CHAPTER 28 SPECIAL RELATIVITY

OpenStax College Physics Instructor Solutions Manual Chapter 28 CHAPTER 28: SPECIAL RELATIVITY 28.2 SIMULTANEITY AND TIME DILATION (a) What is  if v 0.250c ? (b) If v 0.500c ? Solution (a) Using the definition of  , where v 0.250c :  1/  1/  v2   (0.250c)   1   1  1.0328  c2  c    (b) Again using the definition of  , now where v 0.500c :  (0.500c)    1   c2    1/ 1.1547 1.15 (a) What is  if v 0.100c ? (b) If v 0.900c ? Solution  (0.100c)   1  1.00504  c   (a) Showing three digits difference from  1/  (0.900c)    1   c2   (b)  1/ 2.294 2.29 Particles called  -mesons are produced by accelerator beams If these particles travel 8 at 2.70 10 m/s and live 2.60 10 s when at rest relative to an observer, how long they live as viewed in the laboratory? Solution  v2   (2.70 108 m/s)  γ 1   1  2.294, so that 2  c   (3.00 10 m/s)  Δt γΔt (2.294)(2 60 10  s) 5.96 10  s Suppose a particle called a kaon is created by cosmic radiation striking the 8 atmosphere It moves by you at 0.980c , and it lives 1.24 10 s when at rest relative  1/2  1/2 to an observer How long does it live as you observe it? Solution  1/  1/  v2   (0.980c)   1    1  5.025, so that  c2  c    Δt γΔt (5.025)(1.24 10  s) 6.23 10  s OpenStax College Physics Instructor Solutions Manual Chapter 28 A neutral  -meson is a particle that can be created by accelerator beams If one such  16  16 particle lives 1.40 10 s as measured in the laboratory, and 0.840 10 s when at rest relative to an observer, what is its velocity relative to the laboratory? Solution  v2  Δt 1.40 10  16 s    Δt Δt  γ    1.667  Δt 8.40 10  17 s  c   1 v c1    γ  1/   c 1  2  (1.67)   1/2  1 v2  c2 γ2 1/ 0.800c A neutron lives 900 s when at rest relative to an observer How fast is the neutron moving relative to an observer who measures its life span to be 2065 s? Solution  v2   1   t t  c  Using , where   1/  v  t 2065 s  2.2944 1   t 900 s  c  , we see that:  1/ 1  c2  v2  c2      c  c  v2  Squaring the equation gives c2 c2  v2   , and solving for speed finally gives: Cross-multiplying gives  c2  v  c  c1       1/   c 1    (2.2944)  1/ 0.90003c 0.900c If relativistic effects are to be less than 1%, then  must be less than 1.01 At what relative velocity is  1.01 ? Solution  v2  γ 1    c  If relativistic effects are to be less than 3%, then  must be less than 1.03 At what relative velocity is  1.03 ? Solution  v2  γ 1    c  (a) At what relative velocity is  1.50 ? (b) At what relative velocity is  100 ?  1/  1/    v c1         v c1      1/ 1/   c 1    (1.01)  1/   c 1    (1.03)  0.140c 1/ 0.240c OpenStax College Physics Solution Instructor Solutions Manual  v2  γ 1    c  (a)  1/   v  1    (100)  (b)    v c1      1/ Chapter 28    1    (1.50)  1/ 0.745c 1/ 0.99995c (to five digits to show difference from c.) 10 (a) At what relative velocity is  2.00 ? (b) At what relative velocity is  10.0 ? Solution  v2  γ 1    c  (a)  1/    v c1        v  1    (10.0)  (b) 11 Solution 1/   1  2  ( 2.00)  1/ 0.866c 1/ 0.995c Unreasonable Results (a) Find the value of  for the following situation An Earthbound observer measures 23.9 h to have passed while signals from a high-velocity space probe indicate that 24.0 h have passed on board (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent? t t , (a) Using the equation we can solve for  : t 23.9 h   0.9958 0.996 t 24.0 h (b)  cannot be less than (c) The earthbound observer must measure a longer time in the observer’s rest frame than the ship bound observer The assumption that time is longer in the moving ship is unreasonable 28.3 LENGTH CONTRACTION 12 A spaceship, 200 m long as seen on board, moves by the Earth at 0.970c What is its length as measured by an Earth-bound observer? Solution  (0.970 c)  L 200 m 1     L   200 m  v  1/ c2   (1  ) c 13 How fast would a 6.0 m-long sports car have to be going past you in order for it to appear only 5.5 m long? 1/ 48.6 m OpenStax College Physics Solution L Chapter 28 L0 L 6.0 m    1.0909, so that  L 5.5 m  v2  γ 1    c  14 Instructor Solutions Manual  1/    v c1      1/   c 1    (1.0909)  1/ 0.400c (a) How far does the muon in Example 28.1 travel according to the Earth-bound