8 research outputs found
Spectral Properties and Energy Transfer between Ce<sup>3+</sup> and Yb<sup>3+</sup> in the Ca<sub>3</sub>Sc<sub>2</sub>Si<sub>3</sub>O<sub>12</sub> Host: Is It an Electron Transfer Mechanism?
The downshifting
from Ce<sup>3+</sup> blue emission to Yb<sup>3+</sup> near-infrared
emission has been studied in the garnet host Ca<sub>2.8–2<i>x</i></sub>Ce<sub>0.1</sub>Yb<sub><i>x</i></sub>Na<sub>0.1+<i>x</i></sub>Sc<sub>2</sub>Si<sub>3</sub>O<sub>12</sub> (<i>x</i> = 0–0.36).
The downshifting does not involve quantum cutting, but one incident
blue photon is transferred from Ce<sup>3+</sup> to Yb<sup>3+</sup> with an energy transfer efficiency up to 90% when <i>x</i> = 0.36 for the Yb<sup>3+</sup> dopant ion. For <i>x</i> ≤ 0.15, a multiphonon-assisted electric dipole–electric
quadrupole mechanism of energy transfer dominates, while for the highest
concentration of Yb<sup>3+</sup> employed, the electron transfer mechanism
is confirmed. A temperature-dependent increase of the Ce<sup>3+</sup> → Yb<sup>3+</sup> energy transfer rate does not exclusively
indicate the electron transfer mechanism. The application of the material
to solar energy conversion is indicated
Site Occupancies, Luminescence, and Thermometric Properties of LiY<sub>9</sub>(SiO<sub>4</sub>)<sub>6</sub>O<sub>2</sub>:Ce<sup>3+</sup> Phosphors
In this work, we
report the tunable emission properties of Ce<sup>3+</sup> in an apatite-type
LiY<sub>9</sub>(SiO<sub>4</sub>)<sub>6</sub>O<sub>2</sub> compound
via adjusting the doping concentration or temperature. The occupancies
of Ce<sup>3+</sup> ions at two different sites (Wyckoff 6h and 4f
sites) in LiY<sub>9</sub>(SiO<sub>4</sub>)<sub>6</sub>O<sub>2</sub> have been determined by Rietveld refinements. Two kinds of Ce<sup>3+</sup> f–d transitions have been studied in detail and then
assigned to certain sites. The effects of temperature and doping concentration
on Ce<sup>3+</sup> luminescence properties have been systematically
investigated. It is found that the Ce<sup>3+</sup> ions prefer occupying
Wyckoff 6h sites and the energy transfer between Ce<sup>3+</sup> at
two sites becomes more efficient with an increase in doping concentration.
In addition, the charge-transfer vibronic exciton (CTVE) induced by
the existence of free oxygen ion plays an important role in the thermal
quenching of Ce<sup>3+</sup> at 6h sites. Because of the tunable emissions
from cyan to blue with increasing temperature, the phosphors LiY<sub>9</sub>(SiO<sub>4</sub>)<sub>6</sub>O<sub>2</sub>:Ce<sup>3+</sup> are endowed with possible thermometric applications
Combined Experimental and ab Initio Study of Site Preference of Ce<sup>3+</sup> in SrAl<sub>2</sub>O<sub>4</sub>
Low-temperature
photoluminescence properties of Sr<sub>1–2<i>x</i></sub>Ce<sub><i>x</i></sub>Na<sub><i>x</i></sub>Al<sub>2</sub>O<sub>4</sub> (<i>x</i> = 0.001) synthesized
by a solid-state reaction method are measured with excitation energies
in the vacuum ultraviolet (VUV) to ultraviolet (UV) range. Two distinct
activator centers with different emission and excitation intensities
are observed and attributed to Ce<sup>3+</sup> occupying the Sr1 and
Sr2 sites of SrAl<sub>2</sub>O<sub>4</sub> with different probabilities.
