December 1 - 6, 2024
Boston, Massachusetts
Symposium Supporters
2024 MRS Fall Meeting & Exhibit
EL04.13.07

Breaking the Shockley-Queisser (SQ) Limit to Develop a Next Generation of Solar Cell

When and Where

Dec 4, 2024
8:00pm - 10:00pm
Hynes, Level 1, Hall A

Presenter(s)

Co-Author(s)

Tuhin Ghosh1,Jianbo Gao1

Brock University1

Abstract

Tuhin Ghosh1,Jianbo Gao1

Brock University1
<b>Abstract: </b>To overcome the well-known Shockley-Queisser (SQ) limit, one novel approach is to utilize the hot carrier generation and collection mechanism, which can achieve more than 67 % power conversion efficiency. A hot carrier is the photogenerated carrier above band gap, due to its extra energy difference between incident photon energy and optical band gap.[i] One signature of the hot carrier photovoltaic (PV) technology is a higher open-circuit voltage (V<sub>OC</sub>) than the band gap of solar absorbers.<br/>However, hot carrier PV technology still suffers from the difficulty in collection of the ultra-short time scale hot carrier due to their rapid electron-phonon interaction. In the recent time, hybrid organic-inorganic based perovskite-based structure (e.g., APbX<sub>3</sub>, where A = Cs, methylammonium (MA) or formamidinium (FA), X = (Cl, Br, I)) shows their capability in used as hot carrier solar cell due to their prolong carrier lifetime beyond 10s of picosecond or nanosecond, measured by the ultrafast pump-probe and time-resolved photoluminescence.[ii] However, all those characterizations not only investigated the perovskite thin films or solutions, rather than the solar cell working condition (i.e., <i>in-situ</i>), but also limited to the carrier diffusion mechanism, while the photocurrent obey the carrier drift understanding.<br/>Here lies some urgency to characterize the photocurrent within <i>in-situ</i> based perovskite solar cell (PSC) using a novel ultrafast photovoltaic spectroscopy to directly collect the photocurrent, when the solar cell at work.[iii] For the first time, with a sub - 40ps time resolution, we discover a transient V<sub>OC</sub> much larger than the band gap of the mixed cation (CsMAFA) perovskite solar cells with &gt;20% efficiency. We further investigate the hot carrier drift transport property, which depends on film thickness and temperature.<br/><b>Keywords:</b> hot carrier, drift dynamics, charge collection, solar cell<br/><br/><br/>[i] Nozik, A. J. <i>et al.</i>, Semiconductor Quantum Dots and Quantum Dot Arrays and Applications of Multiple Exciton Generation to Third-Generation Photovoltaic Solar Cells. <i>Chem Rev</i> <b>2010</b>, 110, 6873-6890.<br/><br/>[ii] Wang, T. <i>et al.</i>, Protecting hot carriers by tuning hybrid perovskite structures with alkali cations. <i>Sci Adv</i> <b>2020</b>, 6, eabb1336.<br/><br/>[iii] Kobbekaduwa, K.; Liu, E.; Zhao, Q.; Bains, J. S.; Zhang, J.; Shi,Y.; Zheng, H.; Li, D.; Cai, T.; Chen, O.; Rao, A. M.; Beard, M.C.; Luther, J.M.; and Gao, J. Ultrafast Carrier Drift Transport Dynamics in CsPbI<sub>3</sub> Perovskite Nanocrystalline Thin Films. <i>ACS Nano</i><b> 2023</b>, 17, 13997–14004.

Keywords

perovskites | spectroscopy

Symposium Organizers

Anita Ho-Baillie, The University of Sydney
Marina Leite, University of California, Davis
Nakita Noel, University of Oxford
Laura Schelhas, National Renewable Energy Laboratory

Symposium Support

Bronze
APL Materials

Session Chairs

Marina Leite
Nakita Noel

In this Session