Throughout biology, cells and organisms use flagella and cilia to propel fluid and achieve motility. The beating of these organelles, and the corresponding ability to sense, respond to and modulate this beat is central to many processes in health and disease. While the mechanics of flagellum–fluid interaction has been the subject of extensive mathematical studies, these models have been restricted to being geometrically linear or weakly nonlinear, despite the high curvatures observed physiologically. We study the effect of geometrical nonlinearity, focusing on the spermatozoon flagellum. For a wide range of physiologically relevant parameters, the nonlinear model predicts that flagellar compression by the internal forces initiates an effective buckling behaviour, leading to a symmetry-breaking bifurcation that causes profound and complicated changes in the waveform and swimming trajectory, as well as the breakdown of the linear theory. The emergent waveform also induces curved swimming in an otherwise symmetric system, with the swimming trajectory being sensitive to head shape—no signalling or asymmetric forces are required. We conclude that nonlinear models are essential in understanding the flagellar waveform in migratory human sperm; these models will also be invaluable in understanding motile flagella and cilia in other systems.
Spermatozoan motility is critical for fertilization and relies on the whip-like beating of a flagellum. This waveform arises through an intricate balance of internally generated shear, flagellar elastic resistance and hydrodynamic viscous drag. Despite complex beat patterns, aspects of the overall swimming trajectories are simply related to properties of flagellar bending. In particular, averaged over a beat cycle, symmetrical flagellar waveforms propel free swimming cells in relatively straight paths (Gray & Hancock 1955; Katz et al. 1989; Smith et al. 2009a,b), while bending asymmetry drives the cell in curved trajectories, as illustrated in figure 1b. Furthermore, when the sperm head is pinned to a surface, beat asymmetry induces cell rotation about the point of attachment (Goldstein 1977). Asymmetric bending has also been observed to be important in the chemotactic response of sperm (Miller & Brokaw 1970; Wolgemuth et al. 2000) and during hyperactivation (Katz et al. 1989; Kinukawa et al. 2003), a motility change that is thought to be required for successful fertilization. However, despite the vital role of symmetry-breaking phenomena for the flagellar waveform, and consequently for sperm transport, the mechanism by which asymmetric beating is generated is yet to be fully understood.
Domain boundaries can also induce asymmetric dynamics (Katz et al. 1989). When sufficiently close to a solid boundary, typically at a distance of less than the sperm body length, numerous swimming behaviours have been observed. Rodent sperm with hook-like heads often swim with a planar flagellar waveform and a trajectory curvature of fixed chirality relative to the sperm head. This is considered to arise from the influence of head geometry on stable surface swimming (Woolley 2003). Similarly, for sperm with more symmetrical heads, non-planar beating can occur with cell rolling during surface swimming, resulting in circular swimming trajectories in the direction of cell rolling, which is always the same within a species (Woolley 2003).
Surfaces do not always appear to dictate the symmetry breaking of sperm cells. This is illustrated in figure 1a, for non-rolling human sperm that have migrated significant distances within a deep chamber (400 µm) filled with a physiological high-viscosity medium. Here, clockwise (yellow) and counterclockwise (cyan) surface swimmers can be observed together with an approximately straight swimming path (white). In this case, no obvious morphological feature dictates the chirality of path curvature. In figure 1b, the manifest asymmetrical bending associated with circular swimming is also illustrated.
These observations readily establish that symmetry breaking and curved trajectories can occur without cell rolling or asymmetric cell morphology and need not be driven by dominant boundary influences. In such cases, it is not clear that an internal asymmetry of the flagellum is dynamically important and driving symmetry breaking, whether it be due to an asymmetric force generation by the dynein molecular motors, as indicated in hyperactivation arising from elevated intracellular calcium (Suarez & Ho 2003), or the subtle heterogeneities of flagellar structure (Fawcett 1975). This is especially the case for species such as humans that can also exhibit highly symmetric waveforms. Thus, our aim is to explore whether physical principles support the null hypothesis that asymmetric waveforms can be generated within flagella with no intrinsic asymmetry and without asymmetric internal forces via a dynamical instability, as observed with passive filament bending in viscous shear flows (Becker & Shelley 2001). In the following study, we therefore summarize relevant features of flagellar mechanics, construct a simple elastohydrodynamical model exploring flagella waveform symmetry breaking for sperm motility within viscous, Newtonian, fluids and, finally, place the findings in the context of sperm motility through numerical simulations and a parameter study.
