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* 'Phe electrons would actually win the race versus 0¿s2ble light because of the index of |
refraction of air. A gamma ray would make out better. |
--- Trang 300 --- |
paperl When the electrons are going that fast their masses are enormous, but |
their speed cannot exceed the speed oŸ light. |
Now let us look at some further consequences of relativistic change of mass. |
Consider the motion of the molecules in a small tank of gas. When the gas |
is heated, the speed of the molecules is increased, and therefore the mass 1s |
also increased and the gas is heavier. An approximate formula to express the |
Increase of mass, for the case when the velocity is small, can be found by |
expanding mo/1 — 02/c2 = mọ(1 — 02/c2)~1⁄2 in a power series, using the |
binomial theorem. We get |
mạ(1L— t2/cÈ) 8 = mạ(1 + }08/cÊ + 304/et +), |
W© see clearly from the formula that the series converges rapidly when 0 is small, |
and the terms after the first two or three are negligible. So we can write |
~ 1 s( 1 |
m nọ + srnoU 2 (15.11) |
in which the second term on the ripght expresses the increase of mass due to |
molecular velocity. When the temperature inereases the ø2 increases proportion- |
ately, so we can say that the increase in mass is proportional to the increase |
in temperature. But since singu? 1s the kinetic energy in the old-fashioned |
Newtonian sense, we can also say that the increase In mass of all this body of gas |
is equal to the inerease in kinetic energy divided by e2, or Am = A(K.B.)/€2. |
15-9 Equivalence of mass and energy |
The above observation led Einstein to the suggestion that the mass of a body |
can be expressed more simply than by the formula (15.1), if we say that the mass |
is equal to the total energy content divided by c2. If Eq. (15.11) is multiplied |
by c? the result is |
mcŸ = mạc” + 3m0” + - -- (15.12) |
Here, the term on the left expresses the total energy oŸ a body, and we recognize |
the last term as the ordinary kinetic energy. Einstein interpreted the large |
constant term, ?moe2, to be part of the total energy of the body, an intrinsic |
energy known as the “rest energy.” |
Let us follow out the consequences of assuming, with Einstein, that ứhe |
energu oƒ a bod aluas eguals mc2. As an interesting result, we shall find the |
--- Trang 301 --- |
formula (15.1) for the variation of mass with speed, which we have merely assumed |
up to now. W© start with the body at rest, when its energy is mọc”. Then we |
apply a force to the body, which starts it moving and gives it kinetic energy; |
therefore, since the energy has increased, the mass has increased——this is Implieit |
in the original assumption. So long as the force continues, the energy and the |
mass both continue to increase. We have already seen (Chapter 13) that the rate |
of change of energy with time equals the force times the velocity, or |
—— —= È'`-0. 15.13 |
di ° 5.13) |
W© also have (Chapter 9, Eq. 9.1) that ' = d(mo)/dt. When these relations are |
put together with the delnition of , Eq. (15.13) becomes |
d(mc2) d(mb) |
————=U'—.. 15.14 |
dc ””” đ 5.14) |
We wish to solve this equation for ?mm. To do this we first use the mathematical |
trick of multiplying both sides by 2mm, which changes the equation to |
đm d(ựm?®) |
2m) —— = 2m0 - ———. 15.15 |
cm) d‡ TT ' ) |
W© need to get rid of the derivatives, which can be accomplished by integrating |
both sides. The quantity (2m) đưm/đf can be recognized as the từne derivative |
of m2, and (2m0) - d(mo) /dt is the tỉme derivative of (mø)2. So, Eq. (15.15) is |
the same as (m2) (m202) |
d(m d(m“u |
———=—.. 15.16 |
“— dị di (15.16) |
Tf the derivatives of two quantities are equal, the quantities themselves differ at |
most by a constant, say Œ. 'Phis permits us to write |
m°c? = m?u° + Œ. (15.17) |
W© necd to delne the constant Œ more explicitly. Since Eq. (15.17) must be true |
for all velocities, we can choose a special case where ø = 0, and say that in this |
case the mass is mo. Substituting these values into Eq. (15.17) gives |
mặc? =0+ Œ. |
--- Trang 302 --- |
W© can now use thịs value of Ở in Eq. (15.17), which becomes |
mỸc2 = mm 2u” + mặc”. (15.18) |
Dividing by e? and rearranging terms gives |
mÊ(1 — 0Ê/c2) = mã, |
from which we get |
m = mo/W1— 02/c2. (15.19) |
This is the formula (15.1), and is exactly what is necessary for the agreement |
between mass and energy in Eq. (15.12). |
Ordinarily these energy changes represent extremely slight changes in mass, |
because most of the time we cannot generate much energy from a given amount |
of material; but in an atomie bomb of explosive energy equivalent to 20 kilotons |
of NT, for example, it can be shown that the dirt after the explosion is lighter |
by 1 gram than the initial mass of the reacting material, because of the energy |
that was released, I.e., the released energy had a mass of l1 gram, according to |
the relationship AE = A(mc2). Thịis theory of equivalence of mass and energy |
has been beautifully verified by experiments in which matter is annihilated—— |
convcrted totally to energy: An electron and a positron come together at rest, |
cach with a rest mass mmọ. When they come together they disintegrate and bwo |
øamma rays emerge, each with the measured energy of mọc2. This experiment |
furnishes a direct determination of the energy associated with the existence of |
the rest mass of a particle. |
--- Trang 303 --- |
I6 |
Miolqfitisfic Freorgjgg «areeÏ WẤC@rtt©reftrrtt |
16-1 Relativity and the phỉilosophers |
In this chapter we shall continue to discuss the principle of relativity of |
Binstein and Poincaré, as it afects our ideas of physics and other branches of |
human thought. |
Poincaré made the following statement of the principle of relativity: “Ac- |
cording to the principle of relativity, the laws of physical phenomena must be |
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