Quantum Physics. The Quantization of Light §19-1 Thermal Radiation and Plank’s theory of Radiation 热辐射 普朗克的量子假设 §19-2 The Photoelectric Effect and Einstein’s.

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

A potential difference V is maintained between the metal target and the collector cup Electrons ejected from C travel to A and G detects the flow Apply.
Ch6 X-ray Producing X-ray Moseley formula X-ray diffraction
equipment 2. Photoelectric Effect. Einstein’s Photon Theory ( 光电效应、爱因斯坦光子理论 ) R K1K1 K2K2 E G V les, called photons. Einstein assumed that the energy.
Knight - Chapter 28 (Grasshopper Book) Quantum Physics.
光 電 效 應 實 驗光 電 效 應 實 驗. The Interaction of Radiation with Matter( 電磁輻射與物質之間作用 ) The Photoelectric Effect ( 光電效應 ) The Compton Effect ( 康卜吞效應 ) The Pair.
Early Quantum Theory and Models of the Atom
PHOTOELECTRIC EFFECT AND DUAL NATURE OF MATTER AND RADIATIONS 1.Photoelectric Effect 2.Experimental Set-up to study Photoelectric Effect 3.Effect of Intensity,
1 Chapter 38 Light Waves Behaving as Particles February 25, 27 Photoelectric effect 38.1 Light absorbed as photons: The photoelectric effect Photoelectric.
2. The Particle-like Properties Of Electromagnetic Radiation
Blackbody Radiation & Planck’s Hypothesis
Chapter 27 Quantum Physics.  Understand the relationship between wavelength and intensity for blackbody radiation  Understand how Planck’s Hypothesis.
The dual nature of light l wave theory of light explains most phenomena involving light: propagation in straight line reflection refraction superposition,
Chapter 45 The Nature of Light. Light Particle (photon) Wave (electromagnetic wave) Interference Diffraction Polarization.
Introduction to Quantum Physics
Classical vs Quantum Mechanics Rutherford’s model of the atom: electrons orbiting around a dense, massive positive nucleus Expected to be able to use classical.
What is the nature of Part II. Last week we surmised that photons must carry momentum in spite of the fact that they are massless. Last time we learned.
Chapter 2: Particle Properties of Waves
the photoelectric effect. line spectra emitted by hydrogen gas
Young/Freeman University Physics 11e. Ch 38 Photons, Electrons, and Atoms © 2005 Pearson Education.
More About Photoelectricity Quantum Physics Lesson 2.
The Particlelike Properties of Electromagnetics Radiation Wei-Li Chen 10/27/2014.
CHAPTER 40 : INTRODUCTION TO QUANTUM PHYSICS 40.2) The Photoelectric Effect Light incident on certain metal surfaces caused electrons to be emitted from.
Quantum Mechanics. Planck’s Law A blackbody is a hypothetical body which absorbs radiation perfectly for every wave length. The radiation law of Rayleigh-Jeans.
Quantum Physics. Quantum Theory Max Planck, examining heat radiation (ir light) proposes energy is quantized, or occurring in discrete small packets with.
Blackbody Radiation: The light from a blackbody is light that comes solely from the object itself rather than being reflected from some other source. A.
1 PHYS 3313 – Section 001 Lecture #10 Monday, Feb. 17, 2014 Dr. Jaehoon Yu Photoelectric Effect Compton Effect Pair production/Pair annihilation Monday,
Thompson’s experiment (discovery of electron) + - V + - Physics at the end of XIX Century and Major Discoveries of XX Century.
Baby-Quiz 1.Why are diffraction effects of your eyes more important during the day than at night? 2.Will the converging lens focus blue light or red light.
Physics 1C Lecture 28A. Blackbody Radiation Any object emits EM radiation (thermal radiation). A blackbody is any body that is a perfect absorber or emitter.
Quantum Physics Chapter 27!.
Modern Physics Quantum Effects 1773 – 1829 Objectives  Explain the photoelectric effect and recognize that quantum theory can explain it, but wave theory.
Questions From Reading Activity? Assessment Statements  Topic 13.1, Quantum Physics: The Quantum Nature of Radiation Describe the photoelectric.
Chapter 40 Introduction to Quantum Physics. Need for Quantum Physics Problems remained from classical mechanics that relativity didn’t explain Attempts.
4: Introduction to Quantum Physics
Origin of Quantum Theory
Wednesday, Feb. 25, 2015 PHYS , Spring 2014 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #10 Wednesday, Feb. 25, 2015 Dr. Jaehoon Yu Blackbody.
LIGHT and MATTER Chapters 11 & 12. Originally performed by Young (1801) to demonstrate the wave-nature of light. Has now been done with electrons, neutrons,
Dualisme Cahaya Sebagai Gelombang dan Partikel
THE PHOTOELECTRIC EFFECT. When red light is incident on a clean metal surface: no electrons are released, however long light is shone onto it, however.
Light is a Particle Physics 12.
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”:
Chapter 33 Early Quantum Theory and Models of Atom.
Physics 213 General Physics Lecture Exam 3 Results Average = 141 points.
Photon-matter interactions Contents: Photoelectric effect Compton scattering Pair production.
3.1 Discovery of the X-Ray and the Electron 3.2Determination of Electron Charge 3.3Line Spectra 3.4Quantization 3.5Blackbody Radiation 3.6Photoelectric.
Compton Effect X-Ray Scattering Classical Theory (cont’d): c) The scattered radiation should have the same frequency as the incident radiation d) Because.
Lecture_04: Outline Photoelectric Effect  Experimental facts  Einstein’s explanation  Problems.
3.1 Discovery of the X-Ray and the Electron 3.2Determination of Electron Charge 3.3Line Spectra 3.4Quantization 3.5Blackbody Radiation 3.6Photoelectric.
Chapter 38 Photons: Light Waves Behaving as Particles
Origin of Quantum Theory
PHYS 3313 – Section 001 Lecture #10

