum Physics Blackbody radiation Plank s hypothesis http://www.physics.wayne.edu/~apetrov/phy2140/ Chapter 27 1 Quantum Physics 2 Introduction: Need

More information

Physics Lecture 6

Physics Lecture 6 Physics 3313 - Lecture 6 Monday February 8, 2010 Dr. Andrew Brandt 1. HW1 Due today HW2 weds 2/10 2. Electron+X-rays 3. Black body radiation 4. Compton Effect 5. Pair Production 2/8/10 3313 Andrew Brandt

More information

Classical and Planck picture. Planck s constant. Question. Quantum explanation for the Wein Effect.

Classical and Planck picture. Planck s constant. Question. Quantum explanation for the Wein Effect. 6.1 Quantum Physics. Particle Nature of Light Particle nature of Light Blackbody Radiation Photoelectric Effect Properties of photons Ionizing radiation Radiation damage x-rays Compton effect X-ray diffraction

More information

Early Quantum Theory and Models of the Atom

Early 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 information

WAVE PARTICLE DUALITY

WAVE PARTICLE DUALITY WAVE PARTICLE DUALITY Evidence for wave-particle duality Photoelectric effect Compton effect Electron diffraction Interference of matter-waves Consequence: Heisenberg uncertainty principle PHOTOELECTRIC

More information

Chapter 27. Quantum Physics

Chapter 27. Quantum Physics Chapter 27 Quantum Physics Need for Quantum Physics Problems remained from classical mechanics that relativity didn t explain Blackbody Radiation The electromagnetic radiation emitted by a heated object

More information

is the minimum stopping potential for which the current between the plates reduces to zero.

is the minimum stopping potential for which the current between the plates reduces to zero. Module 1 :Quantum Mechanics Chapter 2 : Introduction to Quantum ideas Introduction to Quantum ideas We will now consider some experiments and their implications, which introduce us to quantum ideas. The

More information

Chapter 1. From Classical to Quantum Mechanics

Chapter 1. From Classical to Quantum Mechanics Chapter 1. From Classical to Quantum Mechanics Classical Mechanics (Newton): It describes the motion of a classical particle (discrete object). dp F ma, p = m = dt dx m dt F: force (N) a: acceleration

More information

Physics 2D Lecture Slides Lecture 11: Jan. 27 th Sunil Sinha UCSD Physics

Physics 2D Lecture Slides Lecture 11: Jan. 27 th Sunil Sinha UCSD Physics Physics 2D Lecture Slides Lecture 11: Jan. 27 th 2010 Sunil Sinha UCSD Physics Einstein s Explanation of PhotoElectric Effect What Maxwell Saw of EM Waves What Einstein Saw of EM Waves Light as bullets

More information

The term "black body" was introduced by Gustav Kirchhoff in The light emitted by a black body is called black-body radiation.

The term black body was introduced by Gustav Kirchhoff in The light emitted by a black body is called black-body radiation. Black body (Redirected from Black-body radiation) As the temperature decreases, the peak of the black body radiation curve moves to lower intensities and longer wavelengths. The black-body radiation graph

More information

Modern Physics (Lec. 1)

Modern Physics (Lec. 1) Modern Physics (Lec. 1) Physics Fundamental Science Concerned with the fundamental principles of the Universe Foundation of other physical sciences Has simplicity of fundamental concepts Divided into five

More information

Quantum Mechanics (made fun and easy)

Quantum Mechanics (made fun and easy) Lecture 7 Quantum Mechanics (made fun and easy) Why the world needs quantum mechanics Why the world needs quantum mechanics Why the world needs quantum mechanics Why the world needs quantum mechanics Why

More information

Photoelectric Effect

Photoelectric Effect PC1144 Physics IV Photoelectric Effect 1 Purpose Demonstrate the different predictions of the classical wave and quantum model of light with respect to the photoelectric effect. Determine an experimental

