Birth of Quantum Mechanics Quantum = Specific amount “Probabilities”

Slides:



Advertisements
Similar presentations
Wave-Particle Duality
Advertisements

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.
The Modern Atomic Model After Thomson: Bohr, Placnk, Einstein, Heisenberg, and Schrödinger.
Electromagnetic Radiation
Electronic Structure of Atoms
Quantum Theory of Light A TimeLine. Light as an EM Wave.
1 Chapter 29 Particles and Waves. 2 There is nothing new to be discovered in physics now. All that remains is more and more precise measurement. -- William.
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.
The Photoelectric Effect
Quantum Physics. Black Body Radiation Intensity of blackbody radiation Classical Rayleigh-Jeans law for radiation emission Planck’s expression h =
Chapter 38.
L 33 Modern Physics [1] Introduction- quantum physics Particles of light  PHOTONS The photoelectric effect –Photocells & intrusion detection devices The.
Birth of Quantum Mechanics PHYS 521. Necessity of QM “There is nothing new to be discovered in physics now. All that remains is more and more precise.
Quantum Theory of the Atom
Classical ConceptsEquations Newton’s Law Kinetic Energy Momentum Momentum and Energy Speed of light Velocity of a wave Angular Frequency Einstein’s Mass-Energy.
Electronic Structure of Atoms Chapter 6 BLB 12 th.
Particle Nature of Light
The Bohr Atom. Spectroscopy Kirchhoff/Bunsen – used spectroscope  to identify emission spectra of elements.
Chapter 39 Particles Behaving as Waves
Chapter 4 Arrangement of Electrons in Atoms
Phys141 Principles of Physical Science Chapter 9 Atomic Physics Instructor: Li Ma Office: NBC 126 Phone: (713)
Quantum Mechanics Chapters 27 and 28. The Beginning  Thomson-Cathode Ray Experiments J. J. Thomson experimented with cathode rays and discovered the.
Chapter 4 Arrangement of Electrons in Atoms
Wave Particle Duality Chapter 5
Chapter 6: Electronic Structure of Atoms Pages
27-12 The Bohr Model Bohr studied Rutherford’s planetary model and found it had validityBohr studied Rutherford’s planetary model and found it had validity.
Atomic Particles  Atoms are made of protons, neutrons and electrons  % of the atom is empty space  Electrons have locations described.
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.
As an object gets hot, it gives Off energy in the form of Electromagnetic radiation.
Quantum Physics. Quantum Theory Max Planck, examining heat radiation (ir light) proposes energy is quantized, or occurring in discrete small packets with.
Leading up to the Quantum Theory.  exhibits wavelike behavior  moves at a speed 3.8 × 10 8 m/s in a vacuum  there are measureable properties of light.
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.
Chemistry 330 Chapter 11 Quantum Mechanics – The Concepts.
1 The Quantum Mechanical Model of the Atom Chapter 7.
1 High School Technology Initiative © 2001 Quantum History Pasteurization 1861 Albert Einstein 1905 Louis de Broglie 1924 Max Planck 1900 Columbus discovers.
Topic 13 Quantum and Nuclear physics Atomic spectra and atomic energy states.
Development of Atomic Models
Learning Objectives Who was involved? Who was involved? Which experiments were used to help us understand? Which experiments were used to help us understand?
Quantum Physics   Quantum   The smallest quantity of a substance that still has the specific properties of that substance Discrete vs. Continuous 
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.
Chapter 38C - Atomic Physics © 2007 Properties of Atoms Atoms are stable and electrically neutral.Atoms are stable and electrically neutral. Atoms have.
1 2. Atoms and Electrons How to describe a new physical phenomenon? New natural phenomenon Previously existing theory Not explained Explained New theoryPredicts.
The Quantum Mechanical Model of the Atom. Niels Bohr In 1913 Bohr used what had recently been discovered about energy to propose his planetary model of.
Need for Quantum Physics Problems remained from classical mechanics that relativity didn’t explain Problems remained from classical mechanics that relativity.
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.
Quantum Physics… the world is about to get even weirder!
Topic I: Quantum theory Chapter 7 Introduction to Quantum Theory.
History of Atomic Theory … continued…. Problem with Rutherford If electrons are orbiting around a nucleus, they are continuously accelerating. 19th century.
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.
Chemistry I Chapter 4 Arrangement of Electrons. Electromagnetic Radiation Energy that exhibits wavelike behavior and travels through space Moves at the.
Properties of light spectroscopy quantum hypothesis hydrogen atom Heisenberg Uncertainty Principle orbitals ATOMIC STRUCTURE Kotz Ch 7 & Ch 22 (sect 4,5)
Light CHEM HONORS. The Nature of Light Light is electromagnetic radiation, a wave composed of oscillating, mutually perpendicular electric and magnetic.
History of General Quantum Physics
Electromagnetic Radiation
Introduction to Quantum Theory for General Chemistry
General Physics (PHY 2140) Lecture 27 Modern Physics Quantum Physics
Electronic Structure and Light
2.4 Modern Atomic Structure Objectives 4, 5:b, and 6:a
Chapter 39 Particles Behaving as Waves
Electronic Structure.
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
Chapter 39 Particles Behaving as Waves
Photoelectric Effect And Quantum Mechanics.
Presentation transcript:

