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  2. Conditions for the finiteness of the moments of the ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI17027
    0 < w < 1 implies that 1 cos(w) C0w2. This implies in turn that for τ < 1/b where b has been defined in (11). ... 1 rv(τ) = 0. 1 cos(λτ) dFv(λ). 1/τ0. 1 cos(λτ)dFv(λ). C0τ2 1/τ0.
  3. cats2.dvi

    https://api.newton.ac.uk/website/v0/events/preprints/NI05017
    We considera cat’s eye flow with. ψ = A cos x B cos y, w = ψ, (3.1). ... Finally let us now replace (3.1) by. ψ = A cos x B cos y, w = A cos x B cos(y φ), (3.7).
  4. Submitted to the Annals of Statistics T -OPTIMAL DESIGNS ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI11054
    3.2) ti (b) = (1. |b|n. )cos. (iπ. n. ) |b|n, i = 1,. ... 1+. cos(πn. )) where direct calculations show that the points ti (b), i = 1,.
  5. Vacuum Energy and Repulsive Casimir Forces in Quantum StarGraphs ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI07023
    Second, if cos(ωa) = 0,then ω is one of the numbers (8) and. ... Bj=1. r=1. 1. r2. (2. B 1. )r cos(rθj)aj. , (24).
  6. driver_SA.dvi

    https://api.newton.ac.uk/website/v0/events/preprints/NI11063
    where. 21. T (d,s,a,b) = b. awk{(. 1 d swψ. )cos. ( ... a′)k cos (a′) (b′)k cos (b′) k P1 (k 1,a′,b′) , k 1.
  7. Limit laws for norms of i.i.d. sampleswith Weibull tails ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI04022
    and (7.17) follows withµ = 0, b = Γ(1 α) cos(πα/2) > 0, β = 1.2) Let now1 < α < 2. ... 2+. 1 β. 2exp(b ex. ), (10.9). where, according to (2.9),β 1 andb = Γ(1 α) cos(πα/2) 1.
  8. arX iv:2 212. 0941 6v1 [he p-th ] 1 ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI22017
    i cos(γπκ2. ) sin(γπκ. 2)). , (36). where γ, b are model-dependent constants, while H(κ) is a model-dependent product ofgamma-functions. ... A(x) = cos(γπvx2. )eγvx log x+. k=1 z2k1(vx)2k1. , (37). where zk is proportional to ζk in a
  9. Localized rotating convection with no-slip boundary conditions…

    https://api.newton.ac.uk/website/v0/events/preprints/NI13020
    The general form of these. solutions is. ψ = cos(λ0z)A {cos(λ1z)B c.c.} , (19)θ = i. ... TaAz {iλ11 B sin(λ1z) c.c.} , (26). v = A {B cos(λ1z) c.c.} , (27)where λ21 = σ1μ iTa and μ is the growth rate of the mode.
  10. arX iv:g r-qc /060 6067 v2 11 Jul 2 ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI06032
    The tetrad vectors are. e1(τ ) =(. sinh(aτ ) cos(bτ ) (b/a) cosh(aτ ) sin(bτ ),. cosh(aτ ) cos(bτ ) (b/a) sinh(aτ ) sin(bτ ), (k/a) sin(bτ ), 0). ,. ... e2(τ ) =(. sinh(aτ ) sin(bτ ) (b/a) cosh(aτ ) cos(bτ ), cosh(aτ ) sin(bτ ) (b/a) sinh
  11. Delsarte's Extremal Problem and Packing on Locally Compact…

    https://api.newton.ac.uk/website/v0/events/preprints/NI18015
    trigonometryi.e. applying cos2(γ) = 12(1 cos(2γ))the formula. sYd2(s) =sj2d. 2. (s). ... H(t) = 12A2q2d. 2. (1. (d 1)td1+. t. cos(2s 2β)sd2. ds. )
  12. arX iv:0 711. 0707 v2 [ hep- th] 8 ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI07083
    j1 =12[sin(Φ) dΘ sin(Θ) cos(Θ) cos(Φ) dΦ],. j2 =12[cos(Φ) dΘ sin(Θ) cos(Θ) sin(Φ) dΦ],. ... with (recall that a2 a b2 = 0, see (3.4)). J′1 =12sin(Θ) cos(Θ) (a dΦ b dΦ),.
  13. Multi-target search in bounded andheterogeneous environments: a…

