@Article{PirralhoPSBPFRA:2017:TrNePo,
author = "Pirralho, M. J. P. and Peres, M. L. and Soares, D. A. W. and
Braga, P. C. O. and Pena, F. S. and Fornari, Celso Israel and
Rappl, Paulo Henrique de Oliveira and Abramof, Eduardo",
affiliation = "{Universidade Federal de Itajub{\'a} (UNIFEI)} and {Universidade
Federal de Itajub{\'a} (UNIFEI)} and {Universidade Federal de
Itajub{\'a} (UNIFEI)} and {Universidade Federal de Itajub{\'a}
(UNIFEI)} and {Universidade Federal de Itajub{\'a} (UNIFEI)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)}",
title = "Transition from negative to positive photoconductivity in p -type
P b1-x e uxTe films",
journal = "Physical Review B",
year = "2017",
volume = "95",
number = "7",
pages = "075202",
month = "Feb.",
abstract = "We investigated the photoconductivity effect in p-type Pb1-xEuxTe
films for x=0.01, 0.02, 0.03, 0.05, and 0.06 at T=300K. The
measurements revealed a clear transition from negative to positive
photoconductivity as the Eu content x is increased at room
temperature. This transition is related to the metal-insulator
transition that occurs due to the disorder originated from the
introduction of Eu atoms and it is an Anderson transition. Our
investigation found that, from the potential application point of
view, the sample x=0.06 is more suitable, i.e., it presents an
almost noise-free signal and the higher photoconductivity
amplitude response. The photoconductive amplitude response for the
sample with x=0.06 was investigated further in the temperature
range of 77-300 K and, surprisingly, multiple additional
transitions were observed with amplitudes that reached around 200
times the original value before illumination. We show that this
anomalous behavior is a consequence of the generation and
recombination rates between the bands and the 4f level and a
defect level located inside the band gap.",
doi = "10.1103/PhysRevB.95.075202",
url = "http://dx.doi.org/10.1103/PhysRevB.95.075202",
issn = "1098-0121",
language = "en",
urlaccessdate = "27 abr. 2024"
}