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Electromagnetic Fields and Waves: Including Electric Circuits

Paul Lorrain, Dale R. Corson

Chapter 15

Relativity Iii - all with Video Answers

Educators


Chapter Questions

04:48

Problem 1

(15.3) Burning hydrogen
You ignite a mixture of hydrogen and oxygen inside a closed vessel, and then allow the water vapor to cool.
Sketch graphs of $m c^{2}$ and of $m_{0} c^{2}$ as functions of time.

Jennifer Hudspeth
Jennifer Hudspeth
Numerade Educator
01:42

Problem 2

(15.3) Relativistic effects with 40 -GeV electrons
A linear accelerator accelerates electrons up to energies of 40 gigaelectronvolts ( $40 \times 10^{4}$ electronvolts).
(a) Calculate the mass of an electron that has the full energy. How does this mass compare with that of a proton at rest? See the page facing the back cover.
(b) What is the length of the accelerator in the reference frame of an electron that has the full energy? The length of the accelerator, as measured on the ground, is 3000 meters.
(c) How much time would such an electron take to go from one end of the accelerator to the other (i) in the laboratory frame and (ii) in the electron's frame of reference?
(a) $d m=\gamma\left(1+v_{x}^{\prime} \frac{\mathscr{V}{c}}{c^{2}}\right) d m^{\prime}$,
(b) $d \tau=\frac{d \tau^{\prime}}{\gamma\left(1+v_{x}^{\prime} V / c^{2}\right)^{\prime}}$
(c) $\rho=\gamma^{2}\left(1+\frac{v_{x}^{\prime} \eta}{c^{2}}\right)^{2} \rho^{\prime}, \quad \rho^{\prime}=\gamma^{2}\left(1-\frac{v_{x}}{c^{2}}\right)^{2} \rho$.

Zulfiqar Ali
Zulfiqar Ali
Numerade Educator
04:30

Problem 2

(15.3) Relativistic effects with $40-\mathrm{GeV}$ electrons
A linear accelerator accelerates electrons up to energies of 40 gigaelectronvolts (40 $\times 10^{4}$ electronvolts).
(a) Calculate the mass of an electron that has the full energy. How does this mass compare with that of a proton at rest? See the page facing the back cover.
(b) What is the length of the accelerator in the reference frame of an electron that has the full energy? The length of the accelerator, as measured on the ground, is 3000 meters.
(c) How much time would such an electron take to go from one end of the accelerator to the other (i) in the laboratory frame and (ii) in the electron's frame of reference?

Nathan Prins
Nathan Prins
Numerade Educator
01:41

Problem 3

(15.6) Transformation of a mass density
We use the symbol $\tau$ for a volume in this problem.
A small element in an object has a proper mass $d m_{0}$, a proper volume $d \tau_{0}$, and a proper mass density $\rho_{0}=d m_{0} / d \tau_{0}$. With respect to $S$ and $S^{\prime}$ the mass densities are $\rho=d m / d \tau$ and $\rho^{\prime}=d m^{\prime} / d \tau^{\prime}$, respectively, and the velocities of the element are $v$ and $v^{\prime}$.
Show that, if $\boldsymbol{V}$ is the speed of $S^{\prime}$ with respect to $S$, then (a) $d m=\gamma\left(1+v_{x}^{\prime} \frac{\mathscr{V}{c}}{}\right) d m^{\prime}$,
(b) $d \tau=\frac{d \tau^{\prime}}{\gamma\left(1+v_{x}^{\prime} \mathcal{V} / c^{2}\right)^{\prime}}$
(c) $\rho=\gamma^{2}\left(1+\frac{v_{x}^{\prime} q}{c^{2}}\right)^{2} \rho^{\prime}, \quad \rho^{\prime}=\gamma^{2}\left(1-\frac{v_{x} \eta}{c^{2}}\right)^{2} \rho$.

Narayan Hari
Narayan Hari
Numerade Educator
02:54

Problem 4

(15.5) The relativistic force
In classical mechanics, $\boldsymbol{F}=m a$ if the mass is constant. Show that with relativity,
$$
\boldsymbol{F}=\frac{m_{0}}{\left(1-v^{2} / c^{2}\right)^{3 / 2}} a_{1}+\frac{m_{0}}{\left(1-v^{2} / c^{2}\right)^{1 / 2}} a_{\perp}=\gamma^{2} m a_{1}+m a_{\perp}
$$
where $a_{\|}$and $a_{\perp}$ are the components of the acceleration that are, respectively, parallel and perpendicular to the velocity $v$ of the point of application of the force.

