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1) According to the photon model, light carries its energy in packets called quanta or photons. Why then don't we see a series of flashes when we look at things?2) Most black-and-white photographic film (with the exception of some special-purpose films) is less sensitive to red light than blue light and has almost no sensitivity to infrared. How can these properties be understood on the basis of photons?3) Galaxies tend to be strong emitters of Lyman-alpha photons (from the n=2 to n=1 transition in atomic hydrogen). What can you infer from this observation about the temperature in this environment? Explain. (Lyman alpha photons have a wavelength of 122 nm and it's the longest wavelength line in the Lyman series of UV lines in the H spectrum)4) The emission of a photon by an isolated atom is a recoil process in which momentum is conserved. Thus hf = (energy initial - energy final) should include a recoil kinetic energy for the atom. Why is this energy negligible in that equation?
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