    https://api.newton.ac.uk/website/v0/events/preprints/NI23013
    2) isgiven by B(?): = @cos(2c:/#) 8@6sin(2c:/#) @for the periodic axis, while for the reflective axis wehave B(A)0 = 0 or B. ... A): (=, =0) =. #1 5 (==01)/26(=)6(=0)/[f cos(c:/#)] with6(<) =. 5 sin(c:</#) sin[c:(< 1)/# ] when. : >
  14. hard_hard_test_d_zoom_convergence.eps

    https://api.newton.ac.uk/website/v0/events/preprints/NI09023
    bottom topography considered is described by:. b(x) =. . 0.25 cos(10π(x 1.5)) 1)) m if 1.4 m x 1.6 m,0 otherwise. ... 0. 0.5. 1. 1.5. x (m). (b. b U)/. b ref.
  15. Heteroclinic snaking near a heteroclinic chain in draggedmeniscus…

    https://api.newton.ac.uk/website/v0/events/preprints/NI13030
    stabilising short-range interaction, Π̃2(h̃) = B/h̃6. Here h̃ is the dimensional film thickness,. ... Using cylindrical polar coordinates (r, θ, z), such that y1 = r cos θ, y2 = r sin θ and.
  16. Jupiter’s cloud-level variability triggered by torsional oscillations …

    https://api.newton.ac.uk/website/v0/events/preprints/NI22030
    1/2Pmn1(x) , (5). where x = cos θ, we can rewrite (4) as. ... Bs =n=1. nm=0. (reqr. )n2[gmn cos mφ h. mn sin mφ].
  17. EFFICIENT ADAPTIVE MULTILEVEL STOCHASTIC GALERKINAPPROXIMATION USING…

    https://api.newton.ac.uk/website/v0/events/preprints/NI17021
    a(x, y) = 1. m=1. αm cos(2πβ1mx1) cos(2πβ. 2mx2)ym,. where β1m = mkm(km 1)/2, β2m = km β1m and km = b1/2 (1/4 2m)1/2c ... φij = 2 cos(iπx1) cos(jπx2), νij =1. 4exp(π(i2 j2)l2). We choose the correlation length l = 0.65 and rewrite the sum
  18. Using graphs to find the best block designs R. ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI11047
    For example, Fig. 1 shows two block designs with v = 15, b = 7 and. ... Thus current is defined on( B) (B ) and voltage is defined on T B.
  19. Decay to equilibrium of the filament end density alongthe ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI15068
    For (DBC) another straightforward, although a little longer computation gives thatbifurcation values are of the form α = 1/|cos b|, where b solves. ... Cb tan b = 0. (16). We denote by b0 (π/2,π) the smallest positive solution, set α0 = 1/|cos b0|,
  20. ANALYSIS OF A VARIATIONAL MODEL FOR NEMATIC SHELLS ANTONIO ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI14037
    Wκ(α) =κ. 2. Q. {|sα|2 η cos(2α). }dVol, (1.4). where η is a function which depends only on the geometry of the torus. ... Examples. 1. (γ [0, 1] v(γ)). Let v(x,y) := (cos(y), sin(y)), θ̄ (0, 2π), and γ : [0, θ̄] R2, γ(t) := (0, t)
  21. One-dimensional scaling limits in a planar Laplacian random growth ...