Birth of Quantum Mechanics Quantum = Specific amount “Probabilities”

Necessity of QM By the end of the nineteenth century a number of serious discrepancies had been found between experimental results and classical theory. Blackbody radiation law Photo-electric effect Atom and atomic spectra

Blackbody radiation Exp. Measurements: the radiation spectrum was well determined --- a continuous spectrum with a shape that dependent only on temperature

Blackbody radiation Exp. Measurements: the radiation spectrum was well determined --- a continuous spectrum with a shape that dependent only on temperature Theory: classical kinetic theory (Rayleigh and Jeans) predicts the energy radiated to increase as the square of the frequency. Completely wrong! Ultraviolet catastrophe!

Planck’s solution Planck’s assumption (1900): radiation of a given frequency ν could only be emitted and absorbed in “quanta” of energy E=hν h=6.6261E-34 J·s : Planck’s constant With this assumption, Planck came up with a formula that fits well with the data. Planck called his theory “an act of desperation”.

Planck’s solution Planck’s assumption (1900): radiation of a given frequency ν could only be emitted and absorbed in “quanta” of energy E=hν h=6.6261E-34 J·s : Planck’s constant With this assumption, Planck came up with a formula that fits well with the data. Planck called his theory “an act of desperation”. Planck neither envisaged a quantization of the radiation field, nor did he quantize the energy of an individual material oscillator What Planck assumed is that the total energy of a large number oscillators is made up of finite energy elements hν

Einstein’s interpretation of Planck’s formula Einstein in 1906 interpreted Planck’s result as follows: “Hence, we must view the following proposition as the basis underlying Planck’s theory of radiation: The energy of an elementary resonator can only assume values that are integral multiples of hν; by emission and absorption, the energy of a resonator changes by jumps of integral multiples of hν”

Photo-electric effect Experimental facts Shining light on metal can liberate electrons from metal surface Whether the metal emit electrons depends on the freq. of the light: only light with a freq. greater than a given threshold will produce electrons Increasing the intensity of light increases the number of electrons, but not the energy of each electron Energy of electron increases with the increase of light frequency.

Einstein on photo-electric effects Light consists of a collection of “light quanta” of energy hν The absorption of a single light quantum by an electron increases the electron energy by hν Some of this energy must be expended to separate the electron from the metal (the work function, W), which explains the threshold behavior, and the rest goes to the kinetic energy of the electron. Electron kinetic energy = hν - W

Reactions to Einstein’s light quanta idea For a long, long time, nobody else believed that.

Reactions to Einstein’s light quanta idea For a long, long time, nobody else believed that. Planck and others in their recommendation of Einstein’s membership in Prussian Academy (1913): “One can say that there is hardly one among the great problems in which modern physics is so rich to which Einstein has not made a remarkable contribution. That he may sometimes have missed the target in his speculations, as, for example, in his hypothesis of light quanta, cannot really be held to much against him, for it is not possible to introduce really new ideas even in the most exact sciences without sometimes taking a risk

Experimental confirmation Experimental confirmation came in 1915 by Millikan Millikan didn’t like Einstein’s light quanta idea, which he saw as an attack on the wave theory of light. Tried very hard (for 10 years) to disprove Einstein’s theoretical prediction.