observer? (b) How far does it travel as viewed by an observer moving with it? Base your calculation on its velocity relative to the Earth and the time it lives (proper time) (c) Verify that these two distances are related through length contraction γ = 3.20 Solution Using the values given in Example 28.1: L0 vt (0.950c)( 4.87 10  s) (a) (0.950c )( 2.998 10 m/s )( 4.87 10  s) 1.386 10 m 1.39 km 6 (b) L0 vt (0.950c)( 2.998 10 m/s )(1.52 10 s) 4.329 10 m 0.433 km L0 1.386 10 m L  4.33 10 m 0.433 km γ 3.20 (c) 15 (a) How long would the muon in Example 28.1 have lived as observed on the Earth if its velocity was 0.0500c ? (b) How far would it have traveled as observed on the Earth? (c) What distance is this in the muon’s frame? Solution All answers are reported to significant figures to show the differences:  1/  1/  v2   (0.0500c)  γ 1    1  1.00125  c2  c    (a) Δt  γΔt (1.00125)( 1.52 10  s) 1.5219 10  s 1.522 10  s 6 (b) L0 vt (0.0500c)t (0.0500)( 2.998 10 m/s )(1.5219 10 s) 22.81 m 6 (c) L vt (0.0500)( 2.998 10 m/s )(1.52 10 s) 22.78 m 16 (a) How long does it take the astronaut in Example 28.2 to travel 4.30 ly at 0.99944c (as measured by the Earth-bound observer)? (b) How long does it take according to the astronaut? (c) Verify that these two times are related through time dilation with γ = 30.00 as given Solution (a) Δt  L0 4.30 ly 4.30 y   4.303 y v 0.9994c 0.9994 , to four digits to show any effect OpenStax College Physics (b) (c) 17 L Instructor Solutions Manual Chapter 28 L0 4.30 ly L 0.1433 ly  0.1433 ly, so that Δt   0.1434 y γ 30.0 v 0.99944c Δt  γΔt  γ  Δt 4.303 y  30.0 Δt 0.1434 y (a) How fast would an athlete need to be running for a 100- m race to look 100 yd long? (b) Is the answer consistent with the fact that relativistic effects are difficult to observe in ordinary circumstances? Explain Solution (a) (100 m)(1.0937 yd/m) 109.37 yd , and since L L 109.37 yd L  γ  1.0937 γ L 100 yd  1/ 1/ 1/  v2      γ 1    v c1   c 1  0.405c      c   (1.0937)  This is definitely a world record! (b) Yes, the foot racer would need to travel at extraordinary speeds in order to observe a length contraction of this size; therefore it is difficult to observe relativistic effects in ordinary circumstances 18 Unreasonable Results (a) Find the value of  for the following situation An astronaut measures the length of her spaceship to be 25.0 m, while an Earth-bound observer measures it to be 100 m (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent? Solution (a) γ L0 25.0 m  0.250 L 100 m (b)  must be 1 (c) The earthbound observer must measure a shorter length, so it is unreasonable to assume a longer length 19 Unreasonable Results A spaceship is heading directly toward the Earth at a velocity of 0.800c The astronaut on board claims that he can send a canister toward the Earth at 1.20c relative to the Earth (a) Calculate the velocity the canister must have relative to the spaceship (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent? Solution v  u u   u ; u 1.20c; v 0.800c   v  u v  u   (vu / c ) c  (a) Using  , solving for u: OpenStax College Physics Instructor Solutions Manual Chapter 28 u v vu  vu  u  10.0c u  v u1   u v  u   (uv/c ) c  c  and so that (b) The resulting speed of the canister is greater than c, an impossibility (c) It is unreasonable to assume that the canister will move toward the earth at 1.20c u 28.4 RELATIVISTIC ADDITION OF VELOCITIES 20 Suppose a spaceship heading straight towards the Earth at 0.750c can shoot a canister at 0.500c relative to the ship (a) What is the velocity of the canister relative to the Earth, if it is shot directly at the Earth? (b) If it is shot directly away from the Earth? Solution v  u 0.750c  0.500c u  0.909c / c )  (0.750c)(0.500c ) / c  ( v u (a) 0.750c  0.500c u 0.400c    ( 750 c )(  500 c ) / c (b) 21 Repeat the previous problem with the ship heading directly away from the Earth Solution v  u  0.750c  0.500c u   0.400c / c )  ( 0.750c)(0.500c) / c  ( v u (a)  0.750c  0.500c u  0.909c    (  750 c )(  500 c ) / c (b) 22 If a spaceship is approaching the Earth at 0.100c and a message capsule is sent toward it at 0.100c relative to