More information

Quantum Mechanics: Blackbody Radiation

Quantum Mechanics: Blackbody Radiation Blackbody Radiation Quantum Mechanics Origin of Quantum Mechanics Raleigh-Jeans law (derivation)-ultraviolet catastrophe, Wien s Distribution Law & Wein s Displacement law, Planck s radiation law (calculation

More information

STSF2223 Quantum Mechanics I

STSF2223 Quantum Mechanics I STSF2223 Quantum Mechanics I What is quantum mechanics? Why study quantum mechanics? How does quantum mechanics get started? What is the relation between quantum physics with classical physics? Where is

More information

Dual Nature of Radiation and Matter-I

Dual Nature of Radiation and Matter-I Dual Nature of Radiation and Matter-I Physics Without Fear CONTENTS ELECTRON EMISSION PHOTOELECTRIC EFFECT; HERTZ S OBSERVATIONS HALLWACHS AND LENARD S OBSERVATIONS EXPERIMENTAL STUDY OF PHOTOELECTRIC

More information

CHAPTER 3 The Experimental Basis of Quantum Theory

CHAPTER 3 The Experimental Basis of Quantum Theory CHAPTER 3 The Experimental Basis of Quantum Theory 3.1 3.2 3.3 3.4 3.5 3.6 3.7 3.8 3.9 Discovery of the X Ray and the Electron Determination of Electron Charge Line Spectra Quantization As far as I can

More information

CHAPTER 27 Quantum Physics

CHAPTER 27 Quantum Physics CHAPTER 27 Quantum Physics Units Discovery and Properties of the Electron Planck s Quantum Hypothesis; Blackbody Radiation Photon Theory of Light and the Photoelectric Effect Energy, Mass, and Momentum

More information

We also find the development of famous Schrodinger equation to describe the quantization of energy levels of atoms.

We also find the development of famous Schrodinger equation to describe the quantization of energy levels of atoms. Lecture 4 TITLE: Quantization of radiation and matter: Wave-Particle duality Objectives In this lecture, we will discuss the development of quantization of matter and light. We will understand the need

More information

PHY202 Quantum Mechanics. Topic 1. Introduction to Quantum Physics

PHY202 Quantum Mechanics. Topic 1. Introduction to Quantum Physics PHY202 Quantum Mechanics Topic 1 Introduction to Quantum Physics Outline of Topic 1 1. Dark clouds over classical physics 2. Brief chronology of quantum mechanics 3. Black body radiation 4. The photoelectric

More information

QM all started with - - The Spectrum of Blackbody Radiation

QM all started with - - The Spectrum of Blackbody Radiation QM all started with - - The Spectrum of Blackbody Radiation Thermal Radiation: Any object, not at zero temperature, emits electromagnetic called thermal. When we measure the intensity of a real object,

More information

Chapter One. The Old Quantum Theory. 1-1 Why Quantum Mechanics.

Chapter One. The Old Quantum Theory. 1-1 Why Quantum Mechanics. Chapter One The Old Quantum Theory 1-1 Why Quantum Mechanics. The birth of quantum mechanics can be dated to 1925, when physicists such as Werner Heisenberg and Erwin Schrödinger invented mathematical

More information

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS LSN 12-1A: INTERACTIONS OF MATTER WITH RADIATION Questions From Reading Activity? Essential Idea: The microscopic quantum world offers a range of phenomena,

More information

Exam 2 Development of Quantum Mechanics

Exam 2 Development of Quantum Mechanics PHYS40 (Spring 00) Riq Parra Exam # (Friday, April 1 th, 00) Exam Development of Quantum Mechanics Do NOT write your name on this exam. Write your class ID number on the top right hand corner of each problem

More information

Explain how Planck resolved the ultraviolet catastrophe in blackbody radiation. Calculate energy of quanta using Planck s equation.

