Lecture 1 A Revolution in time Classical Physics Timeline.

Slides:



Advertisements
Similar presentations
ON TIME An Introduction into the theory behind Albert Einsteins Special Relativity.
Advertisements

Special relativity Einstein originally proposed his theory of special relativity in 1905 and it is often taken as the beginning of modern physics. It opened.
Physics Lecture Resources
Caroline Chisholm College
Chapter S2 Space and Time
Addition of velocities in the Newtonian physics V v= speed of the train measured from the platform w 1 =man’s speed measured from the train w1w1 w 2 =man’s.
Theory of Special Relativity
Wednesday, Feb. 4, 2015PHYS , Spring 2014 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #5 Wednesday, Feb. 4, 2015 Dr. Jaehoon Yu Einstein’s.
Black Holes. Outline Escape velocity Definition of a black hole Sizes of black holes Effects on space and time Tidal forces Making black holes Evaporation.
 PROGRAM OF “PHYSICS2B” Lecturer: Dr. DO Xuan Hoi Room A1. 413
Special Relativity (Time and length)
Physics 12 Mr. Jean May 9 th, The plan: Video Clip of the day – UB0http://
A Strange Phenomenon There is a type of unstable particles called Muon. They are produced in the upper atmosphere 14 km above Earth’s surface and travel.
Cosmic Rays Basic particle discovery. Cosmic Rays at Earth – Primaries (protons, nuclei) – Secondaries (pions) – Decay products (muons, photons, electrons)
1 Special Relativity (Ch 37) Modern physics special relativity quantum mechanics Both were developed to explain the “few remaining puzzles” of classical.
Physics 311 Special Relativity Lecture 2: Unity of Space and Time Inertial Frames OUTLINE Same unit to measure distance and time Time dilation without.
SPECIAL RELATIVITY -Postulates of Special Relativity -Relativity of time –> time dilation -Relativity of length –> length contraction © 2005.
Principle of special relativity Their is inconsistency between EM and Newtonian mechanics, as discussed earlier Einstein proposed SR to restore the inconsistency.
Special Theory of Relativity
LIGO-G W Welcome to the World Year of Physics Fred Raab, LIGO Hanford Observatory “One thing I have learned in a long life: that all our science,
Relativity Chapter 26. Introduction Major Physics accomplishments by the end of the 19 th century –Newton’s laws –Universal gravitation –Kinetic-molecular.
Time Dilation, Length Contraction and Doppler
Hubble Diagram: Distribution of Galaxies. Hubble’s Law: v = H o d Velocity increases with distance.
General Relativity For a general audience. Precession of Mercury Mercury’s entire orbit undergoes precession at a known rate. Most of it can be explained.
Contemporary science issues Lesson 16: Has the universe always been there? © 2006 Gatsby Technical Education Projects.
Chapter 26 Relativity. General Physics Relativity II Sections 5–7.
A lecture series on Relativity Theory and Quantum Mechanics The Relativistic Quantum World University of Maastricht, Sept 24 – Oct 15, 2014 Marcel Merk.
Special and General Relativity Marcus Han 3O3 (!0)
A presentation by Nipun Sharma Time dilation is difficult to explain simply, and has different explanations according to the setting. Best put, it is.
Muons are short-lived subatomic particles that can be produced in accelerators or when cosmic rays hit the upper atmosphere. A muon at rest has a lifetime.
The theory of special relativity applies in inertial (i.e., non-accelerating) reference frames. The theory of general relativity generalizes special relativity.
Special Relativity Chapters 15 and 16.
Einstein’s postulates 1.The laws of nature are the same for everyone. 2. The speed of light in a vacuum is constant for all observers.
P2 Topic 10. Learning Objectives For an object to move in a circular path a force must act on it. Energy can be converted from one form into another but.
Special Relativity: “all motion is relative”
Precursors to Modern Physics 1. Introduction to the course. 2. Quiz 0, one hour. 3. Required to read in the text book. 4. Class discussion. 5. Preview.
H.5.1Discuss muon decay as experimental evidence to support special relativity. H.5.2Solve some problems involving the muon decay experiment. H.5.3Outline.
PHYS 221 Recitation Kevin Ralphs Week 12. Overview HW Questions Chapter 27: Relativity – History of Special Relativity (SR) – Postulates of SR – Time.
Special Theory of Relativity Einstein pondered the question, “If I could ride a beam of light, what would I see?” Meaning, if a car moved at the speed.
Origins Lecture 15; May Previously on Origins Time of history/humans vs. time of “god” –What was there before time? –Does this make sense? The.
Relativity: History 1879: Born in Ulm, Germany. 1901: Worked at Swiss patent office. –Unable to obtain an academic position. 1905: Published 4 famous.
Relativity: QuarkNet Lecture. What we know circa 1900: Light travels at a finite velocity. Ole Rømer Galileo was among the first to try and measure.
Relativity Jennifer Keehn. “I want to know how God created this world. I am not interested in this or that phenomena, in the spectrum of this or that.
Astronomy 1143 – Spring 2014 Lecture 18: Special Relativity.
Phy 107 Fall From Last Time Physics changed drastically in the early 1900’s Relativity one of the new discoveries –Changed the way we think about.
Physics 12 MODERN PHYSICS: AN INTRODUCTION.  QUOTE AND CLIP OF.
MUONS!. What are we going to talk about? How muons are created Detecting methods Muon half life and decay rate Muon decay data Problems with the data.
Universal Gravitation. Gravity… Makes things such as leaves and rain fall It made the Earth round Builds up the pressures that kindle every star to shine.
One of Albert Einstein’s Greatest Insights By Larry Kimbrough.
Chapter 37 Relativity Relativity is an important subject that looks at the measurement of where and when events take place, and how these events are measured.
Special Relativity Physics 12 Adv. Einstein’s Postulates  In 1905, while working as a patent clerk in Switzerland, Einstein published his paper on.
Time-dilation experiment Prof Raghava Varma. This experiment is an indirect verification of special theory of relativity using cosmic ray muons. The picture.
RELATIVITY Einstein demonstrated that space and time are entangled. The time between two events depends on how far apart they occur, and vice versa. Also,
X’ =  (x – vt) y’ = y z’ = z t’ =  (t – vx/c 2 ) where   1/(1 - v 2 /c 2 ) 1/2 Lorentz Transformation Problem: A rocket is traveling in the positive.
1.4: Simple Types of Motion: Having the initial conditions(initial position and initial velocity), what is the distance and speed at later time? a. No.
Relativity. Historical Development 1600s Newton discovered his laws of mechanics Applied to a wide variety of problems over the next two decades Worked.
Catalyst Pick up a note sheet. Pick up 1 piece of colored paper. Put “Unit 1 Astronomy” on the front of the colored paper. SIT SILENTLY IN YOUR SEAT.
By: Jennifer Doran. What was Known in 1900 Newton’s laws of motion Maxwell’s laws of electromagnetism.
There is no universal, ‘absolute’ time in relativity Einstein postulated that the velocity of light c is the same for all observers. That led to the consequence.
Space and Time © 2014 Pearson Education, Inc..
Special and General Relativity Marcus Han 3O3 (!0)
A warning light in the engine of a fast-moving train flashes once each second according to a clock on the train. Will an observer on the ground measure.
Physics and Nature Physics studies the fundamental laws of nature. It is based on observations and experimentation, which lead to laws and theories. We.
Some places where Special Relativity is needed
RELATIVITY Einstein demonstrated that space and time are entangled.
Special Relativity II Two-minute movie Quiz Breakdown of simultaneity
The Relativistic Quantum World
General Physics (PHY 2140) Lecture 25 Modern Physics Relativity
Einstein’s Theory of Relativity
Science Notes: Stnd 14 Date Standard 14: 8.ESS1.1 The Big Bang
Presentation transcript:

