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Relativity

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Course of lectures «Contemporary Physics: Part2»Lecture №6Relativity. The Principle of Galilean Relativity. The Michelson-Morley Experiment. Einstein's Principle of Relativity. Consequences of the Special Theory of Relativity.

Слайды и текст этой презентации

Слайд 1Quick Quiz

Write the definitions for

a)Kirchhoff's law
b) Stephen- Boltzmann law

c) Wien's law
d) Rayleigh–Jeans law.

Quick QuizWrite the definitions for 	a)Kirchhoff's law	b) Stephen- Boltzmann law 	c) Wien's law	d) Rayleigh–Jeans law.

Слайд 2Course of lectures «Contemporary Physics: Part2»
Lecture №6

Relativity. The Principle of

Galilean Relativity. The Michelson-Morley Experiment. Einstein's Principle of Relativity. Consequences

of the Special Theory of Relativity.
Course of lectures «Contemporary Physics: Part2»Lecture №6Relativity. The Principle of Galilean Relativity. The Michelson-Morley Experiment. Einstein's Principle

Слайд 3In 1905, at the age of only 26, Einstein published

his special theory of relativity.
Regarding the theory, Einstein wrote:
“The relativity

theory arose from necessity, from serious and deep contradictions in the old theory from which there seemed no escape. The strength of the new theory lies in the consistency and simplicity with which it solves all these difficulties . . .”
In 1905, at the age of only 26, Einstein published his special theory of relativity.Regarding the theory,

Слайд 4The Principle of Galilean Relativity
Principle of Galilean relativity:
The laws of

mechanics must be the same in all inertial frames of

reference.
The Principle of Galilean RelativityPrinciple of Galilean relativity:The laws of mechanics must be the same in all

Слайд 5The Principle of Galilean Relativity
the Galilean space–time transformation equations
The Galilean

velocity transformation equation

The Principle of Galilean Relativitythe Galilean space–time transformation equationsThe Galilean velocity transformation equation

Слайд 6The Principle of Galilean Relativity
The Speed of Light

The Principle of Galilean RelativityThe Speed of Light

Слайд 7The Michelson–Morley Experiment
The most famous experiment designed to detect small

changes in the speed of light was first performed in

1881 by Albert A. Michelson and later repeated under various conditions by Michelson and Edward W. Morley (1838–1923).

No fringe shift of the magnitude required was ever observed.

Light is now understood to be an electromagnetic wave, which requires no medium for its propagation.

The Michelson–Morley ExperimentThe most famous experiment designed to detect small changes in the speed of light was

Слайд 8The Michelson–Morley Experiment
Details of the Michelson–Morley Experiment

The Michelson–Morley ExperimentDetails of the Michelson–Morley Experiment

Слайд 9The Michelson–Morley Experiment
Details of the Michelson–Morley Experiment

The Michelson–Morley ExperimentDetails of the Michelson–Morley Experiment

Слайд 10The Michelson–Morley Experiment
Details of the Michelson–Morley Experiment
It detected no shift

whatsoever in the fringe pattern.

The Michelson–Morley ExperimentDetails of the Michelson–Morley ExperimentIt detected no shift whatsoever in the fringe pattern.

Слайд 11Einstein’s Principle of Relativity
He based his special theory of relativity

on two postulates:
1. The principle of relativity: The laws of

physics must be the same in all inertial reference frames.
2. The constancy of the speed of light: The speed of light in vacuum has the same value, c = 3.00 · 108 m/s, in all inertial frames, regardless of the velocity of the observer or the velocity of the source emitting the light.
Einstein’s Principle of RelativityHe based his special theory of relativity on two postulates:1. The principle of relativity:

Слайд 12Consequences of the Special
Theory of Relativity
In relativistic mechanics there is

no such thing as an absolute length or absolute time

interval. Furthermore, events at different locations that are observed to occur simultaneously in one frame are not necessarily observed to be simultaneous in another frame moving uniformly with respect to the first.
Consequences of the SpecialTheory of RelativityIn relativistic mechanics there is no such thing as an absolute length

Слайд 13Consequences of the Special
Theory of Relativity
Simultaneity and the Relativity of

Time

Consequences of the SpecialTheory of RelativitySimultaneity and the Relativity of Time

Слайд 14Consequences of the Special
Theory of Relativity
Simultaneity and the Relativity of

Time
In other words,
two events that are simultaneous in one

reference frame are in general not simultaneous in a second 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.

Einstein’s thought experiment demonstrates that two observers can disagree on the simultaneity of two events. This disagreement, however, depends on the transit time of light to the observers and, therefore, does not demonstrate the deeper meaning of relativity. In relativistic analyses of high-speed situations, relativity shows that simultaneity is relative even when the transit time is subtracted out.