Explain how Planck resolved the ultraviolet catastrophe in blackbody radiation. Calculate energy of quanta using Planck s equation. Objectives Explain how Planck resolved the ultraviolet catastrophe in blackbody radiation. Calculate energy of quanta using Planck s equation. Solve problems involving maximum kinetic energy, work function,

More information

Photoelectric effect

Photoelectric effect Experimental Physics EP3 Atoms and Molecules Photoelectric effect energy quantization, photons http://research/uni-leipzig.de/valiu/ Experimental Physics III - Photoelectric effect 1 Light-matter interaction

More information

DUAL NATURE OF RADIATION AND MATTER I K GOGIA KV JHARODA KALAN DELHI.

DUAL NATURE OF RADIATION AND MATTER I K GOGIA KV JHARODA KALAN DELHI. DUAL NATURE OF RADIATION AND MATTER AIM: The aim of present self- learning module is to train the minds of the learners in building the concepts by learning on their own. The module is designed to Achieve

More information

CHAPTER 2: POSTULATES OF QUANTUM MECHANICS

CHAPTER 2: POSTULATES OF QUANTUM MECHANICS CHAPTER 2: POSTULATES OF QUANTUM MECHANICS Basics of Quantum Mechanics - Why Quantum Physics? - Classical mechanics (Newton's mechanics) and Maxwell's equations (electromagnetics theory) can explain MACROSCOPIC

More information

Heinrich Hertz, a German physicist, achieved the first experimental demonstration of EM waves in 1887.

Heinrich Hertz, a German physicist, achieved the first experimental demonstration of EM waves in 1887. 9.4.2-1(i) Hertz s first radio wave transmission demonstration Maxwell In 1865 James Clerk Maxwell predicted the existence of electromagnetic waves. He said that an accelerating charge would produce a

More information

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

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

More information

Modern Physics, summer Modern physics. Historical introduction to quantum mechanics

Modern Physics, summer Modern physics. Historical introduction to quantum mechanics 1 Modern physics 2 Gustav Kirchhoff (1824-1887) Surprisingly, the path to quantum mechanics begins with the work of German physicist Gustav Kirchhoff in 1859. Electron was discovered by J.J.Thomson in

More information

1 The Cathode Rays experiment is associated. with: Millikan A B. Thomson. Townsend. Plank Compton

1 The Cathode Rays experiment is associated. with: Millikan A B. Thomson. Townsend. Plank Compton 1 The Cathode Rays experiment is associated with: A B C D E Millikan Thomson Townsend Plank Compton 1 2 The electron charge was measured the first time in: A B C D E Cathode ray experiment Photoelectric

More information

General Physics (PHY 2140) Lecture 14

General Physics (PHY 2140) Lecture 14 General Physics (PHY 2140) Lecture 14 Modern Physics 1. Relativity Einstein s General Relativity 2. Quantum Physics Blackbody Radiation Photoelectric Effect X-Rays Diffraction by Crystals The Compton Effect

More information

Chapter 38. Photons Light Waves Behaving as Particles

Chapter 38. Photons Light Waves Behaving as Particles Chapter 38 Photons Light Waves Behaving as Particles 38.1 The Photoelectric Effect The photoelectric effect was first discovered by Hertz in 1887, and was explained by Einstein in 1905. The photoelectric

More information

Planck s Quantum Hypothesis Blackbody Radiation

Planck s Quantum Hypothesis Blackbody Radiation Planck s Quantum Hypothesis Blackbody Radiation The spectrum of blackbody radiation has been measured(next slide); it is found that the frequency of peak intensity increases linearly with temperature.

More information

CHAPTER 3 The Experimental Basis of Quantum

CHAPTER 3 The Experimental Basis of Quantum CHAPTER 3 The Experimental Basis of Quantum 3.1 Discovery of the X Ray and the Electron 3.2 Determination of Electron Charge 3.3 Line Spectra 3.4 Quantization 3.5 Blackbody Radiation 3.6 Photoelectric

More information

1 Photoelectric effect - Classical treatment. 2 Photoelectric effect - Quantum treatment

1 Photoelectric effect - Classical treatment. 2 Photoelectric effect - Quantum treatment 1 OF 5 NOTE: This problem set is to be handed in to my mail slot (SMITH) located in the Clarendon Laboratory by 5:00 PM Tuesday, 10 May. 1 Photoelectric effect - Classical treatment A laser beam with an

More information

Chapter 2 Problem Solutions

Chapter 2 Problem Solutions Chapter Problem Solutions 1. If Planck's constant were smaller than it is, would quantum phenomena be more or less conspicuous than they are now? Planck s constant gives a measure of the energy at which

More information

Class 21. Early Quantum Mechanics and the Wave Nature of Matter. Physics 106. Winter Press CTRL-L to view as a slide show. Class 21.

