η = 1 - (TC/TH)where TC is the temperature of a cold reservoir, and TH is the temperature of a hot reservoir. When there is no temperature differential, TH is equal to TC, and the efficiency is zero. This idea that a temperature differential provides work is nicely illustrated in the drinking bird toy that I showed in a previous article (Second Law of Thermodynamics, February 7, 2011). That article also discussed the second law and the impossibility of perpetual motion machines. The differential temperature in the drinking bird is provided by evaporative cooling that provides a slightly cooler temperature below ambient. There's a temperature differential, so work (the dipping action) can be done. Hot engines work best, which is somewhat of a battle cry for turbine engine designers. When we want to harvest solar energy, photovoltaics are a good choice for small to medium-sized installations. The largest economical photovoltaic array would be one that powers a large building. Googleplex is a good example, since it has a solar installation that generates 1.6 megawatts, which is about 30% of the power demand for this corporate center.[1] Solar thermal is the next step in power generation. In a recent article (Solar Nevada, June 6, 2011), I discussed the Crescent Dunes Solar Energy Project being constructed near Las Vegas that is rated at 110-megawatts. This installation uses mirrors to focus light onto a reactor that heats molten salt. The heat from the molten salt is used to create steam to drive a turbine generator. There's another solar thermal method that's being developed by materials scientists at the California Institute of Technology (Pasadena, CA) that makes use of the thermodynamics of the equilibrium between cerium oxide and its formative elements.[2-3] Cerium oxide, a stable oxide that's also called ceria, is formed from the elements in a highly exothermic reaction:
Ce + O2 -> CeO2Stable, of course, is a relative term, since, at a given temperature, there is always a small fraction of unreacted cerium available and an associated partial pressure of oxygen. At room temperature, the equilibrium pressure of oxygen over ceria is laughably small. It's just 2.3 x 10-180 atmospheres, so the idea that ceria is a very stable oxide is well founded. When the temperature is increased, ceria starts to decompose, although just very slightly. The graph below shows the partial pressure of oxygen above ceria as a function of temperature, as calculated from its free energy of formation.[4]
Partial pressure of oxygen above ceria as a function of temperature, as calculated from the Gibbs Free Energy of formation. Free energy data from Ref. 4. Graph rendered by Gnumeric. |