Muhammad
Faizan
*a,
Jiahao
Xie
b,
Ghulam
Murtaza
c,
Carlos
Echeverría-Arrondo
d,
Thamraa
Alshahrani
*e,
Kailash Chandra
Bhamu
f,
Amel
Laref
g,
Iván
Mora-Seró
*d and
Shah Haidar
Khan
*a
aDepartment of Physics, University of Peshawar, Peshawar 25120, Pakistan. E-mail: faizanstd@uop.edu.pk; shkhan@uop.edu.pk
bState Key Laboratory of Superhard Materials and School of Materials Science and Engineering, Jilin University, Changchun 130012, China
cMaterials Modeling Lab, Department of Physics, Islamia College University, Peshawar 25120, Pakistan
dInstitute of Advanced Materials (INAM), Universitat Jaume I, Castelló 12006, Spain. E-mail: sero@uji.es
eDepartment of Physics, College of Science, Princess Nourah Bint Abdulrahman University, Riyadh 11671, Saudi Arabia. E-mail: thmalshahrani@pnu.edu.sa
fSchool of Chemical Engineering, University of Ulsan, 93 Daehakro, Nam-Gu, Ulsan 44610, South Korea
gDepartment of Physics and Astronomy, College of Science, King Saud University, Riyadh 11451, Kingdom of Saudi Arabia
First published on 7th July 2021
Correction for ‘A first-principles study of the stability, electronic structure, and optical properties of halide double perovskite Rb2Sn1−xTexI6 for solar cell applications’ by Muhammad Faizan et al., Phys. Chem. Chem. Phys., 2021, 23, 4646–4657, DOI: 10.1039/D0CP05827K.
For Rb2Sn0.75Te0.25I6, the strongest absorption (∼6.9 × 105 cm−1) occurs at approximately 2.93 eV. Similarly, for Rb2Sn0.50Te0.50I6, the maximum absorption (5.82 × 105 cm−1) occurs at ∼3.1 eV.
The Royal Society of Chemistry apologises for these errors and any consequent inconvenience to authors and readers.
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