'Same quantum state' diaporamas de présentation

The Interaction of Light and Matter

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The Interaction of Light and Matter

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hapter S4C Building Blocks of the Universe

hapter S4C Building Blocks of the Universe. How has the quantum revolution changed our world?. The Quantum Realm. Light behaves like particles (photons) Atoms consist mostly of empty space Electrons in atoms are restricted to particular energies

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Chapter 1 Structure and Bonding

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The Ontological Interpretation of Quantum Mechanics and the implications of wholeness on

The Ontological Interpretation of Quantum Mechanics and the implications of wholeness on science and society. Bradley J Nordell Special Topics Seminar Series 1/13/2012 University of Missouri- Kansas City Department of Physics and Astronomy. Table of Contents. Introduction

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Stars and their Physical Properties

Stars and their Physical Properties. Background Information. Name: Isabel Baransky School: Fu Foundation of Engineering and Applied Science Major: Applied Physics Minor: Music. OVERVIEW OF FORCE. THE BIG BANG. Big Bang. Occurred 13.7 billion years ago.

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The History of Quantum Mechanics

The History of Quantum Mechanics. Brittany Hall Aurel Lazar John Hodge Jesse Mahn. This Timeline has much Entropy. 1925: Heisenberg developed the Heisenberg Uncertainty principle Wolfgang Pauli developed the fourth quantum number- the spin number . 1922:

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Lesson 5

Lesson 5. Fundamental Aspects of Nuclear Structure. Fundamental Forces of Nature. Exchange Particles and Force Carriers. Forces occur through the notion of the virtual exchange of bosons that are force carriers.

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Lectures 10-11: Multi-electron atoms

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General Physics (PHY 2140)

General Physics (PHY 2140). Lecture 35. Modern Physics Atomic Physics The periodic table Atomic transitions. http://www.physics.wayne.edu/~apetrov/PHY2140/. Chapter 28. Lightning Review. Last lecture: Atomic physics De Broglie waves/hydrogen atom Quantum mechanics and spin.

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Ultracold Fermi gas near Feshbach resonance with mass and population imbalance

Ultracold Fermi gas near Feshbach resonance with mass and population imbalance. Advisor: Prof. Luming Duan Committee: Prof. Luming Duan Prof. Georg Raithel Prof. Samuel Moukouri. Guin-Dar Lin Department of Physics University of Michigan August 25, 2006. Outline. BEC, Superfluidity

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Chapter 41 Atomic Structure

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Standard Model of Physics

Standard Model of Physics. Project Supervisor: Dr. Babar Qureshi Project by: M. Anadil Saeed Occasional Helper: Dr. Amer Iqbal. What does the information given in the previous slide mean? Let me illustrate a little. What are quarks? What are leptons? What are bosons?. What are quarks?.

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FE-4: Review of materials science for the FE exam

FE-4: Review of materials science for the FE exam. Part 3: Corrosion, thermal and electrical properties. Based on the following:

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Chapter 18

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Atomic Structure

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NON Bolztmann ensembles

y i1. y i2. y i3. y i2. y i2. y i3. y i4. y i5. y i6. NON Bolztmann ensembles. Fermions: 2 particles cannot occupy the same quantum state ?occupation number n k can only be 0 or 1. P 1,2 y =- y antisymmetric.

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