the Earth, what is the speed of the capsule relative to the ship? Solution v  u u  (vu / c ) , we can add the relativistic velocities: Using the equation     v  u 0.100c  0.100c u  0.198c  (vu / c )  (0.100c)( 0.100c ) / c  23  (a) Suppose the speed of light were only 3000 m/s A jet fighter moving toward a target on the ground at 800 m/s shoots bullets, each having a muzzle velocity of 1000 m/s What are the bullets’ velocity relative to the target? (b) If the speed of light was this small, would you observe relativistic effects in everyday life? Discuss OpenStax College Physics Instructor Solutions Manual Chapter 28 Solution v  u 800 m/s  1000 m/s u  1653 m/s 1.65 km/s /c )  (800 m/s)(1000 m/s)/(3000 m/s)  ( v u (a) (b) Yes, if the speed of light were this small, speeds that we can achieve in everyday life would be larger than 1% of the speed of light and we could observe relativistic effects much more often 24 If a galaxy moving away from the Earth has a speed of 1000 km/s and emits 656 nm light characteristic of hydrogen (the most common element in the universe) (a) What wavelength would we observe on the Earth? (b) What type of electromagnetic radiation is this? (c) Why is the speed of the Earth in its orbit negligible here? Solution  λobs λs   u/c  (10 m/s)/(3 108 m/s) (656 nm) 658 nm  u/c  (10 m/s)/(3 108 m/s) (a) (b) The radiation is visible red light  r  (1.496 1011 m) v  2.97 10 m/s t 3.16 10 s (c) , so v 2.97 10 m/s  9.92 10  c 2.998 10 m/s , which is negligible 25 Solution A space probe speeding towards the nearest star moves at 0.250c and sends radio information at a broadcast frequency of 1.00 GHz What frequency is received on the Earth? c f , so f obs  f s  u/c  0.250 (1.00 Ghz) 0.7746 Ghz 775 Mhz  u/c  0.250 26 If two spaceships are heading directly towards each other at 0.800c , at what speed must a canister be shot from the first ship to approach the other at 0.999c as seen by the second ship? Solution v  u u v 0.800c, u 0.999c Find u  Starting with  (vu /c ) , we get: uv u v 0.999 c  0.800 c u  u  v  u   u   0.991c c  (uv/c )  [(0.999 c)(0.800 c)/c ] 27 Two planets are on a collision course, heading directly towards each other at 0.250c A spaceship sent from one planet approaches the second at 0.750c as seen by the second planet What is the velocity of the ship relative to the first planet? Solution v 0.250c, u 0.750c Find u  OpenStax College Physics Instructor Solutions Manual Chapter 28 v  u u v 0.750c  0.250c u  u   0.615 c 2  (vu /c )  (uv/c )  [(0.750c)(0.250 c)/c ] 28 When a missile is shot from one spaceship towards another, it leaves the first at 0.950c and approaches the other at 0.750c What is the relative velocity of the two ships? Solution v  u uu  u u  v v  u ' u ' 0.950c, u 0.750c Starting with  (vu / c ) , c and u  u 0.950c  0.750c v   0.696c (uu / c )  (0.750c)(0.950c) / c    The velocity v is the speed measured by the second spaceship, so the minus sign indicates the ships are moving apart from each other ( v is in the opposite direction as u ) 29 What is the relative velocity of two spaceships if one fires a missile at the other at 0.750c and the other observes it to approach at 0.950c ? Solution u ' 0.750c, u 0.950c Find v v  u u u 0.750c  0.950c u  v  0.696c 2  (vu / c ) (uu / c )  (0.750c)( 0.950c) / c    The velocity v is the speed measured by the second spaceship, so the ships are moving towards each other ( v is in the same direction as u ) 30 Solution Near the center of our galaxy, hydrogen gas is moving directly away from us in its orbit about a black hole We receive 1900 nm electromagnetic radiation and know that it was 1875 nm when emitted by the hydrogen gas What is the speed of the gas? λobs  u/c 1900 nm   1.0133 So λs  u/c 1875 nm (1.0133)  1  u / c (1.0133) (1  u / c )  u / c  1.324 10   u 0.01324c (1.0133)  31 A highway patrol officer uses a device that measures the speed of vehicles by bouncing radar off them and measuring the Doppler shift The outgoing radar has a frequency of 100 GHz and the returning echo has a frequency 15.0 kHz higher What is the velocity of the vehicle? Note that there are two Doppler shifts in echoes Be certain not to