Lecture 12 Special Theory of Relativity II ASTR 340 Fall 2006 Dennis Papadopoulos.

Slides:



Advertisements
Similar presentations
Physics: Principles with Applications, 6th edition
Advertisements

Classical Relativity Galilean Transformations
Physics Lecture Resources
Time dilation D.3.1Describe the concept of a light clock. D.3.2Define proper time interval. D.3.3Derive the time dilation formula. D.3.4Sketch and annotate.
Theory of Special Relativity
P1X*Dynamics & Relativity : Newton & Einstein Chris Parkes October 2005 Special Relativity Postulates Time Dilation Length Contraction Lorentz Transformation.
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 Theory of Relativity
1 Special Relativity 2. 2 Topics l Recap l Length Contraction l Cosmic Ray Muons l Spacetime l Summary.
Relativity Pierre-Hugues Beauchemin PHY 006 –Talloire, May 2013.
1 Special Relativity (Ch 37) Modern physics special relativity quantum mechanics Both were developed to explain the “few remaining puzzles” of classical.
INFINITE SPACE AND ABSOLUTE TIME. Large scale bubble-like structures in the universe. The image contains about 4000 galaxies each representing one luminous.
SPECIAL RELATIVITY -Postulates of Special Relativity -Relativity of time –> time dilation -Relativity of length –> length contraction © 2005.
Lecture 11 Special Theory of Relativity I 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
Chapter 37 Special Relativity. 37.2: The postulates: The Michelson-Morley experiment Validity of Maxwell’s equations.
2. Einstein's postulates in special theory of relativity
A lecture series on Relativity Theory and Quantum Mechanics The Relativistic Quantum World University of Maastricht, Sept 24 – Oct 15, 2014 Marcel Merk.
Introduction to special relativity
Special Theory of Relativity
S-164 Countdown G minus 15 and counting. Relativity AP Physics Supplemental.
Page 1 Phys Baski Relativity I Topic #9: Special Relativity I Transformation of Variables between Reference Frames –Non-relativistic Galilean Transformation.
Special relativity.
Chapter R2 Synchronizing Clocks. Newtonian time Time was held to be universal. Clocks ran the same in all inertial systems. In these systems if one system.
Phy107 Fall From last time… Galilean Relativity –Laws of mechanics identical in all inertial ref. frames Einstein’s Relativity –All laws of physics.
The Special Theory of Relativity. Galilean-Newtonian Relativity Definition of an inertial reference frame: One in which Newton’s first law is valid Earth.
Chapter 26 Relativity © 2006, B.J. Lieb
 Newtonian relativity  Michelson-Morley Experiment  Einstein ’ s principle of relativity  Special relativity  Lorentz transformation  Relativistic.
Special Relativity Einstein messes with space and time.
Relativity Introduction 14.1 Introduction Electrons can be accelerated to 0.99c using a potential difference of 3.1 MV According to Newtonian Mechanics,
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.
Education Physics Deparment UNS
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.
Introduction to special relativity
Special Relativity I wonder, what would happen if I was travelling at the speed of light and looked in a mirror?
Astronomy 1143 – Spring 2014 Lecture 18: Special Relativity.
The Theory of Special Relativity. Learning Objectives  Einstein’s two postulates in his theory of special relativity: The principle of relativity. (Same.
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.
Introduction Classical Physics Laws: Mechanics (Newton), Electromagnetism (Maxwell), Optics, Fluids,.. Etc. Modern Physics: What do we mean? Are the laws.
Chapter 26 Relativity. General Physics Relative Motion (Galilean Relativity) Chapter 3 Section 5
IB Physics – Relativity Relativity Lesson 1 1.Galilean Transformations (one frame moving relative to another) Michelson Morley experiment– ether. 2.Speed.
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.
LECTURE # 2 RELATIVITY II NEWTONIAN RELATIVITY- GALILEAN TRANSFORMATIONS - EINSTEIN PHYS 420-SPRING 2006 Dennis Papadopoulos Acknowledge contributions.
Unit 13 Relativity.
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.
Chapter 1 Relativity 1.
Special Theory of Relativity. Galilean-Newtonian Relativity.
1 PHYS 3313 – Section 001 Lecture #4 Monday, Jan. 27, 2014 Dr. Jaehoon Yu Galilean Transformation Do we need Ether? Michelson-Morley Experiment Einstein’s.
Galileo’s Relativity: Text: The laws of mechanics are the same in all inertial reference frames. More general: The laws of mechanics are the same in all.
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.
PHY 102: Lecture History 12.2 Events and Inertial Reference Frames 12.3 Postulates of Special Relativity 12.4 Relativity of Time: Time Dilation.
Relativity. Historical Development 1600s Newton discovered his laws of mechanics Applied to a wide variety of problems over the next two decades Worked.
Special Relativity How does light behave in moving reference frames?
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.
PHYS 342: More info The TA is Meng-Lin Wu: His is His office hour is 10:30am to 12pm on Mondays His office is Physics.
Quiz: True or False 1.Length and time are absolute. 2.If we only had the technology, spaceships could theoretically travel at twice speed of light. 3.You.
The Relativistic Quantum World
Einstein’s Relativity Part 2
RELATIVITY III SPECIAL THEORY OF RELATIVITY
The Galilean Transformation
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.
Presentation transcript:

Lecture 12 Special Theory of Relativity II ASTR 340 Fall 2006 Dennis Papadopoulos

Centripetal Acceleration t t+  t

Concept Summary Galilean Relativity and Transformation Maxwell’s Equations – speed of light Ether – MM experiment Einstein’s postulates Simultaneity Time dilation Length contraction Lorentz transformation Examples Relativistic Doppler effect

Galilean Relativity “Relativity” refers in general to the way physical measurements made in a given inertial frame are related to measurements in another frame. An inertial observer is one whose rest frame is inertial A quantity is invariant if all inertial observers obtain the same value Under Galilean relativity, measurements are transformed simply by adding or subtracting the velocity difference between frames: v ball (measured on ground)=v train (measured on ground)+v ball (measured on train) 12 m/s = 10m/s + 2 m/s V ball (measured on train)=v ground (measured on train)+ v ball (measured on ground) 2 m/s =  10m/s + 12 m/s 10 m/s 2 m/s 12 m/s

Fig. 1-1, p. 4 Experiment at rest Experiment in moving frame Same result. Ball rises and ends up in the thrower’s hand. Ball in the air the same length of time. Experiment looks different from ground observer (parabolic trajectory, speed as a function of time) and observer on the truck. However, they both agree on the validity of Newton’s laws.

CLOCKS SYNCHRONIZED AT t=0 (t=t’=0) AND ORIGINS COINCIDE Event – Galilean transformation Laws of mechanics invariant under Galilean transformation

The Speed of Light But at what frame is its value 3x10 5 km/sec ? Ether

Electromagnetic waves James Clerk Maxwell ( ) –Developed theory of electromagnetic fields in the 1860’s (Maxwell’s equations).

From T. Ferris : “Coming of Age in the Milky Way” ETHER

from wikipedia Light must travel through a medium: hypothesize that a “luminiferous ether” exists Earth is moving with respect to the ether (or the ether is moving with respect to the earth), so there should be some directional/season dependent change in the speed of light as observed from the reference frame of the earth.

Fig. 1-4, p. 8 MM experiment gave negative result NO ETHER – NO PREFERRED FRAME

THE SPEED OF LIGHT PROBLEM c If no ether we have a problem

Einstein enters the picture… Albert Einstein –Didn’t like idea of Ether –Threw away the idea of Galilean Relativity –Came up with the two “Postulates of Relativity” Postulate 1 – The laws of nature are the same in all inertial frames of reference Postulate 2 – The speed of light in a vacuum is the same in all inertial frames of reference.

The speed of light in vacuum has the same value, c= m/s, in all inertial reference frames, regardless of the velocity of the observer or the velocity of the source emitting the light. All the laws of physics have the same form in all inertial reference frames. The Solution??? Oh my goodness…how can that be right??? Alright … we know that Newtonian mechanics worked in all inertial reference frames under Galilean transformations, but does the same hold true for Maxwell ’ s equations of electromagnetism?

INVARIANCE OF SPEED OF LIGHT

TRUTH AND CONSEQUENCES WHAT IS SPEED ? WHAT DISTANCE AN OBJECT WILL TRAVEL IN A GIVEN DURATION OF TIME V=DX/DT DISTANCE IS A NOTION ABOUT SPACE – HOW MUCH SPACE IS BETWEEN TWO POINTS DURATION IS A NOTION ABOUT TIME – HOW MUCH TIME ELAPSES BETWEEN EVENTS SPEED IS A SPACE-TIME NOTION – CONSTANCY OF SPEED OF LIGHT REQUIRES THAT WE MODIFY CONVENTIONAL CONCEPTS OF SPACE AND TIME

The radical consequences Speed = distance traveled time elapsed If the speed of light is a constant … then … length and time must be variables?? speed of light = miles per hour These effects are known as length contraction and time dilation. How come you never noticed this before, and how come most of the time I can get away with Galilean transformations in your calculations? Most of the time the speed of the object whose motion you are calculating is so slow relative to the speed of light that the discrepancy due to relativity is negligible. (Most, but not all of the time)

Fig. 1-8, p. 13 REFERENCE FRAME -> GRID (3D) + SET OF CLOCKS CLOCKS SYNCHRONIZED

SIMULTANEITY NEWTON -> UNIVERSAL TIMESCALE FOR ALL OBSERVERS –“Absolute, true time, of itself and of its own nature, flows equably, without relation to anything external” EINSTEIN –“A time interval measurement depends on the reference frame the measurement is made”

II. SIMULTANEITY

Fig. 1-9, p. 14

II: TIME DILATION Imagine building a clock using mirrors and a light beam. One “tick” of the clock is the time it takes for light to travel from base to mirror. mirror Bouncing light packet Speaker clicks when light strikes D

