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  2. 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.
  3. 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).
  4. SDLD104 - Extrapolation of local measurements on a complete model \…

    www-mdp.eng.cam.ac.uk/web/CD/engapps/aster_docs/VDocs-HTML/V201104a/V201104a.pdf.html
    m. T. With. T. B. T. T. m. =. -. =. -. cos. sin. sin. cos. sin. sin. éq. 2.1-10. Displacements in physical space are obtained by the formula of Ritz:. ... cos. cos. cos. cos. &. cos. cos. cos. cos. X T.
  5. Modeling of the turbulent excitations

    www-mdp.eng.cam.ac.uk/web/CD/engapps/aster_docs/RDocs-HTML/R40702b/R40702b.pdf.html
    cos. sin. =. éq 2.3.3.2-3. where. N. Yk. and. N. ... RN. m. One a:. (). (). N. K. K. K. =. 0. cos. sin. and. N. m. defined in a similar way.
  6. 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
  7. V203002c

    www-mdp.eng.cam.ac.uk/web/CD/engapps/aster_docs/VDocs-HTML/V203002c/V203002c.pdf.html
    0. 0. cos has. cos has. Z. 0. 0. 0. 0. ... 08/01/98. Author (S):. B. QUINNEZ. Key:. V2.03.002-C. Page:. 4/6. Manual of Validation.
  8. V202100d. Doc.

    www-mdp.eng.cam.ac.uk/web/CD/engapps/aster_docs/VDocs-HTML/V202100d/V202100d.pdf.html
    2. cos. ,. ,. where. S. is the surface of the section. (). ... 2. 1. 1. 1. 1. 2. 2. exp. sin. cos. ,. µ. damping coefficient proportional. C. M. K. =. µ. (. ). µ. µ. 1. 0. 2. 2. 2. 0. 4. 4. 2.
  9. 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.
  10. 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.
  11. SSNL118 - Bar subjected to a field speed of wind

    www-mdp.eng.cam.ac.uk/web/CD/engapps/aster_docs/VDocs-HTML/V602118a/V602118a.pdf.html
    O. O. O. O. O. O. (. cos (. ). sin (. )) /. cos. /. cos. /. sin. /. sin. /. 2. ... Fvent =. L Sin qo Q. Vvy Cos qo Q. Vvx Sin qo Q.

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