PH 103 Dr. Cecilia Vogel Lecture 14 Review Outline  Consequences of Einstein’s postulates  time dilation  simultaneity  Einstein’s relativity  1.

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.
Theory of Special Relativity
Cutnell/Johnson Physics 7th edition
SPECIAL RELATIVITY -Postulates of Special Relativity -Relativity of time –> time dilation -Relativity of length –> length contraction © 2005.
1 Light’s Arrival Starship Enterprise is headed straight for the star Betelgeuse at a speed of 0.6 c. When the Enterprise is 2 light-years (in the Enterprise.
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.
PH 301 Dr. Cecilia Vogel Lecture 2. Review Outline  length contraction  Doppler  Lorentz  Consequences of Einstein’s postulates  Constancy of speed.
PH 301 Dr. Cecilia Vogel Lecture 1. Review Outline  PH  Mechanics  Relative motion  Optics  Wave optics  E&M  Changing E and B fields  Relativity.
PH 103 Dr. Cecilia Vogel Lecture 16. Review Outline  Relativistic Energy  mass energy  kinetic energy  More consequences of constancy of speed of.
PHY 1371Dr. Jie Zou1 Chapter 39 Relativity (Cont.)
PH 103 Dr. Cecilia Vogel Lecture 10. Review Outline  Interference  2-slit  Diffraction grating  spectra  Relativity  classical relativity  constants.
Special Relativity & General Relativity
Chapter 37 Special Relativity. 37.2: The postulates: The Michelson-Morley experiment Validity of Maxwell’s equations.
Lecture 14 Space-time diagrams (cont) ASTR 340 Fall 2006 Dennis Papadopoulos.
PH 103 Dr. Cecilia Vogel Lecture 13 Review Outline  Einstein’s postulates  inertial frames indistinguishable  constancy of speed of light  principle.
SPECIAL RELATIVITY Chapter 28.
Special Relativity Classical Relativity 1,000,000 ms -1 ■ How fast is Spaceship A approaching Spaceship B? ■ Both Spaceships see the other approaching.
Special Relativity Physics 1161: Lecture 35 Sections 29-1 – 29-6.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 29 Physics, 4 th Edition James S. Walker.
Outline - Feb. 8, 2010 Postulates of special relativity State of Motion Reference Frames Consequences of c = constant Time dilation and length contraction.
Chapter 29 Relativity.
Physics 213 General Physics Lectures 20 & Last Meeting: Optical Instruments Today: Optics Practice Problems, Relativity (over two lectures)
A lecture series on Relativity Theory and Quantum Mechanics The Relativistic Quantum World University of Maastricht, Sept 24 – Oct 15, 2014 Marcel Merk.
The Death of High Mass Stars. Quiz #8 On the H-R diagram, a high mass star that is evolving off the main sequence will become redder in color and have.
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.
Mon. Jan. 5 – Physics Lecture #16 Relativity – Basic Postulates 0) Overview of Quarter – Special Relativity, E&M, Unification 1) Basic Postulates 2) Relative.
PH 301 Dr. Cecilia Vogel Lecture 4. Review Outline  Lorentz transformation  simultaneity  twin paradox  Consequences of Einstein’s postulates  length.
Special Theory of Relativity
Special relativity.
Special Theory of Relativity Space and Time. Inertial reference frames Reference frames in which Newton’s first law is valid. –In other words, a reference.
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 Space and Time. Spacetime Motion in space is related to motion in time. Special theory of relativity: describes how time is affected.
The Special Theory of Relativity. Galilean-Newtonian Relativity Definition of an inertial reference frame: One in which Newton’s first law is valid Earth.
PH 301 Dr. Cecilia Vogel Lecture 2. Review Outline  Relativity  classical relativity  Einstein’s postulates  Constancy of speed of light  consequence:
Relativity Introduction 14.1 Introduction Electrons can be accelerated to 0.99c using a potential difference of 3.1 MV According to Newtonian Mechanics,
Goal: To get to know the ins and outs of relativity (relatively speaking) Objectives: 1)To understand how Black holes compare to space-time 2)To learn.
Chapter 9 Relativity Basic Problems The formulation of Newtonian mechanics is based on our daily experience and observation. But, Newtonian mechanics.
The Theory of Special Relativity Ch 26. Two Theories of Relativity Special Relativity (1905) –Inertial Reference frames only –Time dilation –Length Contraction.
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.
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.
1.Simultaneity 2.Time Dilation 3.Length Contraction SPECIAL RELATIVITY Space, time, motion, revisited.
Special Relativity I wonder, what would happen if I was travelling at the speed of light and looked in a mirror?
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.
My Chapter 26 Lecture.
1 Relativity  H3: Relativistic kinematics  Time dilation  Length contraction.
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 102: Lecture 28 Make sure your grade book entries are correct.
Chapter 39 Relativity. A Brief Overview of Modern Physics 20 th Century revolution 1900 Max Planck Basic ideas leading to Quantum theory 1905 Einstein.
Mon. Jan. 28 – Physics Lecture #4 Relativity – Basic Postulates 0) Quiz 1) Basic Postulates 2) Relative velocities 3) Light Clocks 4) Comparing time between.
11.1 – Frames of Reference and Relativity
Time Dilation. Relative Time  Special relativity predicts that events seen as simultaneous by one observer are not simultaneous to an observer in motion.
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.
Special Relativity How does light behave in moving reference frames?
Space and Time © 2014 Pearson Education, Inc..
© 2007 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their.
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
The Relativistic Quantum World
Physics: Principles with Applications, 6th edition
Special Relativity Physics 102: Lecture 28
Wacky Implications of Relativity
General Physics (PHY 2140) Lecture 25 Modern Physics Relativity
Lorentz Transformation
RELATIVITY III SPECIAL THEORY OF RELATIVITY
Physics 1161: PreLecture 26 Special Relativity 1.
Presentation transcript:

PH 103 Dr. Cecilia Vogel Lecture 14

Review Outline  Consequences of Einstein’s postulates  time dilation  simultaneity  Einstein’s relativity  1 st and 2 nd postulates of special relativity  equivalence principle of general relativity

Some Consequences Can be derived from constancy of speed of light:  Time interval between two events is different measured by different observers.  Order of events may be different measured by different observers.  Length of object or length of a trip is different measured by different observers.

Recall Classical Relativity  Suppose two observers time the pretzel you throw and catch. One observer on plane, one on Earth. Same pretzel. Go-stop. t=5 s Go stop. t =?

Recall Classical Relativity  At any point, let the velocity of the pretzel measured by the plane observer be v p.  The velocity measured by Earth observer is v plane + v p. Earth observer measures faster speed:  pretzel goes farther, faster, but same time (5s) Compared to this frame, in this frame, the pretzel goes... farther

Now Einstein’s Relativity  That worked for pretzels, what about light?  Person on super-plane shines light at mirror.  Suppose two observers time the light that shines and reflects. One observer on plane, one on Earth. Same light. Go-stop. t o =5  s Go stop. t=?

Now Einstein’s Relativity Compared to this frame, in this frame, light goes...  At any point, the velocity of the light measured by the plane observer is c  And the velocity measured by Earth observer is c, so Earth observer measures:  Light goes farther, same speed→ farther longer time! t>5  s

Time Dilation  Generalize result:   t and  t o are both the time between same events  measured by different observers  v is relative speed of the two observers  Notice that if v<<c, the two times are .  Hard part: which time is which?

Time Dilation  Units comment  If velocities are given as a fraction of c,  then the “c”units cancel.  Example:  If v= 0.8 c,  then (v/c) =(0.8c/c) = 0.8 (no units)

Proper time  What’s the difference between  t and  t o ?   t o is the “proper time”  It is always less than any other measured time.  Definition : proper time is time in frame in which the two events occur at same place  Events are  single instant in time, single point in space,  Events don’t move.  They don’t have reference frame. Occur in all frames  Time interval is time between two events  One event makes you start your timer  other even makes you stop you timer.

Proper time  What’s the difference between  t and  t o ?   t o is the “proper time”  Definition : proper time is time in frame in which events occur at same place  For example  If the two events happen to someone or something, their frame measures proper time  your heartbeat  If someone is at both events, (or same  x away) their frame measures proper time  person taking trip  particle’s lifetime  you and the clock on the wall

Time Trip  Nikos travels to a planet 12 light-years away at a speed of 0.6 c. Juan stays on Earth. Each measures the trip to take a different amount of time. Note:  A light-year is distance light travels in a yr  1 light-year = (c)(1yr) = 1c-yr  Consistent units: distance in light-years, speed as fraction of c, time in years  The values in example are relative to Earth  In that frame (in any one frame), the laws of physics hold, including d = vt Ex: 12c-yr/24yr = 0.5c

More Example  If Nikos makes a 12 light-year trip at 0.6c, Juan sees him moving at 0.6c for 20 years.  d = vt = (0.6c)(20 y) = 12c-yr.  Nikos sees himself moving at   Nikos sees the planet getting closer at 0.6c for 16 years.  d = vt = (0.6c)(16y) = 9.6 c-yr  Both are measuring the distance between Earth and planet, yet the distances are different!

Proper Length  What’s the difference between the two lengths?  One is the “proper length”  It’s always longer than any other measured length.  Def: proper length is length in frame in which object (or ends of trip) is at rest  For example  Object, or anyone at rest relative to it, measures object’s proper length.  Your own height  Length of ship you are riding on  Someone measures the proper length between two objects, if both are at rest relative to them  person on either planet, for a trip between planets

Just How Proper is it? If there is a proper time and a proper length, is there a proper reference frame?  NO!!!!!!!  Proper time of trip in example: Nikos  Proper length of trip in example: Juan  Proper time of astronaut’s heartbeat: Astronaut  Astronaut’s heartbeat looks SLOW to you.  Proper time of your heartbeat: You  Your heartbeat looks SLOW to astronaut.

Simultaneity  How do we know whether 2 events are simultaneous?  If signals coming from events arrive at the same time, the events might not have been simultaneous  how long did it take the signal to get here? demo

If t arrive, d, and v the same, conclude t event same

If t arrive, is smaller and d/v also smaller, can conclude t event same v eraser +v thrower V eraser -v thrower

If t arrive is earlier and d/v is same, must conclude t event is earlier! one observer says two events are simultaneous, other says they are not!! SIMULTANEITY IS NOT ABSOLUTE