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pnas201217998 3276..3281
www-g.eng.cam.ac.uk/advancedstructures/files/pdf/2013GuestD.pdf6 Feb 2014: 16. Seffen KA (2012) Compliant shell mechanisms. Philos Trans R Soc Lond A 370(1965):2010–2026. -
A stable, power scaling, graphene-mode-locked all-fiber oscillator D. …
www-g.eng.cam.ac.uk/nms/publications/pdf/Popa21.pdf7 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, -
Nano Res (2010) 3: 404–411 404 Ultrafast Stretched-Pulse Fiber ...
www-g.eng.cam.ac.uk/nms/publications/pdf/Sun_naonres_2010.pdf21 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 -
pone.0095695 1..12
www-g.eng.cam.ac.uk/advancedstructures/files/pdf/2014GuestG.pdf23 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 -
Conversionless efficient and broadband laser light diffusers for high …
www-g.eng.cam.ac.uk/nms/publications/pdf/396.pdf7 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 -
doi:10.1098/rspa.2006.1750
www-g.eng.cam.ac.uk/advancedstructures/files/pdf/seffen2007b.pdf8 Jan 2008: Keywords: bistable; orthotropic; elliptical; morphing structures; Gaussian curvature. ka. RecAcc. 1. -
Characterization of carbon nanotube--thermotropic nematic liquid…
www-g.eng.cam.ac.uk/nms/publications/pdf/Trushkevych_JPD2008.pdf29 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 -
nnano.2008.67 210..215
www-g.eng.cam.ac.uk/nms/publications/pdf/Das_NN2008.pdf7 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. -
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.pdf23 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 -
nn5b06631 1..8
www-g.eng.cam.ac.uk/nms/publications/pdf/acsnano.5b06631.pdf27 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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