Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

1.5-μm band quantum-correlated photon pair generation in dispersion-shifted fiber: suppression of noise photons by cooling fiber

Open Access Open Access

Abstract

Spontaneous four-wave mixing in a dispersion-shifted fiber (DSF) is a promising approach for generating quantum-correlated photon pairs in the 1.5 μm band. However, it has been reported that noise photons generated by the spontaneous Raman scattering process degrade the quantum correlation of the generated photons. This paper describes the characteristics of quantum-correlated photon pair generation in a DSF cooled by liquid nitrogen. With this technique, the number of noise photons was sufficiently suppressed and the ratio of true coincidence to accidental coincidence was increased to ~30.

©2005 Optical Society of America

Full Article  |  PDF Article
More Like This
Long-distance distribution of time-bin entanglement generated in a cooled fiber

Hiroki Takesue
Opt. Express 14(8) 3453-3460 (2006)

Generation of high-purity entangled photon pairs using silicon wire waveguide

Ken-ichi Harada, Hiroki Takesue, Hiroshi Fukuda, Tai Tsuchizawa, Toshifumi Watanabe, Koji Yamada, Yasuhiro Tokura, and Sei-ichi Itabashi
Opt. Express 16(25) 20368-20373 (2008)

All-fiber photon-pair source for quantum communications: Improved generation of correlated photons

Xiaoying Li, Jun Chen, Paul Voss, Jay Sharping, and Prem Kumar
Opt. Express 12(16) 3737-3744 (2004)

Cited By

Optica participates in Crossref's Cited-By Linking service. Citing articles from Optica Publishing Group journals and other participating publishers are listed here.

Alert me when this article is cited.


Figures (4)

Fig. 1.
Fig. 1. Experimental setup. PC: polarization controller, D: photon counter.
Fig. 2.
Fig. 2. C value as a function of number of idler photons per pulse. Squares: cooled, x symbols: uncooled. The dotted line shows C when there are no noise photons.
Fig. 3.
Fig. 3. Number of quantum correlated photon pairs per pulse as a function of pump peak power. Squares: cooled, x symbols: uncooled.
Fig. 4.
Fig. 4. Number of noise photons per pulse as a function of pump peak power for (a) Stokes photons (idler channel) and (b) anti-Stokes photons (signal channel). Squares: cooled, x symbols: uncooled.

Tables (1)

Tables Icon

Table I. Loss after DSF and characteristics of photon counters.

Equations (14)

Equations on this page are rendered with MathJax. Learn more.

2 ω p = ω s + ω i
2 k p = k s + k i .
d n s dz = α n s + g e αz 1 P 1 P 0 ,
d n as dz = α n as + g e αz P 0 P 1 1 ,
P 1 P 0 = exp ( k B T ) ,
n s ( T ) = gL e αL 1 exp ( k B T ) ,
n as ( T ) = gL e αL exp ( k B T ) 1 ,
c s = ( μ c + μ sn ) + α s + d s ,
c i = ( μ c + μ in ) + α i + d i ,
p c = μ c α s c s .
R m = c s ( p c α i + c i ) .
R um = c s c i .
C = R m R um = μ c α s α i c s c i + 1 .
ε 1 2 C .
Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.