The present disclosure relates generally to nanoparticles, and more specifically, to exemplary embodiments of systems and method for providing and/or facilitating exemplary giant nonlinear optical responses from photon avalanching nanoparticles.
One of several advantages of the use of photon avalanching (PA) can be its combination of extreme nonlinearity and efficiency, which can be achieved without any periodic structuring or interference effects. PA was first observed over 40 years ago in Pr3+-doped bulk crystals, which exhibited a sudden increase in upconverted luminescence when excited beyond a critical pump laser intensity (IP). (See, e.g., Reference 3). Its discovery led to the development of other lanthanide-based bulk PA materials, utilized for example in efficient upconverted lasers (see, e.g., References 4-6 and 16), and its unique properties continue to spark interest over diverse fields. (See, e.g., References 6 and 7).
Thus, it may be beneficial to provide exemplary giant nonlinear optical responses from photon avalanching nanoparticles which can overcome at least some of the deficiencies described herein above.
To that end, exemplary nanoparticle and method for inducing photon avalanching using a nanoparticle can be provided. The nanoparticle can include, for example, at least 99% thulium doped nanocrystals of the nanoparticle. The nanoparticle can be composed of solely thulium. An atomic concentration of the thulium can be at least 8%. A near infrared excitation wavelength of the nanocrystals can be greater than about 1064 nm. The near infrared excitation wavelength can be between about 1400 nm to about 1490 nm. A passivated shell(s) can be included which can surround the nanocrystals.
A passivated shell(s) can be included which can surround the nanocrystals. For example, a Yb3+ sensitizer can be omitted from the nanoparticle.
Additionally, an exemplary nanoparticle for inducing photon avalanching can include a plurality of nanocrystals, where a combined size of the nanocrystals can be less than about 100 nanometers in three-dimensional space. A near infrared excitation wavelength of the nanocrystals can be greater than about 1064 nm. The near infrared excitation wavelength can be between about 1400 nm to about 1490 nm. A passivated shell(s) can be included, which can surround the nanocrystals.
These and other objects, features and advantages of the exemplary embodiments of the present disclosure will become apparent upon reading the following detailed description of the exemplary embodiments of the present disclosure, when taken in conjunction with the appended paragraphs.
Further objects, features and advantages of the present disclosure will become apparent from the following detailed description taken in conjunction with the accompanying Figures showing illustrative embodiments of the present disclosure, in which:
Throughout the drawings, the same reference numerals and characters, unless otherwise stated, are used to denote like features, elements, components or portions of the illustrated embodiments. Moreover, while the present disclosure will now be described in detail with reference to the figures, it is done so in connection with the illustrative embodiments and is not limited by the particular embodiments illustrated in the figures and the appended claims.
Photon avalanching can be a positive feedback system or method (see, e.g., Reference 6) that can be analogous to the second order phase transition of ferromagnetic spin systems, comparisons that have proven useful for modeling the process. (See, e.g., References 5 and 17). In lanthanide-based PA, a single ground-state absorption (“GSA”) event initiates a chain reaction of excited-state absorption (“ESA”) and cross-relaxation events between lanthanide (“Ln3+”) ions, resulting in the emission of many upconverted photons. (See e.g.,
Exemplary nanocrystal design can be based on: 1) a design paradigm for upconverting nanoparticles (“UCNPs”) emphasizing high Ln3+ content and energy confinement (see, e.g., References 23, 29, and 33-37; 2) the choice of Tm3+ (see, e.g.,