What is the nature of Light ? Part II.
General Physics (PHY 2140) Lecture 27 Modern Physics Quantum Physics
Chapter 38 Photons: Light Waves Behaving as Particles
Atomic Physics & Quantum Effects
Blackbody Radiation All bodies at a temperature T emit and absorb thermal electromagnetic radiation Blackbody radiation In thermal equilibrium, the power.
Photoelectric Effect Maximum kinetic energy of the electron:
Quantization of Light It seemed to be a wave....
PHOTOELECTRIC EFFECT hhhhh 12/4/2018.
Chapter 27 Early Quantum Theory
Introduction and Basic Concepts
Interaction of Electromagnetic Radiation with Matter
Quantization of light, charge and energy Chapter 2-Class5
The Electronic Structure of Atoms
Chapter 29 Photoelectric Effect
Chapter 38 Photons: Light Waves Behaving as Particles
Photoelectric Effect And Quantum Mechanics.
Presentation transcript:

Quantum Physics

The Quantization of Light

§19-1 Thermal Radiation and Plank’s theory of Radiation 热辐射 普朗克的量子假设 §19-2 The Photoelectric Effect and Einstein’s Quantum Theory 光电效应 爱因斯坦的 光子理论 §19-3 The Compton Effect 康普顿效应

I. Thermal radiation §19-1 Thermal Radiation and Plank’s theory of Radiation -- At any temperature, a body emits radiation of all wavelength, but the distribution in wavelength, the spectral distribution, depends on temperature.

Some concepts about thermal radiation 1. The spectral radiancy ( 光谱辐射出射度 ) e (,T) Let de(,T): the energy emitted per unit time in radiation of wavelength in the interval +d from an unit area of the surface at absolute temperature T. e (,T) specifies the spectral distribution of an body radiation at T. Then,

2. Radiancy ( 辐射出射度 ) E(T) The total energy emitted per unit time per unit area from a body at temperature T. The integral of spectral radiancy e (,T) over all.

