2012
DOI: 10.1002/pssa.201228039
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Structural and magnetic properties of Co2MnSi thin films

Abstract: is an open access repository that collects the work of Arts et Métiers ParisTech researchers and makes it freely available over the web where possible. (20, 50, and 100 nm) were grown by radio frequency (RF) sputtering on a-plane sapphire substrates. Our X-rays diffraction (XRD) study shows that, in all the samples, the cubic h110i CMS axis is normal to the substrate and that six well defined preferential in-plane orientations are present. Static and dynamic magnetic properties were investigated using vibrati… Show more

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Cited by 7 publications
(3 citation statements)
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“…Values of the Landé factor measured in experiments for Co 2 MnSi samples are ranging from 2.00 to 2.06, according to Refs. [72][73][74]. These values are of the same order of magnitude as our calculated data.…”
Section: Disorder Dependence Of the Static Magnetic Propertiessupporting
confidence: 88%
“…Values of the Landé factor measured in experiments for Co 2 MnSi samples are ranging from 2.00 to 2.06, according to Refs. [72][73][74]. These values are of the same order of magnitude as our calculated data.…”
Section: Disorder Dependence Of the Static Magnetic Propertiessupporting
confidence: 88%
“…Various deposition techniques such as magnetron sputtering [9][10][11], molecular beam epitaxy [12], laser ablation [8] and plasma-assisted sputtering [13] have been employed for the growth of the CMS films using various substrates such as crystalline Si [5,9,11], Al 2 O 3 [6,14], MgO [6,8], GaAs [15], Ge [12] and amorphous glass [7].…”
Section: Introductionmentioning
confidence: 99%
“…[14][15][16][17] The intrinsic magnetic anisotropy of the well-known FHA films has been found to be dominated by the in-plane anisotropy. [16][17][18] Very recently, the interface-induced PMA was discovered in a Co-based FHA (Co 2 FeAl) in contact with a MgO oxide layer. 19,20 The proposed explanation for the PMA is similar to that of CoFeB or Fe/MgO systems for which interfacial anisotropy induced by hybridization of Fe-, Co-3d and O-2p orbitals causes the a Electronic email: dau@pdi-berlin.…”
Section: Introductionmentioning
confidence: 99%