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Plenarvorträge - DPG-Tagungen

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Halbleiterphysik Montag<br />

HL 12 Poster I<br />

Zeit: Montag 16:30–19:00 Raum: Poster A<br />

HL 12.1 Mo 16:30 Poster A<br />

Herstellung und Charakterisierung optisch gepumpter,<br />

oberflächenemittierender Halbleiterlaser — •S. Hövel 1 , N.C.<br />

Gerhardt 1 , M. Hofmann 1 , J. Yang 2 , D. Reuter 2 und A.D.<br />

Wieck 2 — 1 AG Optoelektronische Bauelemente und Werkstoffe, Ruhr-<br />

Universität Bochum — 2 Lehrstuhl für Angewandte Festkörperphysik,<br />

Ruhr-Universität Bochum<br />

Wir charakterisieren die Emission eines optisch gepumpten<br />

oberflächenemittierenden GaInAs/GaAs-Halbleiterlasers (engl. verticalcavity<br />

surface-emitting laser, VCSEL). Die Struktur wurde mittels<br />

Molekularstrahlepitaxie (engl. Molecular beam epitaxy, MBE) gewachsen.<br />

Sie enthält einen λ-Resonator mit drei 6 nm dicken Ga0.80In0.20As<br />

Quantenfilmen, platziert im Maximum des optischen Feldes. Als Spiegel<br />

wurden symmetrische GaAs/AlAs Bragg-Reflektoren (Oben: 16 Paare,<br />

Unten 19.5 Paare) verwendet. Der Laser emittiert bei 1000 nm mit einer<br />

Schwelle von 2.5kW/cm 2 bei Raumtemperatur und Anregung mit einem<br />

gepulsten Ti:Saphir-Laser (100 fs - Pulse bei 800 nm).<br />

Die Abhängigkeit der Laseremission von den Anregungsbedingungen<br />

wird analysiert und diskutiert.<br />

Wir danken der DFG für Unterstützung im GRK384 und SFB491.<br />

HL 12.2 Mo 16:30 Poster A<br />

Deep level transient spectroscopy on copper indium gallium<br />

diselenide thin film solar cells with different gallium content —<br />

•V. Mertens 1 , R. Reineke-Koch 2 , M. Köntges 2 , and J. Parisi 1 —<br />

1 University of Oldenburg, 26111 Oldenburg — 2 Instiute for Solar Engery<br />

Research, 31860 Emmerthal<br />

One approach to increase the open circuit voltage Voc of Cu(In, Ga)Se2<br />

solar cells is to widen the bandgap Eg by using higher gallium contents<br />

than in the standard composition which has a gallium to gallium plus indium<br />

ratio (GGI) of about 0.28. However further investigations on these<br />

materials showed that their Voc is lower than expected from the empirical<br />

relationship Voc = Eg −0.5V which holds for Eg ≤ 1.3eV . To understand<br />

more about the whole alloy system, we focused on the defects and the<br />

change in their characteristics with composition. For our measurements<br />

we use a home build deep level transient spectrometer based on a Boonton<br />

7200B capacitance bridge. We investigated different samples covering the<br />

whole alloy range with different DLTS techniques as majority and minority<br />

carrier DLTS, reverse-bias pulsed DLTS. We found that the transients<br />

are poorly described by a sum of several monoexponential decays. Therefore<br />

other analyses were conducted to determine the underlying physical<br />

mechanism.<br />

HL 12.3 Mo 16:30 Poster A<br />

Five source PVD for the deposition of CIGSS thin films —<br />

•Mario Gossla 1,2 and William N. Shafarman 1 — 1 Institute of Energy<br />

Conversion, University of Delaware, 451 Wyoming Road, Newark,<br />

DE 19716, USA — 2 Institut für Festkörperphysik, Friedrich-Schiller-<br />

Universität Jena, Max-Wien-Platz 1, 07743 Jena, Germany<br />

CuIn1−xGax(Se1−ySy)2 (CIGSS) films are being investigated as absorber<br />

layer materials for the wide-band-gap cell in a tandem or multijunction<br />

thin-film solar cell. To become a viable option for high performance<br />

photovoltaics, tandem or multijunction solar cells based on polycrystalline<br />

