91探花

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding 91探花
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
91探花
One of the substrate layouts for our organic solar cells
Credit: AFMD Group

Moritz Riede

Professor of Soft Functional Nanomaterials

Research theme

  • Photovoltaics and nanoscience

Sub department

  • Condensed Matter Physics

Research groups

  • Advanced Functional Materials and Devices (AFMD) Group
moritz.riede@physics.ox.ac.uk
Telephone: 01865 (2)72377 (office),01865 (2)82095 (lab)
  • About
  • Research
  • Teaching
  • Publications

Comment on "Roles of donor and acceptor nanodomains in 6% efficient thermally annealed polymer photovoltaics" [Appl. Phys. Lett. 90, 163511 (2007)]

Applied Physics Letters 92:7 (2008)

Authors:

MK Riede, T Mueller, B Maennig, K Leo, KO Sylvester-Hvid, B Zimmermann, M Niggemann, A Gombert

Analyzing poly(3-hexyl-thiophene):1-(3-methoxy-carbonyl)propyl-1-phenyl- (6,6) C61 bulk-heterojunction solar cells by UV-visible spectroscopy and optical simulations

Journal of Applied Physics 102:5 (2007)

Authors:

KO Sylvester-Hvid, T Ziegler, MK Riede, N Keegan, M Niggemann, A Gombert

Abstract:

A nondestructive method for assessing the thickness of the photoactive layer in poly(3-hexyl-thiophene):1-(3-methoxy-carbonyl)propyl-1-phenyl- (6,6) C61 (P3HT:PCBM) solar cells is reported. In the approach the absorption spectrum of the solar cell as derived by optical simulations is fitted to the corresponding measured spectrum, varying only the P3HT:PCBM layer thickness. Within the 50-250 nm thickness range, a linear correlation between the position of a certain spectral minimum and the P3HT:PCBM layer thickness is shown, based on simulated absorption spectra. As an initial application, absorption spectra for 240 P3HT:PCBM solar cells prepared at four different spin-coating speeds were recorded, and the average P3HT:PCBM layer thickness estimated for each spin-coating speed. The simulated fraction of light absorbed in the P3HT:PCBM layer of the solar cells is compared with the P3HT:PCBM absorption spectra measured for films spin coated on simpler substrate types. The latter spectra cannot account for the light harvested in the photoactive layer of P3HT:PCBM solar cells because of substantial optical interference in the solar cells. The measured short circuit current densities Jsc for the solar cells vary with the spin-coating speed in a manner confirmed by optical simulations of the maximal short circuit current densities. The measured efficiencies follow the same pattern. On average the measured Jsc is 1-2 mA cm2 below the simulated maximal short circuit current densities. Based on the resemblance of the measured and simulated absorption spectra such difference can be attributed to recombination exclusively. 漏 2007 American Institute of Physics.

Efficiency limiting factors of organic bulk heterojunction solar cells identified by electrical impedance spectroscopy

Solar Energy Materials and Solar Cells 91:5 (2007) 390-393

Authors:

M Glatthaar, M Riede, N Keegan, K Sylvester-Hvid, B Zimmermann, M Niggemann, A Hinsch, A Gombert

Abstract:

The current-voltage characteristic and the performance of organic bulk-heterojunction solar cells are very sensitive to small variations in the production steps or environmental influences. In our experiments, we found a large variation of the short-circuit current, which does not correspond to the device thickness as one might expect. The fill factor of some devices is below 25% under illumination, while the best devices have a fill factor of about 70%. Electrical impedance spectroscopy can provide information about the conductivity of different regions within the device. In earlier measurements, it was observed that devices with a thick absorber layer might consist of a conductive bulk region and a very poorly conductive depletion region at the metal contact. Using a standard semiconductor device model, it is shown in this paper that this reduces the charge collection efficiency under short-circuit conditions, as there is no electrical field in the bulk region, 91探花ing the charge separation. For devices with the low fill factor, a thin-current limiting layer under forward bias can be identified by electrical impedance spectroscopy and is suggestive of a corroded metal contact. 漏 2006 Elsevier B.V. All rights reserved.

ITO-free wrap through organic solar cells-A module concept for cost-efficient reel-to-reel production

Solar Energy Materials and Solar Cells 91:5 (2007) 374-378

Authors:

B Zimmermann, M Glatthaar, M Niggemann, MK Riede, A Hinsch, A Gombert

Abstract:

Organic solar cells have the potential to make cheap photovoltaic devices feasible. In order to achieve this, material and production costs have to be minimised by using device architectures, which are suited to tap the full potential of reel-to-reel production. The inversion of the layer sequence in organic bulk-heterojunction solar cells is motivated by the possibility to omit the commonly used expensive indium tin oxide electrode utilising the so-called wrap through concept. In this concept, the hole contact is formed by a highly conductive formulation of poly(3,4 ethylenedioxythiophene):poly(styrenesulfonate), which is led through via holes in the solar cell to the backside of the substrate in a regular pattern, where it is contacted with a metal layer with low sheet resistance. In this way, a scalable parallel connexion is realised. If higher voltage is desired, one can also connect several such cell segments in series monolithically. We will show that the inversion of the layer sequence is possible without loss of device performance. Using the results of small area inverted devices, we calculate the optimal dimensions of the wrap through solar cell module. First devices with active areas of 2-4 cm2 with parallel and serial wrap through connexion will be shown as proof of concept. 漏 2006 Elsevier B.V. All rights reserved.

Datamining and analysis of the key parameters in organic solar cells

Proceedings of SPIE the International Society for Optical Engineering 6197 (2006)

Authors:

MK Riede, AW Liehr, M Glatthaar, M Niggemann, B Zimmermann, T Ziegler, G Willeke

Abstract:

The production process of organic solar cells (OSCs) is investigated and the effects of parameter variations on experimental results are analysed with the Principal Component Analysis (PCA). This statistical method is applied to an exemplar data set, in which the materials' concentration in the absorber solution and the spincoating speed of the absorber solution were varied intentionally. In addition to the remaining production parameters, the time intervals between the steps were included in the analysis. A large part of the variance in the experimental results can be explained with the evaporation conditions, the spincoating speed and the concentrations in the absorber solution. The PCA also confirms that the OSC is a complex and interdependent system, where one has to analyse the influence of several parameters at the same time in order to understand their effects on the OSC properties. The PCA results will be used to focus further experiments on the identified key parameters.

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 44
  • Page 45
  • Page 46
  • Page 47
  • Page 48
  • Current page 49
  • Page 50
  • Page 51
  • Page 52
  • Next page Next
  • Last page Last

Footer 91探花

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

91探花,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

漏 91探花 - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Giving to Physics