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46220.dvi
www-g.eng.cam.ac.uk/nms/publications/pdf/Ferrari_EPL1999.pdf14 Dec 2006: The sp3 content of the films isestimated at 10% from X-ray photoemission and electron energy loss spectroscopy [19, 24]. ... P., Phys. Rev. B, 35 (1987) 2946. [24] Li Bassi A., Piseri P., Milani P., Ferrari A. -
PII: S0009-2614(98)01449-3
www-g.eng.cam.ac.uk/nms/publications/pdf/Barborini_CPL1999.pdf14 Dec 2006: Barborini et al.r Chemical Physics Letters 300 1999 633–638 637. w xcoordination 24,25. -
b01330.dvi
www-g.eng.cam.ac.uk/nms/publications/pdf/Bonelli_EJPB2002.pdf12 Dec 2006: 0,24. 0,26. 0,28. 0,30. 0,32. 0,34. G Peak Dispersion (cm-1/nm). Fluence (J/cm-2)Fig. 7. G peak dispersion vs. ... The low frequency Raman spectra of low fluence filmsshow the low frequency double peak structure at about400 and 800 cm1, typical of -
JOURNAL OF APPLIED PHYSICS VOLUME 85, NUMBER 10 15 ...
www-g.eng.cam.ac.uk/nms/publications/pdf/Ferrari_JAP1999.pdf12 Dec 2006: There have been a number of strategies to reducestress in as-depositeda-C:H films, such as incorporatingmetals,24 silicon,25 or multilayers.26 However, metal incor-poration has drawbacks such -
PII: S0022-3093(01)01102-4
www-g.eng.cam.ac.uk/nms/publications/pdf/Fanchini_JNCS2002.pdf11 Dec 2006: Fisica and Unitaa INFM, Politecnico di Torino, Corso Duca degli Abruzzi 24, I-10129 Torino, Italyb Dip. -
42414.dvi
www-g.eng.cam.ac.uk/nms/publications/pdf/Bottani_EPL1998.pdf8 Dec 2006: Our results differ considerably from those reported in [24]. c. e. ... 24] Pailard V., Melinon P., Perez J. P., Dupuis V., Perez A., Loubet J. -
Using APL format
www-g.eng.cam.ac.uk/nms/publications/pdf/Ilie_APL2000.pdf6 Dec 2006: Thepresence of a RamanD peak at;1350 cm21 indicates thatthe s p2 phase is clustering into aromatic rings.18 There is arelationship23,24 between the in-plane correlation lengthL a ofthe ... 2.24 I (D)/I (G) is derived from the Raman spectra -
PII: S0925-9635(99)00271-X
www-g.eng.cam.ac.uk/nms/publications/pdf/Conway_DRM2000.pdf6 Dec 2006: decreases,E0 is measured at lower energies and no longer over a gap defects that could not be measured by ESR [ 24 ]. Robertson [ 25 ] demonstrated that it is possible to fit ... Robertson, Phys. Rev. B 53 (1996 ) 1594. [ 24 ] F. -
PII: S0925-9635(99)00245-9
www-g.eng.cam.ac.uk/nms/publications/pdf/Pastorelli_DRM2000.pdf6 Dec 2006: 85 (av.) 31.4 (av.) 3.24 63.5ta-C:H Homog. 70 28.4 2.35 70 6 30ta-C:H Homog 70 28.4 2.35 43 8.4 ... cm3and a internal layer 63.5 nm thick, with density of3.24 g/cm3[ 12]. -
PII: S0925-9635(99)00233-2
www-g.eng.cam.ac.uk/nms/publications/pdf/LiBassi_DRM2000.pdf6 Dec 2006: Diamond and Related Materials 9 (2000 ) 771–776www.elsevier.com/locate/diamond. Density, sp3 content and internal layering of DLC films byX-ray reflectivity and electron energy loss spectroscopy. A. LiBassi a, A.C. Ferrari b,, V. Stolojan c, B.K.
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