2. Flagellar mechanics
The elastohydrodynamic formulation, which couples the structural mechanics of the flagellum with the surrounding fluid, has been extensively studied (Machin 1958; Brokaw 1971, 1975; Hines & Blum 1978; Lindemann & Kanous 1995; Camalet et al. 1999; Camalet & Jülicher 2000; Riedel-Kruse et al. 2007; Fu et al. 2008; Hilfinger & Jülicher 2008; Hilfinger et al. 2009), both experimentally and theoretically. In the founding study, Machin (1958) proposed that an internal forcing mechanism was required to maintain the flagellar bending observed in spermatozoa experiments. This hypothesis was later established with the discovery of the axoneme internal structure, revealing that sliding microtubules drive active flagellar bending (Satir 1965). Although Brokaw first considered this microtubule sliding mechanism in modelling flagellar locomotion (Brokaw 1971, 1975), the nonlinear flagellar elastohydrodynamic equations were only derived several years later by Hines & Blum (1978). Later, analogous, models have also been proposed in the literature, exploring both linear (Camalet et al. 1999; Camalet & Jülicher 2000; Riedel-Kruse et al. 2007; Fu et al. 2008) and more recently weakly nonlinear dynamics (Hilfinger et al. 2009).
Despite such progress in modelling the internally driven flagellum, the influence of dynamical nonlinear instabilities on the emergent flagellar beat pattern and the consequences for cell swimming have been largely neglected. Nonetheless, nonlinear instabilities are well established for the biophysical dynamics of slender-body systems, including gliding motility assays of cytoskeletal filaments with flow defects (Bourdieu et al. 1995), torque-induced writhing of a rotating elastica (Wolgemuth et al. 2000) and the behaviour of passive filaments within shear flows (Becker & Shelley 2001). The latter in particular highlights that instabilities can emerge from filament compression, with a sharp transition to buckling followed by complicated shape perturbations. Recent studies of flagellar waveform mechanics have initiated explorations of internally generated shear between the microtubules via a linear formulation (Camalet et al. 1999; Camalet & Jülicher 2000; Riedel-Kruse et al. 2007; Fu et al. 2008), as well as considering the lowest order nonlinear effects on the self-organized bending waves (Hilfinger et al. 2009). These investigations highlight that the emergent axonemal beat patterns are a good approximation to the weakly nonlinear problem (Hilfinger et al. 2009). However, except for a brief, perturbative, study on the role of tension owing to an external force (Camalet & Jülicher 2000), the possibility that nonlinear tension dynamics can induce dynamical symmetry breaking has been widely neglected in active flagellar mechanics. Furthermore, this entails that the range of validity of the linear model is not completely explored.
Thus, in contrast to the vast majority of works on the internally driven filament, we investigate whether flagellar tension can induce symmetry breaking via a buckling mechanism and how it may influence flagellar beating and sperm swimming trajectories. This requires considering geometrical nonlinearities in flagellar models coupling internal shear generation via microtubule sliding, the flagellum elastic response and viscous drag. In addition, we also explore the agreement between the geometric nonlinear theory and the linear approximation. This will allow us to delimit the region of validity of linear theory in parameter space, further bridging the gap between linear and nonlinear regimes. In turn, such studies will be important for the formulation of well-founded models for forced elastohydrodynamic problems in the future.
