Introduction

Optical trapping and manipulation is an efficient and precise method for controlling and delivering microscopic objects to a desired position, i.e. it can provide stabilizing, accelerating or directional control of the motion of micro- or nanoparticles1. The purpose of using this method is to apply the high local confinement of an optical trapping field to specimens of biological interest, such as the manipulation and force measurements of DNA- and RNA-based motors involved in transcription and translation processes2,3. Applications include the investigation of cell cytometry4, artificial fertilization of mammalian cells and microsurgery5. Since Ashkin6 first introduced optical trapping using a highly focussed laser beam through a high numerical aperture microscope objective, much work has been done based on the so-called optical tweezers5,7. Along with that technique, substantial research on optical trapping using evanescent fields in the vicinity of optical waveguides, or at the interface of substrates, has also been undertaken8,9,10,11.

The evanescent field of a waveguide can create strong optical forces, which yield a larger trapping volume at its surface compared to the small waist of a focussed beam in an optical tweezers and this phenomenon overcomes the limitations imposed by the Rayleigh range. Such optical waveguides can provide long range controllable transport of micro/nano-objects10,11,12. Among all waveguides, the optical micro/nanofibre (MNF) is fast becoming a common tool for cold atom and particle manipulation experiments13 as it can be fabricated in standard laboratory conditions with relative ease and is readily integrated into other fibre optic-based systems.

Until recently, experimental research using MNFs was mostly based on the fundamental guided mode (FM)13,14,15,16,17. MNFs initially attracted much interest in the field of cold atoms due to their potential for efficiently coupling light from the trapped atoms to the fibre18,19,20. However, though there have been several theoretical proposals that considered higher order modes (HOMs) for cold atom trapping and detection,21,22,23 there was little experimental progress due to the difficulty in fabricating MNFs for efficient HOM propagation. Recently, due to the advances made in higher order mode MNFs fabrication24,25,26 preliminary experimental studies on the interactions between atoms and HOMs have been reported27. All of this work exploits the longer evanescent field extension from the fibre surface, the three dimensional (3D) arrangement of the field and the larger cut-off waist diameter of the fibre compared to that needed for fundamental mode propagation. 3D microtrap arrays can be generated when one considers the interference between FM and HOMs co-propagating through an MNF22,23. Applications of such 3D potential geometries, in combination with light from cold atoms coupled to the fibre modes, provide a promising method to realise the retrieval and storage of light with atomic ensembles near MNF surfaces.

A 3D HOM potential lattice around a microfibre can also be used to investigate particle manipulation. This all-optical manipulation method offers rapid control of trapped microparticle sites around a microfibre through the generation of radially, azimuthally and hybrid polarised HOM light fields. This provides flexible options for practical applications of particle sorting, control and the investigation of the internal structure of large complex cells in an aqueous environment. Moreover, the increased interaction of light in HOMs with particles reduces the challenges of fibre handling and increases the lifetime of the fibre since one can work with a micron-sized fibre rather than the more fragile nanofibre. Using HOMs for particle or atom trapping in a multimode waveguide28 or a hollow core photonic crystal fibre29 has been studied. The main difficulty in performing these experiments is maintaining the polarisation while HOMs propagate in the fibre. Controlling the loss of HOMs due to the presence of complex trapped objects on the fibre surface can also be challenging. The success of these experiments is, therefore, strongly dependent upon understanding the interaction between each individual particle and the HOM's evanescent fields. However, to our knowledge, the study of the interaction between HOM evanescent fields around a microfibre with individual particles has not previously been demonstrated.

In this paper, we take advantage of the stated benefits of HOMs in MNFs and investigate particle propulsion induced by the evanescent field of HOMs propagating in a microfibre. We used a spatial light modulator (SLM) to produce a doughnut-shaped, first order, Laguerre-Gaussian (LG01) beam in free-space. When coupled into suitable optical fibre, LG01 excites the LP11 approximate, first higher order fibre mode and, at the waist region, the true fibre modes, TE01, TM01 and HE21e,o, are generated24. Incorporating the microfibre into an optical tweezers30 allowed us to control the number of particles in the fibre trap very precisely and study the interaction of one or more particles with the evanescent field at the fibre waist. Propulsion speeds of single polystyrene beads with diameters from 1 μm to 5 μm were compared for both FM and HOM propagation. A speed dependence on particle size was also observed and will be discussed here.

