Impact of charge-compensated Fe and Nb co-substitution on BaTiO3: Bandgap and grain size reduction and enhanced bulk photovoltaic power of Al/BFNT/Ag solar cell
•Al/BaTi1-2xFexNbxO3/Ag is an excellent bulk ferroelectric photovoltaic device configuration.•Increment of aliovalent Fe3+and Nb5+ionic substitutions reduces the bandgap of 0.075BFNT ceramics to ∼2.55 eV and broadens the visible spectrum absorption.•The photocurrent density of Al/0.075BFNT/Ag photov...
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Published in | Solar energy Vol. 257; pp. 34 - 44 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Elsevier Ltd
01.06.2023
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Subjects | |
Online Access | Get full text |
ISSN | 0038-092X 1471-1257 |
DOI | 10.1016/j.solener.2023.03.058 |
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Summary: | •Al/BaTi1-2xFexNbxO3/Ag is an excellent bulk ferroelectric photovoltaic device configuration.•Increment of aliovalent Fe3+and Nb5+ionic substitutions reduces the bandgap of 0.075BFNT ceramics to ∼2.55 eV and broadens the visible spectrum absorption.•The photocurrent density of Al/0.075BFNT/Ag photovoltaic cell is about ∼ 2.2 times higher than that of pure BT.•A high photovoltaic power of ∼ 12 μW/cm2 was achieved.
The generation of above bandgap photovoltage using bulk ferroelectric materials has become a subject of great interest, however, their photocurrent density is limited by a broad bandgap and poor conductivity. To overcome this limitation, we replaced aliovalent metal ions (Fe3+and Nb5+)at the B-site of robust ferroelectric BaTiO3and fabricated an Al/BaTi1-2xFexNbxO3/Ag photovoltaic device. Both the experimental and the theoretical studies showed that bandgap was lowered to ∼2.55 eV and hence absorption of wide energy range of the solar spectrum was attained. An apt top electrode, reduced bandgap and domain size resulted in greater photocurrent density of 1.46 μA/cm2 and photovoltage of 8.31 V for Al/0.075BFNT/Ag solar cell in unpoled condition. This research suggest that reduced band gap, mixed structural phases and nano-sized domains suffices greatest PV power output while the large polarization and poling are not necessary prerequisites. |
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ISSN: | 0038-092X 1471-1257 |
DOI: | 10.1016/j.solener.2023.03.058 |