Class 21. Early Quantum Mechanics and the Wave Nature of Matter. Physics 106. Winter Press CTRL-L to view as a slide show. Class 21. Early and the Wave Nature of Matter Winter 2018 Press CTRL-L to view as a slide show. Last Time Last time we discussed: Optical systems Midterm 2 Today we will discuss: Quick of X-ray diffraction Compton

More information

Quantum physics. Anyone who is not shocked by the quantum theory has not understood it. Niels Bohr, Nobel Price in 1922 ( )

Quantum physics. Anyone who is not shocked by the quantum theory has not understood it. Niels Bohr, Nobel Price in 1922 ( ) Quantum physics Anyone who is not shocked by the quantum theory has not understood it. Niels Bohr, Nobel Price in 1922 (1885-1962) I can safely say that nobody understand quantum physics Richard Feynman

More information

1. Historical perspective

1. Historical perspective Atomic and Molecular Physics/Lecture notes presented by Dr. Fouad Attia Majeed/Third year students/college of Education (Ibn Hayyan)/Department of Physics/University of Babylon. 1. Historical perspective

More information

Chapter 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 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 information

B. Sc. Physics (H.R.K) Chapter 49: Light and Quantum Physics LIGHT AND QUANTUM PHYSICS

B. Sc. Physics (H.R.K) Chapter 49: Light and Quantum Physics LIGHT AND QUANTUM PHYSICS LIGHT AND QUANTUM PHYSICS 49.1 Thermal Radiations The radiations emitted by a body due to its temperature are called thermal radiations. All bodies not only emit the thermal radiations, but also absorb

More information

Lecture 2 Blackbody radiation

Lecture 2 Blackbody radiation Lecture 2 Blackbody radiation Absorption and emission of radiation What is the blackbody spectrum? Properties of the blackbody spectrum Classical approach to the problem Plancks suggestion energy quantisation

More information

Modern physics. Historical introduction to quantum mechanics

Modern physics. Historical introduction to quantum mechanics 2012-0-08 Modern physics dr hab. inż. Katarzyna ZAKRZEWSKA, prof. AGH KATEDRA ELEKTRONIKI, C-1, office 17, rd floor, phone 617 29 01, mobile phone 0 601 51 5 e-mail: zak@agh.edu.pl, Internet site http://home.agh.edu.pl/~zak

More information

Learning Objectives and Worksheet I. Chemistry 1B-AL Fall 2016

Learning Objectives and Worksheet I. Chemistry 1B-AL Fall 2016 Learning Objectives and Worksheet I Chemistry 1B-AL Fall 2016 Lectures (1 2) Nature of Light and Matter, Quantization of Energy, and the Wave Particle Duality Read: Chapter 12, Pages: 524 526 Supplementary

More information

29:006 FINAL EXAM FRIDAY MAY 11 3:00 5:00 PM IN LR1 VAN

29:006 FINAL EXAM FRIDAY MAY 11 3:00 5:00 PM IN LR1 VAN L 33 Modern Physics [1] 29:006 FINAL EXAM FRIDAY MAY 11 3:00 5:00 PM IN LR1 VAN Introduction- quantum physics Particles of light PHOTONS The photoelectric effect Photocells & intrusion detection devices

More information

Quantum Theory of Light

Quantum Theory of Light King Saud University College of Applied Studies and Community Service Department of Natural Sciences Quantum Theory of Light General Physics II PHYS 111 Nouf Alkathran nalkathran@ksu.edu.sa Outline Definition

