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Mathematical Methods for Physicists: A concise introduction - Site Map

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A VECTOR TREATMENT OF CLASSICAL ORBIT THEORY<br />

The ®rst vector product vanishes because p ˆ mdr=dt so dr=dt and p are parallel.<br />

The second vector product is simply r F by Newton's second law, and hence<br />

vanishes <strong>for</strong> all <strong>for</strong>ces directed along the position vector r, that is, <strong>for</strong> all central<br />

<strong>for</strong>ces. Thus the angular momentum L is a constant vector in central <strong>for</strong>ce<br />

motion. This implies that the position vector r, and there<strong>for</strong>e the entire orbit,<br />

lies in a ®xed plane in three-dimensional space. This result is essentially Kepler's<br />

second law, which is often stated in terms of the conservation of area velocity,<br />

jLj=2m.<br />

We now consider the inverse-square central <strong>for</strong>ce of gravitational and electrostatics.<br />

Newton's second law then gives<br />

mdv=dt ˆ…k=r 2 †^n;<br />

…1:36†<br />

where ^n ˆ r=r is a unit vector in the r-direction, and k ˆ Gm 1 m 2 <strong>for</strong> the gravitational<br />

<strong>for</strong>ce, and k ˆ q 1 q 2 <strong>for</strong> the electrostatic <strong>for</strong>ce in cgs units. First we note that<br />

Then L becomes<br />

v ˆ dr=dt ˆ dr=dt^n ‡ rd ^n=dt:<br />

L ˆ r …mv† ˆmr 2 ‰^n …d ^n=dt†Š:<br />

Now consider<br />

d<br />

…v L† ˆdv<br />

dt dt L ˆ k<br />

k<br />

…^n L† ˆ<br />

mr2 mr 2 ‰^n mr2 …^n d ^n=dt†Š<br />

ˆk‰^n…d ^n=dt ^n†…d ^n=dt†…^n ^n†Š:<br />

…1:37†<br />

Since ^n ^n ˆ 1, it follows by di€erentiation that ^n d ^n=dt ˆ 0. Thus we obtain<br />

d<br />

…v L† ˆkd ^n=dt;<br />

dt<br />

integration gives<br />

v L ˆ k^n ‡ C;<br />

…1:38†<br />

where C is a constant vector. It lies along, and ®xes the position of, the major axis<br />

of the orbit as we shall see after we complete the derivation of the orbit. To ®nd<br />

the orbit, we <strong>for</strong>m the scalar quantity<br />

L 2 ˆ L …r mv† ˆmr …v L† ˆmr…k ‡ C cos †;<br />

…1:39†<br />

where is the angle measured from C (which we may take to be the x-axis) to r.<br />

Solving <strong>for</strong> r, we obtain<br />

r ˆ<br />

L 2 =km<br />

1 ‡ C=…k cos † ˆ A<br />

1 ‡ " cos : …1:40†<br />

Eq. (1.40) is a conic section with one focus at the origin, where " represents the<br />

eccentricity of the conic section; depending on its values, the conic section may be<br />

19

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