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19 Feb 2015: performs time-ensemble computation, in much the sameway NMR quantum computation performs molecular-ensemble computations.24,25,26 Time-ensemble computa-tion alleviates the demand for single-shot spin measure-ments ... ψ(y,t) = exp[. f1(t) y2 f2(t) y f3(t

14 Feb 2015: Φ = αβiσ2, (3.24). and set E m for all momentum components of the non-relativistic wavepackets,we recover the expected result that the ratio Pu/Pd of the probabilities of ... We take ψ0 to be of the form (3.2), with u = uσ3 and Φ given by equation

19 Feb 2015: 3.24). = 1sin θ(sin(1 λ)θ R0 sin λθ R1. ), (3.25). ... 7.93). 24. As in the 2 camera case, the eigenvalue λ returns the value of S3 that we are tryingto minimise.

18 Feb 2015: S2Q(k) [12] satisfying. Q̇(k) = O(1). Specifically, we have. X (i)a =. k. kX (i)k Q(k)a , Za =. k. k2. SZkQ(k)a (2.24).

16 Feb 2015: h(a) 7 h′(a) = Rh(a)R̃ (1.24). andω(a) 7 ω′(a) = Rω(R̃aR)R̃ 2LR̃aRRR̃, (1.25). ... Using (2.24) and the above constraints, the Einstein equations take thereduced form.

22 Feb 2015: theory (Clifford, 1870s)! R  expB/2. MIT1 2003 24. Rotor Interpolation• How do we interpolate between 2 rotations?• Form path between rotors. •

18 Feb 2015: Hanson. Gravitation, gauge theories anddifferential geometry. Phys. Rep., 66(6):213, 1980. 24. ... Class. Quantum.Grav., 2:919, 1985. [24] A. Barducci, R. Casalbuoni, and L.

15 Feb 2015: This induces the spinor transformation law. ψ 7 R0ψ (3.24). which is the STA equivalent of the quantum transformation law. | ... 3.38). 24. where |ψ〉′ is acted on by matrices in the Weyl representation.

19 Feb 2015: ni =1. 2ρ2(r2 a2, (r2 a2). (. 2Mr(r2 a2))1/2. , 0, a) (24).

19 Feb 2015: 22 E =. d. 2ισ12 ισ. 22 E. (24). It follows that the propagator in the transformed basis can be constructed as. ... 24). Clearlythe observable which measures the amount of a state in any one eigenspinoris a constant of the motion, and more generally,