Quantum Tunneling Ashley Gnoss & Kyle Kucker Physics 43/ May 10th, 2011 Santa Rosa Junior College Spring ‘11 Image:

Slides:



Advertisements
Similar presentations
Pressure and Kinetic Energy
Advertisements

Lecture Outline Chapter 30 Physics, 4th Edition James S. Walker
“velocity” is group velocity, not phase velocity
Wave Particle Duality – Light and Subatomic Particles
The photon, the quantum of light
Unit 12: Part 3 Quantum Mechanics and Atomic Physics.
The Electronic Structures of Atoms Electromagnetic Radiation
Hybridization A Way of Explaining VSEPR Theory. Covalent bonding Modern methods for describing bonding make use of quantum mechanical methods and describe.
Review. The Wave Nature of Light Important: When a light wave travels from one medium to another, its frequency does not change, but its wavelength does.
Nuclear Reactions Lesson 7.
Chapter 9 Notes.  While chemical changes involve changes in the electrons (ex : bonding), nuclear reactions involve changes to the nucleus and involve.
A 14-kg mass, attached to a massless spring whose force constant is 3,100 N/m, has an amplitude of 5 cm. Assuming the energy is quantized, find the quantum.
CHAPTER 2 Introduction to Quantum Mechanics
PH 103 Dr. Cecilia Vogel Lecture 19. Review Outline  Uncertainty Principle  Tunneling  Atomic model  Nucleus and electrons  The quantum model  quantum.
P460 - barriers1 Bound States and Tunneling V 0 0 State A will be bound with infinite lifetime. State B is bound but can decay to B->B’+X (unbound) with.
The Photoelectric Effect
Why are electrons restricted to specific energy levels or quantized? Louis de Broglie – proposed that if waves have particle properties, possible particles.
Almost all detection of visible light is by the “photoelectric effect” (broadly defined.) There is always a threshold photon energy for detection, even.
Modern Physics LECTURE II.
L 33 Modern Physics [1] Introduction- quantum physics Particles of light  PHOTONS The photoelectric effect –Photocells & intrusion detection devices The.
Lecture 10 Energy production. Summary We have now established three important equations: Hydrostatic equilibrium: Mass conservation: Equation of state:
By Kate Hogan.  Born in Wilkes-Barre, Pennsylvania 1917  Studied at Pennsylvania State College and University of California, Berkeley  Manhattan Project.
Ch 9 pages Lecture 18 – Quantization of energy.
Goal: To understand the lifetime of a star and how the mass of a star determines its lifetime Objectives: 1)To learn what defines a Main sequence star.
Chapters 9, 11, 12 Concepts covered that will also be candidates for exam questions.
Chapter 5 Section 5.3 & 5.4 The Quantum Model. Problems with the Bohr Model 1. Worked well for predicting hydrogen spectrum, but not for elements with.
Plan for Fri, 31 Oct 08 Lecture –Emission spectrum of atomic hydrogen (7.3) –The Bohr model of hydrogen (7.4) –Quantum mechanical model (7.5) Quiz 5.
The Nature of Matter Mr. Gilbertson Chemistry Chapter 3 Solids, Liquids, and Gases.
Goal: To understand how stars generate their energy Objectives: To learn about the Proton – Proton Chain To learn about the Carbon – Nitrogen – Oxygen.
 The Bohr model describes definite electron energy levels within atoms  Bohr’s model only applied to hydrogen – it has been replaced by more sophisticated.
PHYS:1200 FINAL EXAM 1 FINAL EXAM: Wednesday December 17, 12:30 P - 2:30 P in LR-1 VAN FE covers Lectures 23 – 36 The study guide, formulas, and practice.
L 33 Modern Physics [1] Introduction- quantum physics Particles of light  PHOTONS The photoelectric effect –Photocells & intrusion detection devices The.