round off until the end of the problem, because the effect is small OpenStax College Physics Solution Instructor Solutions Manual Chapter 28 f obs  u/c  u/c  f obs  f s fs  u/c At the vehicle,  u/c For the echo returning to the  u/c   f s f obs  u/c where the velocities of sources officer, we have a similar equation: are positive in both cases because the source is always moving away from the f f f  u/c  u/c  u/c f s  f obs , then obs  obs obs   fs f s f s  u/c  u/c  u/c observer Since Therefore,  /f s  f obs f  f  1.50 10 Hz u c c s obs (2.998 108 m/s)  22.5 m/s  /f s   f obs f s  f obs 2.00 1011 Hz  1.50 10 Hz The vehicle is therefore travelling at a speed of 22.5 m/s toward the highway patrol officer 32 Prove that for any relative velocity v between two observers, a beam of light sent from one to the other will approach at speed c (provided that v is less than c , of course) Solution u c , so u v  u vc v c c (v  c )    c 2 c v  (vu / c )  (vc / c )  (v / c) 33 Show that for any relative velocity v between two observers, a beam of light projected by one directly away from the other will move away at the speed of light (provided that v is less than c , of course) Solution v  u v c v c c (v  c ) u     c 2 c v  (vu / c )  (vc / c )  (v / c) u  c , so  Similarly u c  u c 34 (a) All but the closest galaxies are receding from our own Milky Way Galaxy If a galaxy 12.0 109 ly away is receding from us at 0.900c , at what velocity relative to us must we send an exploratory probe to approach the other galaxy at 0.990c , as measured from that galaxy? (b) How long will it take the probe to reach the other galaxy as measured from the Earth? You may assume that the velocity of the other galaxy remains constant (c) How long will it then take for a radio signal to be beamed back? (All of this is possible in principle, but not practical.) Solution Note that all answers to this problem are reported to significant figures, to distinguish the results OpenStax College Physics Instructor Solutions Manual Chapter 28 v  u uv , so u  u  v  u  and  (vu / c ) c u v 0.990c  ( 0.900c) u   0.99947c  (uv / c )  [(0.990c)(  0.900c) / c ] u (a) (b) When the probe reaches the other galaxy, it will have traveled a distance (as seen d  x0  vt on Earth) of because the galaxy is moving away from us As seen from d x  vt t  u u Earth, u 0.9995c , so x0 12.0 109 ly (1 y)c   1.2064 1011 y u t  x0  vt  u  v 0.99947 c  0.900 c ly Now, and (c) The radio signal travels at the speed of light, so the return time t  is given by t d x  vt  , c c assuming the signal is transmitted as soon as the probe reaches the other galaxy Using the numbers, we can determine the time: 1.20 1010 ly  (0.900c)(1 2064 1011 y) t  1.2058 1011 y c t  28.5 RELATIVISTIC MOMENTUM 35 Solution  27 Find the momentum of a helium nucleus having a mass of 6.68 10 kg that is moving at 0.200c p mu   36 Solution 1  u / c2  (6.68 10  27 kg)(0.200)(3.00 108 m/s) 1   (0.200 c) /c  4.09 10  19 kg m/s What is the momentum of an electron traveling at 0.980c ? p mu   37 mu mu 1  u / c2  (9.11 10  31 kg)(0.980)(3.00 108 m/s) 1   (0.980 c) /c  1.35 10  21 kg m/s (a) Find the momentum of a 1.00 10 kg asteroid heading towards the Earth at 30.0 km/s (b) Find the ratio of this momentum to the classical momentum (Hint: OpenStax College Physics Instructor Solutions Manual Chapter 28 2 Use the approximation that  1  (1 / 2)v / c at low velocities.) Solution p mu  (a) mu 1  u / c2    (1.00 10 kg)(30.0 10 m/s) 1  (3.00 10 m/s) / 3.00 108 m/s   3.000000015 1013 kg m/s pc mu 1.00 109 kg (3.00 10 m/s) 3.00 1013 kg m/s, so (b) 38 p 1.000000005 pc (a) What is the momentum of a 2000 kg satellite orbiting at 4.00 km/s? (b) Find the ratio of this momentum to the classical momentum (Hint: Use the approximation 2 that  1  (1 / 2)v / c at low velocities.) Solution (a) For low velocities we can use the approximation  1  u2 c2  u2   mu p mu     2c  u3 (0.5) 2000 kg   4.00 10 m/s  mu  m (2000 kg) 4.00 10 m/s   c 3.00 108 m/s  8.00 10 kg m/s  7.11 10  kg m/s 8.00 10 kg m/s (b) The classical momentum, mu , is just the first term above, pc 8.00 10 kg m/s p 8.00 10 kg.m/s  7.111 10  kg m/s  pc 8.00 10 kg