Photoluminescence Analysis of Thin‐Film Solar Cells
Photoluminescence Analysis of Thin‐Film Solar Cells
复制标题
薄膜太阳能电池的光致发光分析
DOI:
10.1002/9783527636280.ch7
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发表时间:
2011
影响因子:
6.9
通讯作者:
L. Gütay
中科院分区:
文献类型:
--
作者:
T. Unold;L. Gütay
The emission of photoluminescence (PL) radiation is caused by the transition of electrons from higher occupied electronic states into lower unoccupied states, under the emission of photons if the transition is dipole allowed. According to the laws of quantum mechanics, the transition rate can be calculated by first‐order perturbation theory using Fermi's golden rule. This chapter describes the most important radiative transitions occurring in semiconductor materials. The shift of transition energy with increasing temperature may be influenced by a shift in the optical gap with temperature. The chapter discusses some typical PL measurement results for chalcopyrite‐type Cu(In,Ga)Se2thin films and also completed solar cells. The chapter also distinguishes between low‐temperature and room‐temperature luminescence analyses. Both techniques have advantages and disadvantages depending on the material and the investigated material properties. When the temperature is raised to room temperature, band‐band transitions become very likely, as the bands are now sufficiently populated by photoexcited carriers.