Hybrid density functional theory (DFT) calculations within the supercell
model are then carried out to optimize the local structures of Ce<sup>3+</sup> located at the two Sr sites of SrAl<sub>2</sub>O<sub>4</sub>, on which wave function-based CASSCF/CASPT2 embedded cluster calculations
with the spin–orbit effect are performed to derive the Ce<sup>3+</sup> 4f<sup>1</sup> and 5d<sup>1</sup> energy levels. On the
basis of the observed relative spectral intensities, the calculated
DFT total energies, and the comparison between experimental and calculated
4f → 5d transition energies, we conclude that, in SrAl<sub>2</sub>O<sub>4</sub>:Ce<sup>3+</sup>, the dopant Ce<sup>3+</sup> prefers
to occupy the slightly smaller Sr2 site, rather than the larger Sr1
site as proposed earlier. Furthermore, by using an established linear
relationship between the lowest 4f → 5d transition energies
of Ce<sup>3+</sup> and Eu<sup>2+</sup> located at the same site of
a given compound, we find that, in SrAl<sub>2</sub>O<sub>4</sub>:Eu<sup>2+</sup>, the dominant green emission observed at room temperature
arises from Eu<sup>2+</sup> located at the Sr2 site of SrAl<sub>2</sub>O<sub>4</sub>
Excitation Wavelength Dependent Luminescence of LuNbO<sub>4</sub>:Pr<sup>3+</sup>î—¸Influences of Intervalence Charge Transfer and Host Sensitization
A series
of LuNbO<sub>4</sub>:Pr<sup>3+</sup> phosphors was prepared
by a solid-state reaction method at high-temperature. Rietveld refinements
were performed based on powder X-ray diffraction (XRD) data. Diffuse
reflectance spectra (DRS), UV–vis photoluminescence (PL), time-resolved
emission spectra (TRES), and fluorescence decays were utilized to
study the luminescence and host sensitization processes of Pr<sup>3+</sup> in LuNbO<sub>4</sub>. Excitation wavelength dependent luminescence
of LuNbO<sub>4</sub>:Pr<sup>3+</sup> was investigated and explained
in consideration of the processes of nonradiation relaxation via cross-relaxation,
multiphonon relaxation, and crossover to the intervalence charge transfer
(IVCT) state. Furthermore, the host sensitization of Pr<sup>3+</sup> emission in LuNbO<sub>4</sub> was confirmed and the energy transfer
efficiency from host to Pr<sup>3+</sup> increased with increasing
Pr<sup>3+</sup> doping concentration/temperature. Because the change
of emission intensities for both blue from the host and red from <sup>1</sup>D<sub>2</sub> is sensitive to temperature, a large variation
of emission color is observed between RT and 500 K
Cellulose-Based Composite Macrogels from Cellulose Fiber and Cellulose Nanofiber as Intestine Delivery Vehicles for Probiotics
Cellulose-based
composite macrogels made by cellulose fiber/cellulose
nanofiber (CCNM) were used as an intestine delivery vehicle for probiotics.
Cellulose nanofiber (CNF) was prepared by a 2,2,6,6-tetramethylpiperidine-1-oxyl
radical (TEMPO)-mediated oxidation system, and the carboxyl groups
in CNF acted as pore size and pH responsibility regulators in CCNMs
to regulate the probiotics loading and controlled release property.
The macrogel presented a porosity of 92.68% with a CNF content of
90%, and the corresponding released viable <i>Lactobacillus plantarum</i> (<i>L. plantarum</i>) was up to 2.68 Ă— 10<sup>8</sup> cfu/mL. The porous structure and high porosity benefited <i>L. plantarum</i> cells to infiltrate into the core of macrogels.
In addition, the macrogels made with high contents of CNF showed sustainable
release of <i>L. plantarum</i> cells and delivered enough
viable cells to the desired region of intestine tracts. The porous
cellulose macrogels prepared by a green and environmental friendly
method show potential in the application of fabricating targeted delivery
vehicles of bioactive agents
Vacuum Referred Binding Energy Scheme, Electron–Vibrational Interaction, and Energy Transfer Dynamics in BaMg<sub>2</sub>Si<sub>2</sub>O<sub>7</sub>:Ln (Ce<sup>3+</sup>, Eu<sup>2+</sup>) Phosphors
The
host structure and the synchrotron radiation VUV–UV
luminescence properties of samples BaMg<sub>2</sub>Si<sub>2</sub>O<sub>7</sub> (BMSO):Ln (Ce<sup>3+</sup>, Eu<sup>2+</sup>) at different
doping levels and different temperatures were investigated in detail.
