Rayat Shikshan Sanstha’s S. M

Slides:



Advertisements
Similar presentations
The Photoelectric Effect Key Points. What is it ? Electrons are emitted from zinc when ultraviolet radiation shines on it. Other metals emit electrons.
Advertisements

An Introduction to Quantum
Chapter 29 - Particles and Waves. 1.Who won the Nobel prize for his explanation of the photoelectric effect? A.Planck B.Bohr C.De Broglie D.Einstein 2.The.
Blackbody Radiation & Planck’s Hypothesis
Black body radiation BBR is the radiation emitted by a non-reflecting solid body. A perfect black body is one which absorbs all the radiations falling.
Wave-Particle Duality: The Beginnings of Quantum Mechanics
Electromagnetic Radiation
The Modern Atom Figure: 05-00CO Caption:
Physics at the end of XIX Century Major Discoveries of XX Century
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.
PH 103 Dr. Cecilia Vogel Lecture 17. Review Outline  Quantum Mechanics  What is quantization?  Photon  Two pieces of evidence:  blackbody radiation.
Chapter 7. Light as a wave  carries energy but doesn’t actually move  Think of a cork on water and surfer. The above diagram is a typical way to visualize.
Index Unit 03 Electron Configuration Module 02: Light as a Particle Based on the PowerPoints By Mr. Kevin Boudreaux, Angelo State Univerisity U03Mod01.
QW *Use the light kits at your tables to perform and answer the following: Shine red, blue, and green lights at glow in the dark material 1. Which one.
Wave-Particle Duality 1: The Beginnings of Quantum Mechanics.
Quantum Mechanics. What is Quantum Physics? Quantum physics takes into account every possible outcome of measurement of physical properties  Quantum.
E = hf E – energy of a quantum (Joules) h – Plank’s constant (6.626 x J  s) f – frequency of absorbed or emitted EMR.
E = hf E – energy of a quantum (Joules) h – Plank’s constant (6.626 x J  s) f – frequency of absorbed or emitted EMR.
Particle Properties of Light. Objectives To discuss the particle nature of light.
Physics 30 – Electromagnetic Radiation – Part 2 Wave-Particle Duality
Light and the Electromagnetic Spectrum. Light Phenomenon Isaac Newton ( ) believed light consisted of particles By 1900 most scientists believed.
Nuclear Atom and Unanswered Questions
Blackbody Radiation And Spectra. Light is a form of _______. Why is this important? With very few exceptions, the only way we have to study objects in.
I II III  Suggested Reading Pages  Section 4-1 Radiant Energy.
As an object gets hot, it gives Off energy in the form of Electromagnetic radiation.
Wave-Particle Duality: The Beginnings of Quantum Mechanics.
Wave-Particle Duality: The Beginnings of Quantum Mechanics.
Thompson’s experiment (discovery of electron) + - V + - Physics at the end of XIX Century and Major Discoveries of XX Century.
Physics and the Quantum Mechanical Model Notes. Light and the Atomic Spectrum Light is composed of waves at different wavelengths The wave is composed.
Wave-Particle Duality: The Beginnings of Quantum Mechanics.
Photons, Electrons, and Atoms. Visible and non-visable light Frequencies around Hz Much higher than electric circuits Theory was about vibrating.
a.k.a. “Classical Physics”
Modern Physics Quantum Effects 1773 – 1829 Objectives  Explain the photoelectric effect and recognize that quantum theory can explain it, but wave theory.
PARTICLE NATURE OF LIGHT. A Black Object Appears black because it absorbs all frequencies of light A black block of iron does this.
Physics 1202: Lecture 30 Today’s Agenda Announcements: Extra creditsExtra credits –Final-like problems –Team in class HW 9 next FridayHW 9 next Friday.
Modern Atomic Theory Quantum Theory and the Electronic Structure of Atoms Chapter 11.
 Waves & Energy H Ch 5&6. Waves  Vibrating disturbance by which energy is transmitted Amplitude (Wavelength) u = λν.
12.8 Light as Particles: The Photoelectric Effect Einstein expanded on Newton and Planck’s idea of light as particles Einstein expanded on Newton and Planck’s.
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.
4-2 Quantum Theory. Planck’s Theory Max Planck predicted accurately how the spectrum of radiation emitted by an object changes with temperature.
Electromagnetic Radiation. Waves To understand the electronic structure of atoms, one must understand the nature of electromagnetic radiation. The distance.
5.3 Atomic Emission Spectra and the Quantum Mechanical Model 1 > Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Chapter 5.
Light and the Electromagnetic Spectrum
Light and the Electromagnetic Spectrum
The Wacky World of Quantum Physics
Light and the Electromagnetic Spectrum
Spectral Lines 3.2.
Quantized Energy and Photons
VISHWAKARMA GOVERNMENT ENGINEERING COLLEGE
Radiation.
Unit 3: Electrons in the Atom
Chapter 5 Electrons In Atoms 5.3 Atomic Emission Spectra
Wien’s Law The Color and Temperature of Stars.
Wien’s Law The Color and Temperature of Stars.
Quantum Mechanics & the Nature of Matter, Motion and Reality
Light and the Electromagnetic Spectrum
Waves and particles Ch. 4.
Basics of Quantum Mechanics
Electronic Structure of Atoms
Continuous, Emission, and Absorption
Light and the Electromagnetic Spectrum
Light and the Electromagnetic Spectrum
Physics at the end of XIX Century Major Discoveries of XX Century
4.6 NOTES Atomic Emission Spectra
Elementary Quantum Mechanics
Light and the Electromagnetic Spectrum
Light and the Electromagnetic Spectrum
Light and the Electromagnetic Spectrum
Photoelectric Effect And Quantum Mechanics.
Quantized Energy and Photons
Presentation transcript:

Rayat Shikshan Sanstha’s S. M Rayat Shikshan Sanstha’s S.M.Joshi College Hadapsar Department of Physics Subject- Quantum Mechanics Dr.R.S.Nimbalkar

Blackbody Radiation Known since centuries that when a material is heated, it radiates heat and its color depends on its temperature • Example: heating elements of a stove: – Dark red: 550ºC – Bright red: 700ºC – Then: orange, yellow and finally white (really hot !) The emission spectrum depends on the material Theoretical description: simplifications necessary Blackbody

Blackbody A material is constantly exchanging heat with its surrounding (to remain at a constant temperature): – It absorbs and emits radiations – Problem: it can reflect incoming radiations, which makes a theoretical description more difficult (depends on the environment) A blackbody is a perfect absorber: – Incoming radiations is totally absorbed and none is reflected

The photoelectric effect provides evidence for the particle nature of light. It also provides evidence for quantization. If light shines on the surface of a metal, there is a point at which electrons are ejected from the metal. The electrons will only be ejected once the threshold frequency is reached . Below the threshold frequency, no electrons are ejected. Above the threshold frequency, the number of electrons ejected depend on the intensity of the light.