Photovoltaics And Artificial Photosynthesis Solar Electricity And .

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Photovoltaics and Artificial Photosynthesis Solar Electricity and Solar FuelF.J. Himpsel, University of Wisconsin Madison

Electricity from the Sun is an ideal source of energy(fully convertible)0.4 TWUS ElectricityConsumption100 100 km2 of solar cells could produce all the electricity for the US.

The required area of solar cells1 kW/m2(Incident solar power) ¼(Useful daylight) 0.16(Efficiency of a solar cell) 1010 m2(100 100 km2) 0.4 TW Electric power consumed in the US0.7 TW could be generated by all the rooftops in the US (NREL study).

How much would it cost ?1 /W (Price of solar cells per Watt) 0.4 TW (Electric power generated in the US) 0.4 T 0.4 Trillion DollarsMechanical support structure adds significant costs.But one can design buildings to provide the support.

Electricity from sunlightAnnual Solar Cell Production(from PVNews)Rapid growth in China.Significant in Europe.US is behind , but greatlyimproved in recent years.

Price comparison: Solar versus fossil energy Solar energy is free, while fossil fuels need to be paid for. /kW versus /kWh Energy payback time matters for solar energy (1-4 years). Typical warranty is 25 years. The price of solar cells is less than 1 3 of the total cost.The rest is for support structure, converter, labor. Higher efficiency keeps support structure small.Forbes

Silicon solar cells dominate, but progress is slow(unlike Moore’s law: no miniaturization, mainly volume)1976SishortageSilicon Wafer TechnologiesModule price decreases by20% for every doubling ofcumulative productionPricewar200520102015NREL IRENA

Si solar cells dominate, but:Little room for improvement, twice the energy payback time Try everything: Nanoparticles, molecules, polymers, perovskites, Less material, low temperature processing Print solar cells roll-to-roll, like newspaperMaintain efficiency! Use existing support structuresThe rooftops in theUS could generateall of our electricity.Nanoparticle ink on metal foil

Cost versus efficiencyGoal1 /WLow endHigh endLow end designs are more cost-effective (less /W).Physics Today,March 2007, p. 37

Efficiency limit: 33% for a single junction(Shockley/Queisser)Lose the kinetic energy ofhot electrons1/3This part is convertedto electrical power1/3Lose photons below theband gap.1/3

Fuel from sunlight via artificial photosynthesisWater splitting 4H photoanodecathodeTachibana, Vayssieres, Durrant,Nature Photonics 6, 511 (2012)Efficient carrier transport by singlecrystal Fe2O3 nanorod photoanode(Vayssieres)

Design a solar cell from scratch.Have 4 energy levels, 3 materials to play with.EFe VOCEFAcceptor Absorber Donor Small energy drop: Large voltageLarge energy drop: Large currentWant both

Dye-sensitized solar cells combine 3 types of materialsNanoparticles Molecules ElectrolyteGrätzel, Nature 414, 338 (2001)and J. Phys. Chem. C 112 (2008)Lose half the voltageon the donor side.

Combine semiconductors with tailored band offsetsCIGSCIGSDiamond film as inert, transparentelectron donorEnergy levels from XAS, XPS, UPS,optical spectroscopyKapilashrami et al., J. Appl.Phys. 116, 143702 (2014).

Two end stations at an undulator beamline (BL8 at the ALS)Wed. Apr. 11, 2006Phy107 Lecture 3016

Need a tunable, polarized source of soft X-raysAdvanced Light Source (ALS)

Swiss Light SourceShanghai Light Source

Absorption spectroscopyLUMOambiguousunique, element‐specific

Polarization dependence Orbital orientationcos2 dipole pattern with a maximum when the polarizationvector is parallel to the orientation of the 2p orbitalTransitions from the C1s core level to C2p valence orbitalsCook et al., J. Chem. Phys. 131, 194701 (2009).

- and - bonds -bond: orbital * orbital- -bond: -orbital *-orbital(bonding)(antibonding)

Different projectionsof the density of statesFilled states:Photoemission: UPS, XPSX-ray emission spectr.: XESXASEmpty states:Inverse photoemission: IPESX-ray absorption spectr.: XASXASXAS: Cook et al., J. Chem. Phys. 134, 204707 (2011).IPES: Gao and Kahn, Org. Electron. 3, 53 (2002).

Calculated projections of the density of statesLevels get very denseat higher energy.Focus on the LUMO.LUMOCook et al., J. Chem. Phys.134, 204707 (2011).

Combine the 3 components of a solar cell in one moleculewith atomic perfectionto AcceptorDonor absorberSet record efficiency for dye-sensitized solar cells (12.3%)Grätzel group: Yella et al. Science 334, 629 (2011).

Probe the components individuallyDonorDonorAcceptor absorberAcceptor absorberCustom synthesis:Ragoussi et al., Eur. J. Org. Chem., Vol. 2013, p. 2832 (2013).

Identify specific atoms by their core levels and orbitals This led to improved synthesis. -A Weak point in the synthesis identifiedby theory (missing Zn atom). -A DDD- -AZegkinoglou et al., J. Phys. Chem. C 117, 13357 (2013).

Beyond energy levels: time-resolutionCarrier lifetime vs. charge transfer rateA dream experiment in photovoltaics and photoelectrochemistryProbe the carriers on theirway out with soft X-rays.The lifetimes of the charge carriersaffect the photocurrent dramatically.When and where are the carriers lost?(inside a molecule, across a device)Pump the center with visible.

“Heroic” experimentsNeed an X-ray laser to make such experiments accessible.Fe 2p edgepumpedDetect an excitationat a specific atom ina molecule.Huse et al., JACS 132, 6809 (2010)

Summary: pros and cons of solar energyNo fuel cost.Avoid paying hostile suppliers.Available everywhere.Avoid shortages, fluctuating oil price.Does not pollute.Avoid smog, mercury, fracking, Can be decentralized.Independence is a great incentive.Up-front investment.Energy storage overnight.Make solar fuel during the day(possibly PV-assisted water splitting),run fuel cell at night (Bloom box).

Solar energy is free, while fossil fuels need to be paid for. /kW versus /kWh Energy payback time matters for solar energy (1-4 years). Typical warranty is 25 years. The price of solar cells is less than 1 3 of the total cost. The rest is for support structure, converter, labor. Higher efficiency keeps support structure small. Price comparison: Solar versus fossil energy

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