To determine whether PA occurs, three definitive criteria were analyzed (see, e.g., References 5 and 6): (i) stronger pump-laser-induced ESA compared to GSA, with the ratio of ESA to GSA rates exceeding 104 (R2/R1 shown in
Plots of Tm3+ emission at 800 nm versus 1064 nm pump intensity measured on nanoparticle ensembles drop-casted onto glass substrates show that as Tm3+ content can be increased from 1% to 4%, the degree of nonlinearity s also increases, but resides firmly in the energy looping regime, with s≤7. (See, e.g.,
To understand why 8% Tm3+ doping gives rise to such non-linear emission, the PA process in ANPs was modelled using coupled nonlinear differential rate equations. (See e.g., DREs; Tables 4-8). (See, e.g., References 17 and 40). Fitting the model to the experimental data for 8% Tm3+ ANPs (see, e.g.,
To observe the signature slow-down in excited-state population rise-times expected for PA (see, e.g., Reference 4, 6, 17 and 42), time-dependent luminescence from the Tm3+ 3H4 level (e.g., 800 nm emission) was measured. (See
The exemplary modeling also predicts PA for even longer-wavelength excitation near 1450 nm, resonant with ESA between 3F4 and 3H4 but not with GSA. (See e.g.,
Recent theoretical treatments show that achieving PA with a large nonlinearity can involve a balance between several coexisting phenomena within the material. (See, e.g., Reference 7). But in the case where the cross-relaxation rate s31>>W2, the DRE model can predict that threshold intensity can be determined entirely by W2. (See e.g., references 5 and 17). In ANPs, s31 can be controlled by Ln3+ concentration, while the nonradiative decay component of W2 can be dominated by losses at surfaces and interfaces. (See, e.g., References 29, 34, 35, 44, and 45). To determine if rebalancing these factors can reduce threshold intensity, two new 8% Tm3+ core/shell structures designed to reduce surface losses and thus W2 were synthesized. These designs include thicker shells as well as larger core size than the 8% ANPs in
Increasing the Tm3+ content can change s31 and W2, and therefore the PA excitation threshold intensity. To study this effect, core/shell ANPs with 20% and 100% Tm3+ were synthesized (e.g., including two sizes of 20% Tm3+ ANPs;
Exemplary models can predict a linear dependence between PA threshold intensity and W2, with a slope that can be determined by s31, W3 (e.g., the excited-state decay rate; see e.g.,
To evaluate the efficiency and relative brightness of ANPs, a kinetic computational model of ET within Ln3+-doped nanoparticles was used, similar to those used to reproduce the experimental upconverting quantum yields (“QYs”) of Er3+/Yb3+ co-doped UCNPs33,47, as well as ELNPs (see, e.g., Reference 22) (“SI”). The exemplary calculations reveal that for fully passivated core-shell nanoparticles, QY can reach approximately 40% for ANPs excited beyond threshold at 105 W cm−2. (See e.g.,
An application for ANPs can be single-particle superresolution imaging, as elucidated by the recently proposed photon-avalanche single-beam superresolution imaging (“PASSI”) concept that exploits the extreme nonlinear response of PA. (See, e.g., Reference 7). The size of the imaging point spread function in scanning confocal microscopy (“SCM”) scales inversely with the square root of the degree of nonlinearity s (e.g., as in multiphoton microscopy) (see, e.g., Reference 7), with the full width at half maximum (“FWHM”) of an imaged nonlinear emitter in SCM given by:
FWHM=λ/(2·NA·√s) (1)
in the Gaussian optics approximation (see, e.g., Reference 48) (e.g., where NA can be numerical aperture and λ can be wavelength). Therefore, deeply sub-wavelength resolution can be realized automatically with ANPs during standard SCM. The imaging may not need complex instrumentation, excitation beam shaping or patterning, image post-processing, or alignment procedures. (See, e.g., Reference 7).
