A path to practical Solar Pumped Lasers via Radiative Energy Transfer

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received: 27 May 2015

accepted: 09 September 2015

Published: 05 October 2015

# A path to practical Solar Pumped Lasers via Radiative Energy Transfer

Philip D. Reusswig 1,* , Sergey Nechayev 2,* , Jennifer M. Scherer 3 , Gyu Weon Hwang 3 ,
Moungi G. Bawendi 3 , Marc. A. Baldo 1 & Carmel Rotschild 2

The optical conversion of incoherent solar radiation into a bright, coherent laser beam enables
the application of nonlinear optics to solar energy conversion and storage. Here, we present an
architecture for solar pumped lasers that uses a luminescent solar concentrator to decouple the
conventional trade-off between solar absorption efficiency and the mode volume of the optical gain
material. We report a 750-μm-thick Nd 3+ -doped YAG planar waveguide sensitized by a luminescent
CdSe/CdZnS (core/shell) colloidal nanocrystal, yielding a peak cascade energy transfer of 14%, a
broad spectral response in the visible portion of the solar spectrum, and an equivalent quasi-CW
solar lasing threshold of 23 W-cm −2 , or approximately 230 suns. The efficient coupling of incoherent,
spectrally broad sunlight in small gain volumes should allow the generation of coherent laser light
from intensities of less than 100 suns.

The conversion of broadband solar radiation into coherent and narrow-band laser radiation has attracted
attention in recent years due to its potential applicability in solar energy conversion. Solar pumped
lasers (SPL) can be used to drive reactions that store solar energy in chemical form 1, or perform efficient wavelength conversion of sub-bandgap sunlight, potentially increasing the efficiency of solar cells
beyond the single junction limit 2 . The first solar pumped laser was reported by RCA Laboratories in
1963 based on a Dy 2+ :CaF2 crystalline system 3 . Since then many advances in optical gain media and
solar collector design have occurred 1,4–8 . The most common optical gain media used in solar pumped
lasers today is the rare earth ion neodymium (Nd 3+ ) due to its natural four-level system, high emission
cross-section, and long excited state lifetime. Despite these favorable optical gain properties, neodymium is not an ideal solar absorber due to poor spectral overlap with sunlight and low peak absorption
coefficients, of < 10 cm −1 at λ ~ 800 nm that necessitate large optical gain media volumes. While larger
gain volumes result in increased solar pump absorption, the equivalent increase in mode volume cancels
out the increase in excitation density of the mode that is essential for reaching population inversion.
Consequently, state-of-the-art solar pumped lasers operate above 1000 suns. Nd 3+ :YAG laser rods, for
example, operate at power thresholds of 275 W-cm −2 utilizing large Fresnel lenses to concentrate sunlight 4 . Nd 3+ :YAG ceramics sensitized by Cr 3+ ions have broad absorption bands in the visible spectrum, and solar lasing thresholds of 160 W-cm −2 1,5 . S. Mizuno _et al._ demonstrated passive cooling of
a solar pumped laser through the use of a small volume Nd 3+ -doped glass fiber operating at a solar
lasing threshold of 370 W-cm −2 8 . Finally, Nd-Doped Active fiber sensitized by Rhodamine solution was
demonstrated to induce gain when pumped by Xenon lamp. Yet, the gain per input power was far from
lasing due to the high self-absorption and poor spectral overlap 9 . In this work we use cascade energy

1Department of Electrical Engineering and Computer Science, Massachusetts Institute of Technology, 77
Massachusetts Avenue, Cambridge, MA 02139, USA. 2 Department of Mechanical Engineering and Russell Berrie
Nanotechnology Institute, Technion-Israel Institute of Technology, Haifa 32000, Israel. 3 Department of Chemistry,
Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139, USA. * These authors
contributed equally to this work. Correspondence and requests for materials should be addressed to M.A.B.
[(email: baldo@mit.edu) or C.R. (email: carmelr@technion.ac.il)](mailto:baldo@mit.edu)

Figure 1. Illustration of cascade energy transfer for solar pumped lasers. A luminescent colloidal
nanocrystal film (yellow) is optically coupled to the planar optical gain waveguide (purple) (not to scale).
Incident sunlight is absorbed by the luminescent layer and largely re-emitted into waveguide modes. As the
luminescence propagates in the waveguide, energy is transferred to the optical gain media through optical
absorption. The optical gain media is then placed into a hemispherical resonator for a solar pumped laser
via cascade energy transfer.