A force that is perpendicular to $v$ changes the direction of $v$, but not the mass, and hence not the speed, as we could expect because the force does no work. Then, if $\boldsymbol{F}$ is perpendicular to $\boldsymbol{v}, \boldsymbol{F}=m \boldsymbol{a}$ applies!

However, a force parallel to $v$ changes the magnitude of $v$ and hence the mass also. The resistance to acceleration is larger because of the $\gamma^{2}$ term.
The quantity $m$ is sometimes called the transverse inertial mass, and $\gamma^{2} m$ the longitudinal inertial mass.

Chai Santi
Chai Santi
Numerade Educator
02:06

Problem 5

(15.7) The gravitational red shift
A photon of energy $h v_{0}$ leaves the surface of a star of radius $R$ and mass $M$
(a) Show that, after the photon has escaped to infinity, $\Delta v / v_{0}$ is equal to $G M /\left(R c^{2}\right)$, where $G$ is the gravitational constant. This change is so small that you can set $v=v_{0}$ in your calculation of the change in potential energy. What is the sign of $\Delta v ?$ This change of frequency is the gravitational red shift.
(b) Calculate $\Delta v / v$ for the sun and for the earth. See the page facing the back cover.
(c) Calculate $\Delta v / v$ for a photon that travels from the surface of the sun to the surface of the earth, taking into account both gravitational fields.
(d) Sirius and a smaller star revolve around each other. The mass of the smaller star is about equal to that of the sun, but its light has a $\Delta v / v$ of $7 \times 10^{-4}$, What is its average density?
(e) The period of rotation of the sun is $24.7$ days. What is the Doppler shift for 500 -nanometer light emitted from the edge of the sun's disk, at its equator? Compare this Doppler shift with the gravitational red shift.
(f) The sun ejects ionized hydrogen. How does the mass of a proton vary as it flies away from the sun?

Suzanne W.
Suzanne W.
Numerade Educator
02:18

Problem 6

(15.8) The mass of a high-energy proton
A proton has a kinetic energy of 500 million electronvolts. Find its mass and velocity.

Zulfiqar Ali
Zulfiqar Ali
Numerade Educator
04:21

Problem 7

(15.9) The conservation laws for colliding particles
In the course of a collision between two particles there is conservation of energy and conservation of momentum.
(a) Show that, if these conservation laws apply in one inertial reference frame, then they apply in any other inertial frame.
(b) Show that if, in a given reaction, relativistic mass is conserved in all inertial frames, then $\boldsymbol{p}$ is also conserved, and inversely.

Suzanne W.
Suzanne W.
Numerade Educator
08:24

Problem 8

(15.10) Transformation of a force Show that
$$
\boldsymbol{F}=\boldsymbol{F}_{\mathrm{i}}^{\prime}+\gamma\left[\frac{\boldsymbol{V} \times\left(\boldsymbol{F}^{\prime} \times \boldsymbol{V}\right)}{\mathcal{V}^{2}}-\frac{\boldsymbol{v} \times\left(\boldsymbol{F}^{\prime} \times \boldsymbol{V}\right)}{c^{2}}\right]
$$

Eduard Sanchez
Eduard Sanchez
Numerade Educator
06:19

Problem 9

(15.10) Force and power
Starting from Eq. 15-17, show that
$$
\boldsymbol{F} \cdot \boldsymbol{v}=\frac{d \mathscr{E}}{d t}
$$

Gopesh Vishwakarma
Gopesh Vishwakarma
Numerade Educator
05:49

Problem 10

$(15.11)$ The ultimate spaceship
The thrust of a spaceship engine is equal fo the product $m^{\prime} v$, where $m^{\prime}$ is the mass of propellant ejected per second and $v$ is the exhaust velocity with respect to the ship. The ultimate spaceship would transform all its propellant into radiation and eject photons backward at the speed of light. The mass of the propellant would then be minimum.
(a) Show that the power-to-thrust ratio $P / F$ for a photon engine is $c$.
Since $P / F$ and $d M / d t$ are independent of the frequency, the source of radiation need not be monochromatic.
(b) Then a photon ship burning 1 gram of matter per second would have a thrust of $3 \times 10^{5}$ newtons. The difficulty is to transform an appreciable fraction of the propellant mass into radiation, as the following example will show.

An ordinary flashlight has a capacity of about 2 ampere-hours at about 2 volts. Show that its terminal velocity is of the order of $10^{-4}$ meter/second.

