Thermal Effects on CH3NH3PbI3 Perovskite from Ab Initio Molecular Dynamics Simulations

We present a molecular dynamics simulation study of CH3NH3PbI3 based on forces calculated from density functional theory. The simulations were performed on model systems having 8 and 27 unit cells, and for a total simulation time of 40 ps in each case. Analysis of the finite size effects, in particu...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Journal of physical chemistry. C 2015-04
Hauptverfasser: Carignano, Marcelo A, Kachmar, Ali, Hutter, Jürg
Format: Artikel
Sprache:eng
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title Journal of physical chemistry. C
container_volume
creator Carignano, Marcelo A
Kachmar, Ali
Hutter, Jürg
description We present a molecular dynamics simulation study of CH3NH3PbI3 based on forces calculated from density functional theory. The simulations were performed on model systems having 8 and 27 unit cells, and for a total simulation time of 40 ps in each case. Analysis of the finite size effects, in particular the mobility of the organic component, suggests that the smaller system is over-correlated through the long-range electrostatic interaction. In the larger system, this finite size artifact is relaxed, producing a more reliable description of the anisotropic rotational behavior of the methylammonium molecules. The thermal effects on the optical properties of the system were also analyzed. The HOMO–LUMO energy gap fluctuates around its central value with a standard deviation of approximately 0.1 eV. The projected density of states consistently place the Fermi level on the p orbitals of the I atoms and the lowest virtual state on the p orbitals of the Pb atoms throughout the whole simulation trajectory.
doi_str_mv 10.1021/jp510568n
format Article
fullrecord <record><control><sourceid>acs</sourceid><recordid>TN_cdi_acs_journals_10_1021_jp510568n</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>d3391990</sourcerecordid><originalsourceid>FETCH-LOGICAL-a251t-8f6832e161e518ba927f561e45b30f9520a65d9cd6e5c2c86aa7aabad4e24abc3</originalsourceid><addsrcrecordid>eNo9UMtKxDAUDaLgOLrwD7JxWc2jN22XQx2nhVEHHN2WmzTB1raRpiP491aUWZ0XnAOHkGvObjkT_K79BM5ApcMJWfBMiiiJAU6PPE7OyUUILWMgGZcL8rZ_t2OPHV07Z80UqB9oXsinQu50KenOjv4rfDSTpW70PV1pWg7N1Hj66DtrDh2O9P57wL4xgb40_WzM4RAuyZnDLtirf1yS14f1Pi-i7fOmzFfbCAXwKUqdSqWwXHELPNWYicTBLGLQkrkMBEMFdWZqZcEIkyrEBFFjHVsRozZySW7-etGEqvWHcZjXKs6q3zOq4xnyB1BpUaM</addsrcrecordid><sourcetype>Publisher</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Thermal Effects on CH3NH3PbI3 Perovskite from Ab Initio Molecular Dynamics Simulations</title><source>American Chemical Society Journals</source><creator>Carignano, Marcelo A ; Kachmar, Ali ; Hutter, Jürg</creator><creatorcontrib>Carignano, Marcelo A ; Kachmar, Ali ; Hutter, Jürg</creatorcontrib><description>We present a molecular dynamics simulation study of CH3NH3PbI3 based on forces calculated from density functional theory. The simulations were performed on model systems having 8 and 27 unit cells, and for a total simulation time of 40 ps in each case. Analysis of the finite size effects, in particular the mobility of the organic component, suggests that the smaller system is over-correlated through the long-range electrostatic interaction. In the larger system, this finite size artifact is relaxed, producing a more reliable description of the anisotropic rotational behavior of the methylammonium molecules. The thermal effects on the optical properties of the system were also analyzed. The HOMO–LUMO energy gap fluctuates around its central value with a standard deviation of approximately 0.1 eV. The projected density of states consistently place the Fermi level on the p orbitals of the I atoms and the lowest virtual state on the p orbitals of the Pb atoms throughout the whole simulation trajectory.</description><identifier>ISSN: 1932-7447</identifier><identifier>EISSN: 1932-7455</identifier><identifier>DOI: 10.1021/jp510568n</identifier><language>eng</language><publisher>American Chemical Society</publisher><ispartof>Journal of physical chemistry. C, 2015-04</ispartof><rights>Copyright © American Chemical Society</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://pubs.acs.org/doi/pdf/10.1021/jp510568n$$EPDF$$P50$$Gacs$$H</linktopdf><linktohtml>$$Uhttps://pubs.acs.org/doi/10.1021/jp510568n$$EHTML$$P50$$Gacs$$H</linktohtml><link.rule.ids>314,780,784,27076,27924,27925,56738,56788</link.rule.ids></links><search><creatorcontrib>Carignano, Marcelo A</creatorcontrib><creatorcontrib>Kachmar, Ali</creatorcontrib><creatorcontrib>Hutter, Jürg</creatorcontrib><title>Thermal Effects on CH3NH3PbI3 Perovskite from Ab Initio Molecular Dynamics Simulations</title><title>Journal