Download presentation

Presentation is loading. Please wait.

Published byRandolf Alexander Modified over 2 years ago

1
Physics 3 for Electrical Engineering Ben Gurion University of the Negev www.bgu.ac.il/atomchipwww.bgu.ac.il/atomchip, www.bgu.ac.il/nanocenterwww.bgu.ac.il/nanocenter Lecturers: Daniel Rohrlich, Ron Folman Teaching Assistants: Daniel Ariad, Barukh Dolgin Week 2. Special relativity – kinematic paradoxes addition of velocities relativistic mass and momentum relativistic energy energy-momentum 4-vector decay and scattering in relativity nuclear energy Sources: Feynman Lectures I, Chap. 15, Sects. 5-6 and Chap. 16; Tipler and Llewellyn, Chap. 1, Sect. 6 and Chap. 2, Sects. 1-4

2
The “Twin Paradox” You go out into space for one year at 0.9 of the speed of light. When you come back, how old will your twin brother be? Is there a paradox here? How would you solve it? Kinematic paradoxes

3
The “Triplet Paradox” Grumpy lives in Haifa; Dumpy and Jump live in Tel Aviv. They are identical triplets with synchronized watches. One day, Jump takes a high-speed (v = c/2) train to visit Grumpy. Grumpy and Dumpy expect Jump’s watch to run slow during the train ride. But Jump expects their watches to run slow! He reasons, “When the train left the station, I saw that my watch was still synchronized with Dumpy’s. So it was still synchronized with Grumpy’s watch. Now I am sitting and they are moving fast relative to me! So their watches must run slower than mine!” Who is right???

4
Event 1: Jump looks at his watch and at Dumpy’s watch. He sees t 1 ′ = 0 and t 1 = 0. Let their location (Tel Aviv) be x 1 ′ = x 1 = 0. Summary of Event 1: t 1 ′ = t 1 = 0, x 1 ′ = x 1 = 0. Event 2: Grumpy looks at his watch and sees t 2 = 0. Let his location (Haifa) be x 2 = 85 km. Summary of Event 2 : t 2 = 0, x 2 = 85 km.

5
Event 1: Jump looks at his watch and at Dumpy’s watch. He sees t 1 ′ = 0 and t 1 = 0. Let their location (Tel Aviv) be x 1 ′ = x 1 = 0. Summary of Event 1: t 1 ′ = t 1 = 0, x 1 ′ = x 1 = 0. Event 2: Grumpy looks at his watch and sees t 2 = 0. Let his location (Haifa) be x 2 = 85 km. Summary of Event 2 : t 2 = 0, x 2 = 85 km. Hence ∆t = t 2 – t 1 = 0, ∆x = x 2 – x 1 = 85 km.

6
Event 1: Jump looks at his watch and at Dumpy’s watch. He sees t 1 ′ = 0 and t 1 = 0. Let their location (Tel Aviv) be x 1 ′ = x 1 = 0. Summary of Event 1: t 1 ′ = t 1 = 0, x 1 ′ = x 1 = 0. Event 2: Grumpy looks at his watch and sees t 2 = 0. Let his location (Haifa) be x 2 = 85 km. Summary of Event 2 : t 2 = 0, x 2 = 85 km. Hence ∆t = t 2 – t 1 = 0, ∆x = x 2 – x 1 = 85 km. What is ∆t′ ?

7
“The barn paradox” According to the farmer, the pole fits into the barn at a single instant. But the runner cannot agree! The pole is 10 m long and the barn is only 2.5 long! The barn is 5 m long to the farmer. The pole is 10 m long to the runner and 5 m long to the farmer, i.e. we have and so v/c

8
What are the events? Event 1: the rear end of the pole reaches the entrance to the barn. Event 2: the front tip of the pole reaches the far end of the barn. In the farmer ’ s reference frame, Event 1 occurs at time t 1 and at place x 1 ; Event 2 occurs at time t 2 and at place x 2 ; t = t 2 – t 1 = 0 and x = x 2 – x 1 = 5 m. In the runner ’ s reference frame: t′ = ( t – v x/c 2 ) m c = 28.9 ns, x′ = ( x – v t) = 10 m.

9
For the runner, the two events are not simultaneous! What does it mean that t′ is negative? What are the events? Event 1: the rear end of the pole reaches the entrance to the barn. Event 2: the front tip of the pole reaches the far end of the barn.

10
What are the events? Event 1: the rear end of the pole reaches the entrance to the barn. Event 2: the front tip of the pole reaches the far end of the barn.

