Physics

The Quantum Reality

 

Periodic Table of Elements Page

 

Physics Lecture Table

 

Lecture

Physics 10

with Richard A. Muller

Thanks to UC Berkeley Educational Technology Services

MIT 8.02

Electricity and Magnetism

 Spring 2002

MIT

Classical Mechanics

Fall 1999

Introduction

MIT 8.03

Vibrations & Waves

Fall 2004

Intro to Vibrations and Waves

Stanford University

Einstein's General Theory

of Relativity

in HD

Modern Physics: Quantum Mechanics (Stanford) click HD

Solid State Physics

01

Atoms and Heat

Coulomb's Law & Electric Force

  Dimensions and Measurements

 Periodic Phenomena

Lecture 01

Lecture 01

Introductory Lectures 1

02

Atoms and Heat II

 Electric Field

Speed, Velocity and Acceleration

  Damped Free Oscillations

Lecture 02

Lecture 02

Introductory Lectures 2

03

Gravity and Satellites

 Gauss's Law & Electric Flux

Vectors

Forced Oscillations with Damping

Lecture 03

Lecture 03

Introductory Lectures 3

04

Gravity and Satellites II

Electric Energy

3D Kinematics

3D Kinematics

Lecture 04

Lecture 04

Introductory Lectures 4

05

Radioactivity

 Conductor & Electrostatic Shielding

Circular Motion

 Coupled Oscillators

Lecture 05

Lecture 05

Introductory Lectures 5

06

Radioactivity II

High-Voltage Breakdown

 Newton's Laws

Triple Pendulum & Cramer's Rule

Lecture 06

Lecture 06

Introductory Lectures 6

07

Nukes

Capacitance & Field Energy

 Weight

 Wave Equation

Lecture 07

Lecture 07

Introductory Lectures 7

08

Review Session

Polarization & Dielectrics

 Friction

Energy in Waves

Lecture 08

Lecture 08

Introductory Lectures 8

09

Electricity and Magnetism

Ohm's Law, Resistivity & Currents

Exam Review

Sound Cavities & Musi...

Lecture 09

Lecture 09

Introductory Lectures 9

10

Electricity and Magnetism II

Kirchhoff's Rule & Power

Hooke's Law & Pendulums

Exam 1 Review

Lecture 10

Lecture 10

 

11

Waves I

Magnetic Field & Lorentz Force

Work - Kinetic Energy

Fourier Analysis

Lecture 11

   

12

Waves II

Review Exam 1

Resistive Forces

Dispersion & Phase Velocity

Lecture 12

Quantum Entanglements

 

13

 Light I

Moving Charges in B-Fields

Potential Energy

 EW and Polarization

 

Lecture 01

 

14

Light II

Biot-Savart Law

 Escape Velocities & Power

Accelerated Charges & Power

 

Lecture 02

 

15

Invisible Light I

Ampere's Law & Solenoids

 Momentum & Center of Mass

Expanding Universe & Stars

 

Lecture 03

 

16

Invisible Light II

Faraday's Law & Lenz Law

 Center of Mass & Collisions

 Reflection & Standing...

 

Lecture 04

 

17

Quantum I

Motional Electromotive Force

Impulse & Rockets

Wave Guides

 

Lecture 05

 

18

Quantum II

Displacement Current

 Exam Review

Exam Review

 

Lecture 06

 

19

Quantum III

Vacation Special

 Rotating Rigid Bodies

Exam 2 Review

 

Lecture 07

 

20

Quantum IV

 Inductance & Magnetic Field Energy

Angular Momentum - Torques

Huygens' Principle & ...

