PHYSICS · Multi-part · Fermi University Physics · Quantum Mechanics · Earth, Climate & Energy Physics · Origins of quantum theory
Energy from Physics, Ch The solar resource resolved: geometry, spectrum and the limits of concentration
Problem
A device has a threshold photon energy of E=1.60eV, one not in the chapter's list. Model the Sun at the Earth's orbit as the diluted 5772K blackbody with f⊙=2.16×10−5.
((a)) Substitute x=ε/kBT⊙ in the photon-flux integral, find the lower limit x0 and the prefactor, and evaluate the integral numerically to three significant figures.
((b)) Find the photon flux Φ(1.60eV) and the current density it would drive at one electron per photon, and check that both lie between the chapter's values at 1.42 and 1.80eV.