Astronauts in three different spaceships are communicating with each other. Those aboard ships A and B agree on the rate at
which time is passing, but they disagree with the ones on ship C.
(a) Describe the motion of the other two ships according to Alice,
who is aboard ship A.
(b) Give the description according to Betty, whose frame of reference
is ship B.
(c) Do the same for Cathy, aboard ship C.
(a) Figure g on page 19 is based on a light clock moving at a
certain speed, v. By measuring with a ruler on the figure, determine
(b) By similar measurements, find the time contraction factor γ, which equals T/t.
(c) Locate your numbers from parts a and b as a point on the graph
in figure h on page 20, and check that it actually lies on the curve.
Make a sketch showing where the point is on the curve.
This problem is a continuation of problem 2. Now imagine that
the spaceship speeds up to twice the velocity. Draw a new triangle
on the same scale, using a ruler to make the lengths of the sides
accurate. Repeat parts b and c for this new diagram.
What happens in the equation for γ
when you put in a negative
number for v? Explain what this means physically, and why it makes
(a) By measuring with a ruler on the graph in figure m on page
24, estimate the γ values of the two supernovae.
(b) Figure m gives the values of v/c. From these, compute γ values
and compare with the results from part a.
(c) Locate these two points on the graph in figure h, and make a
sketch showing where they lie.
The Voyager 1 space probe, launched in 1977, is moving faster
relative to the earth than any other human-made object, at 17,000
meters per second.
(a) Calculate the probe's γ
(b) Over the course of one year on earth, slightly less than one year
passes on the probe. How much less? (There are 31 million seconds
in a year.) p
(a) A free neutron (as opposed to a neutron bound into an
atomic nucleus) is unstable, and undergoes beta decay (which you
may want to review). The masses of the particles involved are as
neutron 1.67495 × 10-27 kg
proton 1.67265 × 10-27 kg
electron 0.00091 × 10-27 kg
antineutrino < 10-35 kg
Find the energy released in the decay of a free neutron.
(b) Neutrons and protons make up essentially all of the mass of the
ordinary matter around us. We observe that the universe around us
has no free neutrons, but lots of free protons (the nuclei of hydrogen,
which is the element that 90% of the universe is made of). We find
neutrons only inside nuclei along with other neutrons and protons,
not on their own.
If there are processes that can convert neutrons into protons, we
might imagine that there could also be proton-to-neutron conversions,
and indeed such a process does occur sometimes in nuclei
that contain both neutrons and protons: a proton can decay into a
neutron, a positron, and a neutrino. A positron is a particle with
the same properties as an electron, except that its electrical charge
is positive (see chapter 7). A neutrino, like an antineutrino, has
Although such a process can occur within a nucleus, explain why
it cannot happen to a free proton. (If it could, hydrogen would be
radioactive, and you wouldn't exist!)
(a) Find a relativistic equation for the velocity of an object in
terms of its mass and momentum (eliminating γ).
(b) Show that your result is approximately the same as the classical
value, p/m, at low velocities.
(c) Show that very large momenta result in speeds close to the speed
(a) Show that for v = (3/5)c, γ comes out to be a simple
(b) Find another value of v for which γ is a simple fraction.
An object moving at a speed very close to the speed of light
is referred to as ultrarelativistic. Ordinarily (luckily) the only ultrarelativistic
objects in our universe are subatomic particles, such
as cosmic rays or particles that have been accelerated in a particle
(a) What kind of number is γ for an ultrarelativistic particle?
(b) Repeat example 5 on page 35, but instead of very low, nonrelativistic
speeds, consider ultrarelativistic speeds.
(c) Find an equation for the ratio E/p. The speed may be relativistic,
but don't assume that it's ultrarelativistic.
(d) Simplify your answer to part c for the case where the speed is
(e) We can think of a beam of light as an ultrarelativistic object -
it certainly moves at a speed that's sufficiently close to the speed
of light! Suppose you turn on a one-watt flashlight, leave it on for
one second, and then turn it off. Compute the momentum of the
recoiling flashlight, in units of kg·m/s.
(f) Discuss how your answer in part e relates to the correspondence
As discussed in book 3 of this series, the speed at which a disturbance
travels along a string under tension is given by
where μ is the mass per unit length, and T is the tension.
(a) Suppose a string has a density ρ, and a cross-sectional area A.
Find an expression for the maximum tension that could possibly
exist in the string without producing v > c, which is impossible
according to relativity. Express your answer in terms of ρ, A, and
c. The interpretation is that relativity puts a limit on how strong
any material can be.
(b) Every substance has a tensile strength, defined as the force
per unit area required to break it by pulling it apart. The tensile
strength is measured in units of N/m2, which is the same as the
pascal (Pa), the mks unit of pressure. Make a numerical estimate
of the maximum tensile strength allowed by relativity in the case
where the rope is made out of ordinary matter, with a density on
the same order of magnitude as that of water. (For comparison,
kevlar has a tensile strength of about 4 × 109 Pa, and there is speculation
that fibers made from carbon nanotubes could have values
as high as 6 × 1010 Pa.)
(c) A black hole is a star that has collapsed and become very dense,
so that its gravity is too strong for anything ever to escape from it.
For instance, the escape velocity from a black hole is greater than
c, so a projectile can't be shot out of it. Many people, when they
hear this description of a black hole in terms of an escape velocity
greater than c, wonder why it still wouldn't be possible to extract
an object from a black hole by other means than launching it out
as a projectile. For example, suppose we lower an astronaut into a
black hole on a rope, and then pull him back out again. Why might
this not work?
The earth is orbiting the sun, and therefore is contracted
relativistically in the direction of its motion. Compute the amount
by which its diameter shrinks in this direction.