Blackbody Radiation All bodies at a temperature T emit and absorb thermal electromagnetic radiation Blackbody radiation In thermal equilibrium, the power.

Slides:



Advertisements
Similar presentations
Physics 2 Chapter 27 Sections 1-3.
Advertisements

Blackbody Radiation & Planck’s Hypothesis
2. The Particle-like Properties Of Electromagnetic Radiation
Blackbody Radiation & 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,
Quantum Theory of Light A TimeLine. Light as an EM Wave.
Chapter 45 The Nature of Light. Light Particle (photon) Wave (electromagnetic wave) Interference Diffraction Polarization.
Introduction to Quantum Physics
The Birth of the Quantum. Blackbody A body that absorbs all the electromagnetic radiation that falls on it. Example: opening of a cave or oven:
What is the nature of Part I. The invention of radio? Hertz proves that light is really an electromagnetic wave. Waves could be generated in one circuit,
Quantum Mechanics Photoelectric Effect. Lesson Aims State the main observations of Millikan’s experiment Explain the failure of classical wave theory.
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.
Black Body radiation Hot filament glows.
Physics at the end of XIX Century Major Discoveries of XX Century
The birth of quantum mechanics Until nearly the close of the 19 th century, classical mechanics and classical electrodynamics had been largely successful.
The Birth of the Quantum Theory Classically: Mechanics (Newton), Electromagnetism (Maxwell), Thermodynamics (Carnot, mayer, Helmholtz, Clausius, Kelvin),
Light as a Particle. Objectives  Define a quantum  Calculate the energy of a photon  Relate photon energy to wavelength and frequency of EMR.
Physics 361 Principles of Modern Physics Lecture 3.
Lecture 1 Quantization of energy. Quantization of energy Energies are discrete (“quantized”) and not continuous. This quantization principle cannot be.
WHAT IS A QUANTUM THEORY ? Quantum theory is the theoretical basis of modern physics that explains the nature and behavior of matter and energy on the.
PHYSICAL CHEMISTRY - ADVANCED MATERIALS Particles and Waves Standing Waves Wave Function Differential Wave Equation Something more about…. X=0 X=L Standing.
Chapter 1 Thermal radiation and Planck’s postulate
Ch 9 pages Lecture 18 – Quantization of energy.
Chapter 3 Light at Particles. Blackbody Radiation.
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.
Thompson’s experiment (discovery of electron) + - V + - Physics at the end of XIX Century and Major Discoveries of XX Century.
Chemistry 330 Chapter 11 Quantum Mechanics – The Concepts.
Photon Statistics Blackbody Radiation 1.The energy loss of a hot body is attributable to the emission of electromagnetic waves from the body. 2.The.
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.
Modern Physics Quantum Effects 1773 – 1829 Objectives  Explain the photoelectric effect and recognize that quantum theory can explain it, but wave theory.
Classical Physics Newton’s laws: Newton’s laws: allow prediction of precise trajectory for particles, with precise locations and precise energy at every.
Lecture 27 — The Planck Distribution Chapter 8, Friday March 21 st Quick review of exam 2 Black-body radiation Before Planck: Wien and Rayleigh-Jeans The.
4: Introduction to Quantum Physics
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.
Lecture_02: Outline Thermal Emission
Modern Atomic Theory Quantum Theory and the Electronic Structure of Atoms Chapter 11.
Dualisme Cahaya Sebagai Gelombang dan Partikel
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”:
IB Physics 12 Mr. Jean February 5 th, The plan: Video clip of the day. Quantum Theory Energy Levels.
QUANTUM AND NUCLEAR PHYSICS. Wave Particle Duality In some situations light exhibits properties that are wave-like or particle like. Light does not show.
Blackbody. Kirchhoff’s Radiation  Radiated electromagnetic energy is the source of radiated thermal energy. Depends on wavelengthDepends on wavelength.
Topic I: Quantum theory Chapter 7 Introduction to Quantum Theory.
Light is a Particle Physics 12 Adv. Blackbody Radiation A blackbody is a perfect emitter; that is it emits the complete EM spectrum Work done by Gustav.
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.
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.
The temperature of a lava flow can be estimated by observing its color
Plan for Today (AP Physics 2) Questions on HW (due tomorrow) Notes/Lecture on Blackbody Radiation.
Instructor: Suchetana Chatterjee Presidency University Physics -0402
PHYS 3313 – Section 001 Lecture #9
The Planck Distribution
Origin of Quantum Theory
PHYS 3313 – Section 001 Lecture #10