Exemplary single-ANP imaging, measuring a PASSI image spot of ≤75 nm average FWHM when excited at 1064 nm at the optimal pump intensity for PASSI was performed, which corresponds to emission intensity at the top of the steep segment of the response curve. (See, e.g., Reference 7). More specifically, the image of the 8% Tm3+ ANP, from the batch with s=26 (e.g.,
Additionally, in characterizing this PA system, an approximately 500-10,000-fold increases in emission intensity was measured when pump intensity can be increased from threshold (IPth) to twice the threshold value, which can be beyond the steep-slope region of the ANP response curve. (See e.g.,
Further, steeply nonlinear nanomaterials, realizing photon avalanching in engineered nanocrystals at room temperature with continuous wave pumping were observed. Core-shell architectures doped with only Tm3+ ions exhibit avalanching behavior for Tm3+ concentrations ≥8% were observed, and that the PA excitation threshold intensity can be fully determined by the 3F4 intermediate state lifetime at higher concentrations. Further, PA can be achieved for excitation in the 1400-1470 nm range in addition to 1064 nm. Along with emission intensities that scale nonlinearly with pump intensity up to the 26th power—enabling sub-70 nm SCM imaging resolution and <2 nm photon localization—these results can open new applications in local environmental, optical, and chemical reporting, and in superresolution imaging.
Sodium trifluoroacetate (e.g., Na-TFA, 98%), sodium oleate, ammonium fluoride (“NH4F”), Yttrium chloride (“YCl3”, anhydrous, 99.99%), thulium chloride (“TmCl3”, anhydrous, 99.9+%), Gadolinium chloride (“GdCl3”, anhydrous, 99.99%), yttrium trifluoroacetate (e.g., 99.99+%), oleic acid (“Office Action”, 90%), and 1-octadecene (“ODE”, 90%) were purchased from Sigma-Aldrich.
The synthesis of NaY1-xTmxF4 ANP cores, with average diameters ranging from d=10 to 18±1 nm (see e.g., Table 1) was based on reported procedures. (See, e.g., Reference 44). For the case of x=0.01 (e.g., meaning 1% Tm3+ doping), YCl3 (e.g., 0.99 mmol, 193.3 mg) and TmCl3 (e.g., 0.01 mmol, 2.8 mg) were added into a 50 ml 3-neck flask, followed by an addition of 6 ml OA and 14 ml ODE. The solution was stirred under vacuum and heated to 100° C. for 1 hour. During this time, the solution became clear. After that, the flask was subjected to three pump/purge cycles, each consisting of refilling with N2 and immediately pumping under vacuum to remove water and oxygen. Thereafter, sodium oleate (e.g., 2.5 mmol, 762 mg) and NH4F (e.g., 4 mmol, 148 mg) were added to the flask under N2 flow. Subsequently, the resealed flask was placed under vacuum for 15 min at 100° C., followed by 3 pump/purge cycles. Subsequently, the flask was quickly heated from 100° C. to 320° C. (e.g., the approximate ramp rate was 25° C./min). The temperature was held at 320° C. for 40-60 min, after which the flask was rapidly cooled to room temperature with a stream of compressed air.
To isolate the nanoparticles, ethanol was added to the solution, and the precipitated nanoparticles were isolated by centrifugation (e.g., 5 min at 4000 rpm). The pellet was suspended in hexanes and centrifuged to remove large and aggregated particles. The nanoparticles remaining in the supernatant were washed two additional times by adding ethanol, isolating by centrifugation, and dissolving the pellet in hexanes. The nanoparticles were stored in hexanes with two drops of oleic acid to prevent aggregation.