More information

Modern Physics- Introduction. L 35 Modern Physics [1] ATOMS and classical physics. Newton s Laws have flaws! accelerated charges radiate energy

Modern Physics- Introduction. L 35 Modern Physics [1] ATOMS and classical physics. Newton s Laws have flaws! accelerated charges radiate energy L 35 Modern Physics [1] Introduction- quantum physics Particles of light PHOTONS The photoelectric effect Photocells & intrusion detection devices The Bohr atom emission & absorption of radiation LASERS

More information

Revision Guide. Chapter 7 Quantum Behaviour

Revision Guide. Chapter 7 Quantum Behaviour Revision Guide Chapter 7 Quantum Behaviour Contents CONTENTS... 2 REVISION CHECKLIST... 3 REVISION NOTES... 4 QUANTUM BEHAVIOUR... 4 Random arrival of photons... 4 Photoelectric effect... 5 PHASE AN PHASORS...

More information

CHAPTER 3 Prelude to Quantum Theory. Observation of X Rays. Thomson s Cathode-Ray Experiment. Röntgen s X-Ray Tube

CHAPTER 3 Prelude to Quantum Theory. Observation of X Rays. Thomson s Cathode-Ray Experiment. Röntgen s X-Ray Tube CHAPTER Prelude to Quantum Theory.1 Discovery of the X Ray and the Electron. Determination of Electron Charge. Line Spectra.4 Quantization.5 Blackbody Radiation.6 Photoelectric Effect.7 X-Ray Production.8

More information

Particle Wave Duality. What is a particle? What is a wave?

Particle Wave Duality. What is a particle? What is a wave? Particle Wave Duality What is a particle? What is a wave? Problems with Classical Physics Nature of Light? Discrete Spectra? Blackbody Radiation? Photoelectric Effect? Compton Effect? Model of Atom? Thomas

More information

Photoelectric Effect & Bohr Atom

Photoelectric Effect & Bohr Atom PH0008 Quantum Mechanics and Special Relativity Lecture 03 (Quantum Mechanics) 020405v2 Photoelectric Effect & Bohr Atom Prof Department of Physics Brown University Main source at Brown Course Publisher

More information

Stellar Astrophysics: The Interaction of Light and Matter

Stellar 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 information

Chapter 27. Quantum Physics

Chapter 27. Quantum Physics Chapter 27 Quantum Physics Need for Quantum Physics Problems remained from classical mechanics that relativity didn t explain Blackbody Radiation The electromagnetic radiation emitted by a heated object

More information

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

Preview. Atomic Physics Section 1. Section 1 Quantization of Energy. Section 2 Models of the Atom. Section 3 Quantum Mechanics Atomic Physics Section 1 Preview Section 1 Quantization of Energy Section 2 Models of the Atom Section 3 Quantum Mechanics Atomic Physics Section 1 TEKS The student is expected to: 8A describe the photoelectric

More information

Chapter 27 Lecture Notes

Chapter 27 Lecture Notes Chapter 27 Lecture Notes Physics 2424 - Strauss Formulas: λ P T = 2.80 10-3 m K E = nhf = nhc/λ fλ = c hf = K max + W 0 λ = h/p λ - λ = (h/mc)(1 - cosθ) 1/λ = R(1/n 2 f - 1/n 2 i ) Lyman Series n f = 1,

More information

Rb, which had been compressed to a density of 1013

Rb, which had been compressed to a density of 1013 Modern Physics Study Questions for the Spring 2018 Departmental Exam December 3, 2017 1. An electron is initially at rest in a uniform electric field E in the negative y direction and a uniform magnetic

More information

SPH4U UNIVERSITY PHYSICS

SPH4U UNIVERSITY PHYSICS SPH4U UNIVERSITY PHYSICS REVOLUTIONS IN MODERN PHYSICS:... L Photons & the Quantum Theory of... (P.620-623) The Work Function Around 1800, Thomas Young performed his double-slit interference experiment

More information

It s a wave. It s a particle It s an electron It s a photon. It s light!

