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3
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85037190530
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A. Steane, e-print quant-ph/9708022.
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Steane, A.1
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7
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4243749278
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R. J. Hughes, D. F. V. James, E. H. Knill, R. Laflamme, and A. G. Petschek, Phys. Rev. Lett. 77, 3240 (1996).
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(1996)
Phys. Rev. Lett.
, vol.77
, pp. 3240
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Hughes, R.J.1
James, D.F.V.2
Knill, E.H.3
Laflamme, R.4
Petschek, A.G.5
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8
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0039776328
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C. Monroe, D. M. Meekhof, B. E. King, W. M. Itano, and D. J. Wineland, Phys. Rev. Lett. 75, 4714 (1995).
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(1995)
Phys. Rev. Lett.
, vol.75
, pp. 4714
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Monroe, C.1
Meekhof, D.M.2
King, B.E.3
Itano, W.M.4
Wineland, D.J.5
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13
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85037194403
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This assumes that there are no degeneracies, i.e., that the state |01〉 is distinguishable from |10〉 even in the absence of interaction. This would hold for the NMR computers because of the chemical shifts. In the degenerate case, the evolution model to be used below would become rather complicated, although I do not expect substantial qualitative differences with the present, simpler one
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This assumes that there are no degeneracies, i.e., that the state |01〉 is distinguishable from |10〉 even in the absence of interaction. This would hold for the NMR computers because of the chemical shifts. In the degenerate case, the evolution model to be used below would become rather complicated, although I do not expect substantial qualitative differences with the present, simpler one.
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14
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85037193917
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See Ref
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See Ref. 1 for details of the algorithm. Note, however, a typographical error in Eq. (20) of 1, which makes it inconsistent with Eq. (22).
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15
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0002565279
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A. Barenco, A. Ekert, K.-A. Suominen, and P. Törmä, Phys. Rev. A 54, 139 (1996).
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(1996)
Phys. Rev. A
, vol.54
, pp. 139
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Barenco, A.1
Ekert, A.2
Suominen, K.-A.3
Törmä, P.4
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16
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85037204713
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I am assuming here that (Formula presented) is “typical,” in that it does not equal a power of 2. Otherwise, (Formula presented) and the factor 0.774 in Eq. (10) below should be equal to 1 instead. My final result (10) may be regarded as a small refinement over the results of
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I am assuming here that (Formula presented) is “typical,” in that it does not equal a power of 2. Otherwise, (Formula presented) and the factor 0.774 in Eq. (10) below should be equal to 1 instead. My final result (10) may be regarded as a small refinement over the results of 9 regarding the performance of the QFT in the presence of random-phase noise.
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