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Study on the time-varying and propagating characteristics of ultrashort pulse Laguerre-Gaussian beam

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Abstract

This work proposes a simple model of pulse Laguerre-Gaussian Beam (LGB) by chopping the incident continuous wave LGB into ultrashort pulse. The pulse LGB is expanded into a series of LGBs with the same angular quantum number (AQN) but different radial quantum number (RQN). The expansion coefficients may show the time-varying and propagating characteristics of the pulse helical beam. Bigger RQN of the incident LGB will cause more serious mode dispersion. This work discusses emphatically the cases that the incident LGBs have zero RQN, in which the original mode, i.e. the same eigen-mode as the incident beam, can be used to approximate the pulse LGB in short propagating range, e.g. 2zR. The original mode decreases, spreads and delays when propagating, and it’s more evident for incident LGB with larger AQN. These conclusions are important for the optical communication that uses the orbital angular momentum division multiplexing (OAM-DM) technology.

©2010 Optical Society of America

1. Introduction

Helical beam is a kind of vortex beams with helical wavefront, and hence it carries the orbital angular momentum (OAM). Allen et al presented that the helical beam with a helical phase term ei, e.g. the Laguerre-Gaussian beam (LGB), possesses OAM quantified with lh̄ per photon [1], where l is an integer called angular quantum number (AQN). In past a decade, the helical beam is paid great attention in many applications, such as optical spanner [2], high density data propagating [3], quantum information processing [4], and etc. Now, several work groups study intensively the optical communication using the helical beams [3,5–11] by virtue of the infinite eigen-states of the OAM operator −iφ [12].

Recently, the ultrafast optics was paid great attention and the pulse width was shorten to the order of a wavelength. This leads to the femtosecond optics, which play significant roles in ultrafast optical switch and the future all optical network. The ultrafast optics may instil new vitality to the OAM division multiplexing (OAM-DM) technology, which is an important channel multiplexing technology first presented by Wei [13]. The OAM-DM technology constructs channels by using the eigen-modes of the OAM operator and transmitting information in each channel. The ultrashort pulse beam operating on the fundamental Gaussian mode was studied intensively in the past decades, while that operating on the helical modes appeared only in numbered works [14, 15]. The time-varying and propagating characteristics of the pulse helical beam are still undiscovered.

This work propose a pulse helical beam model by chopping the incident continuous wave LGB into ultrashort pulse like that used by Porras et al [16], and expand the pulse LGB into a series of LGBs with the same AQN but different angular quantum numbers (RQNs). The expansion coefficients of these decomposed modes show the time-varying and propagating characteristics of the pulse beam. This work details these characteristics and is important for the optical communication by using the OAM-DM technology.

2. Theoretical analysis

2.1. Solution of pulse wave equation in paraxial condition

The paraxial envelope equation of the pulse beam is familiar as [16]

Δψ+2ik0zψ2cztψ=0,

where ∆ = ∂2 x + ∂2 y is the two dimensional Laplace operator and k 0 = ω 0/c the wave number with ω 0 and c the central angular frequency and light velocity, respectively. In case of monochromatic wave, the third term in the right hand of Eq. (1) can be omitted and Eq. (1) can be simplified as

Δψ+2ik0zψ=0.

The solution of Eq. (2) may be the familiar normalized LGBs ψm,n with RQN m nonnegative integer and AQN n integer.

An simple method to solve the pulse equation Eq. (1) is the perturbation method [16], which considers the third term in Eq. (1) as the perturbation to the second term. But in this work we expand the pulse beam as the superposition of LGBs and obtain the expansion coefficients, which contain the time-varying and propagating characteristics of the pulse beam.

The incident beam can be expand as the superposition of LGBs

ψ=m,nam,n(z,t)ψm,n.

Substitute Eq. (3) into Eq. (1) and consider Eq. (2), we can obtain

m,nψm,n(ω0zam,n+iztam,n)+izψm,ntam,n=0.

Multiply the complex conjugation ψ*m′,n′ on Eq. (4) and integrate on the transverse plane, then

mδm,m(iω0t)zam,nHm,ntam,n=0,

where Hm′,m = 〈ψ*m′,nzψm,n〉, with the symbol 〈*〉 denotes the integral on the transverse plane. Equation (5) can also be rewritten as matrix equation

(iω0t)zXHtX=0,

where X = (a 0,n,a 1,n, ⋯,am,n, ⋯)T and H = (Hm′,m).

The matrix equation Eq. (6) can be converted to a group of second order partial differential equations with two variables and several functions. Its solution relies on the properties of the matrix H. According to Zauderers’ work [17] and the property of Laguerre polynomials [18], we can obtain the matrix elements Hm′,m and then the properties of the matrix H:

  1. H does not vary with z or t,
  2. H is a symmetric matrix,
  3. only the elements on the main diagonal and two side minor diagnals of H are nonzero,
  4. and the nonzero elements of H are pure imaginary numbers with negative imaginary part.