Experimental confirmation Experimental confirmation came in 1915 by Millikan Millikan didn’t like Einstein’s light quanta idea, which he saw as an attack on the wave theory of light. Tried very hard (for 10 years) to disprove Einstein’s theoretical prediction. For all his efforts, he confirmed Einstein’s theory and provided a very accurate measurement of Planck’s constant. Millikan got Nobel prize in 1923.

Experimental confirmation Experimental confirmation came in 1915 by Millikan Millikan didn’t like Einstein’s light quanta idea, which he saw as an attack on the wave theory of light. Tried very hard (for 10 years) to disprove Einstein’s theoretical prediction. For all his efforts, he confirmed Einstein’s theory and provided a very accurate measurement of Planck’s constant. Millikan got Nobel prize in Still didn’t like Einstein’s light quanta idea, in a 1916 paper: “This hypothesis may well be called reckless …” “Despite the apparently complete success of the Einstein equation, the physical theory of which it was designed to be the symbolic expression is found so untenable …”

Einstein on light quanta “All these fifty years of conscious brooding have brought me no nearer to the answer to the question `What are light quanta?’ Nowadays every rascal thinks he knows, but he is mistaken.” --- letter to Michel Besso, 1951

Problems with atomic stability Rutherford’s experiment (1911): atom is composed of electrons moving around a heavy nucleus.

Problems with atom stability Rutherford’s experiment (1911): atom is composed of electrons moving around a heavy nucleus. Problem: if the electrons orbit the nucleus, classical physics predicts they should emit electromagnetic waves and loose energy. If this happens, the electron will spiral into the nucleus, no stable atom should exist!

Problems with atomic spectrum Atomic radiation spectrum consists of discrete lines.

Bohr’s solution (1912) An atomic system can only exist in a discrete set of stationary states, with discrete values of energy. Change of the energy, including emission and absorption of light, must take place by a complete transition between two such stationary states.

Bohr’s solution (1912) An atomic system can only exist in a discrete set of stationary states, with discrete values of energy. Change of the energy, including emission and absorption of light, must take place by a complete transition between two such stationary states. The radiation absorbed or emitted during a transition between two states of energies E1 and E2 has a frequency: hν=E1 - E2 Bohr’s formula explains some of the spectral lines in hydrogen atom (but not all), does not do well with other atoms.

Bohr’s solution (1912) An atomic system can only exist in a discrete set of stationary states, with discrete values of energy. Change of the energy, including emission and absorption of light, must take place by a complete transition between two such stationary states. The radiation absorbed or emitted during a transition between two states of energies E1 and E2 has a frequency: hν=E1 - E2 Bohr’s formula explains some of the spectral lines in hydrogen atom (but not all), does not do well with other atoms. A truly revolutionary idea, even Einstein was impressed: “… appeared to me like a miracle. This is highest form of musicality in the sphere of thought.” (1951)

summary Energy quantization is necessary to explain the blackbody radiation, the photo-electric effects, the stability of atoms and their spectra Classical physics must be given up: physical properties that are quantized and not continuous are completely different from the ideas of continuous space and time in classical physics.

Later developments De Broglie: matter wave λ=h/p Exp. with electron diffraction (Davisson and Germer, 1927) Today: interferometers with neutrons, atoms and molecules Born’s statistical interpretation of matter wave Matrix mechanics (Heisenberg, Born and Jordan) Wave mechanics, Schroedinger’s equation (Schroedinger) Relativistic QM (Dirac) Exclusion principle (Pauli)

Birth of QM The necessity for quantum mechanics was thrust upon us by a series of observations. The theory of QM developed over a period of 30 years, culminating in with a set of postulates. QM cannot be deduced from pure mathematical or logical reasoning. QM is not intuitive, because we don’t live in the world of electrons and atoms. QM is based on observation. Like all science, it is subject to change if inconsistencies with further observation are revealed.

Goal of PHYS311 and 312 We will study non-relativistic QM. Our goal is to understand the meaning of the postulates the theory is based on, and how to operationally use the theory to calculate properties of systems. The first semester will lay out the ground work and mathematical structure, while the second will deal more with computation of real problems.