It s a wave. It s a particle It s an electron It s a photon. It s light! It s a wave It s a particle It s an electron It s a photon It s light! What they expected Young s famous experiment using a beam of electrons instead of a light beam. And, what they saw Wave-Particle Duality

More information

Quantum Model Einstein s Hypothesis: Photoelectric Effect

Quantum Model Einstein s Hypothesis: Photoelectric Effect VISUAL PHYSICS ONLINE MODULE 7 NATURE OF LIGHT Quantum Model Einstein s Hypothesis: Photoelectric Effect The photoelectric effect was discovered by Hertz in 1887 as he confirmed Maxwell s electromagnetic

More information

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

Lecture PowerPoints. Chapter 27 Physics: Principles with Applications, 7th edition Giancoli Lecture PowerPoints Chapter 27 Physics: Principles with Applications, 7th edition Giancoli This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching

More information

12.1 Foundations of Quantum Theory

12.1 Foundations of Quantum Theory 1.1 Foundations of Quantum Theory Physics Tool box A blacbody of a given temperature emits electromagnetic radiation over a continuous spectrum of frequencies, with a definite intensity maximum at one

More information

The temperature of a lava flow can be approximated by merely observing its colour. The result agrees nicely with the measured temperatures of lava

The temperature of a lava flow can be approximated by merely observing its colour. The result agrees nicely with the measured temperatures of lava The temperature of a lava flow can be approximated by merely observing its colour. The result agrees nicely with the measured temperatures of lava flows at about 1,000 to 1,200 C. In the late 19 th

More information

QUANTUM MECHANICS AND MOLECULAR SPECTROSCOPY

QUANTUM MECHANICS AND MOLECULAR SPECTROSCOPY QUANTUM MECHANICS AND MOLECULAR SPECTROSCOPY CHEM 330 B. O. Owaga Classical physics Classical physics is based on three assumptions i. Predicts precise trajectory for particles with precisely specified

More information

Photoelectric Effect Worksheet

Photoelectric Effect Worksheet Photoelectric Effect Worksheet The photoelectric effect refers to the emission of electrons from metallic surfaces usually caused by incident light. The incident light is absorbed by electrons thus giving

More information

INTRODUCTION Radiation differs from conduction and convection in that it does not require the presence of a material medium to take place.

INTRODUCTION Radiation differs from conduction and convection in that it does not require the presence of a material medium to take place. RADIATION INTRODUCTION Radiation differs from conduction and convection in that it does not require the presence of a material medium to take place. Radiation: The energy emitted by matter in the form

More information

Lasers PH 645/ OSE 645/ EE 613 Summer 2010 Section 1: T/Th 2:45-4:45 PM Engineering Building 240

Lasers PH 645/ OSE 645/ EE 613 Summer 2010 Section 1: T/Th 2:45-4:45 PM Engineering Building 240 Lasers PH 645/ OSE 645/ EE 613 Summer 2010 Section 1: T/Th 2:45-4:45 PM Engineering Building 240 John D. Williams, Ph.D. Department of Electrical and Computer Engineering 406 Optics Building - UAHuntsville,

More information

Determination of Stefan-Boltzmann Constant.

Determination of Stefan-Boltzmann Constant. Determination of Stefan-Boltzmann Constant. An object at some non-zero temperature radiates electromagnetic energy. For the perfect black body, which absorbs all light that strikes it, it radiates energy

More information

Quantum Mechanics. An essential theory to understand properties of matter and light. Chemical Electronic Magnetic Thermal Optical Etc.