Physics Department Phys 3650 Quantum Mechanics – I Lecture Notes Dr. Ibrahim Elsayed Quantum Mechanics.
Nuclear Reactions AP Physics B Montwood High School R. Casao.
Atomic Particles  Atoms are made of protons, neutrons and electrons  % of the atom is empty space  Electrons have locations described.
Apr 4, 2007 PHYS 117B.02 1 PHYS 117B.02 Lecture Apr 4 The last few lectures we’ve been switching gears from classical to quantum physics This way: The.
In the late years of the 19th century scientists were interested in experiments about the rays that certain elements were emitting. After various experiments.
Physics Lecture 15 10/29/ Andrew Brandt Wednesday October 29, 2014 Dr. Andrew Brandt 0. Hw’s due on next 3 Mondays, test on Nov Wells+Barriers.
Chapter 11 – Intermolecular Forces, Liquids and Solids Homework: 13, 16, 18, 19, 23, 43, 45, 47, 48, 49, 50, 51, 54, 55, 56.
Wave-Particle Duality - the Principle of Complementarity The principle of complementarity states that both the wave and particle aspects of light are fundamental.
Lecture 1 Chemical Bonds: Atomic Orbital Theory and Molecular Orbital Theory Dr. A.K.M. Shafiqul Islam
The Nature of Light Is Light a Particle or a Wave?
Quantum Theory the modern atomic model. Bohr Model of the Atom a quantum model proposed by Niels Bohr in 1913 It helped to explain why the atomic emission.
ATOMIC orbitals!. When the a planet moves around the sun, you can plot a definite path for it which is called an orbit. A simple view of the atom looks.
Quantum Mechanics1 Schrodinger’s Cat. Quantum Mechanics2 A particular quantum state, completely described by enough quantum numbers, is called a state.
Chapter 7 Lecture Lecture Presentation Chapter 7 The Quantum- Mechanical Model of the Atom Sherril Soman Grand Valley State University © 2014 Pearson Education,
Classification of the Elementary Particles
Ludwid Boltzmann 1844 – 1906 Contributions to Kinetic theory of gases Electromagnetism Thermodynamics Work in kinetic theory led to the branch of.
CHEMISTRY 2000 Topic #1: Bonding – What Holds Atoms Together? Spring 2008 Dr. Susan Lait.
 I can identify and describe the five factors that affect reaction rates.
Wednesday, Oct. 31, 2012PHYS , Fall 2012 Dr. Amir Farbin 1 PHYS 3313 – Section 001 Lecture #16 Wednesday, Oct. 31, 2012 Dr. Amir Farbin Reflection.
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.
Physics 213 General Physics Lecture Exam 3 Results Average = 141 points.
Nanoelectronics Chapter 2 Classical Particles, Classical Waves, and Quantum Particles
By the end of this presentation, you should be able to: Select and use Coulomb’s law to determine the force of repulsion, and Newton’s law of gravitation.
1 HEINSENBERG’S UNCERTAINTY PRINCIPLE “It is impossible to determine both position and momentum of a particle simultaneously and accurately. The product.
© 2014 Pearson Education, Inc. Building Blocks of the Universe.
So that k k E 5 = - E 2 = = x J = x J Therefore = E 5 - E 2 = x J Now so 631.
Chapter S4 Building Blocks of the Universe
Chapter 7: The Quantum-Mechanical Model of the Atom ( )
Solutions of Schrodinger Equation
The Uncertainty Principle
Photons: Light Waves Behaving as Particles
CHAPTER 5 The Schrodinger Eqn.
5. Wave-Particle Duality - the Principle of Complementarity
Uncertainty Principle
CHAPTER 5 The Schrodinger Eqn.
Atomic Theory Models and Particles.
Physics Lecture 13 Wednesday March 3, 2010 Dr. Andrew Brandt
5. Wave-Particle Duality - the Principle of Complementarity
Presentation transcript:

Quantum Tunneling Ashley Gnoss & Kyle Kucker Physics 43/ May 10th, 2011 Santa Rosa Junior College Spring ‘11 Image:

Introduction to the concept Quantum tunneling is one of the phenomena displaying the odd nature of Quantum Mechanics. It concerns particles in their wave states, where each observable can be described most acutely by a distribution of probability. This is the main point, that there is no point. Classically, it is assumed that particles that we can observe to be point-like should behave as if under the rules that govern the more massive objects that we have encountered, that is, they should behave deterministically. But due to the nature of Quantum Mechanics, there is a magnitude of size and complexity for which the rules seem to change. Image:

Quantum Mechanics: Introduction to the Concept Particles that we had assumed to be definite in their properties, (position, energy, time, momentum…) can only be described as distributions of probability. These distributions have another limitation. Due to our methods of detection, we are restricted to never knowing two properties of a particle simultaneously. We can never understand fully (with our current knowledge) what the particle/ distribution is doing, nor predict what it will do. This is the reason why we do not yet know what to call these objects. Waves or particles. Quantum mechanics emphasizes the “wave-nature”, because it is through wave mechanics that we can describe these probability distributions and how they could be an adequate description of the particle, though an unintuitive one. A few wave distributions of a hydrogen atom, describing varying positions (or potential positions) of the electron. Image:

Heisenberg’s Uncertainty Principle The inability to know certain multiple properties of an object at the same time is due to the uncertainty principle. This principle is the concept behind quantum tunneling. It is due to this lack of knowledge about the particle that we call the action of tunneling an odd phenomena. Indeed, it makes describing the rules and properties of nature a much more complex activity than once thought. “If the properties of the atom and particle could be known with certainty, then they would decohere and their wave behavior and their ability to interfere would be destroyed”- An interpretation of Quantum Mechanics Equations of the Uncertainty Principle

The Tunneling of a Particle Tunneling refers to the ability of a particle to overcome and cross a potential energy barrier that it would not be able do based on classical understanding. It is only the particle’s wave-nature that allows for this phenomenon. The probability wave describing the particle’s position is an integral that overlaps into the energy barrier, allowing for some finite probability that the particle might actually “tunnel” through. Images: abyss.uoregon.edu/.../ quantum_tunneling.gif

Tunneling in Nature Our sun persists in keeping us warm (and alive) through the process of fusion. Fusion is the creation of larger atomic nuclei/elements from smaller ones. Fusion occurs only at extremely high temperatures, where the Kinetic Energy is high enough to overcome the potential barrier due to the repelling of the nucleons. The only thing is that our sun is not hot enough to produce these high energies. Tunneling is the explanation. Only due to the overlap of the probability waves of the nuclei can they overcome the barrier separating them and fuse. Radioactive decay is another example of how tunneling circumvents the tendencies of nature. Particles such as alpha particles are held in the nucleus by the strong force, which means that they shouldn’t be able to escape. Tunneling again explains how the particles are able to overcome the strongest known force in nature. In the case of the alpha particle for instance, the location of the particle within the nucleus is fairly accurately known, and due to the uncertainty principle, the probability wave for the velocity (and therefore kinetic energy) is greater. The property unable to be defined and the wave description gives it a finite probability to arrive outside of the nucleus.

Technological Applications Once of the most important uses of electron tunneling is the production of current. A new and interesting use is within the new touch screen phones. By applying a force (pressure with the finger), the layers particles of polymer within the screen come closer together. Before they are moved together there is a “large enough” vacuum between the layers and so that the probability of electrons tunneling from one layer to another is very low. By exerting force on the layers, we are able to bring the probability waves of the electrons closer together, increasing the rate of tunneling, enough to produce current on- demand, changing the material from an insulator to a “metal”. The change in tunneling is extreme. For every Angstrom closer (1/10th of a nanometer) the rate of tunneling increases by ten times. And the resistance changes from 10^12 ohms to 1 ohm!

Another strange fact… Fruit flies have been shown to be able to distinguish between a particular molecule (such as acetophenone) and its deuterated version through the process of quantum tunneling via the receptors within the fruit fly’s nose. Within some molecules, deuterium-carbon bond vibrations are similar to the vibrations found in the bonds between carbon and nitrogen, which will result in a similar sent. A majority of fruit flies tend to avoid nitrogen molecules (nitriles), and so too with the deuterated versions of molecules that tend to attract them. Further studies in the nose’s abilities to employ quantum tunneling could lead to artificial noses and more sensitive instruments in the field.

Sources New Ideas in Quantum Tunneling. arxiv/23409/New Ideas in Quantum Tunneling. arxiv/23409/ Explanation of simple concept. um_tunneling.htmlExplanation of simple concept. um_tunneling.html Lecture onQuantumTunneling. ch?v=vMndTqowzqU Molecular vibration-sensing component in Drosophila melanogaster olfaction ). (All researched May 5, 2011)