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Chapter 26 Relativity. General Physics Relative Motion (Galilean Relativity) Chapter 3 Section 5

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Presentation on theme: "Chapter 26 Relativity. General Physics Relative Motion (Galilean Relativity) Chapter 3 Section 5"— Presentation transcript:

1 Chapter 26 Relativity

2 General Physics Relative Motion (Galilean Relativity) Chapter 3 Section 5 http://www.physics.mun.ca/~jjerrett/relative/relative.html

3 General Physics Michelson Interferometer Chapter 25 Section 7

4 General Physics Michelson Interferometer  The Michelson Interferometer is an optical instrument that has great scientific importance  It splits a beam of light into two parts and then recombines them to form an interference pattern  It is used to make accurate length measurements

5 General Physics Michelson Interferometer, schematic  A beam of light provided by a monochromatic source is split into two rays by a partially silvered mirror M  One ray is reflected to M 1 and the other transmitted to M 2  After reflecting, the rays combine to form an interference pattern  The glass plate ensures both rays travel the same distance through glass Active Figure: The Michelson InterferometerThe Michelson Interferometer

6 General Physics Measurements with a Michelson Interferometer  The interference pattern for the two rays is determined by the difference in their path lengths  When M 1 is moved a distance of λ/4, successive light and dark fringes are formed  This change in a fringe from light to dark is called fringe shift  The wavelength can be measured by counting the number of fringe shifts for a measured displacement of M  If the wavelength is accurately known, the mirror displacement can be determined to within a fraction of the wavelength

7 General Physics Luminiferous Ether  Classical physicists (Maxwell, Hertz, etc.) compared electromagnetic waves to mechanical waves  Mechanical waves need a medium to support the disturbance (air, water, string, etc.)  The luminiferous ether was proposed as the medium required (and present) for light waves to propagate  Present everywhere, even in empty space  Massless, but rigid medium  Could have no effect on the motion of planets or other objects

8 General Physics Verifying the Luminiferous Ether  Associated with the ether was an absolute frame of reference in which light travels with speed c  The Earth moves through the ether, so there should be an “ether wind” blowing  If v is the speed of the “ether wind” relative to the Earth, the observed speed of light should have a maximum (a), minimum (b), or in-between (c) value depending on its orientation to the “wind”

9 General Physics Michelson-Morley Experiment  First performed in 1881 by Michelson  Repeated under various conditions by Michelson and Morley  Designed to detect small changes in the speed of light  By determining the velocity of the Earth relative to the ether

10 General Physics Michelson-Morley Equipment  An interference pattern was observed  The interferometer was rotated through 90°  Used the Michelson Interferometer  Arm 2 is initially aligned along the direction of the earth’s motion through space  Should observe small, but measurable, shifts in the fringe pattern as orientation with the “ether wind” changes Active Figure: The Michelson-Morley ExperimentThe Michelson-Morley Experiment

11 General Physics Michelson-Morley Results  Measurements failed to show any change in the fringe pattern  No fringe shift of the magnitude required was ever observed  The addition laws for velocities were incorrect  The speed of light is a constant in all inertial frames of reference  Light is now understood to be an electromagnetic wave, which requires no medium for its propagation  The idea of an ether was discarded

12 General Physics Relativity I Sections 1–4

13 General Physics Basic Problems  The speed of every particle of matter in the universe always remains less than the speed of light  Newtonian Mechanics is a limited theory  It places no upper limit on speed  It breaks down at speeds greater than about 10% of the speed of light (v >.1c)  Newtonian Mechanics becomes a specialized case of Einstein’s Theory of Special Relativity  When speeds are much less than the speed of light v<<c

14 General Physics Galilean Relativity  Choose a frame of reference  Necessary to describe a physical event  According to Galilean Relativity, the laws of mechanics are the same in all inertial frames of reference  An inertial frame of reference is one in which Newton’s Laws are valid  Objects subjected to no forces will move in straight lines

