(Relativistic invariance / Scalar
product / Momentum of a photon)
In this section, Feynman
discusses relativistic invariance, scalar product of
four-vectors, and momentum of a photon (an exception of four-vector).
1. Relativistic invariance:
“...complete the
law of conservation of momentum by extending it to include the time component. This is absolutely
necessary to go with the other three, or there cannot be relativistic
invariance (Feynman et al., 1963, section 17–5 Four-vector algebra).”
According to Feynman,
we must complete the law of conservation of momentum by extending it to include
the conservation of energy (time component) to
obtain a valid four-vector relationship in the space-time geometry. That is, it
is absolutely necessary to have four components
of momentum such that there is relativistic invariance. We can define
relativistic invariance (or Lorentz invariance) in terms of a four-vector aμ under a Lorentz transformation
whereby at′2−ax′2−ay′2−az′2 = at2−ax2−ay2−az2. In chapter 16, Feynman explains that “the conservation of mass which we have deduced above is equivalent to
the conservation of energy” in the context of collisions within the special theory
of relativity. In a sense, this implies that we have a single principle
involving the conservation of momentum, mass, and energy.
In Volume II, Feynman adds that “the quantity which is analogous
to r2 for three dimensions, in
four dimensions is t2−x2−y2−z2. It is an invariant under
what is called the “complete Lorentz group”—which means for transformation of
both translations at constant velocity and rotations
(Feynman et al., 1964, section 25–2 The scalar
product).” He also discusses the four-velocity vector with components vx = dx/dt, vy =
dy/dt, vz =
dz/dt, and mentions that an incorrect guess of the time component is vt = dt/dt = 1. It turns out that the four “velocity”
components that we have written down also have an invariant quantity (the speed
of light) if we include the proper time t in all denominators (cdt/dt, dx/dt, dy/dt, dz/dt). The
invariant quantity of the four-velocity can be calculated easily using (cdt/dt)2 – (dv/dt)2 = g2(c2 – v2) = c2.
2. Scalar
product:
“if aμ is one four-vector and bμ is another four-vector, then
the scalar product is S′aμbμ = atbt−axbx−ayby−azbz. It is the same in all
coordinate systems (Feynman et al., 1963, section 17–5 Four-vector algebra).”
Feynman states the
notations that are used for a scalar product (or inner product) in terms of S′μAμAμ = At2−Ax2−Ay2−Az2. The prime on S′ means that the first term, the “time” term, is
positive, but the other three terms have minus signs. This invariant quantity
is the same in any coordinate system (or inertial frame), and we may call it
the square of the length (or norm) of a four-vector. In addition, Feynman (1964)
mentions that “the only real complication is the notation.” However, some authors complicate the situation by changing the sign of all
the terms and state the square of the length of the four-vector as +ax2+ay2+az2−at2. Alternatively, one may state Saμ2 =
+ax2+ay2+az2+at2 in which all have the same signs, and define at in
terms of ict instead of ct (i
is an imaginary number).
Feynman elaborates
that the square of the length of a four-vector momentum of a single particle is
equal to pt2−px2−py2−pz2, or in short, E2−p2. He says that
the invariant quantity must be the same in every coordinate system (or inertial
frame) and it is purely its energy, which is the same as its rest mass. In
other words, the norm of the four-momentum vector is equal to m02c4 (i.e., E2−p2c2 =m02c4) and the invariant quantity can be stated as rest energy instead of rest mass. In
essence, we may save time in problem-solving if we use the four-momentum vector
with a scalar product (relativistic invariant) that is the same in all inertial frames of reference. Simply put, the
knowledge of an invariant quantity allows us to choose an inertial frame in
which a problem can be solved more easily.
3. Momentum
of a photon:
“Such a photon
also carries a momentum, and the momentum of a photon (or of any other
particle, in fact) is h divided by the
wavelength: p = h/λ (Feynman
et al., 1963, section 17–5
Four-vector algebra).”
Feynman ends
the chapter by discussing the momentum of a photon. This is an interesting
example because the rest mass of a photon is zero. Thus, the equation E2−p2c2 = m02c4 can be simplified as E2−p2c2 = 0 or E = pc. However, Feynman could mention
that the momentum of any (massless) particle is equal to its total energy times
its velocity (p = vE/c2) can be reduced to E = p if c = 1. More importantly, physics teachers should
explain that the equations E = gm0c2 and p = gm0v are not really useful for massless particles because m0 = 0 and g approaches infinity for objects moving at the speed of light (i.e., E and p are not equal to zero). The energy of a photon would change and
this is related to the relativistic Doppler effect that is elaborated later in the
section 34–6 The Doppler effect (Feynman et al., 1963).
Feynman
mentions that the rest mass of a photon is zero and ask whether
the photon’s energy is zero using the formula m0/√(1−v2) instead of E = gm0c2. He adds that the photon really can have energy even though it has
no rest mass, but it possesses energy by always moving at the speed of light. In
Volume II, Feynman states that “the energy E0 has the relativistic mass E0/c2 the photon has a mass (not rest mass) ℏω0/c2, and is ‘attracted’ by the earth (Feynman et al., 1964, section 42–6 The speed of clocks in a gravitational field).” On the other hand, from an interpretation of
Meissner effect, “[t]he photon
mass inside a conventional superconductor is 10–11 proton masses, or less (Wilczek, 2008, p. 213).” It is good to end the chapter by discussing a special case (or
exception) of four-vector using the momentum of a photon.
Questions for discussion:
1. How would you
define the concept of relativistic invariance?
2. Would you define the scalar product of
a four-vector that has the same sign or opposite signs?
3. How would you explain the mass and momentum of a photon?
The moral of the lesson: the relativistic
invariance of a four-vector aμ is related to the principle
of the conservation of momentum, mass, and energy.
References:
1. Feynman, R. P., Leighton, R. B., & Sands, M. (1963). The Feynman Lectures on Physics, Vol I: Mainly mechanics, radiation, and
heat. Reading, MA: Addison-Wesley.
2. Feynman,
R. P., Leighton, R. B., & Sands, M. (1964). The Feynman Lectures on Physics, Vol II:
Mainly
electromagnetism and matter. Reading, MA: Addison-Wesley.
3. Wilczek, F.
(2008). The lightness of being: Mass, ether, and the unification of forces.
New York: Basic Books.
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