Module 1 PDF - Relativity Notes

Chapter 37 Relativity PowerPoint® Lectures for University Physics, 14th Edition – Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow © 2016 Pearson Education Inc.  Learning Goals for Chapter 37 Looking forward at … why different...

Chapter 37 Relativity PowerPoint® Lectures for University Physics, 14th Edition – Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow © 2016 Pearson Education Inc.  Learning Goals for Chapter 37 Looking forward at … why different observers can disagree about whether two events are simultaneous. how relativity predicts that moving clocks run slow, and what experimental evidence confirms this. how the length of an object changes due to the object’s motion. how the theory of relativity modifies the relationship between velocity and momentum. some of the key concepts of Einstein’s general theory of relativity. © 2016 Pearson Education Inc.  Introduction At Brookhaven National Laboratory in New York, atomic nuclei are accelerated to 99.995% of the ultimate speed limit of the universe— the speed of light, c. It is impossible for any object to travel at or beyond c. We shall see some of the far-reaching implications of relativity, such as the effect of motion on time and length. We’ll see that momentum and kinetic energy must be redefined. © 2016 Pearson Education Inc.  Einstein’s first postulate Einstein’s first postulate, known as the principle of relativity, states that the laws of physics are the same in every inertial reference frame. For example, the same emf is induced in the coil whether the magnet moves relative to the coil, or the coil moves relative to the magnet. © 2016 Pearson Education Inc.  Einstein’s second postulate Einstein’s second postulate is that the speed of light in vacuum is the same in all inertial frames of reference and is independent of the motion of the source. Suppose two observers measure the speed of light in vacuum. One is at rest with respect to the light source, and the other is moving away from it. According to the principle of relativity, the two observers must obtain the same result, despite the fact that one is moving with respect to the other. © 2016 Pearson Education Inc.  Relative velocity of slow-moving objects © 2016 Pearson Education Inc.  Relative velocity of light © 2016 Pearson Education Inc.  The Galilean transformation The Galilean transformation is a transformation between two inertial frames of reference. In the figure, and the equations below, the position of particle P is described in two frames of reference. © 2016 Pearson Education Inc.  A thought experiment in simultaneity: Slide 1 of 4 Imagine a train moving with a speed comparable to c, with uniform velocity. Two lightning bolts strike a passenger car, one near each end. © 2016 Pearson Education Inc.  A thought experiment in simultaneity: Slide 2 of 4 Stanley is stationary on the ground at O, midway between A and B. Mavis is moving with the train at in the middle of the passenger car, midway between and. © 2016 Pearson Education Inc.  A thought experiment in simultaneity: Slide 3 of 4 Mavis runs into the wave front from before the wave front from catches up to her. Thus she concludes that the lightning bolt at struck before the one at. © 2016 Pearson Education Inc.  A thought experiment in simultaneity: Slide 4 of 4 The two wave fronts from the lightning strikes reach Stanley at O simultaneously, so Stanley concludes that the two bolts struck B and A simultaneously. Whether or not two events at different locations are simultaneous depends on the state of motion of the observer. © 2016 Pearson Education Inc.  Relativity of time intervals Let’s consider another thought experiment. Mavis, in frame S', measures the time interval between two events. Event 1 is when a flash of light from a light source leaves O'. Event 2 is when the flash returns to O', having been reflected from a mirror a distance d away. The flash of light moves a total distance 2d, so the time interval is: © 2016 Pearson Education Inc.  Relativity of time intervals The round-trip time measured by Stanley in frame S is a longer interval Δt; in his frame of reference the two events occur at different points in space. © 2016 Pearson Education Inc.  Time dilation and proper time Let Δt0 be the proper time between two events. An observer moving with constant speed u will measure the time interval to be Δt, where where the Lorentz factor γ is defined as: © 2016 Pearson Education Inc.  The Lorentz factor When u is very small compared to c, γ is very nearly equal to 1. If the relative speed u is great enough that γ is appreciably greater than 1, the speed is said to be relativistic. © 2016 Pearson Education Inc.  Proper time Proper time is the time interval between two events that occur at the same point. A frame of reference can be pictured as a coordinate system with a grid of synchronized clocks, as in the figure at the right. © 2016 Pearson Education Inc.  