A 0.1 M stock solution of 20% GdCl3 and 80% YCl3 was prepared by adding YCl3 (e.g., 2 mmol, 390.5 mg), GdCl3 (e.g., 0.5 mmol, 131.8 mg), 10 ml OA and 15 ml ODE to a 50 ml 3-neck flask. The solution was stirred and heated to 110° C. under vacuum for 30 min. After that, the flask was filled with N2 and heated to 200° C. for about 1 h, until the solution became clear and no solid was observed in the flask. Subsequently, the flask was cooled to 100° C. and placed under vacuum for 30 min. A 0.2 M solution of Na-TFA was prepared by stirring Na-TFA (e.g., 4 mmol, 544 mg), 10 ml OA and 10 ml ODE in a flask, under vacuum, at room temperature for 2 h, ensuring that all chemicals were dissolved. Using a nanoparticle synthesis robot, the
Workstation for Automated Nanocrystal Discovery and Analysis (“WANDA”), 3-9 nm NaY0.8Gd0.2F4 shells (see Table 1) were grown on ANP cores using a layer-by-layer protocol. (See, e.g., Reference 3). Briefly, for a 3 nm shell thickness, 6 mL ODE and 4 mL OA were added to the dried ANP cores and heated to 280° C. at 20° C./min in the WANDA glove box. The automated protocol alternated between injections of a 0.2 M Na-TFA stock solution and a 0.1 M stock solution of 20% Gadolinium and 80% Yttrium oleate solution. One injection was performed every 20 minutes for a total of 12 injections (e.g., 6 injections for each precursor). Following the last injection, each reaction was annealed at 280° C. for an additional 30 minutes and then cooled rapidly by nitrogen flow. The particles were isolated and purified according to the purification protocol described for ANP cores. Core-shell NaYF4 nanoparticles doped with Tm3+ (e.g., 1-100%) were synthesized using analogous methods.
TEM was performed using a JEOL JEM-2100F field emission transmission electron microscope (“TEM”) at an acceleration voltage of 200 kV, a FEI Themis 60-300 STEM/TEM operating at an acceleration voltage of 300 kV and a Tecnai T20 S-TWIN TEM operating at 200 kV with a LaB6 filament. Size statistics were acquired for approximately 100 nanoparticles using ImageJ software. X-Ray diffraction (“XRD”) measurement was performed using a Bruker D8 Discover diffractometer with Cu Kα radiation. Average core diameter and shell sizes are given in
Nanoparticles (e.g., 40 μL of a 1 μM suspension in hexane) were either drop-cast or spincoated on a coverslip. AFM measurements (e.g., Bruker Dimension AFM) were performed to measure the thicknesses of the films.
For single-ANP imaging, a dilute dispersion of nanoparticles was deposited on a glass coverslip and placed on an inverted confocal microscope (e.g., Nikon, Eclipse Ti-S inverted microscope). A 1064-nm continuous-wave diode laser (e.g., Thorlabs, FELH 750) or a Ti-sapphire pulsed laser (e.g., Coherent, Chameleon OPO Vis, 1390-1510 nm, 80 MHz) were directed into the back aperture of a 1.49 NA 100× immersion oil objective (e.g., Olympus), and focused directly to the sample on an 3D (e.g., XYZ) nanoscanning piezo stage (e.g., Physik Instrumente, P-545.xR8S Plano).
For measurements on film samples, a 0.95 NA 100× air objective lens (e.g., Nikon) was used. Emitted light was collected back through the same objective, filtered by 850-nm short-pass (e.g., Thorlabs, FESH 850) and 750-nm long-pass (e.g., Thorlabs, FELH 750) filters and sent to an EMCCD-equipped spectrometer (e.g., Princeton Instruments, ProEM: 16002 eXcelon™3) or a single-photon avalanche diode (e.g., Micro Photon Device, PDM series). For power dependence measurements, a neutral density wheel with a continuously variable density was used, synchronized with the collection system and automatically rotated by an Arduino-controlled rotator. Powers were simultaneously recorded by a Thorlabs power meter by using a glass coverslip to reflect approximately 10% of the incoming flux. Average excitation power densities were calculated using measured laser powers and using the 1/e2 area calculated from the imaged laser spot.
Samples were excited with a diode laser (e.g., Thorlabs) modulated at frequencies from 0.5 to 5 Hz by a function generator (e.g., Stanford Research Systems DS345). Emitted light collected by the 0.95 NA 100× objective (e.g., Nikon) was detected by a single photon avalanche diode (e.g., Micro Photon Device, PDM series). A time-correlated single-photon counting (“TCSPC”) device (Picoquant, Hydraharp 400) was used to record the timing data.
