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Electron–hole pair creation energy in amorphous selenium: geminate versus columnar recombination

Electron–hole pair creation energy in amorphous selenium: geminate versus columnar recombination

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2316972059

Electron–hole pair creation energy in amorphous selenium: geminate versus columnar recombination

About this item

Full title

Electron–hole pair creation energy in amorphous selenium: geminate versus columnar recombination

Publisher

New York: Springer US

Journal title

Journal of materials science. Materials in electronics, 2019-12, Vol.30 (24), p.21059-21063

Language

English

Formats

Publication information

Publisher

New York: Springer US

More information

Scope and Contents

Contents

Amorphous selenium (a-Se) is one of the most successful photoconductors for direct-conversion X-ray detectors. However, the initial carrier recombination is believed to be responsible for high electron–hole pair (EHP) creation energy in a-Se. The simultaneously generated electron and its hole twin can recombine (
geminate
recombination) or th...

Alternative Titles

Full title

Electron–hole pair creation energy in amorphous selenium: geminate versus columnar recombination

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2316972059

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2316972059

Other Identifiers

ISSN

0957-4522

E-ISSN

1573-482X

DOI

10.1007/s10854-019-02475-7

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