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Below we refer to α as the AB flux in units of Φ0/2π.
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We note that for M=1, in which case there is no leakage to the absorbing channels, Eqs. and reduce to Juv′=0 and Juv′′=Juv, respectively. In that case, Eq. are identical to Eq. of Ref..
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We note that for M = 1, in which case there is no leakage to the absorbing channels, Eqs. and reduce to J u v ′ = 0 and J u v ′ ′ = J u v, respectively. In that case, Eq. are identical to Eq. of Ref..
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We note that the choice of ka=π/2 is a matter of convenience for illustration of the transmission. For any energy, one can tune the interferometer parameters to achieve spin filtering.
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We note that the choice of k a = π / 2 is a matter of convenience for illustration of the transmission. For any energy, one can tune the interferometer parameters to achieve spin filtering.
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43
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84878596824
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-iα(cosω+isinωωî·σ), one extracts the relations for cosω, sinω and the blocked direction nî=ωî.
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- i α (cos ω + i sin ω ω î · σ), one extracts the relations for cos ω, sin ω and the blocked direction n î = ω î.
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