Assessing Carrier Mobility, Dopability, and Defect Tolerance in the Chalcogenide Perovskite Ba Zr S 3
The chalcogenide perovskite Ba Zr S 3 has attracted much attention as a promising solar absorber for thin-film photovoltaics. Here we use first-principles calculations to evaluate its carrier transport and defect properties. We find that Ba Zr S 3 has a phonon-limited electron mobility of 37 cm 2 /...
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creator | Yuan, Zhenkun Dahliah, Diana Claes, Romain Pike, Andrew Fenning, David P. Rignanese, Gian-Marco Hautier, Geoffroy |
description | The chalcogenide perovskite
Ba
Zr
S
3
has attracted much attention as a promising solar absorber for thin-film photovoltaics. Here we use first-principles calculations to evaluate its carrier transport and defect properties. We find that
Ba
Zr
S
3
has a phonon-limited electron mobility of
37
cm
2
/
V s, which is comparable to that in halide perovskites, but lower hole mobility of
11
cm
2
/
V s. The defect computations indicate that
Ba
Zr
S
3
is intrinsically
n
-type due to shallow sulfur vacancies, but that strong compensation by sulfur vacancies will prevent attempts to make it
p
-type. We also establish that
Ba
Zr
S
3
shows some degree of defect tolerance, presenting only few low formation energy, deep intrinsic defects. Among the deep defects, sulfur interstitials are the dominant nonradiative recombination centers but exhibit a moderate capture coefficient. Our work highlights the material’s intrinsic limitations in carrier mobility and
p
-type doping, and suggests focusing on suppressing the formation of sulfur interstitials to achieve longer carrier lifetime. |
doi_str_mv | 10.1103/PRXEnergy.3.033008 |
format | Article |
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Ba
Zr
S
3
has attracted much attention as a promising solar absorber for thin-film photovoltaics. Here we use first-principles calculations to evaluate its carrier transport and defect properties. We find that
Ba
Zr
S
3
has a phonon-limited electron mobility of
37
cm
2
/
V s, which is comparable to that in halide perovskites, but lower hole mobility of
11
cm
2
/
V s. The defect computations indicate that
Ba
Zr
S
3
is intrinsically
n
-type due to shallow sulfur vacancies, but that strong compensation by sulfur vacancies will prevent attempts to make it
p
-type. We also establish that
Ba
Zr
S
3
shows some degree of defect tolerance, presenting only few low formation energy, deep intrinsic defects. Among the deep defects, sulfur interstitials are the dominant nonradiative recombination centers but exhibit a moderate capture coefficient. Our work highlights the material’s intrinsic limitations in carrier mobility and
p
-type doping, and suggests focusing on suppressing the formation of sulfur interstitials to achieve longer carrier lifetime.</description><identifier>ISSN: 2768-5608</identifier><identifier>EISSN: 2768-5608</identifier><identifier>DOI: 10.1103/PRXEnergy.3.033008</identifier><language>eng</language><ispartof>PRX energy, 2024-09, Vol.3 (3), Article 033008</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-crossref_primary_10_1103_PRXEnergy_3_0330083</cites><orcidid>0000-0002-7200-5973 ; 0000-0001-7840-4636 ; 0000-0002-1422-1205 ; 0009-0000-5746-7419 ; 0000-0002-4609-9312 ; 0000-0003-1754-2220</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,860,27901,27902</link.rule.ids></links><search><creatorcontrib>Yuan, Zhenkun</creatorcontrib><creatorcontrib>Dahliah, Diana</creatorcontrib><creatorcontrib>Claes, Romain</creatorcontrib><creatorcontrib>Pike, Andrew</creatorcontrib><creatorcontrib>Fenning, David P.</creatorcontrib><creatorcontrib>Rignanese, Gian-Marco</creatorcontrib><creatorcontrib>Hautier, Geoffroy</creatorcontrib><title>Assessing Carrier Mobility, Dopability, and Defect Tolerance in the Chalcogenide Perovskite Ba Zr S 3</title><title>PRX energy</title><description>The chalcogenide perovskite
Ba
Zr
S
3
has attracted much attention as a promising solar absorber for thin-film photovoltaics. Here we use first-principles calculations to evaluate its carrier transport and defect properties. We find that
Ba
Zr
S
3
has a phonon-limited electron mobility of
37
cm
2
/
V s, which is comparable to that in halide perovskites, but lower hole mobility of
11
cm
2
/
V s. The defect computations indicate that
Ba
Zr
S
3
is intrinsically
n
-type due to shallow sulfur vacancies, but that strong compensation by sulfur vacancies will prevent attempts to make it
p
-type. We also establish that
Ba
Zr
S
3