2.1. Elastohydrodynamic formulation
We consider an internally driven sperm flagellum with a planar waveform, immersed within a viscous fluid. Inertial effects are negligible, because of the very low Reynolds number of sperm swimming, while the hydrodynamic interactions are simplified using resistive-force theory (RFT; Gray & Hancock 1955). This local drag model is the leading order term of the equations of slender-body hydrodynamics (Johnson 1980), and it is simply specified by a local linear relation between the velocity of the flagellum centreline and the force (per unit length) exerted on the fluid, through the anisotropic drag coefficients. Although RFT is only valid for very slender filaments, it is widely used for general elastohydrodynamic problems, including relaxational and forced dynamics of stiff polymers (Machin 1958; Bourdieu et al. 1995; Goldstein & Langer 1995; Goldstein et al. 1998; Wiggins et al. 1998; Wolgemuth et al. 2000; Becker & Shelley 2001; Yu et al. 2006), as well as flagellar dynamics (Machin 1958; Brokaw 1971; Hines & Blum 1978; Johnson & Brokaw 1979; Lindemann & Kanous 1995; Camalet et al. 1999; Camalet & Jülicher 2000; Riedel-Kruse et al. 2007; Fu et al. 2008; Hilfinger & Jülicher 2008; Hilfinger et al. 2009), among others. Theoretical predictions using RFT have previously shown a remarkably good agreement with experimental measurements for actuated filaments (Wiggins et al. 1998; Yu et al. 2006) and the buckling instability exhibited by a single passive filament within a shear flow (Becker & Shelley 2001; Tornberg & Shelley 2004). In addition, microscopy imaging (Riedel-Kruse et al. 2007) has also confirmed that RFT is surprisingly accurate when applied to bull sperm flagellar dynamics, while numerical simulations accounting for non-local hydrodynamic effects support the use of RFT for microswimmers with relatively small cell bodies, including human sperm (Johnson & Brokaw 1979).
Sperm flagellar motion is driven by dynein motor proteins, exerting a relative shearing force between outer adjacent filaments, or microtubules, of the flagellar axoneme: this is referred to as the sliding filament model (Brokaw 1971, 1975; Hines & Blum 1978; Camalet et al. 1999; Camalet & Jülicher 2000; Riedel-Kruse et al. 2007; Fu et al. 2008; Hilfinger & Jülicher 2008; Hilfinger et al. 2009). For planar flagellar waveforms of mammalian sperm, there is a preferred plane of beating imposed by the mammalian flagellar accessory structures (Lindemann et al. 1992). In this context, faithful three-dimensional descriptions of the cylindrical arrangement of microtubule doublets in mammalian sperm have been shown to be equivalent to a simpler two-dimensional representation of the sliding forces within the axoneme, as depicted in figure 2 (Hilfinger & Jülicher 2008; Hilfinger et al. 2009). Here, a pair of parallel elastic filaments may slide relative to each other within the beat plane in response to dynein forces. Each sliding filament is assumed to be homogeneous, inextensible and separated by a constant gap spacing b, which corresponds to the axoneme diameter. At the sperm head junction, we assume for simplicity that no interfilament shear is permitted owing to structural constraints. The axoneme motor proteins induce active shear stresses along the flagellum, which act in opposite directions and force the filaments to locally slide with respect to each other, inducing flagellar bending (figure 2).