15 General Physics Galilean Relativity, cont.  A passenger in an airplane throws a ball straight up  It appears to move in a vertical path  This is the same motion as when the ball is thrown while standing at rest on the Earth  The law of gravity and equations of motion under uniform acceleration are obeyed

16 General Physics Galilean Relativity, cont  There is a stationary observer on the ground  Views the path of the ball thrown to be a parabola  The ball has a velocity to the right equal to the velocity of the plane  The law of gravity and equations of motion under uniform acceleration are still obeyed

17 General Physics Galilean Relativity, final  The two observers disagree on the shape of the ball’s path  Both agree that the motion obeys the law of gravity and Newton’s laws of motion  Both agree on how long the ball was in the air  Conclusion: There is no preferred frame of reference for describing the laws of mechanics

18 General Physics Galilean Relativity – Limitations  Galilean Relativity does not apply to experiments in electricity, magnetism, optics, and other areas  Results do not agree with experiments  According to Galilean relativity, the observer S should measure the speed of the light pulse as v+c  Actually observer S measures the speed as c  What is the problem?

19 General Physics Albert Einstein  1879 – 1955  1905 published four papers:  Brownian motion  Photoelectric effect  2 on Special Relativity  1916 published theory of General Relativity  Searched for a unified theory  Never found one

20 General Physics Einstein’s Principle of Relativity  Resolves the contradiction between Galilean relativity and the fact that the speed of light is the same for all observers  Postulates  The Principle of Relativity: All the laws of physics are the same in all inertial frames  The constancy of the speed of light: The speed of light in a vacuum has the same value in all inertial reference frames, regardless of the velocity of the observer or the velocity of the source emitting the light

21 General Physics The Principle of Relativity  The results of any kind of experiment performed in one laboratory at rest must be the same as when performed in another laboratory moving at a constant velocity relative to the first one  No preferred inertial reference frame exists  It is impossible to detect absolute motion with respect to an absolute frame of reference

22 General Physics The Constancy of the Speed of Light  Been confirmed experimentally in many ways  A direct demonstration involves measuring the speed of photons emitted by particles traveling near the speed of light  Confirms the speed of light to five significant figures  Explains the null result of the Michelson-Morley experiment – relative motion is unimportant when measuring the speed of light  We must alter our common-sense notions of space and time

23 General Physics Consequences of Special Relativity  In relativistic mechanics  There is no such thing as absolute length  There is no such thing as absolute time  Events at different locations that are observed to occur simultaneously in one frame are not observed to be simultaneous in another frame moving uniformly past the first  In Special Relativity, Einstein abandoned the assumption of simultaneity

24 General Physics  Thought experiment  A boxcar moves with uniform velocity v  Two lightning bolts strike the ends  Flashes leave points A’ and B’ on the car and points A and B on the ground at speed c Simultaneity – Thought Experiment Observer O is midway between the points of lightning strikes on the ground, A and BObserver O is midway between the points of lightning strikes on the ground, A and B Observer O’ is midway between the points of lightning strikes on the boxcar, A’ and B’Observer O’ is midway between the points of lightning strikes on the boxcar, A’ and B’

25 General Physics  The light signals reach observer O at the same time  He concludes the light has traveled at the same speed over equal distances  Observer O concludes the lightning bolts occurred simultaneously Simultaneity – Results

26 General Physics Simultaneity – Results, cont  By the time the light has reached observer O, observer O’ on the car has moved  The light from B’ has already moved by observer O’, but the light from A’ has not yet reached him  The two observers must find that light travels at the same speed  Observer O’ concludes the lightning struck the front of the boxcar before it struck the back (they were not simultaneous events)

27 General Physics Simultaneity – Summary  Two events that are simultaneous in one reference frame are in general not simultaneous in a second reference frame moving relative to the first  That is, simultaneity is not an absolute concept, but rather one that depends on the state of motion of the observer  In the thought experiment, both observers are correct, because there is no preferred inertial reference frame