Relativity of length We attach a light source to one end of a ruler and a mirror to the other end. The ruler is at rest in reference frame S', and its length in this frame is l0. © 2016 Pearson Education Inc.  Relativity of length In reference frame S the ruler is moving to the right with speed u. The length of the ruler is shorter in S. © 2016 Pearson Education Inc.  Length contraction and proper length A length measured in the frame in which the body is at rest (the rest frame of the body) is called a proper length. Thus l0 is a proper length in S', and the length measured in any other frame moving relative to S is less than l0. This effect is called length contraction. © 2016 Pearson Education Inc.  Example of length contraction The speed at which electrons traverse the 3-km beam line of the SLAC National Accelerator Laboratory is slower than c by less than 1 cm/s. As measured in the reference frame of such an electron, the beam line (which extends from the top to the bottom of this photograph) is only about 15 cm long! © 2016 Pearson Education Inc.  Lengths perpendicular to the direction of motion There is no length contraction for lengths perpendicular to the direction of relative motion. © 2016 Pearson Education Inc.  The Lorentz transformations This Galilean transformation, as we have seen, is valid only in the limit when u approaches zero. The more general relationships are called the Lorentz transformations. © 2016 Pearson Education Inc.  The Lorentz transformations for coordinates The Lorentz transformations relate the coordinates and velocities in two inertial reference frames. They are more general than the Galilean transformations and are consistent with the principle of relativity. © 2016 Pearson Education Inc.  The Lorentz transformations for velocities The Lorentz velocity transformations show us that a body moving with a speed less than c in one frame of reference always has a speed less than c in every other frame of reference. © 2016 Pearson Education Inc.  Doppler effect for electromagnetic waves When a source moves toward the observer, the observed frequency f is greater than the emitted frequency f0. © 2016 Pearson Education Inc.  Doppler effect for electromagnetic waves This handheld radar gun emits a radio beam of frequency f0, which in the frame of reference of an approaching car has a higher frequency f. The reflected beam also has frequency f in the car’s frame, but has an even higher frequency f ' in the police officer’s frame. The radar gun calculates the car’s speed by comparing the frequencies of the emitted beam and the doubly Doppler-shifted reflected beam. © 2016 Pearson Education Inc.  Relativistic momentum Shown is a graph of the magnitude of the momentum of a particle of rest mass m as a function of speed v. Also shown is the Newtonian prediction, p = mv, which gives correct results only at speeds much less than c. © 2016 Pearson Education Inc.  Relativistic momentum Suppose we measure the mass of a particle to be m when it is at rest relative to us: We call m the rest mass. When such a particle has a velocity v, its relativistic momentum is: We can rewrite this in terms of the Lorentz factor of the particle’s rest frame with respect to the rest frame of the system: © 2016 Pearson Education Inc.  Relativistic work and energy Graph of the kinetic energy of a particle of rest mass m as a function of speed v. Also shown is the Newtonian prediction, which gives correct results only at speeds much less than c. © 2016 Pearson Education Inc.  Relativistic energy and rest energy The relativistic kinetic energy is: Note that the kinetic energy approaches infinity as the speed approaches the speed of light. The rest energy is mc2. © 2016 Pearson Education Inc.  Relativistic energy and momentum The total energy of a particle is: The total energy, rest energy, and momentum are related by: © 2016 Pearson Education Inc.  The general theory of relativity Objects in the space station seem to be weightless, but without looking outside the station there is no way to determine whether gravity has been turned off or whether the station and all its contents are accelerating toward the center of the earth. If we cannot distinguish experimentally between a uniform gravitational field at a particular location and a uniformly accelerated reference frame, then there cannot be any real distinction between the two. In the general theory of relativity the geometric properties of space are affected by the presence of matter. © 2016 Pearson Education Inc.  What happens when an astronaut drops her watch? In gravity-free space, the floor accelerates upward at a = g and hits the watch. © 2016 Pearson Education Inc.  What happens when an astronaut drops her watch? On the earth’s surface, the watch accelerates downward at a = g and hits the floor. © 2016 Pearson Education Inc.  A two-dimensional representation of curved space © 2016 Pearson Education Inc.