2024
DOI: 10.1039/d3dt03244b
|View full text |Cite
|
Sign up to set email alerts
|

Enhancing the inherent NIR photoluminescence in SrLaLiTeO6 through Cr3+–Yb3+ co-substitution for high performance pc-LEDs

Sariga C. Lal,
I. N. Jawahar,
Subodh Ganesanpotti

Abstract: NIR pc-LEDs developed with Cr3+ and Yb3+ co-doped SrLaLiTeO6 phosphor have promising applications in wearable biosensors and food analysis.

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2

Citation Types

0
2
0

Year Published

2024
2024
2025
2025

Publication Types

Select...
7

Relationship

0
7

Authors

Journals

citations
Cited by 9 publications
(2 citation statements)
references
References 66 publications
(106 reference statements)
0
2
0
Order By: Relevance
“…To comprehensively understand the thermal quenching behavior of MgNb 2 O 6 :Cr 3+ , the activation energy (Δ E ) was calculated by means of the Arrhenius equation, 25,52–54 where I 0 is the initial PL intensity of the luminescent materials at room temperature, I T is the PL intensity of a given absolute temperature T , K is the Boltzmann constant, and A is a constant. The thermal disturbance energy Δ E swas calculated to be 0.473 eV by the typical Arrhenius fitting shown in Fig.…”
Section: Resultsmentioning
confidence: 99%
“…To comprehensively understand the thermal quenching behavior of MgNb 2 O 6 :Cr 3+ , the activation energy (Δ E ) was calculated by means of the Arrhenius equation, 25,52–54 where I 0 is the initial PL intensity of the luminescent materials at room temperature, I T is the PL intensity of a given absolute temperature T , K is the Boltzmann constant, and A is a constant. The thermal disturbance energy Δ E swas calculated to be 0.473 eV by the typical Arrhenius fitting shown in Fig.…”
Section: Resultsmentioning
confidence: 99%
“…Furthermore, the activation energy (Δ E ) for thermal quenching is considered as the energy barrier for thermal quenching, which can be obtained by fitting the Arrhenius equation: 58–62 where I t is the emission intensity at temperature T , I 0 is the initial emission intensity, k is the Boltzmann constant (8.617 × 10 −5 eV K −1 ), and A is a constant. The Δ E was fitted to be 0.26 eV (Fig.…”
Section: Resultsmentioning
confidence: 99%