Zachary Warner
Zachary Warner
Numerade Educator
02:42

Problem 11

(15.11) Is interstellar travel possible?
(a) First, time should be dilated by, say, a factor of 10 . Then $\gamma=10$. Calculate $v / c$.
(b) Imagine a spaceship equipped with a photon motor. See Prob. 15-10. You can find the fraction $f$ of the initial mass that remains, after the ship has attained the proper $\beta$, from the conservation of energy and the conservation of momentum. Take into account the energy and momentum of the radiation. You should find that $f=0.05$.
The spaceship must then brake to a stop. This requires $95 \%$ of the remaining mass. At the end of the return trip we are left with $(0.05)^{4}=$ $6.25 \times 10^{-6}$ of the initial mass. If the mass of the ship and its payload is 1 ton, then the propellant has a mass of about 200,000 tons.
(c) In principle, the spaceship could collect and annihilate interstellar matter. There is about one atom of hydrogen per cubic centimeter.

Calculate the mass of hydrogen collected during 1 year if the ship sweeps out a volume 1000 square meters in cross-section at the speed of light,
(d) Now this hydrogen must first be brought up to speed. This slows the ship. Show that the net gain is positive up to $\beta=0.707$ and negative afterward.

Elan Stopnitzky
Elan Stopnitzky
Numerade Educator
00:55

Problem 12

(15.11) The Doppler effect again
Refer to Fig. 14-7. An observer at the origin $O$ of the reference frame $S$ measures the frequency of a source of electromagnetic radiation situated at the origin $O^{\prime}$ of $S^{\prime}$. In Prob. 14-9 we found that $f=\gamma f^{\prime}\left(1+\beta \cos \theta^{\prime}\right)$.
Check this equation by transforming the four-momentum of a photon.

Farhanul Hasan
Farhanul Hasan
Numerade Educator
03:43

Problem 13

(15, 11$)$ The Mössbauer effect
An excited nucleus of ${ }^{57}$ Fe formed by the radioactive decay of ${ }^{57}$ Co emits a gamma ray of $1.44 \times 10^{4}$ electronvolts. In the process, there is conservation of energy and $m_{0} c^{2}=m_{0} c^{2}+h v$, where $m_{0}$ is the initial mass of the nucleus and $m_{\alpha}$ is its mass after the emission of the gamma ray. There is also conservation of momentum, $h v / c=m_{\sigma} u$, where $u$ is the recoil velocity of the iron nucleus. Let $m_{\text {oil }}$ be the rest mass of the nucleus after the reaction. Then the energy released by the reaction is $E=\left(m_{0}-m_{0 a}\right) c^{2}$.
(a) Rewrite the first equation after subtracting $h v$ on both sides, and square. Then square the second equation and substitute. You should find that
$$
h v=\frac{\mathscr{E}\left(m_{0}+m_{u 11}\right)}{2 m_{0}}=\left(1-\frac{\delta}{2 m_{0} c^{2}}\right) \mathscr{E}
$$
So $h v<\mathscr{:}$ part of $\varepsilon$ goes to the photon, and the other part supplies kinetic energy to the recoiling nucleus.
(b) Set $m_{0}=57 \times 1.7 \times 10^{-23}$, and show that $\mathcal{E} /\left(2 m_{0} c^{2}\right)=1.3 \times 10^{-7}$, Thus the fraction of the available energy $\varepsilon$ that appears as recoil is small.
(c) Mossbauer discovered in 1958 that, with solid iron, a significant fraction of the atoms recoil as if they were locked rigidly to the rest of the solid. This is the Mössbauer effect. If the sample has a mass of 1 gram, by what fraction is the gamma ray energy shifted in the recoil process?
(d) A sample of normal ${ }^{57}$ Fe absorbs gamma rays of $14.4$ kiloelectronvolts by the inverse recoilless process much more strongly than it absorbs gamma rays of any nearby energy. The excited nuclei thus formed reemit 14.4-kiloelectronvolt radiation in random directions some time later. This is resonant scattering.

If a sample of activated ${ }^{57} \mathrm{Fe}$ moves in the direction of a sample of normal ${ }^{57} \mathrm{Fe}$, what must be the value of the velocity $v$ that will shift the frequency of the gamma rays, as seen by the normal nuclei, by 3 parts in $10^{13}$ ? This is one line width.
(e) A Doppler shift in the gamma ray results in a much lower absorption by a nucleus if the shift is of the order of one line width or more. What happens to the counting rate of a gamma-ray detector placed behind the sample of normal ${ }^{57}$ Fe when the source of activated ${ }^{57}$ Fe moves (i) toward the normal $^{57} \mathrm{Fe}$, (ii) away from it?
(f) If a $14.4$-kiloelectronvolt gamma ray travels $22.5$ meters vertically upward, by what fraction will its energy decrease?
(g) A normal ${ }^{57} \mathrm{Fe}$ absorber located at this height must move in what direction and at what speed in order for resonant scattering to occur?

Salamat Ali
Salamat Ali
Numerade Educator