author_facet Samsel‐Czekała, M.
Kontrym‐Sznajd, G.
Biasini, M.
Samsel‐Czekała, M.
Kontrym‐Sznajd, G.
Biasini, M.
author Samsel‐Czekała, M.
Kontrym‐Sznajd, G.
Biasini, M.
spellingShingle Samsel‐Czekała, M.
Kontrym‐Sznajd, G.
Biasini, M.
physica status solidi c
Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
Condensed Matter Physics
author_sort samsel‐czekała, m.
spelling Samsel‐Czekała, M. Kontrym‐Sznajd, G. Biasini, M. 1862-6351 1610-1642 Wiley Condensed Matter Physics http://dx.doi.org/10.1002/pssc.200562486 <jats:title>Abstract</jats:title><jats:p>The electronic structure of the isostructural rare‐earth systems TmGa<jats:sub>3</jats:sub>, ErGa<jats:sub>3</jats:sub>, and CeIn<jats:sub>3</jats:sub> has recently been investigated by measurements of two‐dimensional angular correlations of annihilation radiation (2D ACAR). We employ different tomography techniques to reconstruct electron‐positron (e‐p) momentum density <jats:italic>ρ</jats:italic> (<jats:bold><jats:italic>p</jats:italic></jats:bold>) from its line projections. In all these compounds we get very specific shape of <jats:italic>ρ</jats:italic> (<jats:bold><jats:italic>p</jats:italic></jats:bold>). In order to draw the Fermi surface (FS), we perform conversion from the extended <jats:bold><jats:italic>p</jats:italic></jats:bold> to reduced <jats:bold><jats:italic>k</jats:italic></jats:bold> space. In the case of TmGa<jats:sub>3</jats:sub> and ErGa<jats:sub>3</jats:sub> a nesting feature of the FS consistent with the antiferromagnetic structure is observed. On the other hand, in CeIn<jats:sub>3 </jats:sub>we cannot detect any link between the FS topology and the vector of the magnetic propagation. (© 2006 WILEY‐VCH Verlag GmbH &amp; Co. KGaA, Weinheim)</jats:p> Electronic structure of rare‐earth compounds TmGa<sub>3</sub>, ErGa<sub>3</sub>, and CeIn<sub>3</sub> studied by positrons physica status solidi c
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title Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_unstemmed Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_full Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_fullStr Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_full_unstemmed Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_short Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_sort electronic structure of rare‐earth compounds tmga<sub>3</sub>, erga<sub>3</sub>, and cein<sub>3</sub> studied by positrons
topic Condensed Matter Physics
url http://dx.doi.org/10.1002/pssc.200562486
publishDate 2006
physical 179-182
description <jats:title>Abstract</jats:title><jats:p>The electronic structure of the isostructural rare‐earth systems TmGa<jats:sub>3</jats:sub>, ErGa<jats:sub>3</jats:sub>, and CeIn<jats:sub>3</jats:sub> has recently been investigated by measurements of two‐dimensional angular correlations of annihilation radiation (2D ACAR). We employ different tomography techniques to reconstruct electron‐positron (e‐p) momentum density <jats:italic>ρ</jats:italic> (<jats:bold><jats:italic>p</jats:italic></jats:bold>) from its line projections. In all these compounds we get very specific shape of <jats:italic>ρ</jats:italic> (<jats:bold><jats:italic>p</jats:italic></jats:bold>). In order to draw the Fermi surface (FS), we perform conversion from the extended <jats:bold><jats:italic>p</jats:italic></jats:bold> to reduced <jats:bold><jats:italic>k</jats:italic></jats:bold> space. In the case of TmGa<jats:sub>3</jats:sub> and ErGa<jats:sub>3</jats:sub> a nesting feature of the FS consistent with the antiferromagnetic structure is observed. On the other hand, in CeIn<jats:sub>3 </jats:sub>we cannot detect any link between the FS topology and the vector of the magnetic propagation. (© 2006 WILEY‐VCH Verlag GmbH &amp; Co. KGaA, Weinheim)</jats:p>
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author Samsel‐Czekała, M., Kontrym‐Sznajd, G., Biasini, M.