All bodies emit radiation to their surrounding and radiation may fall on a body. 3. Black body( 黑体 ) When radiation falls on a body, absorbed reflected Black body: can absorb all radiation falling on it. no any reflection. ----ideal model.

外壳 热电偶 保温层 加热线圈 腔体 腔芯 热屏蔽套管

II. The experiment results of black body radiation  e (,T) varies continuously with. Each e (,T) curve has a peak.  e (,T) curve increases rapidly with the increasing of T.  m decreases linearly with T increasing

Quantitatively, (1) Stefan’s law  =5.67  W/m 2 ·K 4 --Stefan constant (2) Wien’s displacement law b=2.898  m  K --Wien constant.

[Example] Stefan’s law can be used to determine the radius of a sun in astronomy. It is known that the radiation power of a sun arriving to unit area of the earth is 1.2  W/m 2. The distance between the sun and the earth is 4.3  m. The temperature of the sun’s surface is 5200K. The sun can be regarded as a black body.Find its radius. Solution Let R: sun’s radius, R : distance between sun and earth R : distance between sun and earth Sun earth

Neglecting absorption, we have  The total radiation power of the sun is

III. Classical physics encountered difficulty for explaining the radiation of black body. How can we deduce the quantitative expression of e (,T ) theoretically and make it agree with the experiment?

c 1,c 2 : constants determined by experiment. F Wien’s semi-experiment formula : --It agrees with experiment only in short wavelength range. Wien’s line

F Rayleigh-Jeans formula It agrees with experiment only in longer wavelength range ultraviolet catastrophe ---- “ultraviolet catastrophe” Wein’s l Classical physics cannot explain the radiation of black body. R-J line

IV. Plank’s hypothesis and formula 1. “Quantum of energy ( 能量子 ) ” hypothesis F There are many oscillators in the black body. The energy of an oscillator of a given frequency cannot take arbitrary values, but can only take on the discrete values nh. where n is a positive integer or zero.  = nh is a finite amount, or quantum, of energy.  0 = h is the minimum energy of an oscillator quantum of energy ---- quantum of energy n ---- quantum number( 量子数 )

----Plank’s constant F Applying his hypothesis, Plank obtained ----Plank’s black body radiation formula Plank obtained great agreement with the experiment over the entire range of wavelength.

Furthermore, F Plank got the Nobel Prize in physics in  ---Stenfa’s law  Wien’s displacement law can be obtained.

[Example] A spring-particle oscillator system with k=15N/m, m=1kg and A=0.01m , Calculate  the total energy of the system E=?  the quantum number of the system n= ?  if n changes from n to n+1 or n-1,  E/E=? Solution  Total energy is  According to Plank’s hypothesis,

 n changes an unit, energy changes  If n changes an unit, energy changes F No any instrument can distinguish the changing. ----Quantum effect disappear for macro-system( 宏观系统 ). And

F Electrons are ejected from metal surface when it is radiated by high frequency electromagnetic waves §19-2 The photoelectric effect photoelectron Cathode ( 阴极 ) Quartz window

I. The results of the experiments 光强较强 光强较弱 饱和 电流 截止 电压 G—sensitive ammeter I s —saturated current V 0 —stopping potential

  The saturated current is proportional with the incident light intensity. --the number of photoelectrons ejected from cathode in an unit time is proportional with --the number of photoelectrons ejected from cathode in an unit time is proportional with the incident light intensity.  The photoelectric current =0 when an inverse stopping potential -V 0 is supplied --photoelectrons have the maximum initial kinetic energy.

 V 0 depends linearly on the frequency of the incident light and is independent of its intensity. i.e. cutoff frequency 0 Below 0, no photoelectric effect occurs.

 Electron emission takes place immediately as the light is incident on the surface with no detectable time delay. II. The classical wave theory of light cannot explain the results. According to the classical theory,  the initial kinetic energy would be decided by the intensity of light instead of the frequency of light.

 photoelectric effect would take place for any frequency of light as long as its intensity is large enough instead of existing a cutoff frequency 0.  the photoelectron would not escape from the metal immediately if the intensity of light is very small.