As discussed herein, a single ground-state absorption (“GSA”) event in lanthanide-based PA initiates a chain reaction of excited-state absorption (“ESA”) and cross-relaxation events between lanthanide (“Ln3+″”) ions, resulting in the emission of many upconverted photons. This mechanism amplifies the population of excited states, such as the 800-nm-emitting Tm3+ 3H4 level (
The ESA can be effective because the absorption peak for the electronic 3F2-3F4 transition can be close to the 1064 nm excitation wavelength. However, the 1064 nm photons can have an energy mismatch of approximately 1200 cm−1 for the electronic 3H6-3H5 transition, which decreases the GSA cross section at that wavelength. Due to the energetic mismatch, GSA can be a phonon-assisted process in this case, which makes its oscillator strength very small, approximately 104 times weaker than for excitation resonant with the purely electronic f-f transitions.
PA was first observed at low temperatures—and this can often be the case—though there have now been a fair amount of room temperature demonstrations in bulk systems. (See e.g., references 5-7, 18, and 51-55). In nanomaterials, however, the sensitivity of Ln3+ photophysics to local material properties can preclude the realization of PA and can hinder room temperature operation.
As noted in the main text, four key innovations were combined to design nanocrystals that can be capable of PA. The first can be the recent design paradigm for Ln3+-based upconverting nanoparticles (“UCNPs”), in which high Ln3+ content, engineered energy confinement, and reduced surface losses result in exceptional efficiencies and brightness. (See, e.g., References 23, 29, 33-37, and 56). A second feature can be the choice of Tm3+ (e.g.,
To determine if these design criteria enable nanocrystals to host PA, Tm3+-doped β-NaYF4 core/shell structures 16-33 nm in total diameter were synthesized. (See, e.g., References 29 and 33). As described in synthesis and shell growth sections above, the Tm3+-doped core in each ANP can be surrounded by an optically inert shell to minimize surface losses (see, e.g., Reference 33). (See e.g.,
Differential Rate equation (“DRE”) modelling of the Tm3+ doped system was performed based on the 3-level system. (See, e.g., Reference 1). The integrated rate equations can be expressed as:
These equations may involve the ground-state and excited-state absorption coefficients σGSA and σESA, radiative and non-radiative relaxation rates WiR and WiNR of level i (e.g., excluding cross-relaxation), the branching ratio b32, (e.g., the sum of radiative relaxation rates from the 3H4 level to intermediate levels divided by W3R), and the cross-relaxation rate s31. In addition, to consider the inverse process of the s31 cross relaxation, an inverse process of the cross relaxation (e.g., 3F4+3F4→3H6+3H4) and an upconversion process (e.g., 3F4+3F4→3H6+3F4) can be considered by the Q22n22 and Q23n22 terms, as in the model by S. Guy and F. Joubert.2 The populations ni of level i at steady state can be derived by solving the integrated rate equation with the Runge-Kutta 4th order method.
The radiative relaxation rates can be calculated using crystal Judd-Ofelt parameters for β-NaGdF4:Tm3+ which can have comparable lattice phonon energy3, and reduced matrix elements for Tm3+ ions (e.g., Table 5)4. The parameters that can be related to energy transfer between Tm3+ ions as a function of dopant concentration c can be expressed as, for example:
whereas σESA,W2NR,W3NR,acr,ainv, and auc can be derived from the fitting of simulation results to experimental data as shown in Tables 4 and 5. The nonradiative relaxation. W3NR can be approximately twice as high as W2NR, which seems reasonable considering the fact that the energy gap between the 3F4 and 3H6 level (e.g., approximately 4300 cm−1) can be somewhat smaller than that between the 3H4 and 3H5 levels (e.g., approximately 5700 cm−1). This model assumed W2NR and W3NR can be negligible for sample No. 5 because multiphonon relaxation rates of Ln3+ ions in LaF3 at the 3H4 and 3F4 levels can be calculated to be at least 4 order of magnitude smaller than other parameters,7,8 and the shell thickness of sample No. 5 can be over 6 nm, which was reported to be thick enough to prevent surface quenching.9
The result shows that the ratio of the ESA to GSA rates can be 10667, above 10000, a criterion for a clear avalanche threshold10. This high contrast of The ESA rate can be 1.83 times higher than that for Tm3+ doped silica fiber (e.g., Table 6). (See, e.g., Reference 11). That could be explained by, e.g., the phonon energy difference of the host lattices, along with linewidth narrowing. The coefficients of energy transfer between ions can be estimated at approximately 10% of those measure in YAG5. The decreases can also be attributed to the differences in phonon-assisted energy transfer depending on the host lattices, which has been shown by F. Auzel and F. Pelle12. The narrowing of absorption linewidths decreases the overlap of donor emission spectrum and acceptor absorption spectrum which reduces cross-relaxation energy transfer.
