2009
DOI: 10.1364/aop.2.000001
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Stimulated Brillouin scattering in optical fibers

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Cited by 593 publications
(353 citation statements)
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“…The interaction between the pump light and the backscattered Stokes light forms a forward propagating refractive index grating. 12 This forward propagating grating, in turn, increases the Brillouin Stokes power. Increasing the intensity of the pump light beyond the threshold level P th results in a significant modification in the local refractive index which, in turn, causes a large proportion of the pump power to be transferred to the backward propagating Stokes Brillouin beam.…”
Section: B Brillouin Scatteringmentioning
confidence: 99%
“…The interaction between the pump light and the backscattered Stokes light forms a forward propagating refractive index grating. 12 This forward propagating grating, in turn, increases the Brillouin Stokes power. Increasing the intensity of the pump light beyond the threshold level P th results in a significant modification in the local refractive index which, in turn, causes a large proportion of the pump power to be transferred to the backward propagating Stokes Brillouin beam.…”
Section: B Brillouin Scatteringmentioning
confidence: 99%
“…DOI: 10.1103/PhysRevLett.119.143901 Stimulated Brillouin scattering (SBS) is a third-order (χ 3 ) optical nonlinearity that results from the interaction between photons and acoustic phonons in a medium [1][2][3][4]. SBS has practical importance in optical fiber systems [5,6] where it is an important signal impairment mechanism in long-distance transmission systems [7] and makes possible all-fiber lasers [8] as well as tunable, slow-light generation [9]. Power fluctuation resulting from thermal phonons has also been studied in fiber-optic SBS Stokes wave generation [10], and the intensity and phase noise have been measured in narrow-linewidth Brillouin lasers [11].…”
mentioning
confidence: 99%
“…, where δ n,0(±1) is the Kronecker delta, L the fiber length, P s0 and P f 0 the pump powers launched into the slow and fast optical modes (P 0 = P s0 + P f 0 ), and P noise = k B TΩ j R Γ j R /(2ω 0 ) is the effective input noise power in first-order side-bands 24 where k B is Boltzmann's constant and T is the temperature. We neglect slight differences in noise power for the SRLS and SIMS transitions.…”
Section: Apl Photonics 1 056101 (2016)mentioning
confidence: 99%