Saif Qaid

Dr. Saif Qaid

Physics and Astronomy, King Saud University, Riyadh, Ar Riyāḑ, Saudi Arabia
orcid

Research Focus & Metrics

Academic Career Length

16Years (2011-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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30 September 2024 in Nature
Verified
Journal Article
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SLSaisai Li
Saisai Li
YJYuanzhi Jiang
Yuanzhi Jiang
JXJian Xu
Jian Xu
DWDi Wang
Di Wang
ZDZijin Ding
Zijin Ding
MYMingjian Yuan
Mingjian Yuan

24 March 2020 in ACS Omega
Verified
Journal Article
Open access
Hamid GhaithanHamid Ghaithan
Hamid Ghaithan
ZAZeyad Alahmed
Zeyad Alahmed
SQSaif Qaid
Saif Qaid
MHMahmoud Hezam
Mahmoud Hezam
AAAbdullah S. Aldwayyan
Abdullah S. Aldwayyan
Cesium lead bromide (CsPbBr3) perovskite has recently gained significance owing to its rapidly increasing performance when used for light-emitting devices. In this study, we used density functional theory to determine the structural, electronic, and optical properties of the cubic, tetragonal, and orthorhombic temperature-dependent phases of CsPbBr3 perovskite using the full-potential linear augmented plane wave method. The electronic properties of CsPbBr3 perovskite have been investigated by evaluating their changes upon exerting spin-orbit coupling (SOC). The following exchange potentials were used: the local density approximation (LDA), Perdew–Burke–Ernzerhof generalized gradient approximation (PBE-GGA), Engel–Vosko GGA (EV-GGA), Perdew–Burke–Ernzerhof GGA revised for solids (PBEsol-GGA), modified Becke–Johnson GGA (mBJ-GGA), new modified Becke–Johnson GGA (nmBJ-GGA), and unmodified Becke–Johnson GGA (umBJ-GGA). Our band structure results indicated that the cubic, tetragonal, and orthorhombic phases have direct energy bandgaps. By including the SOC effect in the calculations, the bandgaps computed with mBJ-GGA and nmBJ-GGA were found to be in good agreement with the experimental results. Additionally, despite the large variations in their lattice constants, the three CsPbBr3 phases possessed similar optical properties. These results demonstrate a wide temperature range of operation for CsPbBr3.

19 February 2025 in Nature
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KWKeyu Wei
Keyu Wei
TZTong Zhou
Tong Zhou
YJYuanzhi Jiang
Yuanzhi Jiang
CSChangjiu Sun
Changjiu Sun
YLYulong Liu
Yulong Liu
MYMingjian Yuan
Mingjian Yuan

1 March 2020 in Journal of Colloid and Interface Science
Verified
Journal Article
Closed access
SQSaif Qaid
Saif Qaid
Bandar Al-AsbahiBandar Al-Asbahi
Bandar Al-Asbahi
Hamid GhaithanHamid Ghaithan
Hamid Ghaithan
MAM.S. AlSalhi
M.S. AlSalhi
ADAbdullah S. Al Dwayyan
Abdullah S. Al Dwayyan

27 September 2023 in ACS Energy Letters
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Journal Article
Closed access
BWBaiqian Wang
Baiqian Wang
XYXin Yang
Xin Yang
RLRu Li
Ru Li
SQSaif Qaid
Saif Qaid
WCWensi Cai
Wensi Cai
Zhigang ZangZhigang Zang
Zhigang Zang

16 October 2024 in Nature Communications
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RWRui Wang
Rui Wang
XLXiaoyu Liu
Xiaoyu Liu
SYShan Yan
Shan Yan
NMNi Meng
Ni Meng
XZXinmin Zhao
Xinmin Zhao
THTingwei He
Tingwei He
Wide-bandgap (WBG) perovskite solar cells (PSCs) are employed as top cells of tandem cells to break through the theoretical limits of single-junction photovoltaic devices. However, WBG PSCs exhibit severe open-circuit voltage (Voc) loss with increasing bromine content. Herein, inhomogeneous halogen-phase distribution is pointed out to be the reason, which hinders efficient extraction of carriers. We thus propose to form homogeneous halogen-phase distribution to address the issue. With the help of density functional theory, we construct a double-layer structure (D-2P) based on 2-(9H-Carbazol-9-yl)ethyl]phosphonic acid molecules to provide nucleation sites for perovskite crystallization. Homogeneous perovskite phase is achieved through bottom-up templated crystallization of halogen component. The efficient carrier extraction reduces the Shockley-Read-Hall recombination, resulting in a high Voc of 1.32 V. As a result, D-2P-treated device (1.75 eV) achieves a record power conversion efficiency of 20.80% (certified 20.70%), which is the highest value reported for WBG (more than 1.74 eV) PSCs.