 

Lecture 08

 

21

 Review Session

Dia-, Para- & Ferromagnetism

 Torques & Oscillating Bodies

Diffraction

 

Lecture 09

 

22

Relativity

 Maxwell's Equations

Kepler's Laws

Rainbows, Coronae & Glories

   

23

Relativity II

 Review Exam 2

Doppler Effect and Binary Stars

Final Lecture

 

Special Relativity

click HD

 

24

Universe I

 Transformers & RC Circuits

 Rolling Motion & Gyroscopes

  

Lecture 01

 

25

Universe II

Resonance & Driven LRC Circuits

 Static Equilibrium & Stability

  

Lecture 02

 

26

Review Session

Traveling Waves & Standing Waves

 Elasticity & Young's Modulus

  

Lecture 03

 

27

 

Resonance

Fluid Mechanics

  

Lecture 04

 

28

 

 Polarization & Oscillating Charges

  Archimedes' Principle

  

Lecture 05

 

29

 

Snell's Law

Exam Review

  

Lecture 06

 

30

 

Polarizers Malus's Law

Simple Harmonic Oscillations

  

Lecture 07

 

31

 

Rainbows

Resonance & Forced Oscillations

  

Lecture 08

 

32

 

Review Exam 3

Heat & Thermal Expansion

    

33

 

  Interferometers

Kinetic Gas Theory & Phases

    

34

 

Telescopes

 Breakdown of Classical Mechanics

    

35

A lecture by a monk (extra)

Doppler Effect & The Big Bang

 High-energy Astrophysics

    

36

 

Astronomy Research at MIT

     

 

 

 

 

Caltech

The Mechanical Universe

01

Introduction

This preview introduces revolutionary ideas and heroes from Copernicus to Newton, and links the physics of the heavens and the earth.

02

The Law of Falling Bodies

Galileo's imaginative experiments proved that all bodies fall with the same constant acceleration.

03

Derivatives

The function of mathematics in physical science and the derivative as a practical tool.

04

Inertia

Galileo risks his favored status to answer the questions of the universe with his law of inertia.

05

Vectors

Physics must explain not only why and how much, but also where and which way.

06

Newton's Laws

Newton lays down the laws of force, mass, and acceleration.

07

Integration

Newton and Leibniz arrive at the conclusion that differentiation and integration are inverse processes.

08

The Apple and the Moon

The first real steps toward space travel are made as Newton discovers that gravity describes the force between any two particles in the universe.

09

Moving in Circles

The original Platonic ideal, with derivatives of vector functions. According to Plato, stars are heavenly beings that orbit the Earth with uniform perfection -- uniform speed and perfect circles. Even in this imperfect world, uniform circular motion make perfect mathematical sense.
Instructional Objectives
* Understand the meaning of uniform circular motion. * Describe the vector relationships between the radius, velocity, and acceleration in uniform circular motion. * Be able to use the expressions a = v2/r = omega2r = 4 pi2r/T2 in problems involving circular motion. * Be able to use Newton's laws to describe the dynamics of circular motion and to solve problems involving objects moving in circular paths.

10

Fundamental Forces

All physical phenomena of nature are explained by four forces: two nuclear forces, gravity, and electricity.

11

Gravity, Electricity, Magnetism

Forces at play in the Physics Theater. The gravitational force between two masses, the electric force between two charges, and the magnetic force between two magnetic poles -- all these forces take essentially the same mathematical form. Newton's script suggested connections between electricity and magnetism. Acting on scientific hunches, Maxwell saw the matter in an entirely new light.
Instructional Objectives
* State one connection between electricity and magnetism. * Give examples of the concept of "field." * State some similarities and differences between the force of gravity and electricity. * Explain how the speed of light in "buried" in the forces of electricity and magnetism

12

The Millikan Experiment

How does science progress? Through painstaking trial and error, illustrated with a dramatic re-creation of Robert Millikan's classic oil-drop experiment. Understanding the electric force on a charged droplet and viscosity, the measured the charge of a single electron.
Instructional Objectives
* Be able to describe Millikan's method for measuring the charge of an electron. * Be able to solve problems with viscous forces. * Recognize that all charge is a multiple of fundamental unit of charge, which is the charge of the electron.

13

Conservation of Energy

According to one of the major laws of physics, energy is neither created nor destroyed.

