Coherent backscattering (CBS) is a beautiful physical phenomenon that takes place in a highly scattering medium, which has potential application in noninvasive optical property measurement. The current model that explains the CBS cone shape, however, assumes the incoming beam diameter is infinitely large compared to the transport length. In this paper, we evaluate the effect of a finite scalar light illumination area on the CBS cone, both theoretically and experimentally. The quantitative relationship between laser beam size and the CBS cone shape is established by using two different finite beam models ( uniform top hat and Gaussian distribution). A series of experimental data with varying beam diameters is obtained for comparison with the theory. Our study shows the CBS cone shape begins to show distortion when beam size becomes submillimeter, and this effect should not be ignored in general. In biological tissue where a normal large beam CBS cone is too narrow for detection, this small beam CBS may be more advantageous for more accurate and higher resolution tissue characterization. (C) 2012 Optical Society of America
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Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
Monash Univ, ARC Ctr Excellence Future Low Energy Elect Technol, Clayton, Vic 3800, Australia
Univ New South Wales, Sch Phys, Sydney 2052, AustraliaMonash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
Liu, Hong
Atencia, Rhonald Burgos
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Univ New South Wales, Sch Phys, Sydney 2052, Australia
Univ New South Wales, ARC Ctr Excellence Low Energy Elect Technol, UNSW Node, Sydney 2052, Australia
Univ Sinu, Fac Ingn, Dept Ciencias Bas, Cra1 W 38-153,4536534, Monteria 230002, Cordoba, ColombiaMonash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
Atencia, Rhonald Burgos
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Medhekar, Nikhil
Culcer, Dimitrie
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Univ New South Wales, Sch Phys, Sydney 2052, Australia
Univ New South Wales, ARC Ctr Excellence Low Energy Elect Technol, UNSW Node, Sydney 2052, AustraliaMonash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
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St Petersburg State Univ, Dept Phys, St Petersburg 198504, Russia
St Petersburg Inst Commerce & Econ, Dept Math, St Petersburg 194021, RussiaSt Petersburg State Univ, Dept Phys, St Petersburg 198504, Russia
Kuzmin, V. L.
Valkov, A. Yu
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St Petersburg State Univ, Dept Phys, St Petersburg 198504, Russia
St Petersburg Inst Commerce & Econ, Dept Math, St Petersburg 194021, RussiaSt Petersburg State Univ, Dept Phys, St Petersburg 198504, Russia
机构:
Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
Monash Univ, ARC Ctr Excellence Future Low Energy Elect Technol, Clayton, Vic 3800, Australia
Univ New South Wales, Sch Phys, Sydney 2052, AustraliaMonash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
Liu, Hong
Atencia, Rhonald Burgos
论文数: 0引用数: 0
h-index: 0
机构:
Univ New South Wales, Sch Phys, Sydney 2052, Australia
Univ New South Wales, ARC Ctr Excellence Low Energy Elect Technol, UNSW Node, Sydney 2052, Australia
Univ Sinu, Fac Ingn, Dept Ciencias Bas, Cra1 W 38-153,4536534, Monteria 230002, Cordoba, ColombiaMonash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
Atencia, Rhonald Burgos
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机构:
Medhekar, Nikhil
Culcer, Dimitrie
论文数: 0引用数: 0
h-index: 0
机构:
Univ New South Wales, Sch Phys, Sydney 2052, Australia
Univ New South Wales, ARC Ctr Excellence Low Energy Elect Technol, UNSW Node, Sydney 2052, AustraliaMonash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia
机构:
St Petersburg State Univ, Dept Phys, St Petersburg 198504, Russia
St Petersburg Inst Commerce & Econ, Dept Math, St Petersburg 194021, RussiaSt Petersburg State Univ, Dept Phys, St Petersburg 198504, Russia
Kuzmin, V. L.
Valkov, A. Yu
论文数: 0引用数: 0
h-index: 0
机构:
St Petersburg State Univ, Dept Phys, St Petersburg 198504, Russia
St Petersburg Inst Commerce & Econ, Dept Math, St Petersburg 194021, RussiaSt Petersburg State Univ, Dept Phys, St Petersburg 198504, Russia