28 General Physics Time Dilation, Moving Observer  The vehicle is moving to the right with speed v  A mirror is fixed to the ceiling of the vehicle  An observer, O’, at rest in this system holds a laser a distance d below the mirror  The laser emits a pulse of light directed at the mirror (event 1) and the pulse arrives back after being reflected (event 2)

29 General Physics Time Dilation, Moving Observer  Observer O’ carries a clock  She uses it to measure the time between the events (Δt p )  The p stands for proper  She observes events 1 and 2 to occur at the same place  Light travels distance 2d = cΔt p  The time interval Δt p is called the proper time  The proper time is the time interval between events as measured by an observer who sees the events occur at the same position  You must be able to correctly identify the observer who measures the proper time interval

30 General Physics Time Dilation, Stationary Observer  Observer O is a stationary observer on the Earth  He observes the mirror and O’ to move with velocity v  By the time the light from the laser reaches the mirror, the mirror has moved to the right  The light must travel farther with respect to O than with respect to O’

31 General Physics  Observer O carries a clock  He uses it to measure the time between the events (Δt)  He observes events 1 and 2 to occur at different places  Events separated by distance vΔt  Light travels distance cΔt Time Dilation, Stationary Observer

32 General Physics Time Dilation, Observations  O and O’ must measure the same speed of light  The light travels farther for O  The time interval, Δt, for O is longer than the time interval for O’, Δt p  Observer O measures a longer time interval than observer O’ by the factor gamma Active Figure: Time DilationTime Dilation

33 General Physics Time Dilation, Example  The time interval Δt between two events measured by an observer moving with respect to a clock is longer than the time interval Δt p between the same two events measured by an observer at rest with respect to the clock  For example, when observer O’, moving at v = 0.5c, claims that 1.00 s has passed on the clock, observer O claims that Δt =  Δt p = (1.15)(1.00s) = 1.15 s has passed – Observer O considers the clock of O’ to be reading too low a value – “running to slow”  A clock in motion runs more slowly than an identical stationary clock v O’ O

34 General Physics Time Dilation – Equivalent Views  Initial View: Observer O views O’ moving with speed v to the right and the clock of O’ is running more slowly  Equivalent View: Observer O’ views O as the one who is really moving with speed v to the left and the clock of O is running more slowly  The principle of relativity requires that the views of the two observers in uniform relative motion must be equally valid and capable of being checked experimentally

35 General Physics Time Dilation – Generalization  All physical processes slow down relative to a clock when those processes occur in a frame moving with respect to the clock  These processes can be chemical and biological as well as physical  Time dilation is a very real phenomena that has been verified by various experiments

36 General Physics Time Dilation – Verification  Muons are unstable particles that have the same charge as an electron, but a mass 207 times more than an electron  Muons have a half-life of Δt p = 2.2 µs when measured in a reference frame at rest with respect to them (a) – unlikely to reach the Earth’s surface.  Relative to an observer on earth, muons should have a longer lifetime of Δt p =  Δt p (b) – likely to reach surface  A CERN experiment measured lifetimes in agreement with the predictions of relativity

37 General Physics Length Contraction  The measured distance between two points depends on the frame of reference of the observer  The proper length, L p, of an object is the length of the object measured by someone at rest relative to the object  The length of an object measured in a reference frame that is moving with respect to the object is always less than the proper length  This effect is known as length contraction

38 General Physics Length Contraction – Equation  Length contraction takes place only along the direction of motion Active Figure: Length ContractionLength Contraction

39 General Physics Length Contraction, Example  The length between two points L measured by an observer moving with respect to a ruler is shorter than the length L p between the same two points measured by an observer at rest with respect to the ruler  For example, when observer O’, moving at v = 0.5c, claims that a length of 1.00 m is measured by a ruler, observer O claims that L = L p /  = (1.00 m)/(1.15) = 0.87 m is the measured length between the two points – Observer O considers the length of O’ to be “contracted”  A ruler in motion is contracted compared to an identical stationary ruler v O’ O


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