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19 Feb 2015: spnofikxagoGsKxuHikg=juspnxs7=xaiowoGxu. eCfgh[ikjalYnoeAc0TqAT"H) ¡Cm¢"£ZHeCftoGs=lj}vw¤¥Afhwif{xiky3(fljuspn{o[yªYflOeCfgh[ikjmlYnpoeA«7z)qT. 3K{"3kµK Kp cHE¢"£º"»»/p{¿p¿¿ u K"3 ¡Cm¢£ KÀ ÁÂÂ".

18 Feb 2015: arX. iv:g. r-qc. /040. 5033. v1 6. May. 200. 4. GRAVITY, GAUGE THEORIES ANDGEOMETRIC ALGEBRA. Anthony Lasenby1, Chris Doran2 and Stephen Gull3. Astrophysics Group, Cavendish Laboratory, Madingley Road,Cambridge CB3 0HE, UK. Abstract. A new gauge

19 Feb 2015: Geometric algebra and the causal approachto multiparticle quantum mechanics. Shyamal Somaroo, Anthony Lasenby, and Chris Dorana)Astrophysics Group, Cavendish Laboratory, Madingley Road,Cambridge CB3 0HE, United Kingdom. Received 28 January 1998;

14 Feb 2015: Geometric Algebra and its Applicationto Mathematical Physics. Chris J. L. DoranSidney Sussex College. A dissertation submitted for the degree of Doctor of Philosophy in the University ofCambridge. February 1994. PrefaceThis dissertation is the

5 Feb 2015: It is readily verified that Ka = K2a = a, or, as an operator equation,. ... Ka = Ka = (a) K. (4.52). It follows thatKej = ej, Kej = ej,.

14 Feb 2015: The most important quantities associated with a single 2-spinor κA are its flag-pole Ka = κAκA′, and the flagplane determined by the bivector Pab = κAκBA′B′ ABκA.

5 Feb 2015: where the ka are a set of three Lagrangian multipliers,. R1 = κAκ̇A κ̄A′ ˙̄κA′.

16 Jun 2015: Astrophys., 306, L13-L16. 92. Mackay CD, Parry, IR, Piche, F, Ennico, KA, 1996, "Imaging Spectroscopy for Infra-Red Astronomy", in “Recent Developments in Scientific Optical Imaging”, ed M Bonner Denton, ... 93. Piche, F, Parry IR, Ennico, KA, Ellis,

14 Sep 2015: The ATCA data with the best dynamic range was ob-tained in Ka, i.e. ... The6 km data in Ka were then concatenated with the taskconcat from CASA (McMullin et al.

24 Oct 2015: With the newly upgradedJVLA, it has been possible to begin performing dust polarization studies atcentimeter wavelengths, using the highest-frequency bands available: K, Ka,and Q bands (18–50 GHz). ... Considering that ALMA will eventually have Band 1