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S. O. Park and S. S. Lee, "Forward far-field pattern of a laser beam scattered by a water-suspended homogeneous sphere trapped by a focused laser beam," J. Opt. Soc. Am. A 4, 417-422 (1987).
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Park, S.O.1
Lee, S.S.2
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53
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0000688498
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Internal and near-surface electromagnetic fields for a spherical particle irradiated by a focused laser beam
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J. P. Barton, D. R. Alexander, and S. A. Schaub, "Internal and near-surface electromagnetic fields for a spherical particle irradiated by a focused laser beam," J. Appl. Phys. 64, 1632-1639 (1988).
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Barton, J.P.1
Alexander, D.R.2
Schaub, S.A.3
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54
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36549091673
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Theoretical determination of net radiation force and torque for a spherical particle illuminated by a focused laser beam
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J. P. Barton, D. R. Alexander, and S. A. Schaub, "Theoretical determination of net radiation force and torque for a spherical particle illuminated by a focused laser beam," J. Appl. Phys. 66, 4594-4602 (1989).
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Barton, J.P.1
Alexander, D.R.2
Schaub, S.A.3
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55
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84975647154
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Interpretation of extinction in Gaussian-beam scattering
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J. A. Lock, "Interpretation of extinction in Gaussian-beam scattering," J. Opt. Soc. Am. A 12, 929-938 (1995).
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Lock, J.A.1
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56
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84975659896
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Forward scattering of a Gaussian beam by a nonabsorbing sphere
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J. T. Hodges, G. Gréhan, G. Gouesbet, and C. Presser, "Forward scattering of a Gaussian beam by a nonabsorbing sphere," Appl. Opt. 34, 2120-2132 (1995).
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Hodges, J.T.1
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Presser, C.4
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57
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0009585190
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Reflected image of a strongly focused spot
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L. Novotny, R. D. Grober, and K. Karrai, "Reflected image of a strongly focused spot," Opt. Lett. 26, 789-791 (2001).
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Novotny, L.1
Grober, R.D.2
Karrai, K.3
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58
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0037091515
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Three-dimensional position detection of optically trapped dielectric particles
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A. Rohrbach and E. H. K. Stelzer, "Three-dimensional position detection of optically trapped dielectric particles," J. Appl. Phys. 91, 5475-5488 (2002).
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Rohrbach, A.1
Stelzer, E.H.K.2
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59
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0032181308
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Optimising the image contrast of conventional and confocal microscopes imaging finite sized spherical gold scatterers
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P. Török, P. D. Higdon, R. Juškaitis, and T. Wilson, "Optimising the image contrast of conventional and confocal microscopes imaging finite sized spherical gold scatterers," Opt. Commun. 155, 335-341 (1998).
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Török, P.1
Higdon, P.D.2
Juškaitis, R.3
Wilson, T.4
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60
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27544485737
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P. Li, K. Shi, and Z. Liu, Optical scattering spectroscopy by using tightly focused supercontinuum, Opt. Express 13, 9039 (2005, Equation (3) in this paper has been corrected, cos(θ)]1/2 instead of [cosθ, 1/2
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P. Li, K. Shi, and Z. Liu, "Optical scattering spectroscopy by using tightly focused supercontinuum," Opt. Express 13, 9039 (2005). Equation (3) in this paper has been corrected ([cos(θ)]1/2 instead of [cos(θ)]-1/2).
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61
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84942362646
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Strictly, the amplitude E0 should be corrected to take into account the (weak) energy losses due to reflexion and absorption within the lens. If these losses does not depend noticeably on the azimuthal angle φ, these effects can be easily included in our modeling by modifying the weighting factor [cos(θ)]16/2 appropriately.
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Strictly, the amplitude E0 should be corrected to take into account the (weak) energy losses due to reflexion and absorption within the lens. If these losses does not depend noticeably on the azimuthal angle φ, these effects can be easily included in our modeling by modifying the weighting factor [cos(θ)]16/2 appropriately.
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62
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84894001222
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The center of the Cartesian frame defining the vector spherical harmonics has to be chosen at the particle center. For a given origin, note also that the expansion-coefficient sets of the various fields depend on the orientation of the Cartesian frame
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The center of the Cartesian frame defining the vector spherical harmonics has to be chosen at the particle center. For a given origin, note also that the expansion-coefficient sets of the various fields depend on the orientation of the Cartesian frame.
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63
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84894000593
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Our method, applied in the context of highly convergent light beams, is basically similar to the Bromwich approach used in the context of paraxial Gaussian beams [49,50,53
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Our method, applied in the context of highly convergent light beams, is basically similar to the Bromwich approach used in the context of paraxial Gaussian beams [49,50,53].
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65
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0001106323
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Electromagnetic diffraction in optical systems. II. Structure of the image field in a aplanatic: System
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B. Richards and E. Wolf, "Electromagnetic diffraction in optical systems. II. Structure of the image field in a aplanatic: system." Proc. R. Soc. London, Ser. A 253, 358-379 (1959).
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Richards, B.1
Wolf, E.2
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66
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0000145768
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Electromagnetic field in the neighborhood of the focus of a coherent beam
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A. Boivin and E. Wolf, "Electromagnetic field in the neighborhood of the focus of a coherent beam," Phys. Rev. 138, B1561-131565 (1965).
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(1965)
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Boivin, A.1
Wolf, E.2
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67
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84942362647
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The factor [cos(θ)1/2 is necessary to ensure energy conservation, as the lens, which obeys the sine condition, converts the incoming plane phase front to a spherical phase front in the image space (see [65] for the vector case). This factor is usually set equal to unity since small Angles are implicitly assumed in scalar theory.