m/s 1  39 7.11 10  kg m/s 1  8.89 10  11 8.00 10 kg m/s  21 What is the velocity of an electron that has a momentum of 3.04 10 kg m/s ? Note that you must calculate the velocity to at least four digits to see the difference from c Solution p mu  Beginning with the equation mu 1  u c2  we can solve for the speed u OpenStax College Physics Instructor Solutions Manual Chapter 28 1 u m2  2u c2 p First cross-multiply and square both sides, giving p2 u   m / p   1 / c  m   p / c  Then, solving for u gives p u   m2  p2 / c2 Finally, taking the square root gives Taking the values for the mass of the electron and the speed of light to five significant figures gives: 3.04 10  21 kg m/s u 1/2  9.1094 10  31 kg   3.34 10  21 kg m/s /  2.9979 108 kg  2      2.988 10 m/s  40 Solution   19 Find the velocity of a proton that has a momentum of 4.48 10 kg m/s mu p mu   u2 u 2     p  u / c m u 1  u / c   m   p / c   p 2 2  u p m   p 2 / c2  (4.48 10  19 kg m/s) 1.67 10  27 kg     (4.48 10  19 kg m/s) / 3.00 10 m/s   1.9997 10 m/s 2.00 10 m/s 41 (a) Calculate the speed of a 1.00 - g particle of dust that has the same momentum as a proton moving at 0.999c (b) What does the small speed tell us about the mass of a proton compared to even a tiny amount of macroscopic matter? Solution (a) For the proton: mu p 1 u / c2 (1.673 10  27 kg)(0.999)(2.998 108 m/s)  1.12110  17 kg m/s  (0.999) p 1.121 10 -17 kg m/s  1.12110  m/s 9 1.00 10 kg So, for the particle: m Thus, OpenStax College Physics u Instructor Solutions Manual pm   p / mc 1.121 10  m/s  Chapter 28   1.121 10  m/s 2.998 10 m/s  1.12 10  m/s (b) The small speed tells us that the mass of a proton is substantially smaller than that of even a tiny amount of macroscopic matter! 42 (a) Calculate  for a proton that has a momentum of 1.00 kg m/s (b) What is its speed? Such protons form a rare component of cosmic radiation with uncertain origins Solution p mu  u  (a) u  u / c   p 1.00 kg m/s  5.977 10 26 m/s  27 m 1.673 10 kg 2  p  u   u   1   m  c  Now,  pc / m  so u2  2 c   p / m  u Finally,  p/m   p / mc    (5.977 10 26 m/s)  5.977 10 26 m/s 2.998 10 m/s   2.998 10 m/s p 5.997 10 26 m/s  1.99 1018 mu 2.998 10 m/s 8 (b) As found in part (a), u 2.998 10 m/s 3.00 10 m/s c 28.6 RELATIVISTIC ENERGY 43 Solution  31 What is the rest energy of an electron, given its mass is 9.11 10 kg ? Give your answer in joules and MeV E mc 9.11 10  31 kg 3.00 10 m/s   MeV  8.20 10  14 J 8.20 10  14 J   0.512 MeV  13  1.60 10 J  (according to the number of sig fig stated The exact value is closer to 0.511 MeV.) 44 Find the rest energy in joules and MeV of a proton, given its mass is 1.67 10 Solution E mc 1.67 10  27 kg 3.00 10 m/s  1.50310  10 J  MeV  1.50310  10 J   939 MeV  13  1.60 10 J   27 kg OpenStax College Physics 45 Solution Instructor Solutions Manual Chapter 28 If the rest energies of a proton and a neutron (the two constituents of nuclei) are 938.3 and 939.6 MeV respectively, what is the difference in their masses in kilograms? E mc E mc  E  939.6 MeV  938.3 MeV 1.60 10  13 J/MeV  2.3 10  30 kg 2 c 3.00 10 m/s  To two digits since the difference in rest mass energies is found to two digits m  46 Solution 47 68 The Big Bang that began the universe is estimated to have released 10 J of energy How many stars could half this energy create, assuming the average star’s mass is 4.00 1030 kg ? E   0.500 1.00 10 68 J    5.5610 50 kg 2   c  3.00 10 m/s   50 M 5.56 10 kg   1.39 10 20 30 m 4.00 10 kg E Mc  M  31 44 A supernova explosion of a 2.00 10 kg star produces 1.00 10 kg of energy (a) How many kilograms of mass are converted to energy in the explosion? (b) What is the ratio m / m of mass destroyed to the original mass of the star? Solution E mc  m  (a)    E 1.00 10 44 J  c2 3.00 10 m/s  1.111 10 27 kg 1.11 10 27 kg m 1.111 10 27 kg  5.56 10  5.56 10  31 2.00 10 kg (b) m 48 (a) Using data from Table 7.1, calculate the mass converted to energy by the fission of 1.00 kg of uranium (b) What is the ratio of mass destroyed to the original mass, m / m ? Solution (a) From Table 7.1, the energy released from the nuclear fission of 1.00 kg of uranium 13 is E 8.0 10 J So, E  E released mc , we