Figure 2. ( a ) Measured absorption of the luminescent colloidal film, 10% wt. CdSe/CdZnS:PVB-CVACVAc (blue), overlaid on the AM1.5 solar flux (black). Sunlight can be efficiently absorbed by the colloidal
nanocrystals due to their broad and large absorption coefficients. ( b ) The luminescence of the nanocrystal
(red) is tuned to an absorption peak of the Nd 3+ :YAG (blue), for efficient waveguided luminescent pumping
of optical gain media.

transfer 10 to decouple solar pump absorption and optical gain, thereby enabling solar pumped lasers with
efficient solar absorption in small mode volumes. A schematic of the optical energy transfer process is
shown in Fig. 1. The scheme begins with incident sunlight absorbed by a layer of luminescent colloidal
semiconductor nanocrystals. These are ideal solar down-shifting materials due to their stability 11, narrow
photoluminescence spectrum, and high photoluminescence quantum yield, and broadband absorption
coefficients of - 10 5 cm −1 above an exciton absorption line that is tunable through size and material
composition 12 . The incident light absorbed by the nanocrystals is then re-emitted as photoluminescence.
As in the operation of a luminescent solar concentrator (LSC) 13,14, a fraction of the emitted photoluminescence is trapped within the waveguide formed by the optical gain media and its nanocrystal coating.
The fraction of emitted photons that is subject to total internal reflection is known as the trapping efficiency. A function of the refractive index 14, the trapping efficiency of wave-guided photoluminescence is
approximately 75% for typical dopant hosts such as polymers and glasses with n = 1.5.

The semiconductor nanocrystals are chosen such that their photoluminescence wavelength matches
an absorption peak of the optical gain medium (Fig. 2b). As the photoluminescence propagates in the
waveguide, energy is transferred to the optical gain media through absorption. The optical concentration
achieved in the waveguide can be increased by reducing its thickness, thereby enabling low threshold, small volume solar pumped lasers. This optical pumping scheme is general, and applicable to solar
down-shifting and optical gain materials in the visible and infrared portions of the solar spectrum.
Cascade energy transfer 10 enables large Stokes shifts between solar absorption and optical gain emission, a necessary condition for very-low-threshold daylight-pumped lasers as outlined by Roxio and
Yablonovitch 15 .

Figure 3. ( a ) Excitation spectra of a 750-μ m-thick Nd 3+ :YAG crystal (blue), and the same crystal with
a 10% wt. CdSe/CdZnS:PVB-CVA-CVAc coating (red). Scaled double pass absorption of the colloidal
nanocrystal film is shown as a dashed gray line. ( b ) Modelled Nd 3+ excited state distribution in the
Nd 3+ :YAG coated waveguide for incident photons of wavelength λ = 405 (blue dots), 531 (green dots), and
735 (red dots)nm from the Monte Carlo ray tracing simulation. The pump photon spatial distribution is
shown as a dashed gray line.

As a proof of principle, we constructed a solar-pumped laser based on a conventional 1% atomic Nd 3+
doped Yittrium Aluminum Garnet (YAG) gain medium that we ground and polished to form a planar
waveguide with length, width and thickness of 43 mm × 2 mm × 750 μ m, respectively. The Nd 3+ :YAG
waveguide was coated with a 15-μ m-thick poly(vinyl butyral-co-vinyl alcohol-co-vinyl acetate)
(PVB-CVA-CVAc) thin film containing 10% wt. colloidal CdSe/CdZnS nanocrystals, provided by QD
Vision, Inc. The colloidal nanocrystal quantum efficiency (QE), defined as the ratio between the number
of emitted and absorbed photons, is 75% when doped into PVB-CVA-CVAc, and the film is photostable
in air. The overlap between the solar spectrum and the absorption of the CdSe/CdZnS:PVB-CVA-CVAc
thin film can be seen in Fig. 2a, showing the broad spectral absorption of the nanocrystals between
350 nm and 600 nm. The narrow emission and tunability of the nanocrystal photoluminescence allows
for efficient pumping of the narrow absorption peaks of Nd 3+ :YAG. Indeed, as shown in Fig. 2b, the
CdSe/CdZnS photoluminescence is tuned to neodymium’s main absorption peak in the visible at 585 nm.
A disadvantage of the chosen nanocrystal emitter, however, is the small Stokes shift between absorption
and emission, which leads to reabsorption and eventually loss of the waveguided photoluminescence 16 .
Self-absorption losses can be reduced in future device iterations through energy transfer methods 10,17,
Stokes shift engineered nanocrystals 18,19, and optical techniques 20 to reduce the overlap between absorption and emission of the luminescent emitter.