2.2. Geometrically nonlinear theory: equation of motion
It is convenient to describe the flagellum position, relative to the laboratory frame of reference, by its neutral line X(s,t) (figure 2), noting that t is time and s denotes the distance along the flagellum with 0 ≤ s ≤ L, where L is the filament length. The local flagellum coordinate system is represented as an orthonormal pair with a positive orientation (ŝ(s,t),n̂(s,t)), where ŝ = Xs ≡ ∂X/∂s is the tangent vector and n̂ is the vector normal to the flagellum centreline (figure 2). The flagellar dynamics is inertialess and simply arises via balancing the viscous drag force per unit length with the internal forces per unit length within the flagellum. Non-dimensionalizing with respect to the length scale L, time scale ω−1 and force density E/L3, for a given beating frequency ω and constant flagellum elastic stiffness E, the dimensionless elastohydrodynamic equation of motion for the flagellum neutral line reads 2.1 Here, the subscript t denotes differentiation with respect to time, f(s,t) is shear force density within the flagellum and γ=ξ⊥/ξ∥ is the ratio between the perpendicular, ξ⊥, and parallel, ξ∥, fluid dynamic resistance coefficients. The sperm-compliance parameter 2.2 is dimensionless and characterizes the relative importance of elastic forces to viscous drag (Wiggins et al. 1998). The tensile force T(s,t) is related to the Lagrange multiplier for inextensibility, and it is implicitly determined by the constraint Xs · Xs = 1. Under appropriate variable transformations, these equations are equivalent to earlier models proposed by Hines & Blum (1978), Gueron & Liron (1993) and Camalet & Jülicher (2000). A detailed derivation is presented in the electronic supplementary material as well as the explicit form of the inextensibility constraint.
Although the sliding filament mechanism has been successful in explaining flagellar bending, there is a limited quantitative understanding of the regulation and nature of the internal shear stress f, which represents the coupling between the dynein molecular motor activity and the passive cross-linking proteins within the flagellum (Brokaw 2009; Mitchison & Mitchison 2010). There have been several attempts to explain the observed flagellar beat via different shear-control hypotheses dictating the regulation of internal shear f (Brokaw 1971, 1975, 2009; Hines & Blum 1978; Lindemann & Kanous 1995; Camalet et al. 1999; Camalet & Jülicher 2000; Mitchison & Mitchison 2010), although comparison with experiments has only become possible recently (Riedel-Kruse et al. 2007). Here, it is beyond the scope of the study to consider detailed assessments of the internal shear regulation and the difficulties associated with dynein control mechanisms. Instead, we use a symmetric model, based on observations of shear in situ, to explore the symmetry-breaking event. As detailed in the electronic supplementary material, travelling waves of bending (Smith et al. 2009b), and thus internal shear forces, periodically propagate down the flagellum; given that the dominant mode typically dictates the dynamics (Riedel-Kruse et al. 2007), we therefore model the internal shear density as a simple travelling wave 2.3 with dimensionless force amplitude A and wavenumber k. This particular choice of internal shear will not just isolate the potential for symmetry breaking of a symmetrically driven flagellum, it will also enable us to investigate a wide range of shear distribution k, bringing to light new nonlinear effects within a general framework.
2.3. Boundary conditions
The equations governing the flagellar dynamics are closed by defining the initial cell configuration together with the boundary conditions, in which either the movement of the flagellar endpoints is specified or a balance of forces and torques at each end is imposed. In particular, at the distal boundary, s = L, the flagellum is free to move and, therefore, the external torques and forces are zero, i.e.
At the proximal end of the flagellum, s = 0, we consider three distinct boundary conditions motivated by laboratory examples:
— The clamped head. The sperm head is strongly adhered, with no rotation about its point of attachment, so that both its position and tangent vectors are fixed: Xt|s=0 = Xst|s=0 = 0.
— The pivoting head. The sperm head is adhered so that it does not move except for rotation about its attachment, due to the absence of an external moment: Xt|s=0 = Mext|s=0 = 0.
— The swimming sperm. The cell body experiences a hydrodynamic viscous drag force, Fhead, and moment, Mhead, which are balanced by the contact force and torque between the sperm head and the flagellum at their junction. This balance yields the required boundary condition for the flagellum in terms of the motion of the sperm head via a specification of Xt|s=0 and Xst|s=0.
The full nonlinear numerical scheme, using methods similar to (Tornberg & Shelley 2004), validation and derivation of the boundary equations are summarized in the electronic supplementary material.
