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Introduction to SAT II Physics - FreeExamPapers

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completes four cycles in its orbit around the nucleus, and so represents an electron in the<br />

n = 4 energy state.<br />

The de Broglie wavelength, then, serves <strong>to</strong> explain why electrons can orbit the nucleus<br />

only at certain radii.<br />

EXAMPLE<br />

Which of the following explains why no one has ever managed <strong>to</strong> observe and measure a de<br />

Broglie wavelength of the Earth?<br />

(A) The Earth is traveling <strong>to</strong>o slowly. It would only have an observable de Broglie<br />

wavelength if it were moving at near light speed.<br />

(B) The Earth is <strong>to</strong>o massive. Only objects of very small mass have noticeable wavelengths.<br />

(C) The Earth has no de Broglie wavelength. Only objects on the a<strong>to</strong>mic level have<br />

wavelengths associated with them.<br />

(D) “Wavelength” is only a theoretical term in reference <strong>to</strong> matter. There is no observable<br />

effect associated with wavelength.<br />

(E) The individual a<strong>to</strong>ms that constitute the Earth all have different wavelengths that<br />

destructively interfere and cancel each other out. As a result, the net wavelength of the<br />

Earth is zero.<br />

This is the sort of question you’re most likely <strong>to</strong> find regarding quantum physics on <strong>SAT</strong><br />

<strong>II</strong> <strong>Physics</strong>: the test writers want <strong>to</strong> make sure you understand the theoretical principles<br />

that underlie the difficult concepts in this area. The answer <strong>to</strong> this question is B. As we<br />

discussed above, the wavelength of an object is given by the formula = h/mv. Since h is<br />

such a small number, mv must also be very small if an object is going <strong>to</strong> have a noticeable<br />

wavelength. Contrary <strong>to</strong> A, the object must be moving relatively slowly, and must have a<br />

very small mass. The Earth weighs<br />

kg, which is anything but a small mass. In<br />

fact, the de Broglie wavelength for the Earth is<br />

m, which is about as small a<br />

value as you will find in this book.<br />

Heisenberg’s Uncertainty Principle<br />

In 1927, a young physicist named Werner Heisenberg proposed a counterintuitive and<br />

startling theory: the more precisely we measure the position of a particle, the less<br />

precisely we can measure the momentum of that particle. This principle can be expressed<br />

mathematically as:<br />

334

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