To measure the efficiency of cascade energy transfer from input light to excited Nd 3+ ions, the
Nd 3+ :YAG waveguide is illuminated by monochromatic light at various wavelengths (see METHODS)
with and without a 15-μ m-thick 10% wt. CdSe/CdZnS:PVB-CVA-CVAc thin film. To increase the absorption of the incident light within the sample, a simple backing silver mirror is employed. Luminescence
from the sample is collected with an integrating sphere and 850 nm long pass wavelength filter is used
to discriminate between CdSe/CdZnS and Nd 3+ :YAG emission. The key parameter is the efficiency of
cascade energy transfer, which we define as the fraction of pump photon rate ultimately transferred
to Nd 3+ . Cascade energy transfer depends on the nanocrystal absorption, photoluminescent quantum
yield, the fraction of nanocrystal photoluminescence trapped in the waveguide, and the competition
between photoluminescence reabsorption losses in the nanocrystal film and waveguided pumping of the
optical gain media. As can be seen by the blue line in Fig. 3a, the poor absorption of isolated Nd 3+ :YAG
sample in the visible spectrum leads to very little energy transfer from the pump to the Nd 3+ . With the
addition of the thin film of CdSe/CdZnS:PVB-CVA-CVAc on the Nd 3+ :YAG waveguide, cascade energy
transfer generates a broad visible excitation spectrum with peak value of 14% that follows the absorption
profile of the nanocrystal (gray dotted line). Averaged over the solar spectrum out to the nanocrystal
absorption cutoff at λ = 600 nm, the waveguide pump efficiency due to the nanocrystal is 8.3%, resulting
in total pump efficiency of 9.7%; see grey dashed line and red line in Fig. 3a. For the bare cavity the
pump efficiency at similar spectral range is only 2.35%. This efficiency enhancement by a factor of 4.1
demonstrates the transfer of optical power to small volume optical gain media via a broadly absorbing
luminescent colloidal nanocrystal intermediate. A Monte Carlo ray tracing simulation was developed to
model the effect of cascade energy transfer on the distribution of excited Nd 3+ within the waveguide.
The inputs to the simulation are the sample geometry, the material’s spectral absorption coefficients
and refractive indices, photoluminescence spectrum, and photoluminescence quantum yield. An input
elliptical Gaussian beamshape is used to simulate concentrated input light, with full width half max
of FWHMW = 1 mm and FWHML = 26 mm along the width and length of the sample respectively. In

Figure 4. ( a ) Emission spectrum below (blue) and above (red) threshold. ( b ) Lasing power at λ = 1064 nm
versus pump intensity showing a lasing threshold at 14.54 W-cm −2 local pump intensity. Inset showing
nanocrystal photoluminescence versus pump intensity at t = 0 min and t = 1 min. Above 10 W-cm −2,
the steady-state stability of the polymer doped film is reduced. A quasi-CW pump was used for lasing
experiments.

Fig. 3b, we integrate along the length and the thickness of the Nd 3+ :YAG waveguide, and determine the
density of excited Nd 3+ ions per 100 μ m width across the sample. Normalization of this parameter with
the pump photon flux results in the relative distribution of Nd 3+ excited states. This pump distribution
analysis is done at three different pump wavelengths. Incident light at a wavelength of λ = 735 nm is
beyond the absorption edge of the nanocrystals and only excites neodymium ions. The resultant profile
of Nd 3+ excited states mirrors the non-uniformity of the pump intensity distribution. Absorption of incident light at λ = 405 nm, however, is dominated by the nanocrystals. Subsequent cascade energy transfer
produces a near uniform Nd 3+ population despite the non-uniformity in incident intensity. The improved
uniformity is a result of the relatively long absorption path length of waveguided photoluminescence
compared to the sample thickness. Modelling predicts that 15.3% of incident photons at λ = 405 nm are
transferred to Nd 3+ as compared to the measured 14%. The slight discrepancy between simulation and
experiment may be due to scattering at surfaces which is not included in the model. Finally, for pump
wavelengths such as λ = 531 nm, that excite neodymium and the nanocrystals, the resultant excited state
profile is a weighted average of direct absorption and cascade energy transfer. The modelled total integrated Nd 3+ excited states for pump wavelength of λ = 531 nm is 7.4% compared to the measured 6.3%.
These simulations indicate that cascade energy transfer results in improved uniformity of the excited
state population and thermal dissipation within the optical gain media.

