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10 Oct 2006: n}.How large can we make a family A of subsets of [n] subject to thecondition that for all A, A′ A, there is some B B with B A A′? ... n}.How large can we make a family A of subsets of [n] subject to thecondition that for all A, A′ A, there is some

30 May 2006: D = au3,/B, (10). 274 H. E. Huppert, J. S. Turner and M. ... of the layer. Hence. where B, is the buoyancy flux at the origin.

7 Dec 2006: Large detector – spatially separate particlesHigh B-field – separate charged/neutralsHigh granularity ECAL/HCAL – resolve particles. ... What is optimal detector size/B-field, etc. THIS IS HARD – BUT VERY IMPORTANT!

19 Apr 2006: dashed red line;Model B’ – a flat distribution with r3 as a dashed blue line. ... For the inner part ofthe disk (r 350 AU), Model A/A’ and Model B/B’ givesimilar results, but Model A and A’ give a much betterfit for r >350 AU.

6 Feb 2006: us the joint probability distribution pjk, and thus a joint entropy S(a, b):. ... Ψ〉 = a|00〉 b|01〉 c|10〉 d|11〉 =. . . abcd. .

21 Sep 2006: tances between each point ofA and its closest point inB:. d(A, B) =1. ... The used costterm is thus. de(A, B) =1. Na. Nγ. i=1.

16 Nov 2006: Amsterdam: Elsevier. Clough, G. W. & Schmidt, B. (1981). Design and performance ofexcavations and tunnels in soft clay. ... Géotechnique 43, No.2, 315 – 320. Peck, R. B. (1969). Deep excavations and tunnelling in soft ground.Proc.

25 Sep 2006: 10. DR R. B. B. WARDYHellenistic and Roman Philosophy: knowledge. and fate (8L, weeks 1–4). ... 5–8). GROUP BCourse Directors:B1: Dr R. B. B. WardyB2: Prof. M.

29 Sep 2006: b) SNRe contours at 2.0% strain. 2.5 Dynamic Resolution Selection procedure. ... and uncoloured noise Simulation B-15dB white noise,. etc. mean SNR is appended.

27 Apr 2006: tems. In addition, crystals an d b u b b l es in m ag m as m a y b e distributed so t h at they create stable den- ... G. F. G i b b , C. M. B. H e n d e r s o n , C.

30 May 2006: 8 ). ( 4. 8 b ). = 0 (n-reven), (4 8 c ) and Fnr = t w ' q s ,. , g , , r B B / ( b r - b n ). (,4.9). We again suppress the argument. ... 4.10 b ) N ( - )" 23(nw cosh [)-$ sin ( w cosh inn - &I-) sen(?).

22 Oct 2006: Then there exist a A, b B and c C with ab = c.In particular, this is true if all of A, B and C have size greater than 2n8/9. ... Equivalently, there exist a A and b B suchthat ab = c, as claimed.

16 May 2006: Write B for Bi(A). Then for the set-systems A and B, wehave |A| = |A||A+||A4A+| and |B| = |B||B+||B4B+|.Now, |B| |A| and |B+| |A+| (by the ... system B = Ak satisfies |B| = |A|, |B| |A| and Bi(B) = B forall i.

5 Jun 2006: B Numerical Integration 108. C Derivation of Multi-Variate Gaussian to Log-Normal Mapping 111. ... case of CDHMMs, B will consist of a set of means, variances and mixture com-ponent weights.

28 Nov 2006: limx. µx2 1. x 1ax b. = 0,. what should a and b be? ... c) Find a basis for Null(A) and Col(A). (d) Find a basis for the following set B = {b R4 | Ax = b has nosolution}.

13 May 2006: Then thereis an isomorphism of Brauer-Severi diagrams defined over K,. C //. φ. Pn1. ψ. E|n.0|. // Pn1. with σ(φ)φ1 = τξσ. We lift ψ to a matrix B ... It is evident that yσ =σ(B)B1 is an element of ΘE projecting onto ξσ.

13 Nov 2006: V.B. Golovko a,⁎, M. Cantoro b, S. Hofmann b, B. Kleinsorge b, J. ... Geng a, D. Jefferson a,A.C. Ferrari b, J. Robertson b, B.F.G.

12 May 2006: trivially embed this in the non-abelian theory. B= B?0.( 0( ((q =q? ... B? q? SU(N)diag/SU(N 1) U(1) = CPN1. Simple Idea:. The strings can miss each other in the internal space.

23 May 2006: Secularity condition – resonant sin(θ τ ) and cos(θ τ ). d. dT. (. A. B. ). =. (. a b. b a. )(. ... A. B. ). where. a = 81α/(1 144α2) and b = 3(5 72α2)/2(1 144α2).

6 Jun 2006: ô“ ÎNóx‹ÿTñTy?W#B»Ûvíñ—ÍEíîïrúpžäø¿lD…Ÿ6[Q œ›6«S}öôˆ#{lx£ÎxQcPÃO{óÏZܘ ÌÊwx«/ÒÇÑ08$F‘ÍéÉñç-BÅ{ ... Í–ü