thin films will require a wide band gap top cell with at least<br />

15 % efficiency, optical band gap in the range 1.7 ≤ Eg ≤ 1.9 eV, and<br />

small sub-band gap absorption.<br />

A new five-source deposition system was developed for the deposition<br />

of CIGSS thin films. Thin films within the complete compositional range<br />

of 0 ≤ x ≤ 1, and 0 ≤ y ≤ 1 were deposited on Mo-coated soda lime<br />

glass at different temperatures. The films were analyzed by means of IR,<br />

SEM, and XRD. The incorporation of sulfur in the films depends strongly<br />

on the sulfur concentration in the vapor phase, substrate temperature,<br />

and Cu/In ratio. Complete Mo/CIGSS/CdS/-ZnO/NiAl solar cells with<br />

a typical area of 0.5 cm 2 were prepared. Cell performance was monitored<br />

by QE and I-V measurements and is shown to strongly depend on sulfur<br />

content.<br />

HL 12.4 Mo 16:30 Poster A<br />

Surface-heat-emittance optimization of CIS-based flexible solar<br />

cells — •Carsten Bundesmann 1 , Ferdinand Dürr 1,2 , Mathias<br />

Schubert 1 , and Karsten Otte 2 — 1 Fakultät für Physik und<br />

Geowissenschaften, Institut für Experimentelle Physik II, Universität<br />

Leipzig, Linnéstraße 5, 04103 Leipzig — 2 Solarion GmbH, Ostende 5,<br />

04288 Leipzig<br />

CuInSe2 based flexible thin film solar cells on polyimide substrates are<br />

possible alternatives for crystalline silicon or GaAs based solar cells in<br />

space applications due to their low weight. Still their feasibility has to be<br />

proven. In order to achieve high specific power (W/kg), important optimization<br />

parameters parameters are, for instance, efficiency and surface<br />

heat emittance. The later is studied here for CuInSe2 based thin film solar<br />

cells grown on flexible polyimide substrates in a web-coater based process.<br />

It is shown that the maximum values of the surface heat emittance<br />

depends strongly on the layer structure and the layer optical properties.<br />

The dielectric functions of each single layer is extracted by infrared spectroscopic<br />

ellipsometry. Using these data a layer model is established, the<br />

reflectivity and the surface heat emittance is calculated. Upon varying<br />

the model parameters the maximum of the surface heat emittance is determined.<br />

The simulated results are compared with measured values of<br />

real solar cell structures.<br />

HL 12.5 Mo 16:30 Poster A<br />

Stray current contributions in photo-assisted tunneling spectroscopy<br />

on CIGSe absorbers: an aid or a nuisance? — •U.<br />

Herber 1 , C. Heske 1 , E. Umbach 1 , F. Karg 2 , T. P. Niesen 2 ,<br />

G. Hanna 3 , and U. Rau 3 — 1 Experimentelle Physik II, Universität<br />

Würzburg, 97074 Würzburg — 2 Shell Solar, München — 3 Institut für<br />

Physikalische Elektronik, Universität Stuttgart, 70569 Stuttgart<br />

Polycrystalline Cu(In,Ga)Se2 solar cell absorbers are investigated with<br />

photo-modulated scanning tunneling spectroscopy. For RTP (rapid thermal<br />

processing) absorbers, we find pronounced lateral inhomogeneities of<br />

the photo-induced tunneling current (PITC), as reported earlier [1]. In<br />

addition, similar inhomogeneities are also found on co-evaporated CIGSe<br />

absorbers.<br />

However, every modulated process in scanning probe microscopies is<br />

accompanied by stray effects, in particular by an additional current contribution<br />

via the capacitance between sample and tip. The complex phase<br />

and amplitude of this stray signal can be measured separately, and thus<br />

its contribution can be subtracted from the PITC scan data. On the other<br />

hand, the stray signal is strongly determined by the (chemical) condition<br />

of the surface. The situation within a series of sputter-and-heat cycles<br />

is compared with corresponding photo-emission data and interpreted in<br />

the framework of the equivalent circuit approach.<br />

[1] D. Eich et al., Thin Solid Films 361, 258 (2000)<br />

HL 12.6 Mo 16:30 Poster A<br />

Epitaxial growth of CuGaS2 on Si substrates investigated by<br />

high resolution X-ray diffraction — •J. Cieslak 1 , A. Dietz 1 , J.<br />

Eberhardt 1 , M. Gossla 1 , Th. Hahn 1 , J. Kräusslich 2 , H. Metzner<br />

1 , U. Reislöhner 1 , W. Witthuhn 1 , and F. Wunderlich 2 —<br />

1 Friedrich-Schiller-Universität Jena, Institut für Festkörperphysik, Max-<br />

Wien-Platz 1, 07743 Jena — 2 Friedrich-Schiller-Universität Jena, Institut<br />

für Optik und Quantenelektronik Max-Wien-Platz 1, 07743 Jena<br />

The wide-band gap chalcopyrite semiconductor CuGaS2 (CGS) has recently<br />

attracted some attention since its direct band gap of Egap=2.5eV<br />

(T=5K) makes it suitable for applications in tandem solar cells. We reported<br />

the epitaxial growth of high-quality CGS layers on Si(111) [1].<br />

In this work we elucidate the epitaxial growth and structural properties<br />

of these heteroepitaxial layers. High resolution X-ray diffraction<br />

(HRXRD) was performed at the European Synchrotron Radiation Facility<br />

(ESRF) in Grenoble (France). High-precision ω/2θ-scans with different<br />

in-plane diffraction vectors were carried out.<br />

It was found, that the CGS layers show lattice parameters resembling<br />

those reported in literature for bulk material and that any existence of<br />

metastable ordering, prominent in epitaxial layers of CuInS2, can be ruled<br />

out. This behaviour is discussed within the context of the observed epitaxial<br />

relations between CGS and Si(111) as well as Si(100) substrates.<br />

[1] H. Metzner et al., Appl. Phys. Lett., 81(1), 156 (2002).

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