2013
DOI: 10.1002/pssa.201228721
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Cr incorporation in CuGaS2 chalcopyrite: A new intermediate‐band photovoltaic material with wide‐spectrum solar absorption

Abstract: An intermediate‐band (IB) semiconductor CuGa1−xCrxS2 was investigated by the self‐consistent many‐body GW approach (scGW) and further confirmed by the experimental results. The Cr dopant introduced a partially occupied IB, and the density‐of‐states analysis indicates the electron transfer between the impurities and host lattice would suppress the non‐radiative recombination. The CuGa1−xCrxS2 was synthesized by a high‐temperature solid‐state reaction and the X‐ray photoelectron spectroscopy (XPS) indicated the … Show more

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Cited by 66 publications
(35 citation statements)
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“…Further increasing the number of IBs can raise the efficiency to values as high as 80% [9,10]. This trend is verified in a number of theoretical and experimental works [11][12][13][14].…”
Section: Introductionsupporting
confidence: 60%
“…Further increasing the number of IBs can raise the efficiency to values as high as 80% [9,10]. This trend is verified in a number of theoretical and experimental works [11][12][13][14].…”
Section: Introductionsupporting
confidence: 60%
“…The aim of this paper is to present accurate theoretical results (using hybrid functionals) of the band alignment between the conduction and valence band edges of CuGaS 2 (a light absorber which has interest as possible component of inexpensive chalcopyrite-based tandem cells) and those of semiconductor candidates that can be used as contacts for it in solar cells, in particular, CuAlSe 2 , CdS, ZnSe and ZnS. The results obtained here, may also provide the fundamentals for the design and development of solar cells with an intermediate band [11], based on CuGaS 2 , which has been proposed as a suitable host semiconductor material developing such band when a transition metal is added to substitute the Gallium atoms [12][13][14][15][16].…”
Section: Introductionmentioning
confidence: 61%
“…The ideal widths of the host material for the IBSC are 2.40 and 1.93 eV at 1 sun and full concentration, respectively. As the host materials for the IBSC, many wide gap semiconductors such as III–V, II–VI, spinel and chalcopyrite compounds have been studied and explored.…”
Section: Introductionmentioning
confidence: 99%
“…Owing to the success of chalcopyrite Cu(In,Ga)Se 2 and its cousin Cu 2 ZnSn(S,Se) 4 on the single band gap solar cells, Cu‐based chalcopyrite compounds have been paid much attention as the host for IBSC, for instances, Fe, Cr, Ti, Ge, and Sn doped CuGaS 2 , Ce and Ti doped CuInS 2 , Sn‐doped CuAlS 2 , etc. In order to realize the three‐photon absorption effectively, the intermediate band need to meet two requirements: delocalized and half‐filled .…”
Section: Introductionmentioning
confidence: 99%