2.4. Parallels with the linear theory
For small deflections, Camalet & Jülicher (2000) have shown that the equation of motion (equation (2.1)) simplifies to 2.4 where x ≈ s and X(s,t) ≈ sx̂ + h(s,t)ŷ. The tensile forces only contribute at subleading orders, and hence T(s,t) ≈ 0. In the absence of internal shear, equations (2.1) and (2.4) describe the elastohydrodynamics of a passive filament in a viscous fluid and have already been studied analytically (Machin 1958; Bourdieu et al. 1995; Goldstein & Langer 1995; Goldstein et al. 1998; Wiggins et al. 1998; Wolgemuth et al. 2000; Fu et al. 2008) and experimentally (Bourdieu et al. 1995; Wiggins et al. 1998; Yu et al. 2006). Despite the relative simplicity of the linearized formulation equation (2.4), there has not been a study of its accuracy compared with the full nonlinear framework equation (2.1) given the variation of parameters such as the shear force wavenumber k, shear force amplitude A and the sperm compliance Sp. This was circumvented in Fu et al. (2008) by choosing the sliding force amplitude A, for a given Sp and k, so that the maximum deflection of the filament was no larger than 10 per cent of the total filament length L. More recently, Jülicher and collaborators (Hilfinger et al. 2009) have considered the role of leading nonlinear contributions in a perturbative formulation and demonstrated that the linear theory provided a good estimate, with no evidence of a buckling instability.
Numerical simulations were carried out assuming a fluid dynamic resistance ratio γ = 2. Once the boundary conditions are specified, there are two further degrees of freedom: the sperm-compliance parameter Sp and the wavenumber k. Given these, the force amplitude A is fixed by the constraint that the maximum flagellar displacement does not exceed 10 per cent of the flagellar length in the linear theory, that is, maxxt|h| = 0.1 in equation (2.4), as in Fu et al. (2008). The force amplitude A is plotted for the clamped and pivoting boundary conditions in electronic supplementary material, figure S1, and the parameter regimes considered are consistent with typical physical quantities observed in spermatozoa experiments (Baltz et al. 1990; Lindemann et al. 2005; Smith et al. 2009b). As detailed in the electronic supplementary material, estimates for the human sperm-compliance parameter for various media range from Sp = 4 to Sp = 24, which dictates the choice of Sp in the illustrative examples below. We also display results for smaller Sp, as low as unity, for completeness, when assessing the validity of the linear theory as other flagellates can operate at smaller compliance numbers, as briefly discussed in the electronic supplementary material.
3.1. Clamped head and pivoting head results
We begin our investigation by contrasting the nonlinear flagellar dynamics equation (2.1) with its linear approximation equation (2.4), with illustrations of the symmetry-breaking behaviour, for the clamped and pivoting head boundary conditions. Figure 3a–l shows the time evolution of the linear and nonlinear flagellar shapes for both clamped and pivoting boundary conditions, and six different pairs of wavenumber and sperm compliance parameter (k, Sp). Figure 3m–x additionally illustrates the time evolution of the nonlinear model predictions for the flagellar beat pattern when symmetry breaking occurs for a range of internal shear wavenumbers, k, and sperm compliance Sp = 19 for the clamped head plus sperm compliance Sp = 15 for the pivoting head.
The linear theory provides a good agreement with the full nonlinear problem for cases a, b, g, h and d, e, j, k in figure 3. In contrast, the linear approximation fails for cases c, i, f, l in figure 3 for both the pivoting and clamped boundary conditions, where the nonlinear solutions are characterized by condensed or highly asymmetric waveforms, breaking up–down symmetry in the plane. This is despite the constraint on the maximum flagellum amplitude, as illustrated for k = 5π and Sp = 12 in figure 3f. The symmetry-breaking behaviour within the nonlinear model is further highlighted in figure 3m–x. In particular, at large values of the sperm-compliance parameter, Sp, corresponding to increasing viscous domination of the dynamics, the symmetry-breaking behaviour is particularly enhanced. For clamped head boundary conditions, the emergent asymmetrical waveforms are relatively constrained as the tangent vector is also pinned at s = 0, whereas asymmetrical bending causes the flagellum to rotate about the point of attachment for the pivoting head boundary condition. We also observe that all flagellar patterns are eventually periodic in time, once transients have decayed, despite the complexity in the dynamics, though the period is greatly increased once symmetry breaking has occurred.