Quantized Energy and Photons
General Physics (PHY 2140) Lecture 27 Modern Physics Quantum Physics
Quantum Physics Interaction of matter with energy
Atomic Physics & Quantum Effects
Quantization of Light It seemed to be a wave....
PHOTOELECTRIC EFFECT hhhhh 12/4/2018.
Chapter 27 Early Quantum Theory
Blackbody Radiation All bodies at a temperature T emit and absorb thermal electromagnetic radiation Blackbody radiation In thermal equilibrium, the power.
Physics and the Quantum Model
Quantum Mechanics IB Physics.
Physics at the end of XIX Century Major Discoveries of XX Century
Chapter 29 Photoelectric Effect
Unit 2 Particles and Waves Photoelectric Effect
Photoelectric Effect And Quantum Mechanics.
PHYS 3313 – Section 001 Lecture #10
Presentation transcript:

Blackbody Radiation All bodies at a temperature T emit and absorb thermal electromagnetic radiation Blackbody radiation In thermal equilibrium, the power emitted equals the power absorbed How is blackbody radiation absorbed and emitted?

Blackbody Radiation

Blackbody Radiation A blackbody is a perfect absorber of radiation A simple blackbody is given by a hole in a wall of some enclosure Both absorption and can occur The radiation properties of the cavity are independent of the enclosure material

Blackbody Radiation The y axis is power per area per wavelength

Blackbody Radiation

Blackbody Radiation Wien’s displacement law Stefan-Boltzmann law Wavelength decreases as T increases Stefan-Boltzmann law Total power / area radiated increases as T4

Blackbody Radiation Attempts to calculate the spectral distribution of blackbody radiation from first principles failed The best description was given by the Rayleigh-Jeans formula This described the distribution at long wavelengths but increased without limit as λ→0 Ultraviolet catastrophe

Blackbody Radiation

Blackbody Radiation Planck was able to calculate the correct distribution by assuming energy was quantized (he was desperate) Microscopic (atomic) oscillators can only have certain discrete energies The oscillators can only absorb or emit energy in multiples of

Blackbody Radiation Planck’s radiation law agreed with data It leads directly to Wien’s displacement law and the Stefan-Boltzmann law It agrees with Rayleigh-Jeans formula for large wavelengths See derivations for both in Thornton and Rex

Blackbody Radiation We may derive the radiation law later in the course but for now consider The electromagnetic energy inside the (metallic) cavity must exist in the form of standing waves with nodes at the surfaces Classically, the equipartition theorem gives the average energy of a standing wave Note the same value is predicted for all standing waves independent of their frequency The amount of radiation coming out of the cavity is then the number of different wave modes X the energy per mode

Blackbody Radiation Let E=nhv, then the average energy is

Kinetic Theory of Gases Based on “atomic” theory of matter Results include Speed of a molecule in a gas vrms = (<v2>)1/2 = (3kT/m)1/2 Equipartion theorem Internal energy U = f/2 NkT = f/2 nRT Heat capacity CV = (dU/dT)V = f/2 R Maxwell speed distribution

Blackbody Radiation To evaluate this we use standard “tricks” from statistical mechanics

Blackbody Radiation And note

Blackbody Radiation Putting these together we have

Blackbody Radiation To finish the calculation we’d have to multiply the average energy of a wave of frequency f x the number of waves with frequency f This would give us the Planck distribution

Blackbody Radiation You can how Planck avoided the ultraviolet catastrophe Because the energy is proportional to the frequency The average energy is kT when the possible energies are small compared to kT The average energy is extremely small when the possible energies are large compared to kT (because P(ε) is extremely small)

Blackbody Radiation Planck’s paper is generally considered to be the birthplace of quantum mechanics Revisionist history? Planck did not pay too much attention to energy quantization Neither did anyone else There is controversy of whether he even intended the energy of an oscillator to be nhf

Photoelectric Effect Light incident on a metal will eject electrons Aside, other means of doing this are with temperature, electric fields, and particle bombardment

Photoelectric Effect Experiments showed Kinetic energy of the photoelectrons are independent of the light intensity The maximum kinetic energy of the photoelectrons depends on the light frequency The smaller the work function φ the smaller the threshold frequency to produce photoelectrons The number of photoelectrons is proportional to light intensity

Photoelectric Effect

Photoelectric Effect

Photoelectric Effect Explained by Einstein in one of his annus mirabilis papers In his paper he assumed Electromagnetic field was quantized Light quanta were localized in space (like particles) == photons Energy E = hf In the photoelectric process, the energy quanta (photons) are completely absorbed

Photoelectric Effect Thus photons penetrate the surface of the metal and are absorbed by electrons The electrons overcome attractive forces that normally hold them in the material and escape Conservation of energy gives hf = 1/2mv2max + φ And consequently he predicted 1/2mv2max= eV0 = hf – φ Note h/e can be measured from the slope

Photoelectric Effect This was strange since it involved Planck’s constant h This was a difficult experiment to carry out It took almost a decade to verify Millikan was the principle experimenter (who tried to prove Einstein’s theory wrong) The end result was proof that light energy is quantized and E=hf

Photoelectric Effect