Theory

Maxwell's stress tensor and force calculation

The electromagnetic field distribution can be described using Maxwell's equations. The electric field expression can be determined from equation

Here, E is the electric field, k0 is the wave vector and n is the refractive index of the material (for the case studied here we take n = 1.46 for silica fibre). The interaction between the surface evanescent field of an optical micro/nanofibre and a dielectric micro-object results in three different optical forces acting on the object. The trapping force, also called the gradient force, Fg, is induced due to the temporary polarisation of a dielectric particle in a non-uniform field. The other forces are the result of radiation pressure6. Namely the scattering, Fs and absorption, Fa, forces are responsible for the movement of particles along the optical axis of the fibre. The total force can be described as electromagnetic stress using the Maxwell stress tensor. As particles are transported over a timescale much longer than the optical period of the incident fields coupled into the fibre, the time-independent Maxwell stress-tensor 〈TM〉 can be used to calculate the forces. It is given by31

where E, D, H and B denote the electric field, the electric displacement, the magnetic field and magnetic flux, respectively. I is the isotropic tensor, D* and E* are the complex conjugates.

By applying the relations D = εrε0E and B = μrμ0H, equation (2) can be written

where Ei and Hi are i-th components of the electromagnetic field. μ0, μr, ε0, εr are vacuum and relative permeability and permittivity, respectively.

The total electromagnetic force acting on the particle can be calculated from the integration of the Maxwell stress tensor over the surface of the particle,

where ns is a normal vector pointing in the outward direction from the surface, S.

Here, we consider a system which consists of a particle (with refractive index ) in the evanescent field of a micro/nanofibre in a medium (of refractive index n2). For a non-absorptive particle (i.e. is real), the force acting on the particle can be expressed as the scattering force (FS) along the fibre axis and the gradient force (Fg) perpendicular to it32,33

Here

and α is the electric polarizability of the particle given by , being the conventional Mie coefficient34, ε is the complex amplitude of the electric field.

For nonabsorptive particles α can be approximated as

where a is the particle's radius. We assume that the spin component of the field contributing to the force is negligible; therefore, the scattering force can be described as

where S is the Poynting vector and σext is the extinction cross-section of the Rayleigh particle given by33

Microfluidic effect on particles near a microfibre surface

Since the particles move close to the surface of a microfibre, the standard bulk Stokes' drag coefficient, F = 6πμav, where μ is the viscosity and v is the particle velocity, cannot be used. Two major correction factors have been used in the literature depending on the distance between the trapped particle and the host surface35,36. Assuming h is the distance from the centre of the particle to the fibre surface, Goldman et al.37 used the Faxen correction factor for h > 1.04 a and the deviation was less than 10% compared to experiment. In this case, the force is given by

Alternatively, when h < 1.04 a, the lubrication values of this correction are used, as shown by Krishnan and Leighton38 such that

Numerical techniques

A finite element method (FEM) is used to calculate the E-field distribution along the microfibre (equation 1). The wavelength of the propagating light, λ, was set to 1064 nm. At this wavelength the refractive index of the fibre and water are n = 1.46 and n2 = 1.33, respectively. To simplify our calculations, we assumed that the power coupled into each individual component of the HOM set was identical. For all calculations, the total propagating power of the HOM was normalized to 25 mW.

Figure 1 shows the scattering force, Fs (parallel to the fibre surface) and the gradient force, Fg (perpendicular to the fibre surface), acting on the particle. Light propagates from left to right.

Figure 1
figure 1

Gradient and scattering (Fg, Fs) forces on particles in the evanescent field of a microfibre.

The inner ring represents the physical polystyrene beads with refractive index , positioned 20 nm away from the fibre surface. The outer ring represents a circular surface of the momentum transfer region, which is the integration area of the Maxwell stress tensor on the particle36. The momentum transfer that causes the particle to be trapped and propelled is equal to the momentum difference between the surrounding medium (n2 = 1.33) and the particle. By changing this outer ring region from 1.05 up to twice the particle size, the total force calculated from this momentum transfer area only varies within 1.5%. The Maxwell stress tensor integration area was therefore set to be 1.1 times the particle size in all our experimentally relevant calculations.

