1998
DOI: 10.1016/s0030-4018(98)00428-3
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The phase-sensitivity of a Mach–Zehnder interferometer for Fock state inputs

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Cited by 23 publications
(1 citation statement)
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“…By using classical resources one can arrive at the socalled shot-noise limit, ∆ϕ SNL ∼ 1/ √ N , where N denotes the average number of input photons [12]. Employing quantum resources, such as squeezed [4,[13][14][15], NOON [16] or other non-classical [17,18] states one can approach the ultimate quantum limit ∆ϕ HL ∼ 1/ N also called as the Heisenberg limit (HL) [19].…”
Section: Introductionmentioning
confidence: 99%
“…By using classical resources one can arrive at the socalled shot-noise limit, ∆ϕ SNL ∼ 1/ √ N , where N denotes the average number of input photons [12]. Employing quantum resources, such as squeezed [4,[13][14][15], NOON [16] or other non-classical [17,18] states one can approach the ultimate quantum limit ∆ϕ HL ∼ 1/ N also called as the Heisenberg limit (HL) [19].…”
Section: Introductionmentioning
confidence: 99%