author_facet Samsel‐Czekała, M., Kontrym‐Sznajd, G., Biasini, M., Samsel‐Czekała, M., Kontrym‐Sznajd, G., Biasini, M.
author_sort samsel‐czekała, m.
container_issue 1
container_start_page 179
container_title physica status solidi c
container_volume 3
description <jats:title>Abstract</jats:title><jats:p>The electronic structure of the isostructural rare‐earth systems TmGa<jats:sub>3</jats:sub>, ErGa<jats:sub>3</jats:sub>, and CeIn<jats:sub>3</jats:sub> has recently been investigated by measurements of two‐dimensional angular correlations of annihilation radiation (2D ACAR). We employ different tomography techniques to reconstruct electron‐positron (e‐p) momentum density <jats:italic>ρ</jats:italic> (<jats:bold><jats:italic>p</jats:italic></jats:bold>) from its line projections. In all these compounds we get very specific shape of <jats:italic>ρ</jats:italic> (<jats:bold><jats:italic>p</jats:italic></jats:bold>). In order to draw the Fermi surface (FS), we perform conversion from the extended <jats:bold><jats:italic>p</jats:italic></jats:bold> to reduced <jats:bold><jats:italic>k</jats:italic></jats:bold> space. In the case of TmGa<jats:sub>3</jats:sub> and ErGa<jats:sub>3</jats:sub> a nesting feature of the FS consistent with the antiferromagnetic structure is observed. On the other hand, in CeIn<jats:sub>3 </jats:sub>we cannot detect any link between the FS topology and the vector of the magnetic propagation. (© 2006 WILEY‐VCH Verlag GmbH &amp; Co. KGaA, Weinheim)</jats:p>
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imprint_str_mv Wiley, 2006
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spelling Samsel‐Czekała, M. Kontrym‐Sznajd, G. Biasini, M. 1862-6351 1610-1642 Wiley Condensed Matter Physics http://dx.doi.org/10.1002/pssc.200562486 <jats:title>Abstract</jats:title><jats:p>The electronic structure of the isostructural rare‐earth systems TmGa<jats:sub>3</jats:sub>, ErGa<jats:sub>3</jats:sub>, and CeIn<jats:sub>3</jats:sub> has recently been investigated by measurements of two‐dimensional angular correlations of annihilation radiation (2D ACAR). We employ different tomography techniques to reconstruct electron‐positron (e‐p) momentum density <jats:italic>ρ</jats:italic> (<jats:bold><jats:italic>p</jats:italic></jats:bold>) from its line projections. In all these compounds we get very specific shape of <jats:italic>ρ</jats:italic> (<jats:bold><jats:italic>p</jats:italic></jats:bold>). In order to draw the Fermi surface (FS), we perform conversion from the extended <jats:bold><jats:italic>p</jats:italic></jats:bold> to reduced <jats:bold><jats:italic>k</jats:italic></jats:bold> space. In the case of TmGa<jats:sub>3</jats:sub> and ErGa<jats:sub>3</jats:sub> a nesting feature of the FS consistent with the antiferromagnetic structure is observed. On the other hand, in CeIn<jats:sub>3 </jats:sub>we cannot detect any link between the FS topology and the vector of the magnetic propagation. (© 2006 WILEY‐VCH Verlag GmbH &amp; Co. KGaA, Weinheim)</jats:p> Electronic structure of rare‐earth compounds TmGa<sub>3</sub>, ErGa<sub>3</sub>, and CeIn<sub>3</sub> studied by positrons physica status solidi c
spellingShingle Samsel‐Czekała, M., Kontrym‐Sznajd, G., Biasini, M., physica status solidi c, Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons, Condensed Matter Physics
title Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_full Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_fullStr Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_full_unstemmed Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_short Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
title_sort electronic structure of rare‐earth compounds tmga<sub>3</sub>, erga<sub>3</sub>, and cein<sub>3</sub> studied by positrons
title_unstemmed Electronic structure of rare‐earth compounds TmGa3, ErGa3, and CeIn3 studied by positrons
topic Condensed Matter Physics
url http://dx.doi.org/10.1002/pssc.200562486