The MIT Libraries is completing a major upgrade to DSpace@MIT. Starting May 5 2026, DSpace will remain functional, viewable, searchable, and downloadable, however, you will not be able to edit existing collections or add new material. We are aiming to have full functionality restored by May 18, 2026, but intermittent service interruptions may occur. Please email dspace-lib@mit.edu with any questions. Thank you for your patience as we implement this important upgrade.

Show simple item record

dc.contributor.authorSinsermsuksakul, Prasert
dc.contributor.authorChakraborty, Rupak
dc.contributor.authorKim, Sang Bok
dc.contributor.authorHeald, Steven M.
dc.contributor.authorBuonassisi, Tonio
dc.contributor.authorGordon, Roy G.
dc.date.accessioned2013-04-02T20:25:31Z
dc.date.available2013-04-02T20:25:31Z
dc.date.issued2012-11
dc.date.submitted2012-10
dc.identifier.issn0897-4756
dc.identifier.issn1520-5002
dc.identifier.urihttp://hdl.handle.net/1721.1/78260
dc.description.abstractThin-film solar cells made from earth-abundant, inexpensive, and nontoxic materials are needed to replace the current technologies whose widespread use is limited by their use of scarce, costly, and toxic elements. Tin monosulfide (SnS) is a promising candidate for making absorber layers in scalable, inexpensive, and nontoxic solar cells. SnS has always been observed to be a p-type semiconductor. Doping SnS to form an n-type semiconductor would permit the construction of solar cells with p-n homojunctions. This paper reports doping SnS films with antimony, a potential n-type dopant. Small amounts of antimony (1%) were found to greatly increase the electrical resistance of the SnS. The resulting intrinsic SnS(Sb) films could be used for the insulating layer in a p-i-n design for solar cells. Higher concentrations (5%) of antimony did not convert the SnS(Sb) to low-resistivity n-type conductivity, but instead the films retain such a high resistance that the conductivity type could not be determined. Extended X-ray absorption fine structure analysis reveals that the highly doped films contain precipitates of a secondary phase that has chemical bonds characteristic of metallic antimony, rather than the antimony–sulfur bonds found in films with lower concentrations of antimony.en_US
dc.description.sponsorshipUnited States. Dept. of Energy. Sunshot Initiative (Contract DE-EE0005329)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Grant CBET-1032955)en_US
dc.language.isoen_US
dc.publisherAmerican Chemical Society (ACS)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1021/cm3024988en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alike 3.0en_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/en_US
dc.sourceOther University Web Domainen_US
dc.titleAntimony-Doped Tin(II) Sulfide Thin Filmsen_US
dc.typeArticleen_US
dc.identifier.citationSinsermsuksakul, Prasert et al. “Antimony-Doped Tin(II) Sulfide Thin Films.” Chemistry of Materials 24.23 (2012): 4556–4562.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Mechanical Engineeringen_US
dc.contributor.mitauthorChakraborty, Rupak
dc.contributor.mitauthorBuonassisi, Tonio
dc.relation.journalChemistry of Materialsen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsSinsermsuksakul, Prasert; Chakraborty, Rupak; Kim, Sang Bok; Heald, Steven M.; Buonassisi, Tonio; Gordon, Roy G.en
dc.identifier.orcidhttps://orcid.org/0000-0002-7043-5048
dc.identifier.orcidhttps://orcid.org/0000-0001-8345-4937
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record