option h: relativity h4 consequences of special relativity

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The twin paradox H.4.1 Describe how the concept of time dilation leads to the twin paradox. H.4.2 Discuss the Hafele-Keating experiment. Option H: Relativity H4 Consequences of special relativity

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Option H: Relativity H4 Consequences of special relativity. The twin paradox H.4.1Describe how the concept of time dilation leads to the twin paradox. H.4.2Discuss the Hafele-Keating experiment.. Option H: Relativity H4 Consequences of special relativity. The twin paradox - PowerPoint PPT Presentation

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Page 1: Option H: Relativity H4 Consequences of special relativity

The twin paradox

H.4.1 Describe how the concept of time dilation leads to the twin paradox.

H.4.2 Discuss the Hafele-Keating experiment.

Option H: RelativityH4 Consequences of special relativity

Page 2: Option H: Relativity H4 Consequences of special relativity

The twin paradox

Describe how time dilation leads to the paradox.

This has already been done in Topic H3.

Option H: RelativityH4 Consequences of special relativity

EXAMPLE: The twin paradox: Suppose Einstein has a twin brother who stays on Earth while Einstein travels at great speed in a spaceship. When he returns to Earth Einstein finds that his twin has aged more than himself! Explain why this is so.

SOLUTION: Since Einstein is in the moving spaceship, his clock ticks more slowly. But his twin’s ticks at its Earth rate. The twin is thus older than Einstein on his return!

By the way, this is NOT the paradox. The paradox is on the next slide…

Page 3: Option H: Relativity H4 Consequences of special relativity

EXAMPLE: The twin paradox: From Einstein’s perspective Einstein is standing still, but his twin is moving (with Earth) in the opposite direction. Thus Einstein’s twin should be the one to age more slowly. Why doesn’t he?

SOLUTION: The “paradox” is resolved by general relativity (which is the relativity of non-inertial reference frames). It turns out that because Einstein’s spaceship is the reference frame that actually accelerates, his is the one that “ages” more slowly.

The twin paradox

Describe how time dilation leads to the paradox.

This has already been done in Topic H3.

Option H: RelativityH4 Consequences of special relativity

Page 4: Option H: Relativity H4 Consequences of special relativity

The twin paradox

Discuss the Hafele-Keating experiment.

From Wikipedia: “The Hafele–Keating experiment was a test of the theory of relativity. In 1971, Hafele, a physicist, and Keating, an astronomer, took four atomic clocks aboard commercial airliners.” “They flew twice around the world, first eastward, then westward, and compared the clocks against others that remained at the United States Naval Observatory.”“When reunited, the three sets of clocks were found to disagree with one another, and their differences were consistent with the predictions of special and general relativity.”

Option H: RelativityH4 Consequences of special relativity

This experiment obviously tested time dilation.

Page 5: Option H: Relativity H4 Consequences of special relativity

Velocity addition

H.4.3 Solve one-dimensional problems involving the relativistic addition of velocities.

Option H: RelativityH4 Consequences of special relativity

Page 6: Option H: Relativity H4 Consequences of special relativity

Velocity addition

Solve one-dimensional problems involving the relativistic addition of velocities.

Suppose you are in Car B, shown below.Suppose car A is moving at ux = +20 m s-1 and your car B is moving at v = +40 m s-1 as shown.

As far as you are concerned, the velocity ux’ of car A relative to you is -20 m s-1 , because A is moving backwards relative to you.

Option H: RelativityH4 Consequences of special relativity

A

B

velocity of A relative to Bux’ = ux - v

FYIThis is the Galilean transformation which we learned way back in Topic 2.1.

Page 7: Option H: Relativity H4 Consequences of special relativity

Velocity addition

Solve one-dimensional problems involving the relativistic addition of velocities.

Now consider two spaceships leaving Earth in opposite directions:

Suppose ux = 0.75c and v = 0.50c (to the left).

Then according to the Galilean transformation, the ux’ (the velocity of A relative to B) would be

ux’ = ux – v = 0.80c - -0.50c = 1.3c.

This is in contradiction to the tenet that c is the maximum speed anything can have.

Option H: RelativityH4 Consequences of special relativity

FYIThe Galilean transformation for addition of velocities fails at relativistic speeds.

Page 8: Option H: Relativity H4 Consequences of special relativity

Velocity addition

Solve one-dimensional problems involving the relativistic addition of velocities.

At relativistic speeds we will use:

Option H: RelativityH4 Consequences of special relativity

relativistic velocity addition

ux’ =ux - v

1 - u v c2x

Where ux and v are signed quantities.

EXAMPLE: Spaceship B is travel- ing leftward at 0.50c wrt Earth. Spaceship A is traveling right- ward at 0.80c wrt Earth. What is the speed of A relative to B?