get 8.0 1013 J  8.89 10  kg 0.89 g E  c 3.00 10 m/s  (b) To calculate the ratio, simply divide by the original mass: m 8.89 10  kg   8.89 10  8.9 10  m 1.00 kg   m  OpenStax College Physics 49 Instructor Solutions Manual Chapter 28 (a) Using data from Table 7.1, calculate the amount of mass converted to energy by the fusion of 1.00 kg of hydrogen (b) What is the ratio of mass destroyed to the original mass, m / m ? (c) How does this compare with m / m for the fission of 1.00 kg of uranium? Solution E mc2  m  (a) 6.4 1014 J  7.110 kg E  c 3.00 108 m/s 2 m 7.11 10 -3 kg  7.1 10  7.1 10  kg (b) m m (c) m is greater for hydrogen 50 34 There is approximately 10 J of energy available from fusion of hydrogen in the 33 world’s oceans (a) If 10 J of this energy were utilized, what would be the decrease in mass of the oceans? Assume that about 0.08% of the mass of a water molecule is converted to energy during the fusion of hydrogen (b) How great a volume of water does this correspond to? (c) Comment on whether this is a significant fraction of the total mass of the oceans Solution 1�1033 J   E E  mc � m   �  1.39 �1019 kg �1�1019 kg c 0.0008  3.00 �10 m/s  (a) � m3 � 16 16 V   1.39 �1019 kg  � � 1.39 �10 m �1�10 m 1000 kg � � (b) (c) Since approximately 2/3 of the surface of the earth is covered with water, the surface area of water on Earth is: 2 Asurface  4r  π6.376 10 m  3.411014 m 3 So the volume of water found in part (b) would be equivalent to a thickness of V 1.39 �1016 m t   4.07 �101 m �41 m 14 A 3.41 � 10 m water of: Therefore, no, this mass is not a significant fraction of the total mass of the oceans 51 A muon has a rest mass energy of 105.7 MeV, and it decays into an electron and a massless particle (a) If all the lost mass is converted into the electron’s kinetic energy, find  for the electron (b) What is the electron’s velocity? OpenStax College Physics Solution Instructor Solutions Manual Chapter 28 m  c (  1)me c  m  (  1)me me  me   m   me me (a)  1  (v / c ) 2 105.7 MeV  0.511 MeV  207.85 208 0.511 MeV 1/  1/ (b)    v c1        c 1  2   207.85  1/ 0.999988c (six digits used to show difference from c.) 52 A  -meson is a particle that decays into a muon and a massless particle The  meson has a rest mass energy of 139.6 MeV, and the muon has a rest mass energy of 105.7 MeV Suppose the  -meson is at rest and all of the missing mass goes into the muon’s kinetic energy How fast will the muon move? Solution KE rel mc ( m  m  )c (  1) m c Solving for  will give us a way of calculating the speed of the muon From the equation above, we see that: m  m m  m   m  m 139.6 MeV  1    1.32072 m m m 105.7 MeV 1 v2  , c  so 2 Now, use  1  v c  or 1 v c  c  0.6532c  (1.32072) 1 53 (a) Calculate the relativistic kinetic energy of a 1000-kg car moving at 30.0 m/s if the speed of light were only 45.0 m/s (b) Find the ratio of the relativistic kinetic energy to classical Solution     v c (a) 2  1   30.0 m/s    1     45.0 m/s    1/2 1.342; KE   1 mc  0.3421000 kg  45.0 m/s  6.92 10 J KE KE c  mv (0.5)(1000 kg)(30.0 m/s) 4.50 10 J; 1.54 KE c (b) 54 Alpha decay is nuclear decay in which a helium nucleus is emitted If the helium  27 nucleus has a mass of 6.80 10 kg and is given 5.00 MeV of kinetic energy, what is its velocity? OpenStax College Physics Solution Instructor Solutions Manual KE    1 mc  mc KE  mc    Chapter 28 KE  mc mc 2  5.00 MeV 1.60 10  13 J/MeV  6.80 10  27 kg 3.00 108 m/s   6.80 10     v c 55 2  1  27  kg 3.00 108 m/s    v c1      1/    c 1  2  1.0013  1.0013; 1/ 0.0511c (a) Beta decay is nuclear decay in which an electron is emitted If the electron is given 0.750 MeV of kinetic energy, what is its velocity? (b) Comment on how the high velocity is consistent with the kinetic energy as it compares to the rest mass energy of the electron Solution KE   1 mc  KE  mc  mc  0.750 MeV 1.60 10  13 J/MeV   9.11 10 (a)  31  9.11 10  31 kg 3.00 10 m/s  kg 3.00 10 m/s   2 2.4636;     v c 2  1    v c1      1/   c 1     2.4636  1/ 0.914c (b) The rest mass energy of an electron is 0.511 MeV, so the kinetic energy is approximately 150% of the rest mass energy The electron should be traveling close to the