14

Potential Energy

Potential energy provides a powerful model for understanding why the world has worked the same way since the beginning of time

15

Conservation of Momentum

If The Mechanical Universe is a perpetual clock, what keeps it ticking away till the end of time? Taking a cue from Descartes, momentum -- the product of mass and velocity -- is always conserved. Newton's laws embody the concept of conservation and momentum. This law provides a powerful principle for analyzing collisions, even at the local pool hall.
Instructional Objectives
* Recognize conservation of momentum as a consequence of Newton's Second Law. * Know when the momentum of a system is conserved. * Recognize the connection between kinetic energy and momentum. * Be able to solve problems involving elastic and inelastic collisions. * Know the relationship between impulse and time average of force.

16

Harmonic Motion

The music and mathematics of periodic motion.

17

Resonance

The music and mathematics of nature, Part II. As Galileo noted, the swings of a pendulum increasingly grow with repeated, timed applications of a small force. When the frequency of an applied force matches the natural frequency of a system, large-amplitude oscillations result in the phenomenon of resonance. Resonance explains why a swaying bridge collapsed in a mild wind, and how a wineglass can be shattered by a human voice.
Instructional Objectives
* Be able to define forced oscillations. * Be able to explain resonance and give a few examples. * Understand the relationship between resonance and forced oscillatory motion.

18

Waves

With an analysis of simple harmonic motion and a stroke of genius, Newton extended mechanics to the propagation of sound.

19

Angular Momentum

An old momentum with a new twist. Kepler's second law of planetary motion, which is rooted here in a much deeper principle, imagined a line from the sun to a planet that sweeps out equal areas in equal times. Angular momentum is a twist on momentum -- the cross product of the radius vector and momentum. A force with twist is torque. When no torque acts on a system, the angular momentum of the system is conserved.
Instructional Objectives
* Know the definitions of torque and angular momentum. * Know how to write the angular momentum of a system and a particle. * Understand the connection between Kepler's second law and the law of conservation f angular momentum. * Recognize the role of conservation of angular momentum in the formation of vortices and firestorms.

20

Torques and Gyroscopes

From spinning tops to the precession of the equinoxes.

21

Kepler's Three Laws

The discovery of elliptical orbits helps describe the motion of heavenly bodies with unprecedented accuracy.

22

The Kepler Problem

The deduction of Kepler's laws from Newton's universal law of gravitation is one of the crowning achievements of Western thought.

23

Energy and Eccentricity

The precise orbit of any heavenly body -- a planet, asteroid, or comet -- is fixed by the laws of conservation of energy and angular momentum. The eccentricity, which determines the shape of an orbit, is intimately linked to the energy and angular momentum of the heavenly body.
Instructional Objectives
* Understand the relationship between energy and eccentricity. * Be able to characterize orbits by eccentricity. * Be able to understand the concept of effective potential and how it relates to planetary motion. * Understand how initial conditions affect the orbit of a planet, comet or satellite.

24

Navigating in Space

Voyages to other planets use the same laws that guide planets around the solar system.

25

Kepler to Einstein

From Kepler's laws and the theory of tides, to Einstein's general theory of relativity, into black holes, and beyond.

26

Harmony of the Spheres

A last lingering look back at mechanics to see new connections between old discoveries

27

Beyond the Mechanical Universe

The world of electricity and magnetism, and 20th-century discoveries of relativity and quantum mechanics.

28

Static Electricity

Eighteenth-century electricians knew how to spark the interest of an audience with the principles of static electricity.

29

The Electric Field

Faraday's vision of lines of constant force in space laid the foundation for the modern force field theory.

30

Potential and Capacitance

Franklin proposes a successful theory of the Leyden jar and invents the parallel plate capacitor

31

Voltage, Energy and Force

When is electricity dangerous or benign, spectacular or useful?

32

The Electric Battery

Electricity changed from a curiosity to a central concern of science and technology in 1800, when Alessandro Volta invented the electric battery. Batteries make use of the internal properties of different metals to turn chemical energy directly into electric energy.
Instructional Objectives
* Be able to understand the internal and external potentials of metals. * Be able to explain the internal workings of an electric battery

33

Electric Circuits

The work of Wheatstone, Ohm, and Kirchhoff leads to the design and analysis of how current flows.