SOLUTION: v = -0.50c, ux = +0.80c:

● ux’ = (ux - v) / (1 - uxv/c2)

= (0.8c – -0.5c) / (1 - -0.5c 0.8c / c2)

= 1.3c / (1 + 0.4) = 0.93c.

Page 9: Option H: Relativity H4 Consequences of special relativity

Velocity addition

Solve one-dimensional problems involving the relativistic addition of velocities.

Option H: RelativityH4 Consequences of special relativity

●Use ux’ = (ux – v)/(1 – uxv/c2), where ux = 0.8c and v = -0.8c (since they are traveling in opposite directions.

●Then ux’ = (0.8c – -0.8c)/[1 – (0.8c)(-0.8c)/c2].

ux’ = 1.6c/[1 + 0.64].

ux’ = 0.98c.FYIMake sure you are consistent with your signs and that you get an answer that is LESS THAN c!

Page 10: Option H: Relativity H4 Consequences of special relativity

Velocity addition

Solve one-dimensional problems involving the relativistic addition of velocities.

Option H: RelativityH4 Consequences of special relativity

●A Galilean transformation assumes that time and length are absolute (the same in all reference frames) and fails under conditions of relativistic speeds.●A Galilean transformation simply adds velocities in a straight-forward manner according to “intuition.”

●EXAMPLE: ux’ = ux – v.

Page 11: Option H: Relativity H4 Consequences of special relativity

Velocity addition

Solve one-dimensional problems involving the relativistic addition of velocities.

Option H: RelativityH4 Consequences of special relativity

where ux = 0.9800c and v = -0.9800c (since they are traveling in opposite directions).

●Use ux’ = ux – v,

●Then ux’ = 0.98c – -0.98c = 1.960c.

Page 12: Option H: Relativity H4 Consequences of special relativity

Velocity addition

Solve one-dimensional problems involving the relativistic addition of velocities.

Option H: RelativityH4 Consequences of special relativity

●Use ux’ = (ux – v)/(1 – uxv/c2), where ux = 0.98c and v = -0.98c (since they are traveling in opposite directions.

ux’ = (0.98c – -0.98c)/[1 – (0.98c)(-0.98c)/c2]

= 1.96c/[1 + 0.982]

= 0.9998c.

Page 13: Option H: Relativity H4 Consequences of special relativity

Velocity addition

Solve one-dimensional problems involving the relativistic addition of velocities.

Option H: RelativityH4 Consequences of special relativity

●In (b)(i) v > c which is not possible.

●Thus the Galilean transformation is not applicable to this problem.

Page 14: Option H: Relativity H4 Consequences of special relativity

Mass and energy

H.4.4 State the formula representing the equivalence of mass and energy.

H.4.5 Define rest mass.

H.4.6 Distinguish between the energy of a body at rest and its total energy when it is moving.

H.4.7 Explain why no object can ever attain the speed of light in a vacuum

H.4.8 Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

Page 15: Option H: Relativity H4 Consequences of special relativity

Mass and energy

State the formula representing the equivalence of mass and energy.

●Recall E = mc2. It has been slightly changed:

●We used this formula when we looked at mass defect in nuclear energy problems. It is the energy of a mass m0 in its rest frame.

Option H: RelativityH4 Consequences of special relativity

Equivalence of mass and energy

E0 = m0c2

PRACTICE: A nuclear power plant converts about 30 kg of matter into energy each year. How many joules is this? How many watts?SOLUTION: ●E0 = m0c2 = 30(3108)2 = 2.71018 J.●P = E0/t = 2.71018/[365243600] = 8.61010 W.

Much of this energy is wasted in conversion to electrical power.

Page 16: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Define rest mass.

●It is beyond the scope of this course, but not only do time and length change with speed, but so does mass!

●We call m the relativistic mass. Recall that is the Lorentz factor, and it is instrumental in solving special relativity problems.

●We call m0 the rest mass. This is the mass of the object as measured in a reference frame in which it is at rest.

Option H: RelativityH4 Consequences of special relativity

relativistic mass

m = m0 where = 1

1 - v2/c2

FYINote that as v c that . ●Thus as v c we see that m .

Page 17: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Define rest mass.

Option H: RelativityH4 Consequences of special relativity

relativistic mass

m = m0 where = 1

1 - v2/c2

PRACTICE: At CERN a proton can be accelerated to a speed such that its relativistic mass is that of U238. How fast is it going?SOLUTION: ●First, find the Lorentz factor: m = m0

238mp = mp

= 238.●Then solve for v: (1 – v2/c2)1/2 = 1/238 1 – v2/c2 = 1/2382

1 – 1/2382 = v2/c2

0.9999823 = v2/c2 v = 0.9999912c.

Make sure you can reproduce both of these graphs.

Page 18: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Distinguish between the energy of a body at rest and its total energy when it is moving.

●Since mass increases with velocity according to m = m0, clearly the total energy of a moving mass is E = m0c2.