To delimit the values of the internal shear force wavenumber, k, and sperm compliance parameter, Sp, simulations were performed for 0 ≤ k ≤ 10π, 1 ≤ Sp ≤ 20. A measure of the discrepancy between the linear theory predictions for the flagellar waveform, XL(s,t), and the nonlinear theory predictions, XN(s,t), is given by
When Dmax = 0, the agreement is perfect, while if Dmax ≈ 0.1 or less, the agreement is observed to be qualitatively reasonable. For example in figure 3e,c, Dmax = 0.08 and 0.11, respectively, whereas in figure 3i, Dmax = 0.47.
In figure 4a,b, Dmax is plotted as an interpolated function of Sp and k, with the black contour given by Dmax = 0.1. The linear theory is increasingly inaccurate as the sperm compliance parameter, Sp, increases even for moderate internal shear force wavenumbers, k, especially for the pivoting head boundary conditions. In figure 4c,d, the linear theory prediction for the global maximum curvature, κmax, is plotted as the sperm compliance Sp and wavenumber k are varied, with the contour Dmax = 0.1 once more given by a solid black curve. Clearly, there is a strong positive correlation between the maximum curvature obtained from the linear model and the discrepancy measure, Dmax, for both boundary conditions, explicitly highlighting that the linear theory becomes inaccurate as its predictions for flagellar curvature increase. In particular, once the radius of curvature is less than, approximately, 10 per cent of the flagellar length (κmax = 10), the linear theory is observed to be unreliable.
One should note that figure 4b,d exhibits a blank region in the upper left corner. The high flagellar compliance, slowly varying internal shear distribution and flagella hinging characterizing this region of parameter space allow a local build-up of high curvature and tension, with sudden changes in the force direction. Discretizing the nonlinear equations produces matrices that are too ill-conditioned for reliable simulation. This region of parameter space will not be considered further.
The symmetry-breaking transient dynamics is illustrated in figure 4e,f, where we, respectively, display the flagellar pattern and absolute tension as the buckling instability progresses for the pivoting head boundary conditions with k = 6π and Sp = 15 (figure 3q). During this instability, a common feature is a large absolute tension concentrated towards the sperm cell–flagellum junction at s = 0, noting that the tension is zero at the distal flagellum, s = L. After reaching a critical value of absolute tension, the beating shape instability is followed by a sudden drop in the absolute tension together with an increase in the period (figure 4f). Also, it is noteworthy that the quantity Dmax, displayed in figure 4a,b, or κmax, plotted in figure 4c,d, can be used as a bifurcation diagram to identify the parameter regimes where the buckling-type instability occurs, since inaccuracies of the linear theory are always observed to be accompanied by this dynamic symmetry-breaking behaviour.
3.2. Swimming sperm
We examine the influence of the flagellar buckling instability on swimming sperm. We have considered the effect of two different head morphologies: a ‘human-like’ sperm head (Smith et al. 2009a) with dimensions 4.5 × 2.8 × 1.12 µm and a spherical head with diameter 2.40 µm so that it has the same volume. The swimming sperm was found to be less sensitive to the flagellar buckling instability, although once both the sperm compliance, Sp, and the internal shear wavenumber, k, are large, sperm swimming is observed to be profoundly altered by the symmetry-breaking mechanism. The transition in behaviour is, however, smooth and drives the sperm towards swimming in circular paths of constant radius. Furthermore, a small (large) sperm head viscous drag leads to larger (smaller) circular paths. The sperm trajectories for both human-like (dashed red) and spherical head (dashed blue), when k = 10π and Sp = 20, are illustrated in figure 4g. In addition, the swimming direction in figure 4g changes from clockwise to counterclockwise if f → −f in equation (2.1), illustrating that overall path direction after buckling is sensitive to the phase of the internal shear forcing.