III. Einstein’s quantum theory of the PE-effect l The electromagnetic field itself is quantized and that light consists of corpuscles, called light quanta or photons. Each photon travels with the speed of light c and carries a quantum of energy of magnitude E=h l The electromagnetic field itself is quantized and that light consists of corpuscles, called light quanta or photons. Each photon travels with the speed of light c and carries a quantum of energy of magnitude E=h l The energy flow density ( or intensity ) of light is S =N h l The energy flow density ( or intensity ) of light is S =N h Einstein offered his “photon postulate” for explanation the results of PE-effect in 1905.

the energy of photon the work function of electron --Einstein’s photoelectric effect equation If v m =0, l When a photon falls on a metallic surface, then,

IV.Einstein’s explanation for photoelectric effect  larger intensity of light i.e. larger number of photons larger number of photoelectrons i.e. larger photoelectric current.  as i.e.

 there is a cutoff frequency  there is a cutoff frequency , no photoelectric effect for  W/h ,  A photon is absorbed by an electron immediately if  0 and the electron will eject immediately. F Conclusion : light is the flow of particles. Einstein got Noble prize on physics in 1921

[Example] A beam of ultraviolet light with =2500Å, intensity S=2W/m 2 irradiates on a potassium foil. The work function of potassium is W=2.21eV. Find  the maximum kinetic energy of the photoelectrons,  the maximum number of the photoelectrons per unit time per area from the surface of the potassium foil. Solution  Using Einstein’s equation,

Because one photon can knock out one electron only, the maximum number of the photoelectrons is  The energy of a photon is

I. The Compton effect §19-3 The Compton Effect When a beam of x-rays with sharply defined wavelength 0 falls on some target (such as graphite), it will be scattered and the scattered radiation have two components of wavelength:the origin wavelength 0 and the larger wavelength.

探测器 石墨 光阑 入射光 散射光 x 射 线管 Device Results

Results of experiment   = - 0 increase with the increment of scattering angle .  has nothing to do with 0 and scatter (target).  the intensity of 0 decreases and the intensity of increase with the increment of .

14 S i 16 S 19 K 20 C a 24 C r 26 F e 28 N i 29 C u  the intensity of is larger for the target with lighter atoms than the target with heavier atoms.

Classical theory: x-ray is electromagnetic wave. It acts on the free electrons of the target. There should not be the component of in scattered rays. II.The explanations for Compton effect. Forcing the electrons oscillate at same frequency. radiate electromagnetic wave with same same frequency.

Photon collides with electron in elastic. Photon theory :  Photons collide with the outer bound electrons in the atoms of the target,

outer bound electron looked as free electron Ze          h 0 Ze          h mc 2 Part of energy is transferred to electron

 Photons collide with the inner bound electrons in the atoms of the target, inner bound electron looked as free electron Ze          h 0 equivalent to collide with the whole atoms of target. As m atom >> m photon,  photon does not lose energy. So we have = 0 or = 0

 Ze          h 0 Compton effect is evident for smaller Z than bigger Z.

III. The Compton equation 1.Photons collide with the outer bound electrons Before collision photon : energy momentum electron : After collision photon : electron : E,PE,P Ee,PeEe,Pe

Conservation of momentum Conservation of energy    

Considering relativistic energy and momentum electron : For photon :  and  can be re-written substituting We get : and :

or ----Compton wavelength of the electron Here ----depend on  only The magnitude of c is closer to the magnitude of the wavelength 0 of x-ray (0.1~100Å) =2.43  Å So  is evident.

2.Photon collides with the inner bound electron The mass of atom >> m 0 So Compton effect is not evident.

[Example] x-ray with 0 =1.00  m is scattered by electron. Find  The Compton shift at the scattering angle  =90 0 and  The energy that each electron gets from x-ray. Solution : 

 The energy that each electron gets from x-ray So the energy that each electron gets = the energy that each photon lose