Quantum Mechanics. An essential theory to understand properties of matter and light. Chemical Electronic Magnetic Thermal Optical Etc. Quantum Mechanics An essential theory to understand properties of matter and light. Chemical Electronic Magnetic Thermal Optical Etc. Fall 2018 Prof. Sergio B. Mendes 1 CHAPTER 3 Experimental Basis of

More information

Quantum and Atomic Physics - Multiple Choice

Quantum and Atomic Physics - Multiple Choice PSI AP Physics 2 Name 1. The Cathode Ray Tube experiment is associated with: (A) J. J. Thomson (B) J. S. Townsend (C) M. Plank (D) A. H. Compton 2. The electron charge was measured the first time in: (A)

More information

David J. Starling Penn State Hazleton PHYS 214

David J. Starling Penn State Hazleton PHYS 214 All the fifty years of conscious brooding have brought me no closer to answer the question, What are light quanta? Of course today every rascal thinks he knows the answer, but he is deluding himself. -Albert

More information

The Photoelectric Effect

The Photoelectric Effect 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 information

2. Fingerprints of Matter: Spectra

2. Fingerprints of Matter: Spectra 2. Fingerprints of Matter: Spectra 2.1 Measuring spectra: prism and diffraction grating Light from the sun: white light, broad spectrum (wide distribution) of wave lengths. 19th century: light assumed

More information

Historical Background of Quantum Mechanics

Historical Background of Quantum Mechanics Historical Background of Quantum Mechanics The Nature of Light The Structure of Matter Dr. Sabry El-Taher 1 The Nature of Light Dr. Sabry El-Taher 2 In 1801 Thomas Young: gave experimental evidence for

More information

Chapter 9: Quantization of Light

Chapter 9: Quantization of Light Chapter 9: Quantization of Light Max Planck started the revolution of quantum theory by challenging the classical physics and the classical wave theory of light. He proposed the concept of quantization

More information

Chapter 27 Quantum Physics

Chapter 27 Quantum Physics Key Ideas Two Principles of Relativity: The laws of physics are the same for all uniformly moving observers. The speed of light is the same for all observers. Consequences: Different observers measure

More information

PHY 571: Quantum Physics

PHY 571: Quantum Physics PHY 571: Quantum Physics John Venables 5-1675, john.venables@asu.edu Spring 2008 Introduction and Background Topics Module 1, Lectures 1-3 Introduction to Quantum Physics Discussion of Aims Starting and

More information

5. Light-matter interactions: Blackbody radiation

5. Light-matter interactions: Blackbody radiation 5. Light-matter interactions: Blackbody radiation The electromagnetic spectrum Sources of light Boltzmann's Law Blackbody radiation why do hot things glow? The cosmic microwave background The electromagnetic

More information

Quantum Mechanics. Particle in a box All were partial answers, leading Schrödinger to wave mechanics

Quantum Mechanics. Particle in a box All were partial answers, leading Schrödinger to wave mechanics Chemistry 4521 Time is flying by: only 15 lectures left!! Six quantum mechanics Four Spectroscopy Third Hour exam Three statistical mechanics Review Final Exam, Wednesday, May 4, 7:30 10 PM Quantum Mechanics

More information

Module 5 : MODERN PHYSICS Lecture 23 : Particle and Waves

Module 5 : MODERN PHYSICS Lecture 23 : Particle and Waves Module 5 : MODERN PHYSICS Lecture 23 : Particle and Waves Objectives In this lecture you will learn the following Radiation (light) exhibits both wave and particle nature. Laws governing black body radiation,

More information

Exam 2 Development of Quantum Mechanics

Exam 2 Development of Quantum Mechanics PHYS420 (Spring 2002) Riq Parra Exam #2 (Friday, April 12 th, 2002) Exam 2 Development of Quantum Mechanics Do NOT write your name on this exam. Write your class ID number on the top right hand corner

More information

λ φ φ = hc λ ev stop φ = λ φ and now ev stop λ ' = Physics 220 Homework #2 Spring 2016 Due Monday 4/11/16

λ φ φ = hc λ ev stop φ = λ φ and now ev stop λ ' = Physics 220 Homework #2 Spring 2016 Due Monday 4/11/16 Physics 0 Homework # Spring 06 Due Monday 4//6. Photons with a wavelength λ = 40nm are used to eject electrons from a metallic cathode (the emitter) by the photoelectric effect. The electrons are prevented