    https://api.newton.ac.uk/website/v0/events/preprints/INI1410
    trjt = r. jt. (rjt )2 1. (rjt )2 2rjt cos(ϑ. ... jTt). (rjt )2 2rjt cos(ϑ. jt ξ. jTt) 1. (23). (where we have suppressed the dependence on z to ease notation).By observing that the right hand side of (22)
  22. Perfectly Matched Layers in 1-d : Energy decay for ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI07024
    4.9)On the other hand,. û(t,ξ) = û0(ξ)(cos(tωh(ξ)) itωh(ξ. h0 )sinc(tωh(ξ)). ), (4.10). ... σ. cos(. kπh4. )) Ch.For each h, we dene Kh = b 4hπ arcsin(δ)c.
  23. 1 Misconceptions about quantifying animalencounter and interaction…

    https://api.newton.ac.uk/website/v0/events/preprints/NI23002
    h(N)k (n,n0). [1 s. (N)k. ]t, (10). where. h(N)k (n,n0) =. αkN. cos. [(n 1. 2. )πk. N. ]cos. [(n0. 1. 2. ) ... cos[2πk(x y)/N]/N. Analogously to the reflecting case above, the propagator for both walkers,278that is the solution of Eq.
  24. qscrmtaf.dvi

    https://api.newton.ac.uk/website/v0/events/preprints/NI04011
    Λk =. {. 2a(0) 4(M1)/2. j=1 a(j) cos kj if M is odd. ... TN )jl =2. π. π. k=0. Λk|Λk|. cos kj cos klk M.
  25. MONOTONE UNITARY FAMILIES DANIEL GRIESER Abstract. A unitary family…

    https://api.newton.ac.uk/website/v0/events/preprints/NI09008
    The converse is not true. As an example let A0 =. (. 0 ππ 0. ). , B =. (. b 00 1. ). ... Then eiτ A0 =. (. cos πτ sin πτsin πτ cos πτ. ).
  26. Tzitzeica solitons vs.relativistic Calogero-Moser 3-body clusters J.…

    https://api.newton.ac.uk/website/v0/events/preprints/NI09028
    τn = 1 cos((2n 1)c). i sin ceϕ1(u,v) cos. 2 c. ... H = M0. Nj=1. (cosh(psj) 2 cos(c) cosh(pj/2)), P = M0.
  27. royalsocietypublishing.org/journal/rspa ResearchCite this article:…

    https://api.newton.ac.uk/website/v0/events/preprints/NI19030
    For convenience, we call these functions of r the displacement and stresscomponents, leaving understood a factor of cos 2θ or sin 2θ determined by (2.4). ... ̂σrr, σ̂rθ ) (σ cos 2θ , σ sin 2θ ) (r ), (2.8)or equivalently. (
  28. ALMOST PERIODICITY IN TIME OF SOLUTIONS OF THE KDV ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI16003
    a(n, 0) = 1, b(n, 0) = 2λ cos(2π(nω θ)). This special case is particularly interesting because, as indicated above, the spectral analysis of the initial datais almost complete. ... xψ cos θ ψ sin θ = 0.Using compactness, select a sequence (Ej ,E.
  29. Hitting probabilities for non-linear systemsof stochastic waves by…

    https://api.newton.ac.uk/website/v0/events/preprints/NI12029
    This reference covers the case where, in (1.4),σ = (σi,j)1i,jd is an invertible matrix with constant entries, b = (b. ... Applying twice the inequality (a b)2 12a2 b2 yields. dj=1. di=1.
  30. arXiv:0801.4634v1 [hep-th] 30 Jan 2008

    https://api.newton.ac.uk/website/v0/events/preprints/NI08011
    the following metric. ds2 = 4dudv r+(u). 2ν2(1 cos(u). ) dx2 1 ν4. ... ν2(1 cos(u). ) dxdy r(u). 2ν2(1 cos(u). ) dy2. (1 ν2).
  31. Well-Posedness of Two-Dimensional Hydroelastic Waves David M.…