11
How do we derive time dilation from the Lorentz transformations? x′ = ( x – v t) y′ = y z′ = z t′ = ( t – v x/c 2 ) Further applications of Lorentz transformations

12
How do we derive time dilation from the Lorentz transformations? vtvt L c t/2 ☺ x′ = ( x – v t) y′ = y z′ = z t′ = ( t – v x/c 2 ) If Alice (primed system) moves along the x-axis with velocity v relative to Bob (unprimed system), then

13
vtvt L c t/2 ☺ For Alice, the clock stays in one place. Hence x′ = 0. x′ = ( x – v t) y′ = y z′ = z t′ = ( t – v x/c 2 ) If Alice (primed system) moves along the x-axis with velocity v relative to Bob (unprimed system), then

14
x′ = ( x – v t) Hence x = v t t′ = ( t – v x/c 2 ) ( t – v 2 t/c 2 ) t/ 2 ) t/ vtvt L c t/2 ☺ 0 = If Alice (primed system) moves along the x-axis with velocity v relative to Bob (unprimed system), then For Alice, the clock stays in one place. Hence x′ = 0.

15
x′ = ( x – v t) y′ = y z′ = z t′ = ( t – v x/c 2 ) How do we derive length contraction from the Lorentz transformations? Further applications of Lorentz transformations

16
x′ = ( x – v t) y′ = y z′ = z t′ = ( t – v x/c 2 ) If the runner (primed system) moves along the x-axis with velocity v relative to the farmer (unprimed system), then How do we derive length contraction from the Lorentz transformations?

17
x′ = ( x – v t) y′ = y z′ = z t′ = ( t – v x/c 2 ) For the farmer, x = L and t = 0. For the runner, x′ = L′. If the runner (primed system) moves along the x-axis with velocity v relative to the farmer (unprimed system), then

18
x′ = ( x – v t) = L y′ = y z′ = z t′ = ( t – v x/c 2 ) For the farmer, x = L and t = 0. For the runner, x′ = L′. L′ = If the runner (primed system) moves along the x-axis with velocity v relative to the farmer (unprimed system), then

19
Addition of velocities: u x = dx/dt ; u y = dy/dt ; u z = dz/dt u x ′= dx′/dt′ ; u y ′= dy′/dt′ ; u z ′= dz′/dt′ For inertial reference frames moving with relative velocity v along the x–axis, u x ′= (u x –v)/(1–vu x /c 2 ) u y ′= u y / (1–vu x /c 2 ) u z ′= u z / (1–vu x /c 2 ) Thus you can never surpass the speed of light e.g. by shooting a 0.9c bullet from a 0.9c jet: (0.9c+0.9c)/[1+(0.9c) · (0.9c)/c 2 ] = (1.80/1.81)c = 0.9945c

20
Derivation: apply the Lorentz transformations to the differentials, and substitute them into u x ′, u y ′ and u z ′ to obtain

21
Relativistic mass and momentum We now move from kinematics (pure description of motion) to dynamics (description of forces). We will discover that if momentum (mv) is conserved in one inertial reference frame, it is not conserved in another! But conservation of momentum is a law of physics. And Einstein postulated that the laws of physics are the same in all reference frames ….

22
uxux Two identical particles collide in their center-of-mass frame: The blue particle has mass m and speed v and so does the red particle. In the center-of-mass frame, total momentum is 0 before and after the collision. x y uyuy uyuy

23
Two identical particles collide in their center-of-mass frame: The blue particle has mass m and speed v and so does the red particle. In the center-of-mass frame, total momentum is 0 before and after the collision. But now we go to a reference frame moving to the right with speed u x : uxux x y uyuy uyuy

24
Two identical particles collide in their center-of-mass frame: The blue particle has mass m and speed v and so does the red particle. In the center-of-mass frame, total momentum is 0 before and after the collision. x y But now we go to a reference frame moving to the right with speed u x : uyuy uyuy u y ′ u x ′ = 0 uxux x y uyuy uyuy

25
Since u y ′ + u y ′ ≠ 0, the y-component of momentum is not conserved… uyuy uyuy u y ′ x y u x ′ = 0

26
Since u y ′ + u y ′ ≠ 0, the y-component of momentum is not conserved … unless we redefine momentum! uyuy uyuy u y ′ x y u x ′ = 0

27
Since u y ′ + u y ′ ≠ 0, the y-component of momentum is not conserved … unless we redefine momentum! Let ’ s try p = m f(v) v with f(0)=1. uyuy uyuy u y ′ x y u x ′ = 0

28
uy"uy" x y u y ′ u x ′ = 0 y u y " u x " = 0 x y Boost right u x Boost left u x uxux Boost right v = u x " x

29
x y u y ′ u x ′ = 0 y u y " = – u y ′ u x " = 0 x Boost right v = u x " Addition of velocities with v = u x " and : u y ′ uy"uy" uy"uy" uy"uy" vu x "/ c 2

30
and in the limit u y "→ 0 we replace u x " with v to obtain and therefore p = mγv. So now if we assume p = m f(v) v, then

31
Relativistic momentum: p = mv (or “relativistic mass”?) v/c mv / mv v/c.

32
We accelerate a body using a force F = dp/dt : Relativistic energy

33
If we accelerate the body from rest to a final speed v, we find that the change in kinetic energy of the body is For small v/c the kinetic energy is W = (γ–1) mc 2 ≈ mv 2 /2. But from W we do not learn what the total energy is. Could there really be a huge “rest energy” mc 2 ?