34

Magnetism

William Gilbert, personal physician by appointment to her Majesty Queen Elizabeth I of England, discovered that the earth behaves like a giant magnet. Magnetism as a natural phenomenon, the behavior of magnetic materials, and the motion of charged particles in a magnetic field.

Instructional Objectives
* Be able to calculate the magnetic force on a current element and on a moving charge in a given magnetic field. * Know the definition of torque and potential energy for a magnetic dipole. * Be able to explain the concept of domains in ferromagnetic materials. * Be able to use the definition of magnetic flux and discuss the significance of the result that the net magnetic flux out of a closed surface is zero. * Be able to calculate the magnetic moment of a current loop and the torque exerted on a current loop in a magnetic field. * Be able to discuss the magnetism of the Earth.

35

The Magnetic Field

The law of Biot and Sarvart, the force between electric currents, and Ampère's law.

36

Vector Fields and Hydrodynamics

Force fields have definite properties of their own suitable for scientific study.

37

Electromagnetic Induction

The discovery of electromagnetic induction in 1831 creates an important technological breakthrough in the generation of electric power

38

Alternating Current

Electromagnetic induction makes it easy and natural to generate alternating current. Use of transformers makes it practical to distribute ac over long distances. Although Nikola Tesla understood all this, Thomas Edison chose not to, and thereby hangs a tale. Alternating current circuits obey a differential equation identical to the harmonic oscillator resonance equation.
Instructional Objectives
* Be able to state the definition of rms current and relate it to the maximum current in an ac circuit. * Know the phase relationships between voltages and currents for elements of an LRC circuit. * Be able to discuss the relationship between an LRC circuit and a harmonic oscillator. * Be able to describe a step-up and a step-down transformer. * Be able to discuss the relationship between power transmission and voltage. * Be able to state the resonance condition for an LRC circuit and to sketch the power versus angular frequency

39

Maxwell's Equation

By the 1860s all the pieces of the electricity and magnetism puzzle were in place, except one. The last piece, discovered by James Clerk Maxwell and called (unfortunately) the displacement current was just what was needed to produce electromagnetic waves called (among other things) light.
Instructional Objectives
* Be able to write down Maxwell's equations and discuss the experimental basis of each. * Be able to state the definition of Maxwell's displacement current and discuss its significance. * Realize that Maxwell's equations reveal that light is an electromagnetic wave. * Be able to state the expression for the speed of an electromagnetic wave in terms of electric and magnetic currents. * Be able to comment on the symmetry of Maxwell's equations. * Know the significance of Maxwell's equations in modern technological society. 

40

Optics and Beyond

Maxwell's theory says that electromagnetic waves of all wavelengths, from radio waves to gamma-rays and including visible light, are all basically the same phenomenon. Many of the properties of light are really just properties of waves, including reflection, refraction and diffraction. Ordinary light can be used to see things on a human scale, X-rays to "see" things on an atomic scale.
Instructional Objectives
* Be able to discuss the nature and properties of various parts of the electromagnetic spectrum. * Be able to state the law of reflection and Snell's law of refraction and relate them to the properties of waves. * Be able to explain wave interference and diffraction. * Be able to explain how we can "see" atoms.

41

The Michelson-Morley Experiment

In 1887, an exquisitely designed measurement of the earth's motion through the ether results in the most brilliant failure in scientific history.

42

The Lorentz Transformation @

If the speed of light is to be the same for all observers, then the length of a meter stick, or the rate of a ticking clock, depends on who measures it.

43

Velocity and Time

Einstein is motivated to perfect the central ideas of physics, resulting in a new understanding of the meaning of space and time.