Results

Distribution of LP01 and LP11 modes in a microfibre

According to the weakly guiding approximation39, modes of a standard fibre are approximated as linearly polarised modes or LPlm modes (where the subscripts l and m indicate the radial and azimuthal order, respectively). However, when the fibre is tapered down and immersed in water, the LPlm modes split in to the TElm, TMlm, HElm and EHlm modes. Here, we consider the LP01 or fundamental mode (FM) and the LP11 mode group, i.e. the first higher order modes. The first four HOM profiles and E-field distribution of a 2 μm fibre are shown in figure 2.

Figure 2
figure 2

Mode profiles of the first four true HOMs in 2 μm fibre.

(a-d) Numerical mode intensity profiles of the first four true HOMs. Dashed lines indicate the orientation of the corresponding maximum intensity profile. (e) E-field distributions of each of the individual HOMs (top three distributions), along with a plot showing the distributions superimposed on top of each other (bottom) to show their relative intensities (corresponding to the field along the dashed line).

The calculated decay length for each of the individual HOMs for this fibre shows that all HOMs have approximately the same decay length of 0.52 μm (the decay lengths of TE01, TM01 and HE21 are 0.503 μm, 0.52 μm and 0.525 μm respectively) while the FM has a decay length of 0.33 μm.

Figures 3(a) and (b) present the numerical beam profiles and electric field polarisation direction, while figures 3 (c) and (d) show the experimental beam profiles of the fundamental LP01 and the higher order LP11 mode set, respectively. The LP11 mode set in figure 3(b) represents the total E-field distribution of the HE21,o, HE21,e, TE01 and TM01 modes. As can be seen from the individual mode profiles (Figure 2), each of the HOMs is different. We chose a specific mode combination as a representative field, consisting of equal portions of each mode. This was used as a model to better explain the phenomena at play in our experiments. Figure 3(e) clearly shows that, when one considers the intensity distribution along the horizontal direction, the total evanescent field of the HOMs have larger amplitudes and longer evanescent field extensions when compared to the FM at a given distance from the surface of a 2 μm fibre. The field intensity, which is calculated from the E-field for a given fibre diameter, also indicates that, if the waist power is the same for the HOMs and the FM, the total evanescent portion of the HOMs is three times larger than that of the FM.

Figure 3
figure 3

Field distribution of LP01 and the LP11 mode set.

(a, b) Numerical mode profiles of the LP01 and total E-field distribution of four modes (TE01 and TM01, HE21,e, HE21,o) in the LP11 set, (c, d) experimental beam profiles of the fundamental LP01 and the higher order LP11 modes, respectively. The horizontal dashed lines represent the orientation of maximum intensity (e) E-field distribution of the LP01 and LP11 mode set of a 2 μm microfibre along the direction indicated by the dashed line in (a) and (b).

Optical forces acting on particles in the evanescent field of LP01 and LP11 modes

As mentioned in the Theory section, there are two different optical forces acting on the dielectric particles near the microfibre: the gradient force and the scattering force.

Figure 4(b) presents the calculated scattering (Fs-HOM, Fs-FM) and gradient (Fg-HOM, Fg-FM) forces acting on a single particle touching a microfibre in water for both the HOM and FM cases, respectively. Negative values of the gradient force, Fg, indicate that the particles are attracted to the fibre surface. A positive scattering force, Fs, designates particle propulsion from left to right along the fibre. It is clearly seen that both absolute gradient and scattering forces decrease with fibre size for all cases. By comparing the forces from figure 4(a), it is found that both forces have greater magnitude in the HOM case compared to the FM case for fibre diameters greater than the LP11 cut-off value. This implies an enhancement of particle trapping stability and propulsion speed in the presence of the HOM evanescent field. Figure 4(b) shows that both the scattering and gradient forces increase with increased particle size for a given fibre diameter. However, this particle size dependence is more remarkable for HOMs than for the FM.

Figure 4
figure 4

Calculated optical forces acting on a particle.