speed of light 56 A positron is an antimatter version of the electron, having exactly the same mass When a positron and an electron meet, they annihilate, converting all of their mass into energy (a) Find the energy released, assuming negligible kinetic energy before the annihilation (b) If this energy is given to a proton in the form of kinetic energy, what is its velocity? (c) If this energy is given to another electron in the form of kinetic energy, what is its velocity? Solution 2  31  13 (a) E mc 2me c (2)(9.11 10 kg)(3.00 10 m/s) 1.64 10 J OpenStax College Physics Instructor Solutions Manual KE    1 mc    KE  mc mc 1.64 10 J   1.67 10 kg 3.00 10  1.67 10 kg 3.00 10 m/s   13 - 27 - 27     v c 2  1 (b) 1/  27  27 57 m/s  1.00109;   c 1  2   2.4636  1.64 10 J   1.67 10 kg 3.00 10  1.67 10 kg 3.00 10 m/s   13 8    v c1         v c 1  2  3.00   (c) Chapter 28 m/s  1/ 0.0467c 3.00 1/ 0.943c  16 What is the kinetic energy in MeV of a -meson that lives 1.4010 s as measured  16 in the laboratory, and 0.84010 s when at rest relative to an observer, given that its rest energy is 135 MeV? Solution  1.667 from the result of Exercise 28.5 Thus, KE    1 mc (1.667  1)(135 MeV) 90.0 MeV 58 Find the kinetic energy in MeV of a neutron with a measured life span of 2065 s, given its rest energy is 939.6 MeV, and rest life span is 900s Solution From Exercise 28.6, we know that  = 2.2944, so we can determine the kinetic energy of the neutron: KE rel (  1)mc  2.2944  1 939.6 MeV 1216 MeV 59 2 2 (a) Show that ( pc ) /( mc )   This means that at large velocities pc  mc (b) Is E  pc when  30.0 , as for the astronaut discussed in the twin paradox? Solution   pc    2   (a) E  p c  m c  m c , so that p c   1m c and mc pc  30.0    899   29.98  E  pc mc (b) Yes: , to within part in 2 2 2 1  4 E  pc   5.56 10  899  , Since 60 2 mc  1 2  pc  2   mc      pc 1     pc   One cosmic ray neutron has a velocity of 0.250c relative to the Earth (a) What is the OpenStax College Physics Instructor Solutions Manual Chapter 28 neutron’s total energy in MeV? (b) Find its momentum (c) Is E  pc in this situation? Discuss in terms of the equation given in part (a) of the previous problem Solution v 0.250c    2  E 1 v c (a) E mc , where so E (0.250) E p mc   243 MeV/c c c (b) 1   0.250  (939 MeV) 970 MeV (c) No This is true when pc  mc which is not the case for this situation Here pc  mc 61 What is  for a proton having a mass energy of 938.3 MeV accelerated through an effective potential of 1.0 TV (teravolt) at Fermilab outside Chicago? Solution KE qV (  1) mc so that qV  mc mc 1.60 10  19 C1.00 1012 V  1.60 10  13 J/MeV  938.3 MeV 1.07 10   938.3 MeV γ  62  (a) What is the effective accelerating potential for electrons at the Stanford Linear Accelerator, if  1.00 10 for them? (b) What is their total energy (nearly the same as kinetic in this case) in GeV? Solution    KE (  1)mc  1.00 10  9.11 10  31 kg 3.00 10 m/s KE qV  V  (a)  8.199 10  J KE 8.199 10  J  5.12 1010 V 51.2GV q 1.60 10  19 C  GeV  E mc  1.00 10  0.511 MeV  51.1 GeV 1000 MeV   (b)  63  (a) Using data from Table 7.1, find the mass destroyed when the energy in a barrel of crude oil is released (b) Given these barrels contain 200 liters and assuming the density of crude oil is 750 kg/m , what is the ratio of mass destroyed to original mass, m / m ? Solution E mc  m  (a)   E 5.90 109 J  c2 3.00 108 m/s   6.5610  kg OpenStax College Physics Instructor Solutions Manual Chapter 28 3 (b) m  200 L  1 m /1000 L 750 kg/m  150 kg Δm 4.37 10  10 Therefore, m 64 (a) Calculate the energy released by the destruction of 1.00 kg of mass (b) How many kilograms could be lifted to a 10.0 km height by this amount of energy? Solution 16 16 (a) E released mc 1.00 kg   2.998 10 m/s  8.988 10 J 8.99 10 J m (b) 65 PE 8.99 1016 J  9.17 1011 kg gh 9.80 m/s 10.0 10 m  A Van de Graaff accelerator utilizes a 50.0 MV potential difference to accelerate charged particles such as protons (a) What is the velocity of a proton accelerated by such a potential? (b) An electron? Solution KE qV (  1)mc qV  mc mc 1.60 10  19 C 5.00 10 V MeV 1.60 10  13 J/MeV   938.3 MeV   938.3 MeV 1.0532 γ        v c 2  1 (a) 