    https://api.newton.ac.uk/website/v0/events/preprints/NI14090
    Solving for L, this is. L[η] = 4π2. 2π0 cos(η(α)) dα. ... µε = 2π0 B. ε1 cos(θε) dα. 2π0 cos(θε) dα. = Lε.
  32. Anderson transition at 2 dimensional growth rate on antitrees ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI15039
    ii) Let (a,b) B = and assume that for Lebesgue almost all E (a,b) there is a subordinatesolution wE,n to (2.7) at E such that. ... For part (ii) note that for (a,b) B = we can apply Theorem 2.7 and (2.18).
  33. On algorithms with good mesh properties for problems with ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI15085
    On algorithms with good mesh properties for problems with moving. boundaries based on the Harmonic Map Heat Flow and the. DeTurck trick. Charles M. Elliott and Hans Fritz. Abstract. In this paper, we present a general approach to obtain numerical
  34. The Savage-Hutter Avalanche ModelHow far Can it be Pushed? ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI03072
    b. b bτ xzzzp. τ =. τ =. shea. r st. ... gz λκηu2). εgzb. y,. η := cos (ψ(y) ϕ(x) ϕ0) ,. in which. Kx = Kxact/pass = 2sec2φ(. 1(. 1 cos2 φ/cos2 δ)1/2. ).
  35. Quadratic Weyl Sums, Automorphic Functions, and Invariance Principles …

    https://api.newton.ac.uk/website/v0/events/preprints/NI15010
    such that sin φ, cos φ 6= 0) we apply twice the identity. ... dv, (3.20). where g(v) = 2πi12. (w2v2) cos φwvsin φ. We have.
  36. Approximations to the Stochastic Burgers equation Martin Hairer,…

    https://api.newton.ac.uk/website/v0/events/preprints/NI10015
    1,vDεv〉. =n6=0. σ2ξn(t)ξn(t). 4νπ(in)einaε einbε. (a b)εin. =σ2. 2πν. n>0. |ξn(t)|2cos aεn cos bεn. ... limε0. E〈1,vDεv. 〉=. σ2. 2πν. 0. cos ax cos bx(a b)x2.
  37. The structure of completely positive matrices according to their…

    https://api.newton.ac.uk/website/v0/events/preprints/NI14088
    Consider a, b Rn, and for all θ R let cθ = a sin θ b cos θ anddθ = a cos θ b sin θ. ... Ifeither n 3 or p 2 (or both) then B is nearly positive.
  38. The Symplectic Geometry of Closed Equilateral Random Walks in ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI13054
    π. 0. cos xy sincn1 y dy. Using the angle addition formula for cos(a b), this implies that. ... since. 2 2 cos θ is the length of the vector ̀ = ei ei1.
  39. Imperial-TP-AT-2007-4 Pohlmeyer reductionof AdS5 × S5 superstring…

    https://api.newton.ac.uk/website/v0/events/preprints/NI07093
    1. cos 2ϕϕul) = 0. (4.34). Besides the obvious SO(n 1) symmetry these equations are invariant under the following formaltransformation. ... n , (4.37). one arrives at the system (4.34) for φ,ul with the obvious replacement of cos ϕ, sin ϕ, tan ϕ
  40. Fractional Brownian motion with Hurst index H=0 and the Gaussian…

    https://api.newton.ac.uk/website/v0/events/preprints/NI15015
    φ(η)H (t) =. 1. 2. 0. e2ηs. s12H(1 cos (ts)) ds. ... 1. 4HΓ(1 2H). [(4η2 t2)H cos. (2H arctan. t. 2η. ) (2η)2H. ].
  41. arX iv:1 311. 6101 v2 [ quan t-ph ] ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI14012
    A B min(λ1(A),λ1(B)) (1cos(θ)).with cos(θ) = maxψBker(B),ψAker(A) |〈ψA|ψB〉|. Thus if we can bound the gap of A (see Lemma 2.6 ... F(ρ0A,ρB(k)). 2(n 2)4(n 1). n(1 cos(2πk/D)). 4(n 1). This fidelity is clearly maximized for the lowest
  42. Regularity Analysis for Stochastic Partial Differential Equations…