There must be an invertible matrix U to convert H to a diagonal matrix, i.e. U −1 HU = −iΛ, where the diagonal matrix Λ has positive real diagonal elements λ 0,n, λ 1,n, ⋯, λm,n, ⋯ according to the properties (b), (c) and (d). Then the matrix equation [Eq. (6)] can be simplified as

(iω0t)zY+iΛtY=0,

where Y = (b 0,n,b 1,n, ⋯,bm,n, ⋯)T = U −1 X.

We note that Λ is a diagonal matrix, then the coupled equations in Eq. (5) can be decoupled to some separate equations. Each separate equation reads

(iω0t)zbm,n+iλm,ntbm,n=0.

The solution of the Eq. (8) relies on the boundary condition and initial condition which relate to the pulse model.

2.2. Pulse model, boundary condition and initial condition

In optical communication, fast modulation is needed. The future applications of the OAM in high date rate communication and quantum information processing will deep into the domain of ultrafast optics. A simple model ultrashort LGB can be constructed by chopping a single mode continuous wave LGB into slice.

As shown in Fig. 1, a traveling LGB is chopped by a planner shutter perpendicular to the beam axis and large arbitrarily in transverse plane. The transmittance of the planner shutter is equal in transverse plane and changes quickly.

 figure: Fig. 1.

Fig. 1. Model of ultrashort pulse LGBs generation.

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It’s convenient to let the transmittance or wave envelope f(t) be Gaussian, i.e.

f(t)=exp(t2T2),

where T is related to the pulse duration by Δt=2ln2T .

Consider the case of single incident LGB mode ψm0,n , the boundary condition of Eq. (1) reads

ψ(x,z=0,t)=ψm0,nf(t),

and therefore the boundary condition of Eq. (7) reads

Yz=0=(U¯1,m0U¯2,m0...U¯m,m0...)Tf(t),

where U¯m,m0=(U1)m,m0 denote the matrix element of U −1.

Similarly, the initial condition of Eq. (7) also reads

Yt==0.

According to Eqs. (8), (11) and (12), the problem of pulse LGB can be formulated as

{tzbm,niω0zbm,niλm,ntbm,n=0bm,nz=0=U¯m,m0f(t)bm,nt==0

In this work, the numeric results are given for further discussions.

3. Results and discussions

In this work, the computation is carried out for the single cycle pulse LGBs, i.e. the pulse duration ∆t equals a wave cycle T 0. The incident LGBs are ψ 0,0, ψ 0,3, ψ 0,6 and ψ 3,3, respectively. For a certain incident LGB, the pulse beam may be decomposed into many LGBs. These decomposed beams have the same AQN but different RQNs because of the orthogonal relationship of the LGBs. The following discuss bases on the analysis of the expansion coefficients |am,n(z, t)|2, which shows the power distribution with the time t and along the beam propagation direction z. So |am,n(z, t)|2 may give the time-varying and propagation characteristics of the pulse LGB.

 figure: Fig. 2.

Fig. 2. (color online)Time-varying and propagating of decomposed LGBs, |am,n(z, t)|2. Incident LGBs (rows from top to bottom) are ψ 0,0, ψ 0,3, ψ 0,6, and ψ 3,3; RQN of decomposed LGBs (columns from left to right) are m = 0, 1, 2, but m = 2, 3 and 4 in the last row.

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Figure 2 gives the power distribution with t and along z of the decomposed modes of the pulsed LGBs, i.e. |am,n(z, t)|2. The time axis is scaled by the wave cycle T 0 and the z axis by Rayleigh range zR as denoted in Fig. 2(a). Other subgraphs use the same setting. The inset in each subgraph shows the corresponding top view. Figs. 2(a)–2(c) in the first row are computed in case of pulsed LGB with (m,n) = (0,0), and show |am,n(z, t)|2 of the decomposed LGBs with m = 0, 1 and 2, respectively. Although m is theoretically infinite, |am,n|2 is rather small for m > 2 in range of about −5T 0t ≤ 5T 0 and 0 ≤ z ≤ 10zR. Therefore, the decomposed LGBs with m > 2 are not shown here. This also mean that only numbered terms in expansion Eq. (3) can give acceptable result. There are 8 expansion terms retained in this work and they are sufficient. Because of the orthogonal relation between the helical phase terms exp(i), the AQN does not change in the first row. The other rows from the top down are computed for incident LGBs with (m,n) = (0,3), (0,6) and (3,3),respectively. The RQNs of the decomposed LGBs from left to right in the upper three rows are 0, 1 and 2, respectively. But in the bottom row they are 2, 3 and 4, respectively.