Absorption cross sections (e.g., σint,ESA), integrated over the entire ESA peak, can be calculated from Judd-Ofelt theory using the methods described in a recent review13. The ESA cross section σESA(
Exemplary theoretical quantum yield (“QY”) for the 3H4→3H6 transition (e.g., 800 nm) can be calculated by using the results from the DRE simulation. The equation can be expressed as:
(hv=pump photon energy)
Bulk materials other than NaYF4 have hosted photon avalanching, which suggests that there can be opportunities to develop an entire class of PA probes for imaging and sensing. This can be possible with both other dopants (e.g., Pr3+, Ho3+, Er3+ also possibly co-doped with Yb3+) and other crystalline host materials (e.g., (Li/K)(Y/Gd/Lu)F4, (La/Ce)(Cl/B)3, CdF2, Y2O3, YAG, YAlO3, LnVO4) or even heavy glasses (e.g., ZBLAN)15. Therefore, the demarcated for PA in nanoparticles (e.g., using PA preconditioning, lack of sensitizer, and surface passivation) can facilitate the design of a variety of PA wavelengths and their further biomedical and technological applications.
In general, the same factors that promote photon avalanche can encourage high nonlinearities, such as a high ESA/GSA ratio, high cross-relaxation and energy transfer rates relative to other relaxation pathways, as well as emission branching ratios. Notably, the phonon energy and density of states, and thus crystalline structure of the host also plays a role in the efficiency of the phonon-assisted GSA and CR. Reducing the phonon energy of a host can proportionally increase the number of phonons utilized to bridge energy gaps between excitation radiation and GSA transition energies, and, according to the Energy Gap Law, exponentially decrease GSA transition rates.
The exemplary system, method and computer-accessible medium, according to an exemplary embodiments of the present disclosure, can provide a method to design a library of lanthanide-doped photon avalanche nanoparticles. The CR rate s31 and relaxation rate W2 can be fine-tuned by varying the Ln3+ concentration and by surface passivation, respectively. For larger variations in composition, many material parameters can be interdependent, which can complicate predictions of the optimal materials for PA. Crystal structure can determine both site symmetry and phonon energies. Meanwhile changing dopant type results in different transition energies, cross-relaxation rates, and relaxation rates. Thus, in the future, high-throughput rate equation simulations that account for the above factors can be considered for rapidly screening the many combinations of material parameters for PA behavior.
For the sake of simplicity, but without any limitations, a Gaussian beam was used in all simulations. The Gaussian spot's FWHM can be established with a diffraction limit equation for pump beam λP=1064 nm and microscope objective NA=1.49 (e.g., to match experimental parameters). The definition of the beam was described by the equation S7.
This IG beam was scanned, by changing the position of the center (x0, y0) over either a single or a collection of 19.5×16 nm large homogenous ANPs, defined by a binary image TabNP(x,y) (0=no particle, 1=particle). The size of TabNP image defined the size of ultimate image, where each pixel corresponded to 1 nm in 2D space. The I0 was determined from the experimental “S” curves from
By multiplying the IG by TabNP, a new table can be created that represents the excitation intensity at the location of the NP.
