Severity: Warning
Message: file_get_contents(https://...@gmail.com&api_key=61f08fa0b96a73de8c900d749fcb997acc09&a=1): Failed to open stream: HTTP request failed! HTTP/1.1 429 Too Many Requests
Filename: helpers/my_audit_helper.php
Line Number: 197
Backtrace:
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 197
Function: file_get_contents
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 271
Function: simplexml_load_file_from_url
File: /var/www/html/application/helpers/my_audit_helper.php
Line: 3165
Function: getPubMedXML
File: /var/www/html/application/controllers/Detail.php
Line: 597
Function: pubMedSearch_Global
File: /var/www/html/application/controllers/Detail.php
Line: 511
Function: pubMedGetRelatedKeyword
File: /var/www/html/index.php
Line: 317
Function: require_once
98%
921
2 minutes
20
Tin perovskite solar cells (PSCs) have emerged as a highly promising lead-free alternative, attracting significant research interest owing to their reduced toxicity and excellent optoelectronic characteristics. However, their photovoltaic performance is severely restrained by the uncontrollable crystallization process and the resultant high defect density in the perovskite films. To address these issues, two acetamide derivatives, i.e., 2-cyanoacetamide (2CA) and 2-amino-2-cyanoacetamide (2A2CA), with multifunctional groups are used to improve the film quality of tin perovskites. Theoretical calculations and experimental results jointly demonstrate that 2A2CA molecules with larger dipole moments can significantly enhance the interaction between the carbonyl group and uncoordinatedSn cations. The introduction of 2A2CA effectively increases the formation energy of tin vacancy defects (), regulates the crystallization of tin perovskites, and produces high-quality tin perovskite films with smooth morphology, compact structure, increased crystallinity, and low defect density. Thereby, the 2A2CA-modified tin PSCs achieve a champion efficiency of 14.98% and maintain 90% after storing for over 2200 h in a nitrogen atmosphere.
Download full-text PDF |
Source |
---|---|
http://dx.doi.org/10.1021/acsnano.5c07298 | DOI Listing |