In each row in Fig. 2, the power of the original mode is much bigger that others. For example, in the second row the original mode is shown in Fig. 2(d) with (m,n) = (0,3) and the power in the range of −5T 0t ≤ 5T 0 and 0 ≤ z ≤ 10zR is rather bigger than others in the same row. The original mode decays along the z axis while other modes arise. In near area with little z, the original mode is dominant. With increasing z, the power distribution spreads and delays in time axis. The mode dispersion also indicates that the pulse beam will spread in transverse plane, because higher order modes have bigger transverse dimension. From top to bottom, the incident mode with the same RQN m = 0 but larger AQN n shows bigger delay in time and decay in z direction, and larger pulse spread in time and transverse plane. In spite of the difference, they show similar time-varying and propagating characteristics. But for the incident LGBs with nonzero RQN m, even with the same AQN n, the original modes decay much faster. For example, the incident LGBs in the second and fourth rows are ψ 0,3 and ψ 3,3, respectively. The original mode ψ 3,3 in Fig. 2(k) decays much faster than ψ 3,3 in Fig. 2(d).

 figure: Fig. 3.

Fig. 3. Time-varying of decomposed LGBs, |am,n(z, t)|2, at different distances. Incident LGBs (rows from top to bottom) are ψ 0,0, ψ 0,6, and ψ 3,3; Distances (columns from left to right) are z = zR, 2zR, and 4zR.

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We also note that for the incident LGBs with zero RQN, the original mode is dominant in rather long range, e.g. z < 2zR, along z axis. There the pulse beam may be processed as the original mode provided that the time delay and spread been dealt with properly. This is important for ultra fast modulation of the channels in the OAM-DM technology.

Figure 3 shows the time-varying of decomposed LGBs at different distances. The incident LGB modes in the rows from top to bottom are ψ 0,0, ψ 0,6 and ψ 3,3, respectively. The columns from left to right are obtained at z = zR, 2zR, and 4zR, respectively. It’s clear that bigger AQN causes faster decay along z direction, and larger pulse spread and delay on the original modes (denoted by solid lines). For example, for incident LGB with m = 0 at z = 4zR, the peak values of the original modes decay to about 0.8 [Fig. 3(c)] and 0.3 [Fig. 3(f)] for incident LGBs ψ 0,0 and ψ 0,6,respectively. The corresponding pulse widths are about 2.4T 0 and 3.5T 0, respectively. And the corresponding pulse delays are about 0.4T 0 and 2.0T 0, respectively. But for incident LGB with m = 3 in the lowest row, the original mode is flooded by other modes quickly with increasing z, e.g. in Fig. 3(i). In the optical communication using the OAM-DM technology large RQN should be avoid because of serious decay and pulse spread. The original mode with zero RQN will be dominant in rather long range, e.g. z < 2zR.

4. Conclusion

This work expands the pulse beam as superposition of a series of LGBs. The expansion coefficients vary with time and longitudinal coordinate, and show the time-varying and propagating characteristics of the pulse beam. For the incident LGBs with nonzero RQN the original modes decrease seriously along longitudinal coordinate and are flooded by other modes. For the incident LGBs with zero RQN, the original modes are dominant in rather long range, e.g. z < 2zR, and the pulse delay and spread increase gradually with the longitudinal coordinate increasing. This mean that in near area the original modes also can approximate the pulse LGB with zero RQN.

Acknowledgement

This work was partly supported by the National Science Foundation of China (60908034), the National Science Foundation of China (60778002), and the Doctoral Fund of Ministry of Education of China (20090185120016).

References and links

1. L. Allen, M. W. Beijersbergen, R. J. C. Spreeuw, and J. P. Woerdman, “Orbital angular momentum of light and the transformation of Laguerre-Gaussian laser modes,” Phys. Rev. A 45, 8185–8190 (1992). [CrossRef]   [PubMed]  

2. H. He, M. E. J. Friese, N. R. Heckenberg, and H. Rubinsztein-Dunlop, “Direct observation of transfer of angular momentum to absorptive particles from a laser beam with a phase singularity,” Phys. Rev. Lett. 75, 826–829 (1995). [CrossRef]   [PubMed]  

3. G. Gibson, J. Courtial, M. J. Padgett, M. Vasnetsov, V. Pas’ko, S. M. Barnett, and S. Franke-Arnold, “Free-space information transfer using light beams carrying orbital angular momentum,” Opt. Express 12, 5448–5456 (2004). [CrossRef]   [PubMed]  

4. A. Mair, A. Vaziri, G. Weihs, and A. Zeilinger, “Entanglement of the orbital angular momentum states of photons,” Nature 412, 313–316 (2001). [CrossRef]   [PubMed]  

5. Z. Bouchal and R. Celechovsky, “Mixed vortex states of light as information carriers,” N. J. Phys. 6, 131 (2004). [CrossRef]  

6. C. Paterson, “Atmospheric turbulence and orbital angular momentum of single photons for optical communication,” Phys. Rev. Lett. 94, 153901 (2005). [CrossRef]   [PubMed]  

7. Z. Bouchal, V. Kollarova, P. Zemanek, and T. Cizmar, “Orbital angular momentum of mixed vortex beams,” Proc. SPIE 660907, 1–8 (2007).

