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30 Dec 2019: Let (M,g) be an ASD Einstein manifold with scalar curvature 24 admitting a parallel ASD totally nulldistribution.

18 Dec 2019: The predominant approach to this problem has been througha Lagrangian formulation [3, 10], which is the most appropriate for computationalstudies [2, 24, 29, 30]. ... Phys. 203 (2005), no. 2, 539–571. doi:10.1016/j.jcp.2004.08.023. [24] Hou, T. Y.;

8 Dec 2019: cy. I. 1cIδγMa. Bi Peχk. g. 1Bi Peχ. δ. (3.24). 3.3. ... and dΓ /dx|x0 γMa. For the lastterm, we use (3.24) to scale the integral.

6 Dec 2019: ca,β ca′,β. (10.24). If the original state |Ψ〉 was simple, so that (say) the ca,β are non–zero only for a singlevalue of β, for which ca, ... However, if |Ψ〉 is a more general, entangledstate then the sum in (10.24) means that ρA is the

4 Dec 2019: t0〈k||m〉eiωkmt′ dt′ = km. Ek Em(1 eiωkmt. ), (9.24). where km = 〈k||m〉 and ωkm = (Ek Em)/. ... k|†|m〉(ωkm ω). [ei(ωkmω)t 1. ]. (9.32). This is very similar to our result (9.24), with the time–dependence of the perturbation.

30 Nov 2019: P ψ = ψ ⟨v,ψ⟩v. (2.24). These equations have initial conditions α(0) and η(0,r) such that. ... ˙̃η1 = η̃2 O3(A,η̃), ˙̃η2 = Lη̃1 O3(A,η̃). (2.27). 24 The φ4 kink on a wormhole spacetime.

26 Nov 2019: 24). The computational effectiveness of these equations has been demonstrated [107]by tackling small size Ising type problems of order up to 20. ... A variety of potential landscapes to confinepolariton or photons have also been engineered [96, 4, 24].

23 Nov 2019: c2v E = 1. µc2p. (er̂. 4π0r2. )= e. 4π0µc21. r3L (8.24). ... The first ionisationenergy is thus the difference (54.4 79.0) eV = 24.6 eV.

23 Nov 2019: Similarly,. |1, 0〉H =12. (|x〉e |x〉p |x〉e |x〉p) (6.24). as one can check straightforwardly.

23 Nov 2019: ijkSk [Si, S2] = 0. (5.24). as well as [Si,Lj] = 0.