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11 - 20 of 24 search results for KA :PC53 |u:www-g.eng.cam.ac.uk where 0 match all words and 24 match some words.
  1. Results that match 1 of 2 words

  2. pnas201217998 3276..3281

    www-g.eng.cam.ac.uk/advancedstructures/files/pdf/2013GuestD.pdf
    6 Feb 2014: 16. Seffen KA (2012) Compliant shell mechanisms. Philos Trans R Soc Lond A 370(1965):2010–2026.
  3. A stable, power scaling, graphene-mode-locked all-fiber oscillator D. …

    www-g.eng.cam.ac.uk/nms/publications/pdf/Popa21.pdf
    7 Aug 2017: A stable, power scaling, graphene-mode-locked all-fiber oscillator. D. Popa,1,a) Z. Jiang,1 G. E. Bonacchini,1 Z. Zhao,1 L. Lombardi,1 F. Torrisi,1 A. K. Ott,1. E. Lidorikis,2 and A. C. Ferrari11Cambridge Graphene Centre, University of Cambridge,
  4. Nano Res (2010) 3: 404–411 404 Ultrafast Stretched-Pulse Fiber ...

    www-g.eng.cam.ac.uk/nms/publications/pdf/Sun_naonres_2010.pdf
    21 Jun 2010: In metallic tubes, the LO mode is affected by a Kohn anomaly (KA) [43, 44], which causes the softening of this phonon [43, 44]. ... Since KA are not present in semiconducting SWNTs, the G+, G– assignment in metallic SWNTs is the opposite of
  5. pone.0095695 1..12

    www-g.eng.cam.ac.uk/advancedstructures/files/pdf/2014GuestG.pdf
    23 Apr 2015: Contractile and Mechanical Properties of Epithelia withPerturbed Actomyosin DynamicsSabine C. Fischer1, Guy B. Blanchard2, Julia Duque4, Richard J. Adams2, Alfonso Martinez Arias1,. Simon D. Guest3, Nicole Gorfinkiel4. 1 Buchmann Institute for
  6. 7 Apr 2020: However, the so-called “efficiency droop”still limits the operation of LEDs to very low input power den-sities, with current densities 0.01 kA cm2 2,9. ... In contrast to LEDs, laser diodes (LDs) can be operatedat much higher current densities (>10
  7. doi:10.1098/rspa.2006.1750

    www-g.eng.cam.ac.uk/advancedstructures/files/pdf/seffen2007b.pdf
    8 Jan 2008: Keywords: bistable; orthotropic; elliptical; morphing structures; Gaussian curvature. ka. RecAcc. 1.
  8. Characterization of carbon nanotube--thermotropic nematic liquid…

    www-g.eng.cam.ac.uk/nms/publications/pdf/Trushkevych_JPD2008.pdf
    29 May 2008: Inmetallic tubes, the LO mode is affected by a Kohn anomaly(KA), which causes the softening of this phonon [43, 44].Since KA are not present in semiconducting SWNTs, theG+, G
  9. nnano.2008.67 210..215

    www-g.eng.cam.ac.uk/nms/publications/pdf/Das_NN2008.pdf
    7 Apr 2008: at 514 nm, the influence ofdynamic effects is expected to be negligible, because the phononsgiving rise to the 2D peak are far away from the KA at K.
  10. Exp Astron (2009) 23:809–847DOI 10.1007/s10686-008-9115-8 O R I G ...

    www-g.eng.cam.ac.uk/nms/publications/pdf/Kuppers_EA2008.pdf
    23 Feb 2009: An additional Ka-band link for Doppler measurementsis proposed in order to allow a precise determination of the comet’s gravityfield even at low angles between the Earth and the Sun
  11. nn5b06631 1..8

    www-g.eng.cam.ac.uk/nms/publications/pdf/acsnano.5b06631.pdf
    27 Feb 2016: edge K,5,12,13 is activeby double resonance (DR),14,15 and is strongly dispersive withexcitation energy due to a Kohn Anomaly (KA) at K.16 DR canalso happen as

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