More information

ugrad/361

ugrad/361 Quantum Mechanics and Atomic Physics Monday & Wednesday 1:40-3:00 SEC 209 http://www.physics.rutgers.edu/ugrad/361 Sean Oh ohsean@physics.rutgers.edu sics ed Serin W121 http://www.physics.rutgers.edu/

More information

Welcome back to PHY 3305

Welcome back to PHY 3305 Welcome back to PHY 3305 Today s Lecture: Double Slit Experiment Matter Waves Louis-Victor-Pierre-Raymond, 7th duc de Broglie 1892-1987 AnNouncements Reading Assignment for Thursday, Sept 28th: Chapter

More information

PHYSICS 3204 PUBLIC EXAM QUESTIONS (Quantum pt.1)

PHYSICS 3204 PUBLIC EXAM QUESTIONS (Quantum pt.1) PHYSICS 3204 PUBLIC EXAM QUESTIONS (Quantum pt.1) NAME: August 2009--------------------------------------------------------------------------------------------------------------------------------- 11 41.

More information

5. Light-matter interactions: Blackbody radiation

5. Light-matter interactions: Blackbody radiation 5. Light-matter interactions: Blackbody radiation REMINDER: no lecture on Monday Feb. 6th The electromagnetic spectrum Sources of light Boltzmann's Law Blackbody radiation The cosmic microwave background

More information

Introduction to Modern Physics NE 131 Physics for Nanotechnology Engineering

Introduction to Modern Physics NE 131 Physics for Nanotechnology Engineering Introduction to Modern Physics NE 131 Physics for Nanotechnology Engineering Dr. Jamie Sanchez-Fortún Stoker Department of Physics, University of Waterloo Fall 2005 1 Introduction to Modern Physics 1.1

More information

Atomic Physics and Lasers. The idea of a photon. Light from a hot object... Example of a Blackbody. Example of a Blackbody

Atomic Physics and Lasers. The idea of a photon. Light from a hot object... Example of a Blackbody. Example of a Blackbody Atomic Physics and Lasers The idea of a photon Black body radiation Photoelectric Effect The structure of the atom How does a Laser work? Interaction of lasers with matter Laser safety Applications Spectroscopy,

More information

27-1 Planck Solves the Ultraviolet Catastrophe

27-1 Planck Solves the Ultraviolet Catastrophe 27-1 Planck Solves the Ultraviolet Catastrophe By the end of the 19 th century, most physicists were confident that the world was well understood. Aside from a few nagging questions, everything seemed

More information

Physics 2D Lecture Slides. Oct 15. UCSD Physics. Vivek Sharma

Physics 2D Lecture Slides. Oct 15. UCSD Physics. Vivek Sharma Physics 2D Lecture Slides Oct 15 Vivek Sharma UCSD Physics Properties of EM Waves: Maxwell s Equations Power incident on an area A Intensity of Radiation I = Larger t Energy Flow in EM W aves : 1 Poy nting

More information

Part I. Quantum Mechanics. 2. Is light a Wave or Particle. 3a. Electromagnetic Theory 1831 Michael Faraday proposes Electric and Magnetic Fields

Part I. Quantum Mechanics. 2. Is light a Wave or Particle. 3a. Electromagnetic Theory 1831 Michael Faraday proposes Electric and Magnetic Fields Quantized Radiation (Particle Theory of Light) Dr. Bill Pezzaglia Part I 1 Quantum Mechanics A. Classical vs Quantum Theory B. Black Body Radiation C. Photoelectric Effect 2 Updated: 2010Apr19 D. Atomic

More information

Complementi di Fisica Lectures 7-9

Complementi di Fisica Lectures 7-9 Complementi di Fisica Lectures 7-9 Livio Lanceri Università di Trieste Trieste, 07/09-10-2012 Course Outline - Reminder Quantum Mechanics: an introduction Waves as particles and particles as waves (the

More information