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The factor [cos(θ)1/2 is necessary to ensure energy conservation, as the lens, which obeys the sine condition, converts the incoming plane phase front to a spherical phase front in the image space (see [65] for the vector case). This factor is usually set equal to unity since small Angles are implicitly assumed in scalar theory.
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68
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84942362648
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For small u=kp sin(θ) value the Bessel functions Jn>0( u) are close to zero. Moreover, the leading θ-function factor in the integrals In is the one entering the I0 expression. The electric field is thus accurately calculated in retaining only the main term KI0ex ≈ Escalar.
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For small u=kp sin(θ) value the Bessel functions Jn>0( u) are close to zero. Moreover, the leading θ-function factor in the integrals In is the one entering the I0 expression. The electric field is thus accurately calculated in retaining only the main term KI0ex ≈ Escalar.
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70
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84942362649
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When the properties of the associated Legendre polynomials are used, the integral involving the function πn1(θ) in Eq. (26) is found to be equal to (θmax)2 (2n + 1)1/2/4 (only terms with the lowest order in 2qmax are kept in the calculations). An identical result is obtained for the integral involving the function τn1(θ). The field amplitude at the focus, given by Eq. (11), is equal to Kπ (θmax)2. The plane-wave expansion Eq. (B11) in Appendix B is thus recovered.
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When the properties of the associated Legendre polynomials are used, the integral involving the function πn1(θ) in Eq. (26) is found to be equal to (θmax)2 (2n + 1)1/2/4 (only terms with the lowest order in 2qmax are kept in the calculations). An identical result is obtained for the integral involving the function τn1(θ). The field amplitude at the focus, given by Eq. (11), is equal to Kπ (θmax)2. The plane-wave expansion Eq. (B11) in Appendix B is thus recovered.
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71
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11944275123
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Symmetry relations of the translation coefficients of the spherical scalar and vector multipole fields
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K. T. Kim, "Symmetry relations of the translation coefficients of the spherical scalar and vector multipole fields," Prog. Electromagn. Res. 48, 45-66 (2004).
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(2004)
Prog. Electromagn. Res
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, pp. 45-66
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Kim, K.T.1
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72
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0000577165
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Efficient evaluation of vector translation coefficients in multiparticle light-scattering theories
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Y. Xu, "Efficient evaluation of vector translation coefficients in multiparticle light-scattering theories," J. Comput. Phys. 139, 137-165 (1998).
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(1998)
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Xu, Y.1
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74
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84894004375
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In the present context the sine condition implies that the emergent ray meets the focal sphere (sphere of centre O and radius equal to f) in the image space at the same height at which the corresponding ray in the object space entered the objective lens; see [65, and [37, p. 180. This property is illustrated in Fig. 1 the gray sphere, in fact a small portion of it, is assumed to be of radius f
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In the present context the sine condition implies that the emergent ray meets the focal sphere (sphere of centre O and radius equal to f) in the image space at the same height at which the corresponding ray in the object space entered the objective lens; see [65], and [37], p. 180. This property is illustrated in Fig. 1 (the gray sphere - in fact a small portion of it - is assumed to be of radius f).
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75
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84942362650
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In general a0/2 is small as compared with the second term in the denominator of Eq. (51).
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In general a0/2 is small as compared with the second term in the denominator of Eq. (51).
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76
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84893996740
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All the calculations have been performed with a standard PC (Intel Pentium 4 processor with 3.2 GHz clock speed, computational code written in the C language, Typically the spectra or error parameter curves (as a function of λ) displayed in the manuscript involve roughly Nλ=280 wavelengths and a maximum order Nmax in the expansion of the fields equal to 15 i n=1,2,3, Nmax in Eqs, B1, B3, Actually this large Nmax value is not necessary for particles of radius equal to or smaller than 100 nm. Besides the Lorenz-Mie coefficients [Eqs, B4, B7, the present theory requires the Bessel functions Jm(x =kpp sin(2q, and Legendre polynomials Pnm(θ) to be computed for each θ value in the integral of Eq, 32, Typically 800-1200 θ values are retained, depending on the parameter kpp in the argument of the B
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All the calculations have been performed with a standard PC (Intel Pentium 4 processor with 3.2 GHz clock speed, computational code written in the C language). Typically the spectra or error parameter curves (as a function of λ) displayed in the manuscript involve roughly Nλ=280 wavelengths and a maximum order Nmax in the expansion of the fields equal to 15 i n=1,2,3,..., Nmax in Eqs. (B1)-(B3)]. Actually this large Nmax value is not necessary for particles of radius equal to or smaller than 100 nm. Besides the Lorenz-Mie coefficients [Eqs. (B4)-(B7)] the present theory requires the Bessel functions Jm(x =kpp sin(2q)) and Legendre polynomials Pnm(θ) to be computed for each θ value in the integral of Eq. (32). Typically 800-1200 θ values are retained, depending on the parameter kpp in the argument of the Bessel function Jm (and also on kpp in the exponential factor), though this quite large number is unnecessary in most cases of interest. Thanks to efficient recurrence relations obeyed by the Bessel functions and the Legendre polynomials [64], a spectrum is obtained within 3-4 s for an arbitrary particle location (pp ≠ 0; zp ≠ 0). This time obviously depends on the Nλ, Nmax, and θ step values that are selected. This high speed is rooted in the simple mathematical ingredients (standard analytical functions) involved in the theory.
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