Although the dynamics of an internally driven filament in viscous fluids has been widely studied, the possible influence of a nonlinear buckling instability on the ultimate flagellar patterns has not been explored. Here, we consider the physical principles of this instability in the context of flagellar dynamics, incorporating the influence of the surrounding fluid through RFT. The structural response of the flagellum is governed by geometrically nonlinear filament elasticity theory and the internal forcing is represented via the sliding filament model of eukaryotic flagellar motility. The coupling of these three physical phenomena leads to the emergence of complex flagellar waveforms, which were examined in detail through numerical simulations for a large spectrum of internal shear wavenumber, k, sperm compliance, Sp, and different boundary conditions.
While weakly nonlinear analyses (Hilfinger et al. 2009; Mitchison & Mitchison 2010) support the use of geometrically linear elasticity theory in recent models of flagellar dynamics (Camalet et al. 1999; Camalet & Jülicher 2000; Riedel-Kruse et al. 2007; Fu et al. 2008), we have demonstrated that the linear theory can be unreliable in general. On varying the internal shear wavenumber k and the sperm compliance, Sp, the linear theory yields inaccurate predictions for reasonably large values of Sp and a wide range of wavenumbers k (figure 4a,b). While the linear model demonstrates a plausible behaviour in this parameter regime (Fu et al. 2008), the nonlinear simulation exposes the higher order effects and exhibits complex flagellar beating (figure 3). Physically, it is reasonable to expect an increasing inaccuracy of the linear model for larger values of k and Sp, even with constraints on flagellar waveform amplitude. In particular, higher wavenumbers continuously force the flagellum to increase its curvature locally. With higher sperm compliance parameters Sp (equation (2.2)), and thus a sufficient viscous resistance to prevent the tendency of elastic forces to reduce this curvature, high tangential forces are induced, which are nominally a second-order contribution (Camalet & Jülicher 2000; Hilfinger et al. 2009). Hence, the validity of the linear theory requires a larger flagellum radius of curvature, observed to be at least 10 per cent of flagellum length, rather than constraints on the amplitude of flagellar deflection (Fu et al. 2008).
Our main result from this nonlinear investigation is that asymmetric flagellar waveforms may arise dynamically from intrinsically symmetric flagellar dynamics; this is not captured by linear or weakly nonlinear theories. Consequently, an asymmetric flagellar waveform can be initiated and maintained without any change in cell signalling or the presence of flagellar heterogeneity. The asymmetric flagellar bending is caused by a common phenomenon in elastic filament dynamics, the buckling instability (Becker & Shelley 2001), which is frequently found in passive filaments when subjected to high tangential forces. This mechanism is also manifested in driven flagellar dynamics (figure 3), though, conversely, it is triggered by the internal shear force via the fn̂s contribution in equation (2.1). This causes the absolute tension to rise; once beyond a critical value that the flagellum elastic structure cannot support, asymmetric bending is observed (figure 4e,f). Furthermore, the flagellum is still driven by the same internal shear after buckling, which continuously forces the flagellum to maintain the emerging asymmetric bending pattern: roughly an ‘S’ shape for a fixed head and a ‘C’ shape for both the pivoting head case and the swimming sperm (figures 3 and 4g). This represents a markedly distinct buckling instability from those reported in the literature (Bourdieu et al. 1995; Becker & Shelley 2001; Tornberg & Shelley 2004).