1.60 10   19     v c1         1/   c 1  2  1.0532   1/ 0.314c  C 5.00 10 V MeV 1.60 10  13 J/MeV   0.511 MeV  0.511 MeV 98.85   v c 1  2   98.85  (b) 1/ 0.99995c (Five digits used to show difference from c ) 66 Suppose you use an average of 500 kW h of electric energy per month in your home (a) How long would 1.00 g of mass converted to electric energy with an efficiency of 38.0% last you? (b) How many homes could be supplied at the 500 kW h per month OpenStax College Physics Instructor Solutions Manual Chapter 28 rate for one year by the energy from the described mass conversion? Solution (a) The monthly energy use is  500 kW h  3600 s/hr  1.80 10 J -3 13 The energy available is  0.381.00 10 kg 3.00 10 m/s  3.42 10 J 3.42 1013 J 1.9 10 month 1.58 103 years Thus, 1.8 10 J/month (b) 1.58 10 homes 67 (a) A nuclear power plant converts energy from nuclear fission into electricity with an efficiency of 35.0% How much mass is destroyed in one year to produce a continuous 1000 MW of electric power? (b) Do you think it would be possible to observe this mass loss if the total mass of the fuel is 10 kg ? Solution  3600s  24h  365.24d   3.156 1016 J 0.350mc E 1000 10 J/s    1h 1d 1y     (a) E 3.1561016 J  m  1.00 kg 0.350c  0.350 3.00 10 m/s  (b) This much mass would be measurable, but probably not observable just by looking because it is 0.01% of the total mass 68 Nuclear-powered rockets were researched for some years before safety concerns became paramount (a) What fraction of a rocket’s mass would have to be destroyed to get it into a low Earth orbit, neglecting the decrease in gravity? (Assume an orbital altitude of 250 km, and calculate both the kinetic energy (classical) and the gravitational potential energy needed.) (b) If the ship has a mass of 1.00 10 kg (100 tons), what total yield nuclear explosion in tons of TNT is needed? OpenStax College Physics Solution Instructor Solutions Manual Chapter 28 r rE  rO 6.37 10 m  2.50 10 m 6.62 10 m  mv  GMm  r  KE  2r  2r  6.67 10  11 N m /kg 5.98 10 24 kg 1.00 10 kg  3.012 1012 J  2(6.62 10 m) PE mgrO 1.00 10 kg 9.80 m/s  2.50 10 m  2.45 1011 J; E tot KE  PE 3.257 1012 J E mc  m  (a) E 3.257 1012 J  3.618 10  kg c 3.00 10 m/s  Δm 3.618 10  kg  3.62 10  10 m 1.00 10 kg Thus, 3.257 1012 J 775 tons of TNT (b) 4.20 10 J/tonTNT 69 26 The Sun produces energy at a rate of 4.00 10 W by the fusion of hydrogen (a) How many kilograms of hydrogen undergo fusion each second? (b) If the Sun is 90.0% hydrogen and half of this can undergo fusion before the Sun changes character, how long could it produce energy at its current rate? (c) How many kilograms of mass is the Sun losing per second? (d) What fraction of its mass will it have lost in the time found in part (b)? Solution 4.00 10 26 J/s 6.25 1011 kg/s 6.3 1011 kg/s 14 (a) 6.4 10 J/kg 30 18  0.450 1.99 10 11 kg 1.431018 s  1.43 10 s 4.5 1010 y 6.25 10 kg 3.153610 s/y (b) E mc  m  (c) (d) 70 Solution 4.44 10 E 4.00 10 26 J  4.44 10 kg 2 c 3.00 10 m/s    kg/s 1.43 1018 s 0.32% 1.99 1030 kg  27 Unreasonable Results A proton has a mass of 1.67 10 kg A physicist measures the proton’s total energy to be 50.0 MeV (a) What is the proton’s kinetic energy? (b) What is unreasonable about this result? (c) Which assumptions are unreasonable or inconsistent? (a) E mc , so that  E 50.0 MeV  0.0532 938.3 MeV mc OpenStax College Physics Instructor Solutions Manual  Chapter 28  KE    1 mc  9.47 10   938.3 MeV  888.3 MeV (b) The kinetic energy, KE, must be greater than or equal to Here it is negative (c) The proton’s total energy must be mc 938.3 MeV This file is copyright 2016, Rice University All Rights Reserved  ... College Physics Instructor Solutions Manual Chapter 28 v  u u v 0.750c  0.250c u  u   0.615 c 2  (vu /c )  (uv/c )  [(0.750c)(0.250 c)/c ] 28 When a missile is shot from one spaceship...  v2  γ 1    c  (a)  1/   v  1    (100)  (b)    v c1      1/ Chapter 28    1    (1.50)  1/ 0.745c 1/ 0.99995c (to five digits to show difference from c.)... in order for it to appear only 5.5 m long? 1/ 48.6 m OpenStax College Physics Solution L Chapter 28 L0 L 6.0 m    1.0909, so that  L 5.5 m  v2  γ 1    c  14 Instructor Solutions