April 22 - 26, 2024
Seattle, Washington
May 7 - 9, 2024 (Virtual)
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2024 MRS Spring Meeting & Exhibit
EN11.03.08

Photoluminescence of BaCd2P2 as a New Defect-Insensitive Solar Material

When and Where

Apr 24, 2024
5:00pm - 7:00pm
Flex Hall C, Level 2, Summit

Presenter(s)

Co-Author(s)

Gideon Kassa1,Smitakshi Goswami1,Zhenkun Yuan1,Muhammad Hasan2,Andrew Pike1,Shaham Quadir3,Yihuang Xiong1,Victoria Kyveryga2,Diana Dahliah4,Gian-Marco Rignanese4,Romain Claes4,Andriy Zakutayev3,David Fenning5,Obadiah Reid6,Sage Bauers3,Kirill Kovnir2,Geoffroy Hautier1,Jifeng Liu1

Dartmouth College1,Iowa State University of Science and Technology2,National Renewable Energy Laboratory3,Université Catholique de Louvain4,University of California, San Diego5,University of Colorado Boulder6

Abstract

Gideon Kassa1,Smitakshi Goswami1,Zhenkun Yuan1,Muhammad Hasan2,Andrew Pike1,Shaham Quadir3,Yihuang Xiong1,Victoria Kyveryga2,Diana Dahliah4,Gian-Marco Rignanese4,Romain Claes4,Andriy Zakutayev3,David Fenning5,Obadiah Reid6,Sage Bauers3,Kirill Kovnir2,Geoffroy Hautier1,Jifeng Liu1

Dartmouth College1,Iowa State University of Science and Technology2,National Renewable Energy Laboratory3,Université Catholique de Louvain4,University of California, San Diego5,University of Colorado Boulder6
Searching for earth-abundant, defect-insensitive solar materials can play a significant role in future photovoltaics. Here we experimentally verify BaCd<sub>2</sub>P<sub>2</sub> as a promising candidate for low-cost, high-efficiency photovoltaic material, as predicted by high-throughput screening of nearly 40,000 semiconductors. Its optimal band gap of 1.45 eV and properties such as temperature stability and long carrier lifetime make BaCd<sub>2</sub>P<sub>2</sub> a strong photovoltaic candidate. We were able to experimentally demonstrate the optical performance of BaCd<sub>2</sub>P<sub>2</sub> by comparing its photoluminescence (PL) intensity with that of GaAs. The relatively low-purity (99.9%) BaCd<sub>2</sub>P<sub>2 </sub>powder had direct gap PL intensity in the same order as GaAs powder obtained from a prime single crystalline wafer, suggesting that it is insensitive to impurities and defects. We further present an in-depth investigation of the PL spectrum of this promising material by studying the impact of temperature, excitation laser power, and composition variations. Nearly all our experimental data have agreed with our theoretically calculated properties of BaCd<sub>2</sub>P<sub>2</sub>. The calculated band structure suggested a direct gap of 1.45 eV and an indirect gap of 1.48 eV. The PL spectrum of BaCd<sub>2</sub>P<sub>2</sub> at 298 K, had a peak at 847 nm (1.46 eV), aligning well with the predicted band structure, and another, broader, peak at 980 nm. At 78 K we observed a separate peak on the lower wavelength side of the 847 nm peak resulting from the indirect gap transition, further validating our computed band structure. This material also showed great temperature stability, increasing the temperature to 368 K had only a slight decrease in the PL emission by ~5%, which fully recovered when going back to 298 K. Our work on excitation power dependence of PL intensity has enabled us to confirm the nature of 847 nm peak and gain a better understanding of the 980 nm peak. We did this by modifying the well-known equation I<sub>PL</sub>= C * (P<sub>laser</sub>)<sup>α</sup> (meant to model the change in PL peak intensity with power) to account for competing nonradiative processes such as Auger recombination at higher excitation powers and consider the potential saturation of available states. We developed a more generalized equation that treats PL intensity as a function of thermal excitation, laser excitation, and nonradiative recombination. For the 847 nm peak, we repeatedly got a value of the α parameter that was strongly indicative of a band-to-band transition. We saw that the 980 nm peak does not blueshift with decreasing temperature and that it had a strikingly similar response to PL laser excitation power variations as the radiative defect of Si-doped GaAs, appearing at 950 nm, leading us to hypothesize that the 980 nm peak of BaCd<sub>2</sub>P<sub>2</sub> is due to a shallow radiative defect. We conducted an evaluation of the change in the 950 nm defect PL peak when using off-stoichiometric BaCd<sub>2</sub>P<sub>2</sub> samples. We observed that the peak intensifies and is slightly redshifted in Ba-poor samples. We further used the data from our studies of PL intensity change with temperature to calculate the activation energy of the prominent nonradiative defects.

Keywords

Raman spectroscopy

Symposium Organizers

Andrea Crovetto, Technical University of Denmark
Annie Greenaway, National Renewable Energy Laboratory
Xiaojing Hao, Univ of New South Wales
Vladan Stevanovic, Colorado School of Mines

Session Chairs

Annie Greenaway
Vladan Stevanovic

In this Session