This flagellar buckling instability is readily found for large values of the internal shear wavenumber k and the sperm compliance parameter Sp; it is also apparent for moderate wavenumbers, in particular, for constrained sperm especially when the sperm head is pivoting. While the clamped boundary condition restrains the motion, the free torque condition in the pivoting head simulations allows the sperm to rotate around its fixed point; analogously, the free head swimmer boundary conditions induce waveform asymmetries that drive circular trajectories. Furthermore, the swimming sperm trajectories are sensitive to sperm head morphology. Morphologies may subtlety alter the net viscous drag on the swimming flagellum, in turn altering the tension via the boundary conditions. However, in the context of the emergent behaviour from a tension-driven buckling instability, this can have a substantial effect on the emergent waveform, and hence the resulting swimming trajectory (figure 4g). Furthermore, the swimming direction is a non-trivial consequence of the force and torque balance during the bifurcation to asymmetric waveforms and, in particular, exhibits a dependence on the phase of the internal sliding forces.
These results demonstrate that asymmetric flagellar beating does not necessarily require an intrinsic asymmetric forcing mechanism. Thus, observations of circular swimming or flagellar waveform asymmetry are not sufficient to infer the presence of hyperactivation or any other asymmetric physiological regulation or signalling influencing the internal dynein molecular motors within the flagellum. Similarly, one cannot immediately infer that subtle flagellar structural asymmetries, such as the 5–6 microtubule bridging (Satir 1965; Olson & Linck 1977), are dynamically critical and driving symmetry breaking. Moreover, high wavenumbers are commonly exhibited by sperm migrating in high viscosity fluids (Smith et al. 2009b) and circling cells (figure 1). The results we have presented indicate that it is physically plausible for this behaviour to be caused by excessive tangential forces on the flagellum owing to both internal shear forces and the viscous drag on the sperm cell. Nonetheless, the influences of ultrastructural, histological and physiological complications are currently unexplored. For example, we have not considered the role of tapering in the accessory flagellar structures commonly found in mammalian sperm cells, such as the outer dense fibres. These accessory structures reinforce the flagellum in regions where high tensions are expected, and may also act to prevent the flagellar buckling instability; likewise, subtle structural asymmetries of the sperm flagellum could encourage buckling. Similarly, possible dynein detachment mechanisms at high flagellar curvature, such as the geometric clutch hypothesis (Lindemann & Kanous 1995), may influence the emergent waveform and require exploration. Further work could also account for non-local hydrodynamic effects.
In summary, our formulation is the first to explore the buckling instability of a filament driven by internal shear forces within viscous fluids. It has firstly delimited the validity of geometrically linear elastic filament theory. Secondly, the study has demonstrated the physical plausibility of dynamical symmetry breaking of filaments. Our demonstration that the asymmetric waveforms (figure 1 and electronic supplementary material, movie S1) that characterize specialized sperm behaviours, such as hyperactivation or chemotaxis, can also emerge dynamically without recourse to variations in structure or signalling (figures 3 and 4g), emphasizes the importance of being alert to this symmetry-breaking mechanism when interpreting observations of sperm flagella. These findings are crucial when considering motility at these scales in physiological fluids and their analogues, because of the fact that increased viscosity induces a higher sperm compliance number, as defined in equation (2.2). Furthermore, mathematical models exploring the oscillatory behaviour of cilia and flagella beating should also consider geometrically nonlinear dynamics to accommodate the high curvatures observed physiologically. We hope these findings will stimulate future mathematical research, which considers the role for geometrically nonlinear dynamics and buckling instabilities in other systems exhibiting flagellar motility, such as protozoa, algae and artificial microswimmers.
The authors thank Mr Henry Shum for many helpful discussions and Professor John R. Blake for continued insight. H.G. acknowledges the Capes Foundation (Brazilian sponsor) for financial support through grant no. BEX 4676/06-8, and also through the Hester Cordelia Parsons Fund and Timothy Bailey Trust. D.J.S. thanks the Medical Research Council through grant no. G0600178. This publication is based on work supported in part by Award no. KUK-C1-013-04, made by King Abdullah University of Science and Technology (KAUST).
- Received March 5, 2010.
- Accepted April 23, 2010.
- © 2010 The Royal Society