(a) Magnitude of gradient and scattering (Fg-HOM, Fs-HOM) forces for the LP11 mode set and (Fg-FM, Fs-FM) forces for LP01 mode, respectively, on a 3 μm polystyrene particle. Scattering and gradient forces of HOMs are considerably stronger than those of the FM at the HOM cut-off or larger fibre diameter. (b) Particle size dependence of optical forces for the 2 μm fibre diameter. Larger particles experience stronger optical forces. The waist power was 25 mW.

Speed of microparticles near a microfibre surface

Along with the theoretical analysis, an experimental setup was built as in figure 5. A 1064 nm laser was coupled into the microfibre which was immersed in water dispersion. A polystyrene particle was trapped with an optical tweezers and approached to the microfibre. When the tweezers was turned off, the particle was propelled along the fibre. (See Methods and Supplementary Information). To obtain the average particle speed, the position of each particle was recorded for a distance of 75 μm along the microfibre. Each measurement was repeated at least three times.

Figure 5
figure 5

Experimental setup for particle propulsion.

L1, L2, L3, L4 are lenses, LP and HWP are a linear polariser and a half wave plate, respectively, BS is a beam splitter, CCD is a camera and PC is a computer. The red lines represent the free beam path. The inset shows the magnified image of the interaction region.

Figures 6(a) and (b) show the consecutive images of a propelled 3 μm polystyrene particle captured by the CCD camera under both FM and HOMs conditions. In this time interval (1.2 s), when the waist power was at 25 mW, the particle underwent very slow propulsion under FM propagation while the speed of the particle was greatly increased under HOM propagation. The frame rate of the camera used was not fast enough to track propelled particles at high speed. This caused the particles to appear elongated along the propulsion axis (see Figure 6(b)).

Figure 6
figure 6

Micrograph of 3 μm polystyrene particle propulsion under.

(a) FM and (b) HOMs propagation. In both cases the waist power was 25 mW. Table 1 gives the speed of a 3 μm particle at a fixed waist power of 25 mW obtained experimentally and by three different theoretical methods. The experimental results confirm that, under identical powers at the microfibre waist, the particle speed is approximately 8 times faster under LP11 mode set propagation than in the LP01 case. Such an increase in speed is indicative of the stronger evanescent field and larger field extension of the HOMs.

It is apparent from the values in Table 1 that the bulk Stokes drag coefficient cannot be used to describe the experimental results. In order to better understand the phenomenon of microfluidic approach on particles moving along a microfibre surface, two correction factors were used to calculate the particle velocities37,38. It is clearly shown in Table 1 that, for the FM case, the Krishnan model is in reasonable agreement with the experiment for low particle speeds when the particle is close to the fibre surface (h = 1.52 μm). On the other hand, under the HOM's evanescent field, the speed of the particle is relatively fast compared to the FM case. This leads to strong hydrodynamic interactions that may push the particle to float at a considerable distance from the microfibre surface due to the hydrodynamic lift force. Here, the Krishnan approximation does not hold and the experimentally obtained speed seems to be closer to the value approximated in the Faxen region for h = 1.56 μm.

Table 1 Hydrodynamic velocities of single 3 μm polystyrene beads. Speed of particles is calculated using different correction factors for the LP01 and LP11 microfibre modes. The power at the fibre waist regions Pwaist was fixed at 25 mW

Figure 7 shows the change in the speed of a single 3 μm polystyrene sphere under the evanescent field of both FM and HOMs with varying power as measured from the recorded video files. The agreement between the experimental results and the Krishnan and Faxen corrections is evident in the FM case. However, the particle speeds for the HOMs is slightly higher than those obtained by the Faxen approximation for waist powers less than 25 mW. We assume that the increase in speed due to the increase in waist power causes the particle to move further away from the fibre surface. As this distance increases, the surface and/or hydrodynamic interaction between the particle and the fibre walls weakens allowing the particle to reach a higher speed.

Figure 7
figure 7

Measured speed of a 3 μm polystyrene particle under the evanescent field of the FM (blue circles) and HOM (red stars) as a function of waist power, Pwaist.

The speed is significantly higher for HOM propagation. The filled circles and unfilled stars represent the experimental data and the lines are the theoretical plots.

