1 Special Relativity 2. 2 Topics l Recap l Length Contraction l Cosmic Ray Muons l Spacetime l Summary.

Slides:



Advertisements
Similar presentations
Einsteins Special Theory of Relativity. Relative Motion ALL motion is relative Speeds are only measured in relation to other objects No way to determine.
Advertisements

Lecture 20 Relativistic Effects Chapter Outline Relativity of Time Time Dilation Length Contraction Relativistic Momentum and Addition of Velocities.
Classical Relativity Galilean Transformations
Physics Lecture Resources
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.
Lecture 13 Space Time Diagrams ASTR 340 Fall 2006 Dennis Papadopoulos.
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.
SPECIAL RELATIVITY Background (Problems with Classical Physics) Classical mechanics are valid at low speeds But are invalid at speeds close to the speed.
1 Relativity part 1. 2 Where Do We Come From? What Are We? Paul Gauguin (1897) Where Are We Going? Museum of Fine Arts, Boston.
Harrison B. Prosper Florida State University Young Scholars Program.
Physics 3 for Electrical Engineering Ben Gurion University of the Negev
1 Special Relativity (Ch 37) Modern physics special relativity quantum mechanics Both were developed to explain the “few remaining puzzles” of classical.
SPECIAL RELATIVITY -Postulates of Special Relativity -Relativity of time –> time dilation -Relativity of length –> length contraction © 2005.
Lecture 12 Special Theory of Relativity II ASTR 340 Fall 2006 Dennis Papadopoulos.
PHY 1371Dr. Jie Zou1 Chapter 39 Relativity. PHY 1371Dr. Jie Zou2 Outline The principle of Galilean relativity Galilean space-time transformation equations.
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
Special Relativity & General Relativity
Time Dilation, Length Contraction and Doppler
Special Relativity. Topics Motion is Relative Michelson-Morley Experiment Postulates of the Special Theory of Relativity Simultaneity Spacetime Time Dilation.
Special Relativity The Death of Newtonian Physics.
Amanda Dorsey Faranak Islam Jose Guevara Patrick Conlin
Chapter 29 Relativity.
A lecture series on Relativity Theory and Quantum Mechanics The Relativistic Quantum World University of Maastricht, Sept 24 – Oct 15, 2014 Marcel Merk.
Page 1 Phys Baski Relativity I Topic #9: Special Relativity I Transformation of Variables between Reference Frames –Non-relativistic Galilean Transformation.
Special relativity.
The Special Theory of Relativity. Galilean-Newtonian Relativity Definition of an inertial reference frame: One in which Newton’s first law is valid Earth.
Special Relativity Einstein (1905): Three Nobel-Prize worthy publications On unrelated subjects: Brownian motion Photo-electric effect (Nobel prize) “On.
Special Relativity Contents: The End of Physics Michelson Morley Postulates of Special Relativity Time Dilation.
Special Relativity The Failure of Galilean Transformations
Special Relativity Einstein messes with space and time.
Chapter 9 Relativity Basic Problems The formulation of Newtonian mechanics is based on our daily experience and observation. But, Newtonian mechanics.
PHYS 221 Recitation Kevin Ralphs Week 12. Overview HW Questions Chapter 27: Relativity – History of Special Relativity (SR) – Postulates of SR – Time.
Time Dilation We can illustrate the fact that observers in different inertial frames may measure different time intervals between a pair of events by considering.
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.
Chapter 28 Special Relativity Events and Inertial Reference Frames An event is a physical “happening” that occurs at a certain place and time. To.
Consequences of Lorentz Transformation. Bob’s reference frame: The distance measured by the spacecraft is shorter Sally’s reference frame: Sally Bob.
Physics Lecture 2 1/26/ Andrew Brandt Monday January 26, 2009 Dr. Andrew Brandt 1.Special Relativity 2.Galilean Transformations 3.Time.
Chapter 28: Special Relativity
Modern Physics Relativity 1 Space is defined by measurements of length and depends on what “ruler” is used to measure the length. Time is defined by measurements.
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.
Chapter 7 Relativity n Special Theory of Relativity – Einstein 1905 – space contraction and time dilation n General Theory of Relativity – Einstein 1916.
My Chapter 26 Lecture.
IB Physics – Relativity Relativity Lesson 1 1.Galilean Transformations (one frame moving relative to another) Michelson Morley experiment– ether. 2.Speed.
Handy Dandy Chart  = 1v = 0  = 2v =.866 c  = 2.5v =.92 c  = 7v =.99 c  = 10v =.995 c  = 100v = c.
Mr. BaldwinPHYSICS 5/23/2014Relativity Aim: What does it mean to travel at light speed? Do Now: What happens when an object’s length (dimensions) as it.
Consequences of Special Relativity Simultaneity: Newton’s mechanics ”a universal time scale exists that is the same for all observers” Einstein: “No universal.
Special Relativity Physics 12 Adv. Einstein’s Postulates  In 1905, while working as a patent clerk in Switzerland, Einstein published his paper on.
Chapter 39 Relativity. A Brief Overview of Modern Physics 20 th Century revolution 1900 Max Planck Basic ideas leading to Quantum theory 1905 Einstein.
11.1 – Frames of Reference and Relativity
Chapter 1 Relativity 1.
Special Theory of Relativity. Galilean-Newtonian Relativity.
Special Relativity By Jackson Andrews.
1 1.Time Dilation 2.Length Contraction 3. Velocity transformation Einstein’s special relativity: consequences.
Time Dilation. Relative Time  Special relativity predicts that events seen as simultaneous by one observer are not simultaneous to an observer in motion.
Consequences of Relativism SPH4U. Wind Back the Clock Two consequences of relativism discussed: To a stationary observer, time appears to slow down in.
Special Relativity /- 5 The End of physics: Black Body Radiation -> Quantum mechanics Velocity of light With Respect to ether Maxwell’s Equations…
By: Jennifer Doran. What was Known in 1900 Newton’s laws of motion Maxwell’s laws of electromagnetism.
Chapter 28 Special Relativity Events and Inertial Reference Frames An event is a physical “happening” that occurs at a certain place and time. To.
Some places where Special Relativity is needed
Special Relativity II Two-minute movie Quiz Breakdown of simultaneity
Physics: Principles with Applications, 6th edition
Special Relativity Contents: The End of Physics Michelson Morley
Einstein’s Relativity Part 2
26-1 Galilean-Newtonian Relativity
RELATIVITY III SPECIAL THEORY OF RELATIVITY
Part 2: Time Dilation.
Aim: How do we explain the special theory of relativity?
Presentation transcript:

1 Special Relativity 2

2 Topics l Recap l Length Contraction l Cosmic Ray Muons l Spacetime l Summary

3 Recap l Postulates of Relativity l Laws of physics are the same in all inertial (that is, non-accelerating) frames l The speed of light in vacuum is independent of the motion of source and observer l Relativity of Simultaneity l Events simultaneous for one observer need not be simultaneous for another moving relative to the first

4 Recap -Time Dilation If t V is the elapsed time measured by a clock moving at speed v relative to a clock that measures an elapsed time of t R and is at rest relative to an observer then where

5 Recap -Time Dilation Very Important Point (VIP): By Principle 1, the time dilation effect must be perfectly symmetrical: If Betty and Ann are moving at a constant velocity relative to each other, Betty sees Ann’s clock run slower and Ann sees Betty’s clock run slower

6 Length Contraction You : d Y = v t Y d P = v t P Prof Consider the measurement of the length of a table by You and your professor who moves at speed v from A to B A B

7 Length Contraction Prof The ratio of your elapsed time t Y to the elapsed time t P measured by your professor is t Y / t P = , so A B You : d Y = v t Y d P = v t P

8 Summary: Moving clocks tick more slowly Moving lengths contract Again, it is important to understand that these statements must hold true for all inertial observers: every inertial observer will see moving clocks run more slowly and moving lengths contracted longitudinally Time Dilation & Length Contraction

9 Cosmic Ray Muons ~ 9 km Mean muon lifetime 2 ~ 2 microsecond Time to the ground 9km / 300,000 km/s 30 ~ 30 microsecond 15 For every 15 microseconds of our clock, the muon’s “clock” advances 1 only 1 microsecond!

10 Muon Decay – Detailed Example Muons decay according to the statistical law of radioactivity where N 0 is the initial number of muons, N(t) is the number remaining after an elapsed time t and  is the mean muon lifetime of 2.2  s

11 Muon Decay – Detailed Example The time to reach the ground is about 15 times the mean muon lifetime. Therefore, according to Newtonian physics only a fraction will reach the ground. But because of time dilation and length contraction the fraction reaching the ground is predicted to be about

12 Space + Time = Spacetime The distinction between past, present and future is only an illusion, even if a stubborn one. Albert Einstein Space: is a (3-D) hyper-surface through spacetime on which all events are simultaneous, for someone Time: is the direction perpendicular to this hyper-surface

13 Earth’s Time Axis 3008 AD 2008 AD 2508 AD y x now Event: A place at a given time Spacetime: The set of all events (t,x,y,z) A B CD O worldline

14 Summary l Clocks and Rulers l Moving clocks run more slowly l Moving lengths contract longitudinally l Spacetime l Space is a hyper-surface of simultaneous events and time is the direction perpendicular to it l Worldline l A trajectory through spacetime