Chapter 12: Q30P (page 537)
particle’s kinetic energy is ntimes its rest energy, what is its speed?
Short Answer
The speed is.
Chapter 12: Q30P (page 537)
particle’s kinetic energy is ntimes its rest energy, what is its speed?
The speed is.
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Get started for freeThe twin paradox revisited. On their birthday, one twin gets on a moving sidewalk, which carries her out to star X at speed ; her twin brother stays home. When the traveling twin gets to star X, she immediately jumps onto the returning moving sidewalk and comes back to earth, again at speed . She arrives on her birthday (as determined by her watch).
(a) How old is her twin brother?
(b) How far away is star X? (Give your answer in light years.) Call the outbound sidewalk system and the inbound one (the earth system is S). All three systems choose their coordinates and set their master clocks such that at the moment of departure.
(c) What are the coordinates of the jump (from outbound to inbound sidewalk) in S?
(d) What are the coordinates of the jump in ?
(e) What are the coordinates of the jump in ?
(f) If the traveling twin wants her watch to agree with the clock in , how must she reset it immediately after the jump? What does her watch then read when she gets home? (This wouldn’t change her age, of course—she’s still —it would just make her watch agree with the standard synchronization in .)
(g) If the traveling twin is asked the question, “How old is your brother right now?”, what is the correct reply (i) just before she makes the jump, (ii) just after she makes the jump? (Nothing dramatic happens to her brother during the split second between (i) and (ii), of course; what does change abruptly is his sister’s notion of what “right now, back home” means.)
(h) How many earth years does the return trip take? Add this to (ii) from (g) to determine how old she expects him to be at their reunion. Compare your answer to (a).
In classical mechanics, Newton’s law can be written in the more familiar form . The relativistic equation, , cannot be so simply expressed. Show, rather, that
where is the ordinary acceleration.
As an illustration of the principle of relativity in classical mechanics, consider the following generic collision: In inertial frame S, particle A (mass, velocity ) hits particle B (mass, velocity ). In the course of the collision some mass rubs off A and onto B, and we are left with particles C (mass, velocity ) and D (mass , velocity ). Assume that momentum is conserved in S.
(a) Prove that momentum is also conserved in inertial frame, which moves with velocity relative to S. [Use Galileo’s velocity addition rule—this is an entirely classical calculation. What must you assume about mass?]
(b) Suppose the collision is elastic in S; show that it is also elastic in .
Use the Larmor formula (Eq. 11.70) and special relativity to derive the Lienard formula (Eq. 11. 73).
In the past, most experiments in particle physics involved stationary targets: one particle (usually a proton or an electron) was accelerated to a high energy E, and collided with a target particle at rest (Fig. 12.29a). Far higher relative energies are obtainable (with the same accelerator) if you accelerate both particles to energy E, and fire them at each other (Fig. 12.29b). Classically, the energy of one particle, relative to the other, is just (why?) . . . not much of a gain (only a factor of ). But relativistically the gain can be enormous. Assuming the two particles have the same mass, m, show that
(12.58)
FIGURE 12.29
Suppose you use protons with . What do you get? What multiple of E does this amount to? [Because of this relativistic enhancement, most modern elementary particle experiments involve colliding beams, instead of fixed targets.]
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