34
Here’s the answer: consider a head-on collision between two bodies of mass m and relativistic momentum ±mγv forming a body of mass M at rest: Momentum is conserved. Now let’s look at the collision in a frame that moves perpendicular to v with a small, nonrelativistic velocity u: From conservation of momentum in the u-direction, we have where the factor γ' differs slightly from γ = because there is a component of velocity u added to v. mm mm

35
Now divide both sides by u; in the limit u → 0 we get where γ depends only on v. We see that the body at rest having mass M contains the kinetic energy of the colliding particles! A body at rest contains energy! Since Mc 2 = 2γmc 2 the energy E of a body of mass m and speed v must equal E = γmc 2. mm

36
v

37
E = mγc 2, so E and pc form a 4-vector u = (E, pc) and (Note E and pc have the same units.) The energy-momentum 4-vector transforms like any other 4-vector under Lorentz transformations. Hence both the energy E and the momentum p are conserved in each inertial reference frame. Energy-momentum 4-vector

38
A heavy particle of mass M decays into two lighter particles of mass m. What is the velocity of each of the lighter particles? How much kinetic energy is released? Let us treat this problem in the rest frame of the heavy particle. Energy-momentum conservation: (Mc 2, 0) = (mγ 1 c 2, mγ 1 v 1 c) + (mγ 2 c 2, mγ 2 v 2 c) = (E 1, p 1 c) + (E 2, p 2 c) Hence p 1 = – p 2 and γ 1 = γ 2 = γ from momentum conservation, and Mc 2 = 2mγc 2 from energy conservation. Therefore γ = M/2m and since we get. Decay and scattering in relativity A fateful example

39
So in the rest frame of the heavy particle, the lighter particles come out back to back with opposite velocities and equal speeds There is no kinetic energy initially. The final kinetic energy is More generally, if the heavy particle decays into several lighter particles of masses m i, the kinetic energy released is

40
Application: fission of U 235 into Ba 141 and Kr 92 and also two neutrons yields how much kinetic energy? mass (a.m.u.) U 235 Ba 141 Kr 92 n 235.043923 140.914411 91.926156 1.008665 Kinetic energy yield = (235.043923 – 140.914411 – 91.926156 – 2 × 1.008665) a.m.u. × (1.660539 × 10 – 27 kg/a.m.u.) × (2.997925 × 10 8 m/s) 2 = 2.77629 × 10 – 11 J

41
One gram of U 235 contains 2.56 × 10 21 atoms of U 235, so fission of one gram of pure U 235 yields (2.56 × 10 21 ) × (2.78 × 10 – 11 J) = 7.12 × 10 10 J of kinetic energy. By way of comparison, consider two cars, each with 1500 kg mass, at speed 90 km/hour = 25 m/s, in a head-on collision. The total kinetic energy lost in the collision is (3000 kg) × (25 m/s) 2 = 1.875 × 10 6 J. So fission of one gram of U 235 has the destructive power of about 40,000 such collisions.

42
The bomb dropped on Hiroshima caused about 800 grams of U 235 to undergo fission …

43
...and about 80,000 deaths on that day, two to three times as many within five years.

44
Relativistic scattering: another fateful example Two deuterium ( 1 H 2 ) nuclei collide and produce a helium-3 ( 2 He 3 ) nucleus and a neutron. What are the velocities and energies of the helium nucleus and the neutron?

45
The easiest way to solve this problem is to go to the “center-of- momentum” frame, i.e. the inertial frame in which the total momentum is zero:

47
In this case the problem reduces to the previous problem, with the initial mass M of the decaying particle replaced by the initial energy of the two deuterium nuclei divided by c 2.

48
What is the minimum amount of kinetic energy produced by this scattering process (in the center-of-momentum frame)?

49
It is [2 × m(deuterium) – m(helium-3) – m(neutron)] × c 2

50
Note: In fission of uranium-235, the fraction of mass converted into energy is

51
In fusion of two deuterium nuclei to helium-4, it is

52
Nuclear energy: the curve of binding energy Average binding energy ∆E/A vs. mass number A

53
Nuclear energy: the curve of average nucleon mass m/Am/A Average mass of nucleon m/A vs. mass number A

Similar presentations

OK

Nuclear Fission and Fusion Unit 8 – Part B. Nuclear Balance Delicate balance between attractive strong nuclear forces and repulsive electric forces. In.

Nuclear Fission and Fusion Unit 8 – Part B. Nuclear Balance Delicate balance between attractive strong nuclear forces and repulsive electric forces. In.

© 2017 SlidePlayer.com Inc.

All rights reserved.

Ads by Google