I
P(x0, y0)=TabNP(x, y)·IG(x, y, x0, y0, I0, 1064) (10)
The experimental “S” shaped dependence between pump and emission intensities was used in the simulations ((IEMI=fun(IP)), and emission intensity at the position of the Gaussian excitation beam (x0, y0) was calculated (e.g.,
I
L(x0, y0)=Σx
The simulations of multi-point excitation PASSI parallel imaging were performed in a very similar way, with some modifications to emulate detection combined with photon localization analysis. Briefly, a hexagonal pattern of Gaussian beams was generated. (See e.g.,
At this point, these data were treated in a different way as compared to raster scanned imaging. Use of a 2D photodetector (e.g., a 2D pixel array) was assumed. Thus, every nanoparticle, excited with local pump intensity IP, became a source of a new diffraction limited Gaussian spot, whose luminescence intensity IP, was determined by the experimental “S” shaped power dependence, and FWHM was calculated for emission wavelength (e.g., λ=800 nm). These diffraction limited spots were cumulated on a virtual CCD imager. Due to the very steep power dependence of ANPs, the hexagonal beam excitation pattern stimulated reasonable avalanche luminescence only from those ANPs that were matching exact centers of excitation beams (e.g., green spots in
By then adopting the photon localization method and searching for local maxima, the positions of individual ANPs can be determined accurately. By shifting the hexagonal pattern (e.g.,
Photon avalanching materials were originally developed within the context of realizing new (e.g., efficient) lasers, and a number of successful demonstrations exist in literature. These bulk-material based PA results have been reviewed elsewhere. (See, e.g., References 1 and 2). As one can note, there can be many claims for PA (e.g., as slopes can be higher than 4 and simple ESA/ETU may not be enough to explain the UC process), but many can be unjustified as PA occurs when a few conditions can be satisfied simultaneously, for example, quasi linear power dependence below threshold AND saturation of luminescence at high pumping power and very high slopes (e.g., >10) above threshold AND power dependent slow rise times.
As shown in
Further, the exemplary processing arrangement 1805 can be provided with or include an input/output ports 1835, which can include, for example a wired network, a wireless network, the interne, an intranet, a data collection probe, a sensor, etc. As shown in
The foregoing merely illustrates the principles of the disclosure. Various modifications and alterations to the described embodiments can be apparent to those skilled in the art in view of the teachings herein. It can thus be appreciated that those skilled in the art can be able to devise numerous systems, arrangements, and procedures which, although not explicitly shown or described herein, embody the principles of the disclosure and can be thus within the spirit and scope of the disclosure. Various different exemplary embodiments can be used together with one another, as well as interchangeably therewith, as can be understood by those having ordinary skill in the art. In addition, certain terms used in the present disclosure, including the specification, drawings and claims thereof, can be used synonymously in certain instances, including, but not limited to, for example, data and information. It can be understood that, while these words, and/or other words that can be synonymous to one another, can be used synonymously herein, that there can be instances when such words can be intended to not be used synonymously. Further, to the extent that the prior art knowledge has not been explicitly incorporated by reference herein above, it can be explicitly incorporated herein in its entirety. All publications referenced can be incorporated herein by reference in their entireties.
3H6 → 3F4
3F4 → 3H5
3H5→ 3H4
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@593 nm
@535 nm
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The following references are hereby incorporated by reference, in their entireties:
This application relates to and claims priority from U.S. patent application Ser. No. 63/116,216, filed on Nov. 20, 2020, the entire disclosure of which is incorporated herein by reference.
This invention was made with government support under Grant Nos. DE-SC0019443 and DE-ACO2-02CH11231, awarded by the Department of Energy. The government has certain rights in the invention.
Number | Date | Country | |
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63116216 | Nov 2020 | US |
Number | Date | Country | |
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Parent | 17531266 | Nov 2021 | US |
Child | 18531271 | US |