Physics: Principles with Applications (7th Edition)

Published by Pearson
ISBN 10: 0-32162-592-7
ISBN 13: 978-0-32162-592-2

Chapter 27 - Early Quantum Theory and Models of the Atom - General Problems - Page 801: 74

Answer

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Work Step by Step

a. Start by calculating the intensity of the light at a distance of R = 1.0 meters. We divide the power (in the visible spectrum) by the surface area of a sphere of radius R. $$I=\frac{P}{4\pi R^2}$$ To find the energy entering the eye each second, multiply the intensity by the area of the pupil (assume its diameter is d) $$P_2=I\pi (d/2)^2=\frac{Pd^2}{16 R^2}$$ Divide this by the energy of a single photon to find the number of visible light photons that enter the eye each second, n. $$n=\frac{P_2}{hc/ \lambda}=\frac{P\lambda d^2}{16hc R^2}$$ $$n=\frac{(0.030)(100W)(550\times10^{-9}m)(0.004m)^2} {16(6.626\times10^{-34}J s)(3.00\times10^8 m/s) (1.0m)^2}=8.3\times10^{12}photons/s$$ b. Repeat, using R = 1.0 km. $$n=\frac{(0.030)(100W)(550\times10^{-9}m)(0.004m)^2} {16(6.626\times10^{-34}J s)(3.00\times10^8 m/s) (1.0\times 10^3 m)^2}=8.3\times10^{6}photons/s$$
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