To determine the laser threshold, the sample is placed in a hemispherical resonator as shown in
Fig. 1 and excited by a λ = 531 nm laser with spot size as defined in the Monte Carlo ray tracing simulation. We observe that the doped PVB-CVA-CVAc polymer films used in this study are thermally
stable for CW pumping below 10 W-cm −2 without active cooling, as seen in the inset of Fig. 4b. The
instability we observe at 10 W-cm −2 is due to the low glass transition temperature Tg ~ 75 °C 21 of the
host used. Consequently, we employ a quasi-CW scheme with pump pulse widths of approximately
10 ms to eliminate the possibility of thermal degradation of the down-shifting films. We observe both
spectral narrowing of the main Nd 3+ transition at λ = 1064 nm, as depicted in Fig. 4a, and threshold
behavior at an incident power of 7.9 W. Taking into account the illumination distribution, as simulated in
Fig. 3b, the maximal local flux of such pump at threshold is 14.54 W-cm −2 . Figure 4b shows the threshold characterization in terms of maximal local flux. This induces maximal local population inversion of
Nt = 8.45 × 10 21 Nd 3+ -m −3 . Because the excitation distribution occupies only part of the sample, a conservative estimation of the 531 nm pump that is required for lasing at the entire sample would be equal to
maximal photon flux of 14.54 W-cm −2 . Calculating the solar concentration required to induce the same
maximal flux must take into account the difference between the pumping efficiency at 531 nm (6.3%) and
the average pumping efficiency over the solar spectrum between 350 nm and 825 nm (6.8%; see red line
in Fig. 3a). In addition, because only 46% of the total solar flux is within this wavelength range the overall
solar pumping efficiency is 3.12%, leading to the required solar flux of 23 W-cm 2 or 230 suns. Averaging
the pump contribution of the NCs (gray line in Fig. 3a) over the solar spectrum shows that in the case
of Nd 3+ excitations generated only by NC emission, the laser will operate at pump threshold of 415 suns.

The lasing threshold, efficiency, and stability of the cascade energy transfer scheme can be improved
through three methods: (i) enhanced solar absorption with near-infrared (NIR) rather than visible spectrum colloidal nanocrystals 22, (ii) higher efficiency waveguide pumping using colloidal nanocrystals
with lower self-absorption through an increased Stokes shift 18,19 and higher photoluminescence quantum yield, and (iii) smaller mode volume optical gain media 23 . The dependence of the laser threshold
on the properties of the luminescent concentrator can be seen in Fig. 5. By moving to a NIR absorbing

Figure 5. The calculated lasing threshold of the presented system as a function of the absorption edge
of the luminescent colloidal nanocrystals and the efficiency of energy transfer to the gain medium,
disregarding direct solar absorption by Nd 3+ . The measured equivalent threshold solar concentration due
to cascade energy transfer reported in this work is marked as a star.

and emitting colloidal nanocrystal, the amount of photons available to the gain material would double,
reducing the gain threshold by a factor of two. However, a larger benefit is expected from improving
the waveguide pump efficiency, plotted on the x-axis in Fig. 5, which can be increased by improving
the in-film photoluminescence quantum yield of the colloidal nanocrystals and optimizing the Stokes
shift to reduce self-absorption of waveguided photoluminescence. Such improvements should not only
result in a reduced threshold power, but should also result in a reduction in heat generation within the
down-shifting film. The improvement of waveguide pumping efficiency and solar absorption in the NIR
could result in significant reduction in solar concentration threshold from this proof of principal system.

