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the entire system together. * This model must then exhibit properties that are the combined effects of the Pauli principle, relativistic dynamics, and the gravitationallaw. First let us work out the pressure exerted by a Fermi gas of relativistic electrons in the ground state. The states for a single electron are specified by the momentum p and the spin quantum number s = ~. The single-particle energy levels are independent of s:

y(pc) + (m ec 2 )

PF=h(3: f/3

(11.33)

depths of the depression in 1932 to the peak of the Internet bubble in January of 2000. There are a variety of astounding things to note in this chart: The point where the two major lines intersect in 1974 predicted the precise bottom of the massive 1973 1974 bear market. The steady climb from 1990 to 1995 was perfectly bounded by two of the fan lines. Most impressive of all, the ultimate market top in 2000 was established by the rst fan (which, remember, began 97 years before). Figure 1.2 is a close-up view of late 1999 and early 2000; as you can see, the almost century-old fan line creates impressive resistance to these prices moving higher on four different occasions. If we were in stocks at this time, this would be a vital warning signal that the top was established. This is an extreme example, but the point is that being able to gain insight into the most likely future of a particular price is a vehicle for real trading pro ts. It is an edge that those not using charts effectively simply will not have.

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7T;h 3V!(X F)

(11.34)

Click the Home tab on the Ribbon. Click the Advanced button. Click Filter By Form. A blank form appears.

(11.35)

( 1 + -12 + ... )

(X F 1)

(11.36)

-The temperature in an actual white dwarf star is so high that electron-positron pairs can be created in electron-electron collisions. These pairs in tum annihilate into radiation. Therefore in equilibrium there should be a certain number of electron-positron pairs and a certain amount of radiation present. We neglect the effects of these. It has been speculated that neutrinos can also be created in electron-electron, electron-positron, and photon-photon collisions with appreciable probability. This leads to some interesting phenomena, for neutrinos interact so weakly with matter that they do not come to thermal equilibrium with the rest of the system. They simply leave the star and cause a constant drain of energy. (H. Y. Chiu and P. Morrison, Phys. Rev. Lett. 5, 573 (1960).) Our model is based on the neglect of these effects.

(~:r/3

FIGURE 1.2 Highlighted here four times is the Dow bouncing off the fan line established over a century earlier.

(11.37)

where m p is the mass of a proton. In terms of M and R we have 8'7T m p R 3 u=--3

(11.38)

Click in the field by which you want to filter. Click the that appears and choose a criterion. Repeat Steps 5 and 6 to add more criteria to the filter.

M=---

(11.40)

F )]

(11.41)

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