Consequences of Lorentz Transformation. Bob’s reference frame: The distance measured by the spacecraft is shorter Sally’s reference frame: Sally Bob.

Slides:



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

Space Fight.
O’ O X’ X Z’ Z 5. Consequences of the Lorentz transformation
Lecture 20 Relativistic Effects Chapter Outline Relativity of Time Time Dilation Length Contraction Relativistic Momentum and Addition of Velocities.
Classical Relativity Galilean Transformations
Classical Doppler Shift Anyone who has watched auto racing on TV is aware of the Doppler shift. As a race car approaches the camera, the sound of its engine.
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.
Derivation of Lorentz Transformations
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.
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.
PHY 1371Dr. Jie Zou1 Chapter 39 Relativity (Cont.)
Special Relativity & General Relativity
Chapter 37 Special Relativity. 37.2: The postulates: The Michelson-Morley experiment Validity of Maxwell’s equations.
Time Dilation, Length Contraction and Doppler
2. Einstein's postulates in special theory of relativity
IB Physics – Relativity Relativity Lesson 2 1.Time dilation 2.Lorentz Factor 3.Proper time 4.Lorentz contraction 5.Proper length 6.Twin paradox and symmetric.
A lecture series on Relativity Theory and Quantum Mechanics The Relativistic Quantum World University of Maastricht, Sept 24 – Oct 15, 2014 Marcel Merk.
Time Dilation and Lorentz Contraction Physics 11 Adv.
Introduction to special relativity
Page 1 Phys Baski Relativity I Topic #9: Special Relativity I Transformation of Variables between Reference Frames –Non-relativistic Galilean Transformation.
Special relativity.
Phy107 Fall From last time… Galilean Relativity –Laws of mechanics identical in all inertial ref. frames Einstein’s Relativity –All laws of physics.
Special Relativity: “all motion is relative”
Module 4Relativity of Time, Simultaneity & Length1 Module 4 Relativity of Time, Simultaneity and Length As written, the Lorentz transformation equations.
Announcements Special Relativity Test on class period after lab
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.
Physics 2170 – Spring Special relativity Homework solutions are on CULearn Remember problem solving sessions.
Chapter 28 Special Relativity Events and Inertial Reference Frames An event is a physical “happening” that occurs at a certain place and time. To.
Education Physics Deparment UNS
Physics Lecture 2 1/26/ Andrew Brandt Monday January 26, 2009 Dr. Andrew Brandt 1.Special Relativity 2.Galilean Transformations 3.Time.
Lecture_06: Outline Special Theory of Relativity  Principles of relativity: length contraction, Lorentz transformations, relativistic velocity  Relativistic.
Special Relativity I wonder, what would happen if I was travelling at the speed of light and looked in a mirror?
My Chapter 26 Lecture.
1 Relativity  H3: Relativistic kinematics  Time dilation  Length contraction.
Handy Dandy Chart  = 1v = 0  = 2v =.866 c  = 2.5v =.92 c  = 7v =.99 c  = 10v =.995 c  = 100v = c.
Special Relativity Additional reading: Higher Physics for CfE, p.64 – 69. Notes p.38 The idea of relativity goes back a long way … Gallileo was one of.
Consequences of Special Relativity Simultaneity: Newton’s mechanics ”a universal time scale exists that is the same for all observers” Einstein: “No universal.
Spacetime diagrams can help you to visualize relativity. They are similar to scale diagrams and freebody diagrams.
Special Relativity = Relatively Weird
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.
Special relativity Part II Recall Einstein’s Postulates (1905) First Postulate –The laws of physics are the same in any inertial frame of reference (principle.
1 PHYS 3313 – Section 001 Lecture #5 Wednesday, Sept. 11, 2013 Dr. Jaehoon Yu Time Dilation & Length Contraction Relativistic Velocity Addition Twin Paradox.
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,
Derivation of Lorentz Transformations Use the fixed system K and the moving system K’ At t = 0 the origins and axes of both systems are coincident with.
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…
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.
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.
Key Areas covered The speed of light in a vacuum is the same for all observers. The constancy of the speed of light led Einstein to postulate that measurements.
Chapter 28 Special Relativity Events and Inertial Reference Frames An event is a physical “happening” that occurs at a certain place and time. To.
Problem: A rocket travels away from earth at constant speed v to planet Q. The trip takes 100 years, as measured on earth but only 25 years as measured.
Some places where Special Relativity is needed
PHYS 3313 – Section 001 Lecture #6
Einstein’s Relativity Part 2
Special Relativity: Time Dilation and Length Contraction
Special Relativity Lecture 2 12/3/2018 Physics 222.
RELATIVITY III SPECIAL THEORY OF RELATIVITY
Time Dilation Observer O is on the ground
Key Areas covered The speed of light in a vacuum is the same for all observers. The constancy of the speed of light led Einstein to postulate that measurements.
Special Relativity Chapter 1-Class3.
Chapter 37 Special Relativity
Presentation transcript:

Consequences of Lorentz Transformation

Bob’s reference frame: The distance measured by the spacecraft is shorter Sally’s reference frame: Sally Bob The relative speed v is the same for both observers:

Length contraction only occurs in the direction of motion— lengths in the perpendicular directions do not change. V = 0 v = 0.87c v=0.995c v=.999c v=c

 The inertial frame of reference in which the observed body is at rest is called the proper frame.

 The length of a rod as measured in the inertial frame in which it is at rest is called the PROPER LENGTH, the relation between the proper length L 0 and the apparent or non- proper length L is as follows 

 The time interval recorded by a clock fixed with respect to the observed event is called the Proper Time,the relation between the proper time t 0 and the apparent or non-proper time t is as follows

One consequence: Time Changes Equipment needed: a light clock and a fast space ship.

In Bob’s reference frame the time between A & B is Δ t 0 Sally on earth Bob Beginning Event A Ending Event B Δt0Δt0

Bob In Sally’s reference frame the time between A & B is Δ t Bob AB Sally on earth Length of path for the light ray: and ΔtΔt

Δt 0 = the time between A & B measured by Bob Δt = the time between A & B measured by Sally v = the speed of one observer relative to the other Time Dilation = Moving clocks slow down If Δt 0 = 1s, v =.999 c then:

Bob’s watch always displays his proper time Sally’s watch always displays her proper time How do we define time? The flow of time each observer experiences is measured by their watch – we call this the proper time If they are moving relative to each other they will not agree

A Real Life Example: Lifetime of muons Muon’s rest lifetime = 2.2x10 -6 seconds Many muons in the upper atmosphere (or in the laboratory) travel at high speed. If v = c. What will be its average lifetime as seen by an observer at rest?

  – meson Decay: Time dilation has been verified in experiments on nuclear particle, called  -mesons. Fast moving  -mesons, are created in the cosmic rays at a height of about 10 kilometers from the surface of the earth and reach the earth in large numbers. Theses m- meson have a typical speed of 2.994x10 8 m/s, which is of the speed of light c. A  -meson is found to have an average life – time of 2x10 -6 s after which it decays into an electron. Obviously, a  -meson in its life-time can travel a distance of only 2.994x10 8 m/s x 2x10 -6 s≈ 600m or 0.6 km.

 Rossi and Hall in 1941 attributed this result to the time dilation effect. The  -mesons has a life –time t 0 ≈ 2x10 -6 s in its own frame of reference, in observer`s frame of reference on the earth, however, the life time is lengthened owing to the relative motion, to the value t given by

 In, a meson whose speed is 0.998c ( ) can travel a distance  Hence, despite their brief life-time it is possible for the  -mesons to reach the ground from the large altitudes at which they are actually formed. More recently, the dilation caused by the thermal vibration of the nuclei in certain crystals has also been verified.  A similar experiment was done with pions by Ayres in 1971, the proper life time measured for point at rest is known to be 26  s

 What will be the apparent length of a meter stick measured by an observer at rest when the stick is moving along its velocity equal  Solution