Moving clock Now suppose we put the same “clock” on a spaceship that is cruising (at constant velocity, V) past us. How long will it take the clock to “tick” when we observe it in the moving spacecraft? Use Einstein’s postulates… Total distance travelled by light beam is  s=c  t Therefore time  t=  s/c By Pythagorean theorem, Can solve to obtain  t= (D/c)  (1  V 2 /c 2 ) 1/2 > D/c Clock appears to run more slowly!!  x=V  t  y=D  s=c  t

Fig. 1-10, p. 15

Now change the point of view… For ground-based observer, clock on spaceship takes longer to “tick” than it would if it were on the ground But, suppose there’s an astronaut in the spacecraft –the inside of the spacecraft is also an inertial frame of reference – Einstein’s postulates apply… –So, the astronaut will measure a “tick” that lasts –This is just the same time as the “ground” observers measured for the clock their own rest frame So, different observers see the clock going at different speeds! Time is not absolute!!

Time dilation This effect called Time Dilation. Clock always ticks most rapidly when measured by observer in its own rest frame Clock slows (ticks take longer) from perspective of other observers When clock is moving at V with respect to an observer, ticks are longer by a factor of This is called the Lorentz factor, 

Lorentz factor Lorentz factor goes to infinity when V->c! But it is very close to 1 for V/c small Notice that the clock ticks longer and as a result the moving person ages less

Clocks and time Does this “time dilation” effect come about because we used a funny clock? No, any device that measures time would give the same effect! The time interval of an event as measured in its own rest frame is called the proper time Note that if the astronaut observed the same “light clock” (or any clock) that was at rest on Earth, it would appear to run slow by the same factor , because the dilation factor depends on relative speed This is called the principle of reciprocity

Why don’t we ordinarily notice time dilation? Some examples of speeds in m/s 464 m/s Earth's rotation at the equator. 559 m/s the average speed of Concorde's record Atlantic crossing (1996)Concorde m/s the speed of a typical rifle bulletrifle 1400 m/s the speed of the Space Shuttle when the solid rocket boosters separate.Space Shuttle 8000 m/s the speed of the Space Shuttle just before it enters orbit. 11,082 m/s High speed record for manned vehicle, set by Apollo 10 29,800 m/s Speed of the Earth in orbit around the Sun (about 30 km/s) 299,792,458 m/s the speed of light (about 300,000 km/s)speed of light

III: LENGTH CONTRACTION The only way observers in motion relative to each other can measure a single light ray to travel the same distance in the same amount of time relative to their own reference frames is if their ``meters'' are different and their ``seconds'' are different! Seconds and meters are relative quantities.

LENGTH CONTRACTION Consider two “markers” in space. Suppose spacecraft flies between two markers at velocity V. A flash goes off when front of spacecraft passes each marker, so that anyone can record it Compare what would be seen by observer at rest w.r.t. markers, and an astronaut in the spacecraft… Observer at rest w.r.t. markers says: –Time interval is t; distance is L o =V  t Observer in spacecraft says: –Time interval is t o ; distance is L S =V  t o We know from before that t = t o  Therefore, L S =V  t o = V  t  (t o /t)=L o /  The length of any object is contracted in any frame moving with respect to the rest frame of that object, by a factor 

Fig. 1-13, p. 19

So, moving observers see that objects contract along the direction of motion. Length contraction… also called –Lorentz contraction –FitzGerald contraction Note that there is no contraction of lengths that are perpendicular to the direction of motion –Recall M-M experiment: results consistent with one arm contracting

Fig. 1-15, p. 21

Fig. 1-14, p. 20

Muon Experiment The Muon Experiment –Muons are created in upper atmosphere from cosmic ray hits –Typical muon travel speeds are  c, giving  =100 –Half-life of muons in their own rest frame (measured in lab) is t h = 2 microseconds = s –Travelling at  c for t h = s, the muons would go only 600 m –But travelling for  t h = s, the muons can go 60 km –They easily reach the Earth’s surface, and are detected! –Half-life can be measured by comparing muon flux on a mountain and at sea level; result agrees with  t h

Muon experiment, again Consider atmospheric muons again, this time from point of view of the muons –i.e. think in frame of reference in which muon is at rest –Decay time in this frame is 2  s (2/1000,000 s) –How do they get from top of mountain to sea level before decaying? From point of view of muon, mountain’s height contracts by factor of  to 600 m –Muons can then travel reduced distance (at almost speed of light) before decaying.

Fig. 1-11, p. 17 Examples of time dilation The Muon Experiment

New velocity addition law Einstein’s theory of special relativity was partly motivated by the fact that Galilean velocity transformations (simple adding/subtracting frame velocity) gives incorrect results for electromagnetism Once we’ve taken into account the way that time and distances change in Einstein’s theory, there is a new law for adding velocities For a particle measured to have velocity V p by an observer in a spaceship moving at velocity V s with respect to Earth, the particle’s velocity as measured by observer on Earth is Notice that if V p and V s are much less than c, the extra term in the denominator ->0 and therefore V ->V p + V s Thus, the Galilean transformation law is approximately correct when the speeds involved are small compared with the speed of light This is consistent with everyday experience Also notice that if the particle has V p = c in the spaceship frame, then it has V p =c in the Earth frame. The speed of light is frame-independent!