    https://api.newton.ac.uk/website/v0/events/preprints/NI10056
    dXt(x) =. [κ2. x2Xt(x) f(x, Xt(x)). ]dt. j=1. [2ν. jr2. b(x, Xt(x)) cos(jπx). ... Theorem 1 finally shows that, under condition (31),the SPDE. dXt(x) =. [κ2. x2Xt(x) f(x, Xt(x)). ]dt. j=1. [2ν. j32. b(x, Xt(x)) cos(jπx).
  43. arX iv:1 208. 4677 v1 [ mat h.SP ] ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI13008
    W(f,v)(a) = 0 iff BC1a(f) cos(θa) BC2a(f) sin(θa) = 0, f dom (Tmax). ... that. Sf = τf,. f dom (S) ={g dom (Tmax). BC1a(g) cos(θa) BC2a(g) sin(θa) = 0}.
  44. A NONLOCAL DIFFUSION PROBLEM ON MANIFOLDS CATHERINE BANDLE, MARIA ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI15088
    Moreover,. ρ cos(λρ) = λ sin λρ = λ2ρsin λρλρ. and the results follows. ... sinh ρ. )N12 cos λρ. C N1n=2. λn. so that, if t 1,.
  45. Floquet stability and Lagrangian statistics of a non-linear…

    https://api.newton.ac.uk/website/v0/events/preprints/NI22019
    U0 = (sin(z sin(t)) cos(y sin(t)),. sin(x sin(t)) cos(z sin(t)),. sin(y sin(t)) cos(x sin(t))). ... 0 1000 2000 3000t. 1010. 106. 102. E. KE. ME. (b) = 1.0.
  46. INVERSE SPECTRAL AND SCATTERING THEORYFOR THE HALF-LINE LEFT DEFINITE …

    https://api.newton.ac.uk/website/v0/events/preprints/NI07030
    û(λ) = 〈u, ϕ(, λ)〉 = b. 0. uλϕ(, λ)w u(0) cos α,. ... Thereforewe find λ(Lϕ̆(, λ))(0) = λf (0)ϕ̆(0, λ) = sin α and (Lϕ̆(, λ))′(0) =. 18 C. BENNEWITZ, B. M. BROWN, R. WEIKARD. ϕ̆′(0, λ)/f (0) = cos
  47. ∗-COMPATIBLE CONNECTIONS IN NONCOMMUTATIVERIEMANNIAN GEOMETRY E.J.…

    https://api.newton.ac.uk/website/v0/events/preprints/NI09036
    Now applying E E′ to δE.a = a.δE and using (b) gives (c). ... Then:. a) gij gjk = ev(ei ek). b) gij gjk = ev(ek ei).
  48. PLANE WAVE DISCONTINUOUS GALERKIN METHODS C. J. GITTELSON∗, R. ...

    https://api.newton.ac.uk/website/v0/events/preprints/NI07088
    x)n. =γn0 (x). 2+. n. j=1. [γnj (x) cos(jϕ) σ. ... Using (4.4) this permits us to rewrite. ((cos ϕksin ϕk. ) x)n. =.
  49. APPROXIMATE CONE FACTORIZATIONSAND LIFTS OF POLYTOPES JOÃO GOUVEIA,…

    https://api.newton.ac.uk/website/v0/events/preprints/NI13069
    The duality statement Ka = Kb is perhaps geometrically obvious, since Ka and Kb arespherical cones with “center” ω and half-angles θa and θb, respectively, with cos θa = a,cos θb = ... Thetriangle inequality in spherical geometry gives γ α β.
  50. Automatic Construction and Natural-Language Descriptionof…

    https://api.newton.ac.uk/website/v0/events/preprints/NI14020
    cos is a special case of our reparametrised PER. 3 Model Search and EvaluationAs in Duvenaud et al. ... SE cos. Both demonstrate, using Bochner’s theorem(Bochner, 1959), that these kernels can approximate anystationary covariance function.
  51. EFFECTIVE RELAXATION FOR MICROSTRUCTURE SIMULATIONS:ALGORITHMS AND…

    https://api.newton.ac.uk/website/v0/events/preprints/NI03087
    The nonconvex minimization problem theninvolves eigen-strains. E1 = 0.0113m m 0.0102n n and E2 = 0.0102m m 0.0113n n,for m = (cos(π/3), sin(π/3)) and ... n = ( sin(π/3), cos(π/3)), and the material tensor Cdefined for cubic anisotropy by.

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