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CMP
Credit: Jack Hobhouse

Robin Nicholas

Emeriti

Sub department

  • Condensed Matter Physics
Robin.Nicholas@physics.ox.ac.uk
Telephone: 01865 (2)72250
Clarendon Laboratory, room 053,151
  • About
  • Publications

Breakdown of the quantum Hall effect in epitaxial graphene

Institute of Electrical and Electronics Engineers (IEEE) (2014) 40-41

Authors:

TJBM Janssen, S Rozhko, A Tzalenchuk, JA Alexander-Webber, RJ Nicholas

Low-temperature processed electron collection layers of graphene/TiO2 nanocomposites in thin film perovskite solar cells.

Nano Lett 14:2 (2014) 724-730

Authors:

Jacob Tse-Wei Wang, James M Ball, Eva M Barea, Antonio Abate, Jack A Alexander-Webber, Jian Huang, Michael Saliba, Iv谩n Mora-Sero, Juan Bisquert, Henry J Snaith, Robin J Nicholas

Abstract:

The highest efficiencies in solution-processable perovskite-based solar cells have been achieved using an electron collection layer that requires sintering at 500 掳C. This is unfavorable for low-cost production, applications on plastic substrates, and multijunction device architectures. Here we report a low-cost, solution-based deposition procedure utilizing nanocomposites of graphene and TiO2 nanoparticles as the electron collection layers in meso-superstructured perovskite solar cells. The graphene nanoflakes provide superior charge-collection in the nanocomposites, enabling the entire device to be fabricated at temperatures no higher than 150 掳C. These solar cells show remarkable photovoltaic performance with a power conversion efficiency up to 15.6%. This work demonstrates that graphene/metal oxide nanocomposites have the potential to contribute significantly toward the development of low-cost solar cells.

An ultrafast carbon nanotube terahertz polarisation modulator

Journal of Applied Physics American Institute of Physics 115:20 (2014) 203108-203108

Authors:

Callum J Docherty, Sam Stranks, Severin N Habisreutinger, Hannah Joyce, Laura Herz, Robin Nicholas, Michael Johnston

Abstract:

We demonstrate ultrafast modulation of terahertz radiation by unaligned optically pumped single-walled carbon nanotubes. Photoexcitation by an ultrafast optical pump pulse induces transient terahertz absorption in nanowires aligned parallel to the optical pump. By controlling the polarisation of the optical pump, we show that terahertz polarisation and modulation can be tuned, allowing sub-picosecond modulation of terahertz radiation. Such speeds suggest potential for semiconductor nanowire devices in terahertz communication technologies.

Phase space for the breakdown of the quantum Hall effect in epitaxial graphene.

Phys Rev Lett 111:9 (2013) 096601

Authors:

JA Alexander-Webber, AMR Baker, TJBM Janssen, A Tzalenchuk, S Lara-Avila, S Kubatkin, R Yakimova, BA Piot, DK Maude, RJ Nicholas

Abstract:

We report the phase space defined by the quantum Hall effect breakdown in polymer gated epitaxial graphene on SiC (SiC/G) as a function of temperature, current, carrier density, and magnetic fields up to 30 T. At 2 K, breakdown currents (I(c)) almost 2 orders of magnitude greater than in GaAs devices are observed. The phase boundary of the dissipationless state (蟻(xx)=0) shows a [1-(T/T(c))2] dependence and persists up to T(c)>45鈥夆�塊 at 29 T. With magnetic field I(c) was found to increase 鈭滲(3/2) and T(c)鈭滲2. As the Fermi energy pproaches the Dirac point, the 谓=2 quantized Hall plateau appears continuously from fields as low as 1 T up to at least 19 T due to a strong magnetic field dependence of the carrier density.

Ultrahigh magnetic field study of layer split bands in graphite.

Phys Rev Lett 111:9 (2013) 096802

Authors:

RJ Nicholas, PY Solane, O Portugall

Abstract:

We report studies of the magnetospectroscopy of graphite into a new regime of high energies and ultrahigh magnetic fields which allows us to perform the first spectroscopic studies of the interlayer split-off bands, E1 and E2. These bands can be well described by an asymmetric bilayer model and have only a small interlayer band gap asymmetry. We show that all of the properties of the electrons and holes can be described by a simple relativistic behavior determined by 纬0 and 纬1.

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