Consequences of the SpecialTheory of RelativitySimultaneity and the Relativity of TimeIn other words, two events that are

Слайд 15Consequences of the Special
Theory of Relativity
Time Dilation

Consequences of the SpecialTheory of RelativityTime Dilation

Слайд 16Consequences of the Special
Theory of Relativity
Time Dilation
Because γ is always

greater than unity, this result says that the time interval

Δt measured by an observer moving with respect to a clock is longer than the time interval Δtp measured by an observer at rest with respect to the clock. This effect is known as time dilation.
Consequences of the SpecialTheory of RelativityTime DilationBecause γ is always greater than unity, this result says that

Слайд 17Consequences of the Special
Theory of Relativity
Time Dilation
Δtp is the proper

time interval.
The proper time interval is the time interval

between two events measured by an observer who sees the events occur at the same point in space.
Consequences of the SpecialTheory of RelativityTime DilationΔtp is the proper time interval. The proper time interval is

Слайд 18Consequences of the Special
Theory of Relativity
Time Dilation
Decay curves for muons

at rest and for muons traveling at a speed of

0.999 4c.
Consequences of the SpecialTheory of RelativityTime DilationDecay curves for muons at rest and for muons traveling at

Слайд 19Consequences of the Special
Theory of Relativity
The Twin Paradox

Consequences of the SpecialTheory of RelativityThe Twin Paradox

Слайд 20Consequences of the Special
Theory of Relativity
Length Contraction
The proper length Lp

of an object is the length measured by someone at

rest relative to the object. The length of an object measured by someone 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.

If an object has a proper length Lp when it is measured by an observer at rest with respect to the object, then when it moves with speed v in a direction parallel to its length, its length L is measured to be shorter according to

Consequences of the SpecialTheory of RelativityLength ContractionThe proper length Lp of an object is the length measured

Слайд 21Consequences of the Special
Theory of Relativity
Length Contraction
Note that length contraction

takes place only along the direction of motion.

Consequences of the SpecialTheory of RelativityLength ContractionNote that length contraction takes place only along the direction of

Слайд 22Space–Time Graphs
Consequences of the Special
Theory of Relativity
It is sometimes helpful

to make a space–time graph, in which ct is the

ordinate and position x is the abscissa.

A path through space–time is called a world-line. At the origin, the world-lines of Speedo and Goslo coincide because the twins are in the same location at the same time. After Speedo leaves on his trip, his world-line diverges from that of his brother. Goslo’s world-line is vertical because he remains fixed in location. At their reunion, the two world-lines again come together.

Space–Time GraphsConsequences of the SpecialTheory of RelativityIt is sometimes helpful to make a space–time graph, in which

Слайд 23The Relativistic Doppler Effect
Consequences of the Special
Theory of Relativity
Another important

consequence of time dilation is the shift in frequency found

for light emitted by atoms in motion as opposed to light emitted by atoms at rest. This phenomenon, known as the Doppler effect. In the case of sound, the motion of the source with respect to the medium of propagation can be distinguished from the motion of the observer with respect to the medium. Light waves must be analyzed differently, however, because they require no medium of propagation, and no method exists for distinguishing the motion of a light source from the motion of the observer.
The Relativistic Doppler EffectConsequences of the SpecialTheory of RelativityAnother important consequence of time dilation is the shift

Слайд 24The Relativistic Doppler Effect
Consequences of the Special
Theory of Relativity
If a

light source and an observer approach each other with a

relative speed v, the frequency fobs measured by the observer is

The most spectacular and dramatic use of the relativistic Doppler effect is the measurement of shifts in the frequency of light emitted by a moving astronomical object such as a galaxy. Light emitted by atoms and normally found in the extreme violet region of the spectrum is shifted toward the red end of the spectrum for atoms in other galaxies—indicating that these galaxies are receding from us. The American astronomer Edwin Hubble (1889–1953) performed extensive measurements of this red shift to confirm that most galaxies are moving away from us, indicating that the Universe is expanding.

The Relativistic Doppler EffectConsequences of the SpecialTheory of RelativityIf a light source and an observer approach each

Слайд 25Quick Quiz 1

A baseball pitcher with a 90-mi/h fastball throws

a ball while standing on a railroad flatcar moving at

110 mi/h. The ball is thrown in the same direction as that of the velocity of the train. Applying the Galilean velocity transformation equation, the speed of the ball relative to the Earth is (a) 90 mi/h
(b) 110 mi/h (c) 20 mi/h (d) 200 mi/h (e) impossible to determine.
Quick Quiz 1A baseball pitcher with a 90-mi/h fastball throws a ball while standing on a railroad

Слайд 26Quick Quiz 2

A crew watches a movie that is two

hours long in a spacecraft that is moving at high

speed through space. Will an Earthbound observer, who is watching the movie through a powerful telescope, measure the duration of the movie to be (a) longer than, (b) shorter than, or (c) equal to two hours?
Quick Quiz 2A crew watches a movie that is two hours long in a spacecraft that is

Слайд 27Quick Quiz 3

Suppose astronauts are paid according to the amount

of time they spend traveling in space. After a long

voyage traveling at a speed approaching c, would a crew rather be paid according to (a) an Earth-based clock, (b) their spacecraft’s clock, or (c) either clock?
Quick Quiz 3Suppose astronauts are paid according to the amount of time they spend traveling in space.

Слайд 28Quick Quiz 4
You are packing for a trip to another

star. During the journey, you will be traveling at 0.99c.

You are trying to decide whether you should buy smaller sizes of your clothing, because you will be thinner on your trip, due to length contraction. Also, you are considering saving money by reserving a smaller cabin to sleep in, because you will be shorter when you lie down. Should you (a) buy smaller sizes of clothing, (b) reserve a smaller cabin, (c) do neither of these, or (d) do both of these?
Quick Quiz 4You are packing for a trip to another star. During the journey, you will be

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