8. J. Lin, X.-C. Yuan, S. H. Tao, and R. E. Burge, “Multiplexing free-space optical signals using superimposed collinear orbital angular momentum states,” Appl. Opt. 46, 4680–4685 (2007). [CrossRef]   [PubMed]  

9. Y. D. Liu, C. Gao, X. Qi, and H. Weber, “Orbital angular momentum (OAM) spectrum correction in free space optical communication,” Opt. Express 16, 7091–7101 (2008). [CrossRef]   [PubMed]  

10. J. A. Anguita, M. A. Neifeld, and B. V. Vasic, “Turbulence-induced channel crosstalk in an orbital angular momentum-multiplexed free-space optical link,” Appl. Opt. 47, 2414–2429 (2008). [CrossRef]   [PubMed]  

11. G. A. Tyler and R. W. Boyd, “Influence of atmospheric turbulence on the propagation of quantum states of light carrying orbital angular momentum,” Opt. Lett. 34, 142–144 (2009). [CrossRef]   [PubMed]  

12. G. Molina-Terriza, J. P. Torres, and L. Torner, “Management of the angular momentum of light: Preparation of photons in multidimensional vector states of angular momentum,” Phys. Rev. Lett. 88, 013601 (2002). [CrossRef]   [PubMed]  

13. H. Wei, X. Xue, J. Leach, M. J. Padgetc, S. M. Barnett, S. Franke-Arnoldd, E. Yao, and J. Courtial, “Simplified measurement of the orbital angular momentum of single photons,” Opt. Commun. 223, 117–122 (2003). [CrossRef]  

14. S. Feng and H. G. Winful, “Higher-order transverse modes of ultrashort isodiffracting,” Phys. Rev. E 63, 046602 (2001). [CrossRef]  

15. J. Lekner, “Helical light pulses,” J. Opt. A 6, L29–L32 (2004).

16. M. A. Porras, “Pulse correction to monochromatic light-beam propagation,” Opt. Lett. 26, 44–46 (2001). [CrossRef]  

17. E. Zauderer, “Complex argument Hermite - Gaussian and Laguerre - Gaussian beams,” J. Opt. Soc. Am. A 3, 465–469 (1986). [CrossRef]  

18. http://en.wikipedia.org/wiki/Laguerre_polynomials

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Figures (3)

Fig. 1.
Fig. 1. Model of ultrashort pulse LGBs generation.
Fig. 2.
Fig. 2. (color online)Time-varying and propagating of decomposed LGBs, |am,n (z, t)|2. Incident LGBs (rows from top to bottom) are ψ 0,0, ψ 0,3, ψ 0,6, and ψ 3,3; RQN of decomposed LGBs (columns from left to right) are m = 0, 1, 2, but m = 2, 3 and 4 in the last row.
Fig. 3.
Fig. 3. Time-varying of decomposed LGBs, |am,n (z, t)|2, at different distances. Incident LGBs (rows from top to bottom) are ψ 0,0, ψ 0,6, and ψ 3,3; Distances (columns from left to right) are z = zR , 2zR , and 4zR .

Equations (13)

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Δ ψ + 2 i k 0 z ψ 2 c z t ψ = 0 ,
Δ ψ + 2 i k 0 z ψ = 0 .
ψ = m , n a m , n ( z , t ) ψ m , n .
m , n ψ m , n ( ω 0 z a m , n + i z t a m , n ) + i z ψ m , n t a m , n = 0 .
m δ m , m ( i ω 0 t ) z a m , n H m , n t a m , n = 0 ,
( i ω 0 t ) z X H t X = 0 ,
( i ω 0 t ) z Y + i Λ t Y = 0 ,
( i ω 0 t ) z b m , n + i λ m , n t b m , n = 0 .
f ( t ) = exp ( t 2 T 2 ) ,
ψ ( x , z = 0 , t ) = ψ m 0 , n f ( t ) ,
Y z = 0 = ( U ¯ 1 , m 0 U ¯ 2 , m 0 . . . U ¯ m , m 0 . . . ) T f ( t ) ,
Y t = = 0 .
{ t z b m , n i ω 0 z b m , n i λ m , n t b m , n = 0 b m , n z = 0 = U ¯ m , m 0 f ( t ) b m , n t = = 0
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