Search

Search Funnelback University

Search powered by Funnelback
21 - 30 of 48 search results for katalk:za33 24 |u:www-g.eng.cam.ac.uk where 0 match all words and 48 match some words.
  1. Results that match 1 of 2 words

  2. PRL 95, 236802 (2005) P H Y S I ...

    www-g.eng.cam.ac.uk/nms/publications/pdf/Lazzeri_PRL2005.pdf
    20 Nov 2006: DFTcalculations are done with the gradient corrected functionalof Ref. [24]. We use plane waves (40 Ry cutoff ) andpseudopotential approaches [25]. ... 24] J. P. Perdew, K. Burke, and M. Ernzerhof, Phys. Rev.
  3. doi:10.1016/j.diamond.2003.12.018

    www-g.eng.cam.ac.uk/nms/publications/pdf/Casiraghi_DRM2004b.pdf
    27 Nov 2006: Fig. 2b shows the G peakdispersion of HCA(t)a-C:N films against N content.Here the G dispersion decreases from 0.24 to 0.1cm ynm, with increasing N ... b). This can be understood if we consider the crosssectional structure of ta-C filmsw13,24,25x.
  4. doi:10.1016/j.diamond.2005.10.052

    www-g.eng.cam.ac.uk/nms/publications/pdf/Pisana_DRM2006.pdf
    13 Nov 2006: Peng et al. [24] reported a root. mean square (rms) roughness of 0.11 nm in a-C:H deposited. ... Technol. 174–175 (2003) 1135. [24] X.L. Peng, Z.H. Barber, T.W. Clyne, Surf.
  5. PII: S0009-2614(98)01449-3

    www-g.eng.cam.ac.uk/nms/publications/pdf/Barborini_CPL1999.pdf
    14 Dec 2006: Barborini et al.r Chemical Physics Letters 300 1999 633–638 637. w xcoordination 24,25.
  6. doi:10.1016/j.diamond.2004.12.028

    www-g.eng.cam.ac.uk/nms/publications/pdf/Piazza_DRM2005.pdf
    22 Nov 2006: obtained here compared to previous films produced by the. small ECWR [24] can be explained by the relatively high. ... 24] A.C. Ferrari, J. Robertson, M.G. Beghi, C.E. Bottani, R. Ferulano, R.
  7. doi:10.1016/j.diamond.2006.01.007

    www-g.eng.cam.ac.uk/nms/publications/pdf/Cantoro_DRM2006.pdf
    13 Nov 2006: like,thick CNFs at temperatures as low as 200 C [24]. ... Phys. 44 (2005) 1558. [24] M. Cantoro, S. Hofmann, et al.
  8. No Job Name

    www-g.eng.cam.ac.uk/nms/publications/pdf/Arenal_NL2006.pdf
    13 Nov 2006: corresponding bulkmaterial.24 However, an increasing temperature softens theE2g phonons,25 whereas we observe a hardening of the Ramanline in the nanotube-rich areas, Figure 3a. ... 24) Piscanec, S.; Cantoro, M.; Ferrari, A. C.; Zapien, J. A.; Lifshitz, Y
  9. PII: S0022-3093(01)01102-4

    www-g.eng.cam.ac.uk/nms/publications/pdf/Fanchini_JNCS2002.pdf
    11 Dec 2006: Fisica and Unitaa INFM, Politecnico di Torino, Corso Duca degli Abruzzi 24, I-10129 Torino, Italyb Dip.
  10. PII: S0925-9635(99)00245-9

    www-g.eng.cam.ac.uk/nms/publications/pdf/Pastorelli_DRM2000.pdf
    6 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].
  11. /home/journal/dvi/APA3708-AP-neu.dvi

    www-g.eng.cam.ac.uk/nms/publications/pdf/Colli_APA2006.pdf
    13 Nov 2006: Nominally sub-eutectic NW syn-thesis using Au as catalyst has been achieved for severalsemiconductor materials, including Ge [22], InP [23], andZnSe [24]. ... 5, 761 (2005)24 A. Colli, S. Hofmann, A.C. Ferrari, C. Ducati, F.

Refine your results

Search history

Recently clicked results

Recently clicked results

Your click history is empty.

Recent searches

Recent searches

Your search history is empty.