With the FM waist power less than 20 mW, particles tend to move in discrete jumps or appear at stable positions along the fibre surface. This is probably due to surface roughness effects that can easily dominate over optical forces at low powers.

Effect of particle size on speed of a particle in the microfibre evanescent field

In order to better understand the power/speed relationship described above and characterize the speed changes with different size particles under HOM and FM propagation, polystyrene particles with diameters of 1 μm, 2 μm, 3 μm and 5 μm were experimentally examined under the same conditions. Figure 8 shows the speed dependence on the particle size for both HOM and FM evanescent field.

Figure 8
figure 8

Measured speed dependence on particle size for HOM (blue circles) and FM (red stars) propagation.

Here, the waist power was set to 25 mW for all cases. The lines are theoretical curves.

It is evident that, for HOMs, an increase in particle size is consistently matched with an increase in speed. This size dependence of particle speed has also been observed for the fundamental mode when the fibre size is comparable to the guided wavelength14. It is well known that larger particles have larger scattering cross-sections compared to smaller particles. Consequently, they have a greater interaction with a given evanescent field, causing them to have faster speeds than smaller particles14. It is interesting to note that the experimentally observed increase in speed with larger particle size is not linear. In figure 8, the speed of a 5 μm particle was smaller compared to the theoretical estimates for both HOMs and FM. This could be due to the fact that, as the particle diameter increases, the surface interaction between the particles and the fibre surface also increases leading to lower propulsion speeds along the fibre.

Discussion

Fabrication of high-quality tapered optical fibres for FM propagation is now a routine practice, with laboratories reporting up to 99.95% light transmission through the fibre at the structure waist40. However, tapered fibres that support HOMs with high transmission have only recently been experimentally realized24,25,26. This work presents the first experimental results using highly transmitted HOMs for particle propulsion. The experimental setup combines three subsystems which allowed us to overcome the challenge of generating and obtaining high quality HOMs through an adiabatic microfibre while minimising system interference to study single particle dynamics.

A complete microfluidic system would include the particle's angular rotation, the change of intensity ratio between the HOM components while propagating along the waist region of the microfibre, the surface roughness and the optical torque. It is known that the FM evanescent power of a 2 μm fibre diameter is small and particle speed is relatively slow. Particles that propel with a low speed are closer to the fibre surface due to weak hydrodynamic interactions. In this case, the surface roughness may cause the particle motion to suffer from frictional forces38. The lubrication correction factor, therefore, seems to fit with experiment.

The ratio of the HOMs to the FM velocities, as calculated, is found to be around 5.7 using either method while in experiments this ratio is around 8. This discrepancy can be explained in terms of hydrodynamic interactions. When a particle is moving along a fibre, there are many parameters such as translational speed, particle rotation, surface roughness, etc. which can contribute to the separation distance between the particle and fibre surface; this in turn influences the particle speed. Moreover, when a particle is propelled at high speed, the hydrodynamic lift force can oppose the attractive optical gradient force. This allows the particle to have a larger separation distance from the fibre35,37,38,41. Therefore, under high HOM power (>20 mW), the particle speed may be faster than that calculated in simulations (see Figure 7).

Furthermore, changes in the ratio between the HOM components while propagating along the fibre will change the amplitude of the LP11 set due to the mode interference. In an ideal situation the proportion of each of the modes in the LP11 mode set in the fibre is assumed to be equally distributed. In reality, the proportion of each mode in the fibre may change, leading to a change in the total optical force. In the simulations where Fs and Fg were calculated it was assumed that this ratio remained constant; this may be introducing further inconsistency with the experimental results. The interaction of each of the individual modes in the HOM set with the particle is beyond the scope of this work.

In conclusion, we have successfully demonstrated particle propulsion under the evanescent field of the HOM of a microfibre and compared it with the FM case. Both theoretical analysis and experimental observations showed a higher speed for microparticles under the influence of the evanescent field of HOMs. We also used different sizes of polystyrene beads to address speed dependence on particle size. The hydrodynamic interaction between particles and fibre surface has been studied and discussed. Two correction factors of the hydrodynamic interaction effect have been used to predict the particle speed for the HOM and FM cases. Apart from these, a number of other parameters need to be addressed for a complete understanding of the experiment such as optical torque and surface roughness. An important experimental feature of this work consists of the integration of a MNF within a standard optical tweezers. Specifically, this facilitated the study of individual particle propulsion. As this experimental framework provides exact control of the number of particles that interact with the fibre, in future we plan on studying optical binding and collective propulsion17on interaction with HOMs.