Lecture 1 A Revolution in time

Classical Physics Timeline

Modern Physics Timeline

At the age of 16, Einstein puzzled over what it would be like to travel at the speed of light. In particular, what would one see in a mirror that is also moving at the speed of light? Einstein’s Mirror

In 1905, at the age of 26, Einstein published his theory of Special Relativity...

“I was sitting in a chair in the patent office at Bern when all of a sudden a thought occurred to me: If a person falls freely he will not feel his own weight... I was startled. This simple thought made a deep impression on me. It impelled me towards a theory of gravitation.” The “Happiest Thought” of Einstein’s Life (1907)

Almost a decade later, in 1916, Einstein completed his theory of General Relativity...

And both theories completely revolutionised our concept of time...

“What, then, is time? I know well enough what it is, provided that nobody asks me; but if I am asked what it is and try to explain, I am baffled.” St. Augustine (5 th Century A.D.) Easier question: How do we measure time?

The ‘second’ is the duration of 9,192,631,770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the cesium-133 atom Definition of a Second

Accurate to seconds! Modern Atomic Clock (NIST-7)

In a galaxy far, far away...

Fact 1

Fact 2

Fact 3

Conclusion:  Time is not absolute, as common sense and everyday experience might suggest  It depends on the observer  In other words, it is relative “When the Special Theory of Relativity began to germinate in me, I was visited by all sorts of nervous conflicts... I used to go away for weeks in a state of confusion.”

Evidence for ‘Time Dilation’  Atomic clock travelling around the world in a plane  Muons reaching Earth from a cosmic ray shower  Muons travelling round in a storage ring  Global Positioning System (GPS)

Hafele and Keating’s Classic Experiment Hafele and Keating taking the atomic clocks around the world to test Einstein’s relativity theory

Muons  Muons are a type of subatomic particle  Same family as electron, but 200 times more massive  They are unstable, with a lifetime of about 2 x seconds

Cosmic Ray Shower

Cosmic Ray Shower (cont’d)  Muons are created in a cosmic ray shower, and travel near the speed of light down to the ground  They should only travel about 600 m before dis- integrating in the upper atmosphere  But from experiments, they can travel 4.8 km to ground level — because of time dilation!

Muon Storage Ring  Can make muons ‘last longer’ by keeping them circulating round a ring at very high speeds  If there were no time dilation, muons can only orbit the ring around 15 times before decaying  Instead, muons are observed to orbit hundred of times before decaying A muon storage ring at CERN

The Global Positioning System (GPS)  24 satellites in orbit  4 of them visible from any point on Earth  Accurate to less than a few metres Hand-held GPS Receiver

GPS Accuracy Depends on Relativity  A clock error of seconds would result in a position error of around 30 m!  Motion of satellite would slow clock by but the reduced gravity would speed it up slightly  Thus effects of special and general relativity need to be accounted for