Quantum Theory By: Lucas, Steven, Brandon and Kristen.

Slides:



Advertisements
Similar presentations
Energy and Electrons. Wave-Particle Duality JJ Thomson won the Nobel prize for describing the electron as a particle. His son, George Thomson won the.
Advertisements

Electromagnetic Spectrum Light as a Particle. Learning Objectives Understand the electromagnetic spectrum Understand the relationships between wavelength,
Electromagnetic Radiation
The Electronic Structures of Atoms Electromagnetic Radiation
Blackbody Radiation. Blackbody: an object that absorbs and emits all radiations of all possible frequencies Kirchhoff observed that when heated to incandescence,
Electronic Structure of Atoms
ENERGY & LIGHT THE QUANTUM MECHANICAL MODEL. Atomic Models What was Rutherford’s model of the atom like? What is the significance of the proton? What.
Quantum Theory of the Atom Chapter 7 Dr. Victor Vilchiz.
Properties of Light Is Light a Wave or a Particle?
Light, Photon Energies, and Atomic Spectra
Black body radiation and ultraviolet catastrophe
November 22, Name of the Game: ENERGY And also: NOBEL PRIZES FOR PHYSICS.
Down The Rabbit Hole: Quantum Physics Lesson 8. Objectives Define a quantum Calculate the energy of a photon Relate photon energy to wavelength and frequency.
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.
Black Body radiation Hot filament glows.
Modern Physics (PC300) Class #9: Introductory Stuff towards Quantum Mechanics.
Quantum Physics. Black Body Radiation Intensity of blackbody radiation Classical Rayleigh-Jeans law for radiation emission Planck’s expression h =
The Photoelectric Effect Textbook: 12.1 Homework: pg. 608 #2, 8,
Electromagnetic Spectrum. Quantum Mechanics At the conclusion of our time together, you should be able to:  Define the EMS (electromagnetic spectrum.
Light as a Particle. Objectives  Define a quantum  Calculate the energy of a photon  Relate photon energy to wavelength and frequency of EMR.
Light and Electrons October 27, 2014.
Particle Properties of Light. Objectives To discuss the particle nature of light.
 Radiation emitted by hot objects is called thermal radiation.  Recall that the total radiation power emitted is proportional to T 4, where T is the.
Particle Nature of Light
Advanced Heat Transfer - Prof. Dr.-Ing. R. Weber - Winter 2005/ Lecture 1 (Governing Laws) Lecture-1. Governing Laws for Thermal Radiation Contents.
Electromagnetic Spectrum Light as a Wave - Recap Light exhibits several wavelike properties including Refraction Refraction: Light bends upon passing.
Lecture 5 Abiol 574 Blackbody Radiation/ Planetary Energy Balance This material is from Ch. 3 of The Earth System, ed. 3, by Kump, Kasting, and Crane.
As an object gets hot, it gives Off energy in the form of Electromagnetic radiation.
Interaction of Light with Matter (1900) in the early 1900’s, there were three key behaviors associated with the interaction of light with matter that could.
Blackbody A black body is an ideal system that absorbs all radiation incident on it The electromagnetic radiation emitted by a black body is called blackbody.
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 Theory I An Overview. Introduction The development of classical physics (based on Newton’s laws) culminated in James Clerk Maxwell’s equations:
1 PHYS 3313 – Section 001 Lecture #9 Wednesday, Feb. 12, 2014 Dr. Jaehoon Yu Determination of Electron Charge Line Spectra Blackbody Radiation Wednesday,
Photons, Electrons, and Atoms. Visible and non-visable light Frequencies around Hz Much higher than electric circuits Theory was about vibrating.
MAX PLANCK By: Puneet Sekhon and Navreet Brar. PERSONAL LIFE OF PLANCK  Born in Kiel, Holstein on April 23/ 1858  Would have become a musician  Studied.
Spectra. White Light Light from many colors mixes to form white light. Different colors have different wavelengths. Shorter wavelengths bend more through.
The wave theory of light was unable to explain something known as the “photoelectric effect”
Light and Electrons! Ch 11. Light & Atomic Spectra A Brief Bit of History (development of the quantum mechanical model of the atom) Grew out of the study.
Physics 1202: Lecture 31 Today’s Agenda Announcements: Extra creditsExtra credits –Final-like problems –Team in class HW 9 this FridayHW 9 this Friday.
Physics 1202: Lecture 30 Today’s Agenda Announcements: Extra creditsExtra credits –Final-like problems –Team in class HW 9 next FridayHW 9 next Friday.
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.
6.1.1 Photons, Photoelectric Effect, and Particle Nature of Light Did the Greeks Invent Everything?!?
Chapter 7: Quantum theory of the atom Chemistry 1061: Principles of Chemistry I Andy Aspaas, Instructor.
Modern Atomic Model and EMR
Radiation Heat Transfer
1 2. Atoms and Electrons How to describe a new physical phenomenon? New natural phenomenon Previously existing theory Not explained Explained New theoryPredicts.
Vocabulary Review New radiation electromagnetic radiation wavelength
Chapter 5 “Electrons in Atoms”. Section 5.3 Physics and the Quantum Mechanical Model l OBJECTIVES: Describe the relationship between the wavelength and.
IB Physics 12 Mr. Jean February 5 th, The plan: Video clip of the day. Quantum Theory Energy Levels.
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.
Using Planck’s Constant…. Picture credit: He was a German physicist and is considered as the founder.
Intro to Modern Physics Aim: How did we arrive to our most recent physics discoveries?
Down The Rabbit Hole: Quantum Physics
Chapter 6 Electronic Structure of Atoms
PHYS 3313 – Section 001 Lecture #9
The Planck Distribution
Alec Sauers and Corrina Kissel
Light: Electromagnetic Spectrum
Why Light, why now?.
Early Quantum Theory and Models of the Atom
Chapter 11 “The Electromagnetic Spectrum”
Light, Photon Energies, and Atomic Spectra
QM2 Concept Test 8.1 The total energy for distinguishable particles in a three dimensional harmonic oscillator potential
6.1.1 Photons, Photoelectric Effect, and Particle Nature of Light
Physics and the Quantum Model
Waves and Particles Nuclear Physics
Photoelectric Effect And Quantum Mechanics.
PHYS 3313 – Section 001 Lecture #10
Presentation transcript:

Quantum Theory By: Lucas, Steven, Brandon and Kristen

Vocabulary Spectra: the range of colors that a object will give off when it is heated or burned. Blackbody: An object that will absorb all light and can radiate it will almost no gaps in its spectrum. Discrete: Apart from, or separate from others of its kind. Spectra: the range of colors that a object will give off when it is heated or burned. Blackbody: An object that will absorb all light and can radiate it will almost no gaps in its spectrum. Discrete: Apart from, or separate from others of its kind.

Vocab cont… Quantum: a discrete amount of energy, given by the product of Planck's constant(h) and the frequency of the radiation (f) Empirical equation: an equation that fits the observed data but is not based on any theory Postulate: a claim, something said without proof of consept. Quantum: a discrete amount of energy, given by the product of Planck's constant(h) and the frequency of the radiation (f) Empirical equation: an equation that fits the observed data but is not based on any theory Postulate: a claim, something said without proof of consept.

Properties of light The color of light is determined by the its wavelength. Increasing or decreasing the temperature of an object will change the color of the light it emits. Each color of light can only have a a set number of different energy levels. The color of light is determined by the its wavelength. Increasing or decreasing the temperature of an object will change the color of the light it emits. Each color of light can only have a a set number of different energy levels.

Blackbody radiation When a blackbody is heated it follows a color path until it reaches a certain temperature limit. The pattern stops once you reach the ultraviolet end of the spectrum. When a blackbody is heated it follows a color path until it reaches a certain temperature limit. The pattern stops once you reach the ultraviolet end of the spectrum.

Max Planck A German physicist that is credited with creating the founding for quantum theory. He won the Nobel Prize in 1918 for his work in quantum mechanics. Now he is known for: 1. Planck ’ s postulate 2. Planck ’ s constant 3. Planck's law of black body radiation

Planck’s constant and postulate He used pervious theory about blackbody radiation and experiments done with the blackbody radiation spectrum to derive this constant. H= x 10^(-34) j*s His postulate Allows use to find the energy of light at any frequency E=nhv n is a discrete value that depends on the color of light you are dealing with, h is Planck's constant and v is the frequency. He used pervious theory about blackbody radiation and experiments done with the blackbody radiation spectrum to derive this constant. H= x 10^(-34) j*s His postulate Allows use to find the energy of light at any frequency E=nhv n is a discrete value that depends on the color of light you are dealing with, h is Planck's constant and v is the frequency.