In conclusion, cascade energy transfer presents a path to efficient solar powered lasers operating
under passive cooling, and potentially in the non-tracking regime 24 . The pairing of luminescent colloidal nanocrystals with traditional optical gain media such as Nd 3+ and Tm 3+ allows the decoupling
of solar absorption from mode volume and enables solar laser operation from the visible to the near
infrared. Solar powered Tm 3+ lasers are especially notable because they potentially enable the efficient
up-conversion of sub-bandgap infrared sunlight for silicon solar cells.

Methods
The Nd 3+ :YAG slab waveguide was formed through conventional polishing techniques from commercial
laser rods of diameter 3 mm and length of 43 mm with λ = 1064 nm antireflection coatings on both
faces. Organic soluble CdSe/CdZnS colloidal semiconductor nanocrystals that emit at 585 nm were provided by QD Vision, Inc. The PVB-CVA-CVAc host was purchased from Sigma Aldrich. A solution of
100 mg/mL 10% wt. CdSe/CdZnS:PVB-CVA-CVAc in chloroform was drop cast onto the Nd 3+ :YAG
waveguide producing a film of 15 μ m thickness. The nanocrystal doped polymer film on glass was excited
at λ = 405 nm and the photoluminescence spectrum was recorded using a calibrated Ocean Optics spectrometer positioned perpendicular to the substrate. The Nd 3+ :YAG and Nd 3+ :YAG with CdSe/CdZnS:
PVB-CVA-CVAc film was excited with monochromatic light. An evaporated silver mirror was used
behind the sample to double the optical path length of incident light. The monochromatic light was generated using a tungsten bulb, monochromator with a spectral resolution of 3.5 nm full width at half maximum, and a mechanical chopper. The sample photoluminescence was measured with a lock-in amplifier,
spectrally calibrated photodetector, and long wavelength filters with a cutoff at λ = 850 nm were used
to discriminate between Nd 3+ :YAG and CdSe/CdZnS emission in the integrating sphere. Although the
fine structure of the Nd 3+ absorption is partly obscured by the resolution of the monochromator, its
spectral resolution does not affect calculations of the equivalent solar threshold obtained by integrating
the product of solar and device excitation spectra. The laser resonator is a hemispherical cavity with a
planar mirror of reflectivity 99.8% and an output mirror with a radius of curvature of 15 cm and reflectivity of 98%. A 18 W λ = 531 nm CW laser was used to optically excite the NC film coated Nd 3+: YAG
slab in air. An Acton spectrometer with a grating of 1000 grooves per mm and a calibrated Newport
photodetector and neutral density filter were used to measure the lasing spectrum and power threshold
of the laser respectively.

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Acknowledgments
This work was initially supported under the Center for Excitonics, an Energy Frontier Research Center
funded by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences and
subsequently by the Cooperative Agreement between the Masdar Institute of Science and Technology
(Masdar Institute), Abu Dhabi, UAE and the Massachusetts Institute of Technology. J.M.S. acknowledges
governmental support, awarded by the Department of Defense, Air Force Office of Scientific Research,
National Defense Science and Engineering Graduate (NDSEG) Fellowship. G.W.H. acknowledges
support by the US Army through the Institute of Soldier Nanotechnology. C.R. acknowledges the partial
supported by the Russell Berrie Nanotechnology Institute (RBNI), and the Grand Technion Energy
Program (GTEP) and comprises part of The Leona M. and Harry B. Helmsley Charitable Trust reports
on Alternative Energy series of the Technion, Israel Institute of Technology and the Weizmann Institute
of Science. Funding: U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, DESC0001088 (MIT); Cooperative Agreement between the Masdar Institute of Science and Technology
(Masdar Institute), Abu Dhabi, UAE and the MIT, 02/MI/MI/CP/11/07633/GEN/G/. Department of
Defense, Air Force Office of Scientific Research, National Defense Science and Engineering Graduate
(NDSEG) Fellowship, 32 CFR 168a, FA9550-11-C-0028. US Army, Institute of Soldier Nanotechnology,
W911NF-13-D-0001.

Author Contributions
P.D.R. and S.N. preformed the experiments, J.M.S. and G.W.H. made the quantum dots. M.G.B., M.A.B.
and C.R. conceived the idea and contributed to the writing of the paper.

Additional Information
Competing financial interests: The authors declare no competing financial interests.

How to cite this article : Reusswig, P. D. _et al._ A path to practical Solar Pumped Lasers via Radiative
Energy Transfer. _Sci. Rep._ 5, 14758; doi: 10.1038/srep14758 (2015).

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