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no force at this point, and so it is the equilibrium point. Another way to see |
that it is the equilibrium poïnt is that it takes work to move away from đin |
either direction. When the two oxygen atoms have settled down, so that no more |
--- Trang 275 --- |
U(r) œ 1/rŠ |
(IF r> đ) |
Fig. 14-3. The potential energy between two atoms as a function of |
the distance between them. |
energy can be liberated from the force between them, they are in the lowest |
energy state, and they will be at this separation d. 'This is the way an oxygen |
mmolecule looks when it is cold. When we heat it up, the atoms shake and move |
farther apart, and we can in fact break them apart, but to do so takes a certain |
amount of work or energy, which is the potential energy difference bebween r = đ |
and r = œ. When we try to push the atoms very close together the energy goes |
up very rapidly, because they repel each other. |
The reason we bring this out is that the idea of force is not particularly |
suitable for quantum mechanics; there the idea of energw is most natural. We fnd |
that although forces and velocities “dissolve” and disappear when we consider |
the more advanced forces between nuclear matter and between molecules and so |
on, the energy concept remains. 'Pherefore we fnd curves of potential energy In |
quantum mechanies books, but very rarely do we ever see a curve for the Íorce |
between two molecules, because by that time people who are doing analyses are |
thinking in terms of energy rather than of force. |
Next we note that if several conservative Íorces are acting on an object at the |
same time, then the potential energy of the object is the sum of the potential |
energies from each of the separate forces. This is the same proposition that we |
mentioned before, because i1f the force can be represented as a vector sum of |
forces, then the work done by the total force is the sum of the works done by |
the partial forces, and it can therefore be analyzed as changes in the potential |
energies of each of them separately. Thus the total potential energy 1s the sum |
of all the little pieces. |
W© could generalize this to the case oŸ a system of many objects interacting |
with one another, like Jupiter, Saturn, Ủranus, etc., or oxygen, nitrogen, carbon, |
--- Trang 276 --- |
etc., which are acting with respect to one another in pairs due to forces all of |
which are conservative. In these circumstances the kinetic energy in the entire |
system is simply the sum of the kinetic energies of all of the particular atoms or |
planets or whatever, and the potential energy of the system is the sum, over the |
pairs of particles, of the potential energy of mutual interaction of a single pair, |
as though the others were not there. (This is really not true for molecular forces, |
and the formula is somewhat more complicated; it certainly is true for NÑewtonian |
gravitation, and ït is true as an approximation for molecular forces. For molecular |
forces there is a potential energy, but it is sometimes a more complicated function |
of the positions of the atoms than simply a sum oŸ terms from pairs.) In the |
special case of gravity, therefore, the potential energy is the sum, over all the |
pairs ? and 7, of —ŒGm¿m;/r¡;, as was indicated in Eq. (135.14). Equation (13.14) |
expressed mathematically the following proposition: that the total kinetic energy |
plus the total potential energy does not change with time. As the various planets |
wheel about, and turn and twist and so on, IŸ we calculate the total kinetic energy |
and the total potential energy we fñnd that the total remains constant. |
14-4 Nonconservative Íorces |
We have spent a considerable time discussing conservative forces; what about |
nonconservative forces? We shall take a deeper view of this than is usual, and state |
that there are no nonconservative forcesl As a matter of fact, all the fundamental |
forces in nature appear to be conservative. This is not a consequence of Ñewton”s |
laws. In fact, so far as Newton himself knew, the forces could be nonconservative, |
as Íriction apparently is. When we say friction øpparenfly 1s, we are taking a |
modern view, in which it has been discovered that all the deep forces, the forces |
between the particles at the most fundamental level, are conservative. |
Tí, for example, we analyze a system like that great globular star cluster that |
we saw a picture of, with the thousands of stars all interacting, then the formula |
for the total potential energy is simply one term plus another term, etc., summed |
over all pairs oŸ stars, and the kinetic energy is the sum of the kinetic energies of |
all the individual stars. But the globular cluster as a whole is drifting in space |
too, and, if we were far enough away from it and did not see the details, could |
be thought of as a single object. Then if forces were applied to i%, some of those |
forces might end up driving it forward as a whole, and we would see the center |
of the whole thing moving. Ôn the other hand, some of the forces can be, so to |
speak, “wasted” in increasing the kinetic or potential energy of the “particles” |
--- Trang 277 --- |
inside. Let us suppose, for instance, that the action of these forces expands the |
whole cluster and makes the particles move faster. 'Phe total energy of the whole |
thing is really conserved, but seen from the outside with our crude eyes which |
cannot see the confusion of motions inside, and just thinking of the kinetic energy |
of the motion of the whole object as though it were a single particle, it would |
appear that energy is not conserved, but this is due to a lack of appreciation of |
what it is that we see. And that, it turns out, is the case: the total energy of the |
world, kinetic plus potential, is a constant when we look closely enough. |
'When we study matter in the ñnest detail at the atomic level, it is no always |
cøs+ to separate the total energy of a thing into two parts, kinetic energy and |
potential energy, and such separation is not always necessary. It is aửnos‡ always |
possible to do it, so let us say that it 7s always possible, and that the potential- |
plus-kinetic energy of the world is constant. 'Phus the total potential-plus-kinetic |
energy inside the whole world is constant, and if the “world” is a piece of isolated |
material, the energy is constant if there are no external forces. But as we have |
seen, some of the kinetic and potential energy of a thing may be internal, for |
instance the internal molecular motions, in the sense that we do not notice ït. |
W©e know that in a glass of water everything is jiggling around, all the parts are |
moving all the time, so there is a certain kinetic energy inside, which we ordinarily |
may not pay any attention to. We do not notice the motion of the atoms, which |
produces heat, and so we do not call it kinetic energy, but heat is primarily |
kinetic energy. Internal potential energy may also be in the form, for instance, of |
chemical energy: when we burn gasoline energy is liberated because the potential |
energies of the atoms in the new atomic arrangement are lower than in the old |
arrangement. Tt is not strictly possible to treat heat as being pure kinetic energy, |
for a little of the potential gets in, and vice versa for chemical energy, so we |
put the ©wo together and say that the total kinetic and potential energy inside |
an object is partly heat, partly chemical energy, and so on. Anyway, all these |
diferent forms of internal energy are sometimes considered as “lost” energy in the |
sense described above; this will be made clearer when we study thermodynamics. |
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