of physical chemistry. C</title><addtitle>J. Phys. Chem. C</addtitle><description>We present a molecular dynamics simulation study of CH3NH3PbI3 based on forces calculated from density functional theory. The simulations were performed on model systems having 8 and 27 unit cells, and for a total simulation time of 40 ps in each case. Analysis of the finite size effects, in particular the mobility of the organic component, suggests that the smaller system is over-correlated through the long-range electrostatic interaction. In the larger system, this finite size artifact is relaxed, producing a more reliable description of the anisotropic rotational behavior of the methylammonium molecules. The thermal effects on the optical properties of the system were also analyzed. The HOMO–LUMO energy gap fluctuates around its central value with a standard deviation of approximately 0.1 eV. The projected density of states consistently place the Fermi level on the p orbitals of the I atoms and the lowest virtual state on the p orbitals of the Pb atoms throughout the whole simulation trajectory.</description><issn>1932-7447</issn><issn>1932-7455</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><sourceid/><recordid>eNo9UMtKxDAUDaLgOLrwD7JxWc2jN22XQx2nhVEHHN2WmzTB1raRpiP491aUWZ0XnAOHkGvObjkT_K79BM5ApcMJWfBMiiiJAU6PPE7OyUUILWMgGZcL8rZ_t2OPHV07Z80UqB9oXsinQu50KenOjv4rfDSTpW70PV1pWg7N1Hj66DtrDh2O9P57wL4xgb40_WzM4RAuyZnDLtirf1yS14f1Pi-i7fOmzFfbCAXwKUqdSqWwXHELPNWYicTBLGLQkrkMBEMFdWZqZcEIkyrEBFFjHVsRozZySW7-etGEqvWHcZjXKs6q3zOq4xnyB1BpUaM</recordid><startdate>20150430</startdate><enddate>20150430</enddate><creator>Carignano, Marcelo A</creator><creator>Kachmar, Ali</creator><creator>Hutter, Jürg</creator><general>American Chemical Society</general><scope/></search><sort><creationdate>20150430</creationdate><title>Thermal Effects on CH3NH3PbI3 Perovskite from Ab Initio Molecular Dynamics Simulations</title><author>Carignano, Marcelo A ; Kachmar, Ali ; Hutter, Jürg</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a251t-8f6832e161e518ba927f561e45b30f9520a65d9cd6e5c2c86aa7aabad4e24abc3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Carignano, Marcelo A</creatorcontrib><creatorcontrib>Kachmar, Ali</creatorcontrib><creatorcontrib>Hutter, Jürg</creatorcontrib><jtitle>Journal of physical chemistry. C</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Carignano, Marcelo A</au><au>Kachmar, Ali</au><au>Hutter, Jürg</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Thermal Effects on CH3NH3PbI3 Perovskite from Ab Initio Molecular Dynamics Simulations</atitle><jtitle>Journal of physical chemistry. C</jtitle><addtitle>J. Phys. Chem. C</addtitle><date>2015-04-30</date><risdate>2015</risdate><issn>1932-7447</issn><eissn>1932-7455</eissn><abstract>We present a molecular dynamics simulation study of CH3NH3PbI3 based on forces calculated from density functional theory. The simulations were performed on model systems having 8 and 27 unit cells, and for a total simulation time of 40 ps in each case. Analysis of the finite size effects, in particular the mobility of the organic component, suggests that the smaller system is over-correlated through the long-range electrostatic interaction. In the larger system, this finite size artifact is relaxed, producing a more reliable description of the anisotropic rotational behavior of the methylammonium molecules. The thermal effects on the optical properties of the system were also analyzed. The HOMO–LUMO energy gap fluctuates around its central value with a standard deviation of approximately 0.1 eV. The projected density of states consistently place the Fermi level on the p orbitals of the I atoms and the lowest virtual state on the p orbitals of the Pb atoms throughout the whole simulation trajectory.</abstract><pub>American Chemical Society</pub><doi>10.1021/jp510568n</doi></addata></record>
fulltext fulltext
identifier ISSN: 1932-7447
ispartof Journal of physical chemistry. C, 2015-04
issn 1932-7447
1932-7455
language eng
recordid cdi_acs_journals_10_1021_jp510568n
source American Chemical Society Journals
title Thermal Effects on CH3NH3PbI3 Perovskite from Ab Initio Molecular Dynamics Simulations
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-20T00%3A13%3A59IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-acs&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Thermal%20Effects%20on%20CH3NH3PbI3%20Perovskite%20from%20Ab%20Initio%20Molecular%20Dynamics%20Simulations&rft.jtitle=Journal%20of%20physical%20chemistry.%20C&rft.au=Carignano,%20Marcelo%20A&rft.date=2015-04-30&rft.issn=1932-7447&rft.eissn=1932-7455&rft_id=info:doi/10.1021/jp510568n&rft_dat=%3Cacs%3Ed3391990%3C/acs%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true