44

Mass, Momentum, & Energy

The new meaning of space and time make it necessary to formulate a new mechanics. Starting from the conservation of momentum, it turns out among other things that E = mc 2.
Instructional Objectives
* Be able to state the definition of relativistic momentum and e equations relating kinetic energy and the total energy of a particle to its speed. * Be able to discuss the relation between mass and energy in Special Relativity and compute the binding energy of various systems from the known rest masses of their constituents. * Be able to discuss the concept of relativistic mass

45

Temperature and Gas Laws

The ups and downs of scientific research are reflected in Boyle's experiments, and Charles' investigations. Hot new discoveries about the behaviors of gases make the connection between temperature and heat, and raise the possibility of an absolute scale. Text Assignment: Chapter 15
Instructional Objectives
* Be able to state the definitions of the Celsius temperature scale and the Fahrenheit temperature scale and convert temperatures given on one scale into those of the other. * Be able to convert temperatures given on either the Celsius scale or the Fahrenheit scale into kelvins. * Be able to state the equation of state for an ideal gas and give the value of the universal gas constant in joules per kelvin. * * Know that the average energy of a gas molecule at temperature T is of the order of kT, where k is Boltzmann's constant. * Know that the absolute temperature T is a measure of the kinetic energy of a gas.

46

Engine of Nature

The Carnot engine, part one, beginning with simple steam engines

47

Entropy

The Carnot engine, part two, with profound implications for the behavior of matter and the flow of time through the universe.

48

Low Temperatures

Solids, liquids, and gases are the substance of every substance in the physical world. With the quest for low temperatures came the discovery that, under the right conditions of temperature and pressure, all elements can exist in each of the basic states of matter.
Instructional Objectives
* Explain how you make something colder. * Be able to list and give examples of the three basic states of matter. * Be able to explain what a phase diagram is. * Be able to reproduce a phase diagram fro water and explain why it is so unique. * Know how gases are liquefied. * Be able to explain the Joule-Thomson effect.

49

The Atom

This program explores the history of the atom, from the ancient Greeks to the early 20th century, when discoveries by J.J. Thomson and Ernest Rutherford created a new crisis for the world of physics.
Instructional Objectives
* Be able to summarize the kinetic theory and discuss the size of atoms. * Be able to compare Thomson's model of an atom with Rutherford's planetary model of an atom. * Be able to discuss why Rutherford's model of an atom conflicted with Maxwell's theory of charged particles. * Be able to discuss the significance of Brownian motion in providing evidence for the existence of atoms.

50

Particles and Waves

Evidence that light can sometimes act like a particle leads to quantum mechanics, the new physics.

51

From Atoms to Quarks

Electron waves attracted to the nucleus of an atom help account for the periodic table of the elements and ultimately lead to the search for quarks.

52

The Quantum Mechanical Universe & Beyond

 

 

 

Various 4 to 5 star Physics Lectures found with Google video search

   Lost Secrets of the Sacred Ark - Quantum Physics Science

  Supermassive-blackholes

  Animated Quantum Video

  Free Energy - Zero-Point Energy Extraction from the Quantum Vacuum

  Imagining the 10th Dimension part1

  Imagining the 10th Dimension part2

  What The Bleep Do We Know

  Elementary Particles and the Laws of Physics - Richard Feynman

  End of Semiconductor Roadmap: Collision of Physics, Economics, & Sociology

  On Getting Creative Ideas

  Invention and History of the Bubble Chamber

  SMALL WONDERS - THE WORLD OF NANOSCIENCE A LECTURE OF NOBEL PHYSICS LAUREATE

  Should Google Go Nuclear? Clean, cheap, nuclear power (no, really)

 Minnesota Channel - The Legacy of Einstein : Sylvester James Gates Jr

THE INVISIBLE MACHINE - ELECTROMAGNETIC WARFARE

Fermat's Last Theorem (1996)

Philosophy, Physics, Mathematics - “Dangerous Knowledge”

 
 
 

 

  The Science of Intention Pt.1

  The Science of Intention Pt.2

  The Science of Intention Pt.3

  The Science of Intention Pt.4

  The Science of Intention Pt.5

  The Science of Intention Pt.6

  The Science of Intention Pt.7

  The Science of Intention Pt.8

  The Science of Intention Pt.9

   
    

 

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