The HOMs have the advantage of possessing a strong evanescent field, thus increasing the sensitivity of interaction between the field and the particles at robust microfibre diameters compared to more fragile nanofibres. The larger evanescent field decay and the field distribution of HOMs can be utilised for particle and refractive index sensing where high sensitivity is required42,43. Additionally, this work can be developed beyond colloidal particles to study novel cold atom traps.

Methods

Generation of higher order modes

To excite the HOMs in the fibre, a beam with a doughnut-shaped intensity cross-section was created in free space. Linearly polarised 1064 nm laser light (Ventus 1064 3W) was launched onto the display of an SLM to create a first-order Laguerre-Gaussian beam (LG01) at the far field44. Two-mode fibre (Thorlabs, SM1250G80) operating at 1064 nm wavelength with a cladding diameter of 80 μm was chosen for this experiment. The fibre supports the fundamental LP01 and the LP11 family of higher order modes. By coupling the LG01 beam to this fibre, a two-lobed pattern corresponding to the LP11 mode can be obtained at the fibre output. By switching the vortex phase grating on the SLM on and off, the propagating mode in the fibre can be easily switched between LP01 and LP11 with high purity. By choosing an appropriate objective lens, 45% coupling efficiency to the LP11 mode was achieved. A charge-coupled device (CCD) camera was used to image the quality of the beam profile. Figure 4 shows the schematic of the experimental setup.

Preparation of higher-mode tapered fibre

Tapered fibres were made on a fibre pulling rig system that uses the flame brush technique, with an oxygen/hydrogen gas source26. The taper shapes may be custom designed with a Matlab code, based on analysis of the required shape26,45. Tapered fibres which support HOMs have been experimentally realised for the above mentioned 80 μm cladding diameters. Based on recent theoretical work24,45 and using improved experimental methods for fabricating adiabatic HOM tapers, an 80 μm fibre was tapered down to a diameter of 2 μm with two consecutive taper angles of 0.6 mrad and 1 mrad26. These taper angles were used to reduce loss caused by undesired coupling of the modes to higher order symmetric cladding modes and to avoid having an excessively long taper. During the tapering process, the output transmission was measured and recorded simultaneously by using a photodiode connected to an oscilloscope. By slowly tapering the fibre, typical transmission of 80% of the LP11 mode was obtained at the fibre output. By switching back to the FM mode via SLM modulation, we observed that the microfibre still transmitted 95% of the fundamental mode.

According to the commonly accepted analysis used for determining the power propagating through the waist of a homogeneous tapered fibre, the total power loss of a uniformly tapered fibre originates only from the transition regions of the microfibre which are symmetrically located on either side of the microfibre waist. The total power at the microfibre waist can therefore be estimated as equal to the square root of the product of the input and output powers.

Integrating the optical tweezers with the tapered fibre

To introduce a single particle to the microfibre surface30 and minimise system interference from unwanted particles, an optical tweezers was built. Trapping was done via an inverted 100× microscope objective (NA = 1.25). A thin glass coverslip was positioned at the focal plane of the objective to support the liquid sample and trap particles. A Ti: Sapphire laser source operating at 820 nm was used to provide a stiff trap.

The prepared microfibre was fixed to a mount on a 3D translation stage to allow both vertical and horizontal fibre adjustment over the trapping plane (Fig. 5). A CCD camera and a white light source were used to observe the system via the tweezers objective.

Polystyrene particles with diameters of 1 μm, 2 μm, 3 μm and 5 μm were prepared in deionized water dispersion that prevents particles from sticking on the surface of the fibre causing undesirable power loss. The optical tweezers was used to trap a single particle and convey it to the evanescent field of the microfibre. As soon as the trapped particle is released from the tweezers, the evanescent field of the microfibre propels the particle in the direction of light propagation. By observing these dynamics, the speed of each single particle under both the HOM and FM transmission was investigated (see Supplementary Information).