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Effect of co-doping on proton conductivity in perovskite oxides BaZr0.9In0.05M0.05O3-δ (M = Yb3+ or Ga3+)

Author
AHMED, Istaq1 2 ; RAHMAN, Seikh M. H1 ; STEEGSTRA, Patrick3 ; NORBERG, Stefan T1 2 ; ERIKSSON, Sten-G1 ; AHLBERG, Elisabet3 ; KNEE, Chris S3 ; HULL, Stephen2
[1] Department of Chemical and Biological Engineering, Chalmers University of Technology, 412 96 Gothenburg, Sweden
[2] ISIS Facility, Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire OX11 OQX, United Kingdom
[3] Department of Chemistry, University of Gothenburg, 412 96 Gothenburg, Sweden
Source

International journal of hydrogen energy. 2010, Vol 35, Num 12, pp 6381-6391, 11 p ; ref : 46 ref

CODEN
IJHEDX
ISSN
0360-3199
Scientific domain
General chemistry, physical chemistry; Energy
Publisher
Elsevier, Kidlington
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
Impedance spectroscopy Neutron diffraction Proton conductor Rietveld analysis SEM TGA
Keyword (fr)
Conductivité protonique Diffraction neutron Etat solide Hydrogène Microscopie électronique balayage Perovskite Spectrométrie impédance électrochimique Thermogravimétrie
Keyword (en)
Proton conductivity Neutron diffraction Solid state Hydrogen Scanning electron microscopy Perovskite Electrochemical impedance spectroscopy Thermogravimetry
Keyword (es)
Conductividad protónica Difracción neutrónica Estado sólido Hidrógeno Microscopía electrónica barrido Perovskita Termogravimetría
Classification
Pascal
001 Exact sciences and technology / 001D Applied sciences / 001D06 Energy / 001D06B Fuels / 001D06B06 Alternative fuels. Production and utilization / 001D06B06B Hydrogen

Discipline
Energy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
22907663

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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