shows some degree of defect tolerance, presenting only few low formation energy, deep intrinsic defects. Among the deep defects, sulfur interstitials are the dominant nonradiative recombination centers but exhibit a moderate capture coefficient. Our work highlights the material’s intrinsic limitations in carrier mobility and
p
-type doping, and suggests focusing on suppressing the formation of sulfur interstitials to achieve longer carrier lifetime.</description><issn>2768-5608</issn><issn>2768-5608</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNqdj8FqwkAURYeiUFF_oKv3ATW-OGjSZY2KG0FaF-JmmMaXOG06I-8FIX8vopauXd2zuGdxlHqJMYpj1MP1x3buicsm0hFqjZg-qc4omaSD8QTT1j9-Vn2Rb8TLK0nexh1F7yIk4nwJmWV2xLAKX65ydfMKs3C0d7Z-DzMqKK9hEypi63MC56E-EGQHW-WhJO_2BGvicJIfVxNMLewYPkH3VLuwlVD_tl01Wsw32XKQcxBhKsyR3a_lxsRoLk3mr8loc23SD0ln651XtQ</recordid><startdate>202409</startdate><enddate>202409</enddate><creator>Yuan, Zhenkun</creator><creator>Dahliah, Diana</creator><creator>Claes, Romain</creator><creator>Pike, Andrew</creator><creator>Fenning, David P.</creator><creator>Rignanese, Gian-Marco</creator><creator>Hautier, Geoffroy</creator><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0002-7200-5973</orcidid><orcidid>https://orcid.org/0000-0001-7840-4636</orcidid><orcidid>https://orcid.org/0000-0002-1422-1205</orcidid><orcidid>https://orcid.org/0009-0000-5746-7419</orcidid><orcidid>https://orcid.org/0000-0002-4609-9312</orcidid><orcidid>https://orcid.org/0000-0003-1754-2220</orcidid></search><sort><creationdate>202409</creationdate><title>Assessing Carrier Mobility, Dopability, and Defect Tolerance in the Chalcogenide Perovskite Ba Zr S 3</title><author>Yuan, Zhenkun ; Dahliah, Diana ; Claes, Romain ; Pike, Andrew ; Fenning, David P. ; Rignanese, Gian-Marco ; Hautier, Geoffroy</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-crossref_primary_10_1103_PRXEnergy_3_0330083</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Yuan, Zhenkun</creatorcontrib><creatorcontrib>Dahliah, Diana</creatorcontrib><creatorcontrib>Claes, Romain</creatorcontrib><creatorcontrib>Pike, Andrew</creatorcontrib><creatorcontrib>Fenning, David P.</creatorcontrib><creatorcontrib>Rignanese, Gian-Marco</creatorcontrib><creatorcontrib>Hautier, Geoffroy</creatorcontrib><collection>CrossRef</collection><jtitle>PRX energy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Yuan, Zhenkun</au><au>Dahliah, Diana</au><au>Claes, Romain</au><au>Pike, Andrew</au><au>Fenning, David P.</au><au>Rignanese, Gian-Marco</au><au>Hautier, Geoffroy</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Assessing Carrier Mobility, Dopability, and Defect Tolerance in the Chalcogenide Perovskite Ba Zr S 3</atitle><jtitle>PRX energy</jtitle><date>2024-09</date><risdate>2024</risdate><volume>3</volume><issue>3</issue><artnum>033008</artnum><issn>2768-5608</issn><eissn>2768-5608</eissn><abstract>The chalcogenide perovskite
Ba
Zr
S
3
has attracted much attention as a promising solar absorber for thin-film photovoltaics. Here we use first-principles calculations to evaluate its carrier transport and defect properties. We find that
Ba
Zr
S
3
has a phonon-limited electron mobility of
37
cm
2
/
V s, which is comparable to that in halide perovskites, but lower hole mobility of
11
cm
2
/
V s. The defect computations indicate that
Ba
Zr
S
3
is intrinsically
n
-type due to shallow sulfur vacancies, but that strong compensation by sulfur vacancies will prevent attempts to make it
p
-type. We also establish that
Ba
Zr
S
3
shows some degree of defect tolerance, presenting only few low formation energy, deep intrinsic defects. Among the deep defects, sulfur interstitials are the dominant nonradiative recombination centers but exhibit a moderate capture coefficient. Our work highlights the material’s intrinsic limitations in carrier mobility and
p
-type doping, and suggests focusing on suppressing the formation of sulfur interstitials to achieve longer carrier lifetime.</abstract><doi>10.1103/PRXEnergy.3.033008</doi><orcidid>https://orcid.org/0000-0002-7200-5973</orcidid><orcidid>https://orcid.org/0000-0001-7840-4636</orcidid><orcidid>https://orcid.org/0000-0002-1422-1205</orcidid><orcidid>https://orcid.org/0009-0000-5746-7419</orcidid><orcidid>https://orcid.org/0000-0002-4609-9312</orcidid><orcidid>https://orcid.org/0000-0003-1754-2220</orcidid></addata></record> |
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language | eng |
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source | DOAJ Directory of Open Access Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals |
title | Assessing Carrier Mobility, Dopability, and Defect Tolerance in the Chalcogenide Perovskite Ba Zr S 3 |
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