Three important aspects are studied to elucidate the luminescence
properties of samples: (1) the vacuum referred binding energy (VRBE)
scheme is constructed with the electron binding in the BMSO host bands
and in the Ce<sup>3+</sup> and Eu<sup>2+</sup> impurity levels with
the aim to explain the different thermal stabilities of Ce<sup>3+</sup> and Eu<sup>2+</sup> emissions; (2) the electron–vibrational
interaction analysis on the narrow Eu<sup>2+</sup> emission indicates
a weak electron–phonon interaction in the current case; (3)
by using three models (Inokuti–Hirayama, Yokota–Tanimoto,
and Burshteĭn models) at different conditions, the energy transfer
dynamics between Ce<sup>3+</sup> and Eu<sup>2+</sup> was analyzed.
It reveals that the energy transfer from Ce<sup>3+</sup> to Eu<sup>2+</sup> via electric dipole–dipole (EDD) interaction is dominant
while energy migration between Ce<sup>3+</sup> is negligible. Finally,
the X-ray excited luminescence spectra of samples BMSO:Ce<sup>3+</sup>/Eu<sup>2+</sup> are collected to evaluate their possible scintillator
applications
Spectroscopy and Luminescence Dynamics of Ce<sup>3+</sup> and Sm<sup>3+</sup> in LiYSiO<sub>4</sub>
The lithium yttrium silicate series
of LiY<sub>1–<i>x</i></sub>Ln<sub><i>x</i></sub>SiO<sub>4</sub> exhibits
superb chemical and optical properties, and with Ln = Ce<sup>3+</sup>, Sm<sup>3+</sup>, its spectroscopic characteristics and luminescence
dynamics are investigated in the present work. Energy transfer and
nonradiative relaxation dramatically influence the Ln<sup>3+</sup> luminescence spectra and decay dynamics, especially in the Ce<sup>3+</sup>–Sm<sup>3+</sup> codoped phosphors. It is shown that
thermal-quenching of the blue Ce<sup>3+</sup> luminescence is primarily
due to thermal ionization in the 5d excited states rather than multiphonon
relaxation, whereas cross-relaxation arising from electric dipole–dipole
interaction between adjacent Sm<sup>3+</sup> ions is the leading mechanism
that quenches the red Sm<sup>3+</sup> luminescence. In the codoped
systems, Ce<sup>3+</sup>–Sm<sup>3+</sup> energy transfer in
competing with the thermal quenching enhance the emission from Sm<sup>3+</sup>. The combined influences of concentration quenching, thermal
ionization, and energy transfer including cross-relaxation on the
luminescence intensity of single-center and codoped phosphors are
analyzed based on the theories of ion–ion and ion–lattice
interactions
Spectral Properties and Energy Transfer of a Potential Solar Energy Converter
The
energy transfer between Ce<sup>3+</sup> and Eu<sup>2+</sup> has been
investigated in the host Ca<sub>3</sub>Sc<sub>2</sub>Si<sub>3</sub>O<sub>12</sub> (CSS), prepared by a modified sol–gel
method. Excitation and emission measurements from the near-infrared
to the vacuum ultraviolet spectral regions have been performed upon
CSS, Ce<sup>3+</sup>-doped CSS, Eu<sup>2+</sup>-doped CSS and Ce<sup>3+</sup>, Eu<sup>2+</sup>-co-doped CSS, at various concentrations,
including experiments at temperatures range of 15–460 K. The
energy transfer efficiency from Ce<sup>3+</sup> to Eu<sup>2+</sup> can approach 90%, and the Ce<sup>3+</sup> donor decay curves for
different Eu<sup>2+</sup> acceptor concentrations in the codoped system
were fitted by the Inokuti–Hirayama method, indicating that
it is energy transfer induced by electric dipole interaction. The
use of the Ce<sup>3+</sup>, Eu<sup>2+</sup> couple in the CSS host
as a wideband harvester with an emission profile tailored to the response
of the silicon solar cell in solar energy conversion suffers from
two main drawbacks relating to valence instability and emission quenching
of Eu<sup>2+</sup>. Possible solutions are suggested