Option H: RelativityH4 Consequences of special relativity

relativistic energy

E0 = m0c2 where = 1

1 - v2/c2E = m0c2

PRACTICE: Show that the relativistic energy E reduces to the rest energy E0 when v = 0.SOLUTION: ●If v = 0 then = 1/(1 - 02/c2)1/2 = 1/11/2 = 1.●Then E = m0c2 = 1m0c2 = m0c2

= E0.

FYIThus E = m0c2 is the total energy of the object, whether the object is moving or not.

Page 19: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Explain why no object can ever attain the speed of light in a vacuum

●Various arguments can be presented to show that no object with a non-zero rest mass can attain the speed of light.

Option H: RelativityH4 Consequences of special relativity

EXAMPLE:

Argument 1: m as v c.●If v = c then = 1/(1 - c2/c2) = 1/0 = .●Since m = m0

then m also.

●But there is not even an infinite amount of mass in the universe. (Reductio ad absurdum).

Argument 2: E as v c.●Since E = m0c2 then as so does E.

●But there is not even an infinite amount of energy in the universe. (Reductio ad absurdum).

Page 20: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

●Recall that the acceleration of a charge e through a potential difference V produces a kinetic energy given by EK = eV.

●The total energy E of a particle of rest mass m0 is just the sum of its rest energy E0 and its kinetic energy EK = eV.

Option H: RelativityH4 Consequences of special relativity

total energy of an accelerated

particle

E = E0 + EK

where m = m0 mc2 = m0c2 + eV

FYIWe can not use (1/2)mv2 = eV at relativistic speeds to find v because it assumes all of the energy eV is going into the velocity. But the mass also changes at large speeds.

Page 21: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

●Use E = m0c2 = E0. Then

3E0 = E0 = 3.

●Since = 1/(1 – v2/c2)1/2 = 3, then(1 – v2/c2)1/2 = 1/3

1 – v2/c2 = 1/9v2/c2 = 8/9

v = 0.94c.

Page 22: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

●The mass as measured by an observer at rest with respect to the mass.●The mass as measured by an observer in the rest frame of the mass.

●From the formula we see that v V.

●Thus if V is large enough, v > c, which cannot happen.

Page 23: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

●Use E = E0 + EK.

mc2 = eV m = eV/c2

m = e(5.0106 V)/c2

m = 5.0 MeV c-2

m = (1.610-19)(5106)/(3108)2

m = 8.910-30 kg.

●Alternate method…

●Then mc2 = m0c2 + eV.mc2 - m0c2 = eV.

Page 24: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

●Use E = E0 + eV. Then

mc2 = m0c2 + eV.

m0c2 = m0c2 + eV.

= 1 + eV/(m0c2)

Page 25: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

●Use = 1 + eV/(m0c2). = 1 + e(500 MV)/(938 MeVc-2c2) = 1 + 500 MeV/(938 MeV) = 1 + 500/938 = 1.53 = 1/(1 – v2/c2)-1/2 = 1.53

1 – v2/c2 = 1/1.532 = 0.427

1 - 0.427 = v2/c2

v2 = 0.573c2

v = 0.76c.

Page 26: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

●As v c, .

●Since E = m0c2 we see that

●As , E .●Since there is not an infinite amount of energy in the universe, you cannot accelerate an object with a rest mass to the speed of light.

Page 27: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

E = E0 + EK = 0.51 MeV + 6.00 MeV = 6.51 MeV.

EK = eV = e(6.00106) V = 6.00 MeV.

(For an electron, E0 = m0c2 = 0.51 MeV.)

Page 28: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

●E = m0c2 = (0.51 MeV) = 6.51 MeV● = 6.51 MeV / 0.51 MeV = 12.17.

= 1/(1 – v2/c2)-1/2 = 12.171 – v2/c2 = 1/12.172 = 1/12.172

1 - 0.0067 = v2/c2

v2 = 0.9933c2

v = 0.997c.

Page 29: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

●Rest mass energy is E0 = m0c2 and is the energy that a particle has in its rest frame.

●Total energy is E = m0c2 + EK and is the sum of the rest mass energy and the kinetic energy EK = eV.●For these problems we always assume there is no potential energy.

Page 30: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

●E0 = m0c2 = (938 MeV c-2)c2 = 938 MeV.

Page 31: Option H: Relativity H4 Consequences of special relativity

Mass and energy

Determine the total energy of an accelerated particle.

Option H: RelativityH4 Consequences of special relativity

● = 1/(1 – v2/c2)-1/2 = 1/(1 – 0.9802c2/c2)-1/2 = 5.03.

●E = m0c2 = m0c2 + eV

eV = ( - 1)m0c2

V = ( - 1)m0c2/eV = (5.03 - 1)(938 MeV)/eV = 3780 MeV.