2014
DOI: 10.1134/s1063783414020267
|View full text |Cite
|
Sign up to set email alerts
|

Luminescence of LaBr3: Ce,Hf crystals under photon excitation in the ultraviolet, vacuum ultraviolet, and X-ray ranges

Abstract: Abstract-This study has been carried out using synchrotron radiation, time resolved luminescence ultraviolet and vacuum ultraviolet spectroscopy, optical absorption spectroscopy, and thermal activation spectroscopy. It has been found that, in scintillation spectrometric crystals LaBr 3 : Ce,Hf characterized by a low hygroscopicity, along with Ce 3+ centers in regular lattice sites, there are Ce 3+ centers located in the vicinity of the defects of the crystal structure. It has also been found that the studied c… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2

Citation Types

0
1
0
1

Year Published

2015
2015
2024
2024

Publication Types

Select...
6
1

Relationship

0
7

Authors

Journals

citations
Cited by 13 publications
(2 citation statements)
references
References 17 publications
0
1
0
1
Order By: Relevance
“…Cerium ions are in favor for industry, but praseodymium has shorter decay time, and its emission is located at shorter wavelengths. In comparison with impurity Ce 3+ ions, praseodymium emission is located in higher energy region and has shorter lifetime (20-30 ns instead of 30-60) [4][5][6][7][8][9].…”
Section: Introductionmentioning
confidence: 98%
“…Cerium ions are in favor for industry, but praseodymium has shorter decay time, and its emission is located at shorter wavelengths. In comparison with impurity Ce 3+ ions, praseodymium emission is located in higher energy region and has shorter lifetime (20-30 ns instead of 30-60) [4][5][6][7][8][9].…”
Section: Introductionmentioning
confidence: 98%
“…В сцинтилляционной практике в настоящее время чаще используются примесные ионы Ce 3+ , но у соединений с примесью ионов Pr 3+ наблюдается более короткое время распада, и спектр излучения локализован в более коротковолновой области спектра. По сравнению с примесными ионами Ce 3+ кинетика затухания межконфигурационных d− fпереходов в ионах Pr 3+ характеризуется временем затухания 20−30 ns вместо 30−60 ns у ионов Ce 3+ [4][5][6][7][8][9].…”
Section: Introductionunclassified