Hostname: page-component-7dd5485656-2pp2p Total loading time: 0 Render date: 2025-10-22T13:07:13.691Z Has data issue: false hasContentIssue false

Aquatic locomotion due to a flexible foil flapping in a perfect fluid

Published online by Cambridge University Press:  20 October 2025

Giorgio Graziani*
Affiliation:
Department of Mechanical and Aerospace Engineering, Sapienza Università di Roma, Via Eudossiana, 18, 00184 Roma, Italy
Damiano Paniccia
Affiliation:
Department of Mechanical and Aerospace Engineering, Sapienza Università di Roma, Via Eudossiana, 18, 00184 Roma, Italy Leonardo S. p. A., Piazza Monte Grappa 4, Roma 00195, Italy
Renzo Piva
Affiliation:
Department of Mechanical and Aerospace Engineering, Sapienza Università di Roma, Via Eudossiana, 18, 00184 Roma, Italy
*
Corresponding author: Giorgio Graziani, g.graziani@uniroma1.it

Abstract

Can a fish-like body swim in a perfect fluid – one that is purely inviscid and does not release vorticity? This question was raised by Saffman over fifty years ago, and he provided a positive answer by demonstrating a possible solution for an inhomogeneous body. In this paper, we seek to determine a suitable deformation for oscillatory fish swimming that enables slight locomotion in a perfect fluid, relying solely on tail flapping motion. This swimming style, typical of carangiform and thunniform species, allows for a separate analysis of the tail’s interaction with the surrounding fluid. As a preliminary approach, the tail is approximated as a rigid plate with prescribed heave and pitch motions, while the presence of a virtual body placed in front is considered to evaluate the locomotion. Analytical solutions provide exact results while avoiding singular behaviour at sharp edges. A phase shift is shown to be strictly necessary for generating locomotion. A more refined approximation of a real fish is achieved by modelling the tail as a flexible foil, connected to the main body via a torsional spring with tuneable stiffness at the peduncle. While the heave motion remains prescribed, the pitch amplitude and phase are passively determined by flow interaction. A plausible solution reveals an optimal stride length as a function of dimensionless stiffness, driven by resonance phenomena. A small structural damping must be considered to induce a phase shift – essential for self-propulsion in the absence of vorticity release.

Information

Type
JFM Papers
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2025. Published by Cambridge University Press

1. Introduction

In the present paper we focus on fish-like bodies that achieve self-propulsion by flapping their tails. The rest of the body, containing the larger part of the total mass, essentially contributes to the stability of locomotion, by keeping control of the recoil motions, while it gives rise to the major part of the resistance, which in the present study is not considered. This behaviour, characteristic of carangiform or thunniform fish, is well known in the literature as oscillatory swimming in contrast to undulatory swimming which involves the deformation of a larger portion of the body to generate propulsion.

Due to its nature, the oscillatory swimming allows us to analyse separately the fish tail as the main propulsive tool, whose interaction with the surrounding fluid was frequently studied by considering its motion under an incoming uniform stream, especially in the field of experimental investigation. In case a direct analysis of self-propulsion is believed more appropriate, simplified theoretical models are easily devised to obtain significant results in a neat form, either by analytical or by numerical methods.

For instance, in the following, we consider the motion of a virtual body (Akoz & Moored Reference Akoz and Moored2018, Moored & Quinn Reference Moored and Quinn2019, Paniccia et al. Reference Paniccia, Padovani, Graziani and Piva2021c ) with prescribed integral properties, at the end of which the flapping tail is attached, with its proper heave and pitch motion, see figure 1. More details are reported in the Supplementary Materials in Paniccia et al. (Reference Paniccia, Padovani, Graziani and Piva2021c ). Within this kind of approximation, we may study the interaction with the surrounding fluid of the isolated tail, by recovering the presence of the main body only in terms of its inertial effects on locomotion, as lateral and angular recoil motions are supposed to be prevented by the prevailing size of the main body itself. In general, self-propulsion occurs when the thrust generated by the flapping tail balances the prescribed drag of the main body (Smits Reference Smits2019) while in the present study both drag and thrust are null, as expected in perfect fluid.

Figure 1. Sketch of the virtual body with the flat plate attached through a torsional spring. The ground frame ( $X\!-\!Y$ ) and the body-fixed one ( $x\!-\!y$ ) are shown.

In previous studies (Paniccia et al. Reference Paniccia, Graziani, Lugni and Piva2021a , Reference Paniccia, Graziani, Lugni and Piva2021b ) we adopted this model to analyse the axial motion of fish body propelled by a flapping tail in the framework of inviscid flows in the presence of non-diffusing vorticity. As a plus, potential theory is able to identify clearly the added mass responsible for the reactive forces, as discussed in Lighthill (Reference Lighthill1960, Reference Lighthill1969) and Wu (Reference Wu1961). Furthermore, the application of an unsteady Kutta condition mimicking the effect of viscosity at the trailing edge singularity implies the release of concentrated vorticity as the main mechanism for the exchange of momentum with the fluid. Particular attention was given to the different roles played by the added mass and by the vortical terms of the governing equations, but also to their couplings which have a positive influence not only on the locomotion, but also on the manoeuvrability of the fish body. See Limacher (Reference Limacher2019) and our previous contribution on the C-start maneuver, i.e., the rapid escape motion with a C-shape bending of the swimmer (Paniccia et al. Reference Paniccia, Graziani, Lugni and Piva2022).

The effort to extend this procedure to include flexible tails, resembling the thin tails of real fish (Quinn & Lauder Reference Quinn and Lauder2022), led to the further modelling proposed by Moore (Reference Moore2014, Reference Moore2015), which considers the flexibility to be fully concentrated at the leading edge by a local torsional spring with a proper stiffness, while the rest of the tail is treated as a rigid body.

The reactive forces, expressed in terms of potential flow and added-mass coefficients, have a primary role in the transfer of energy from the flexible tail to the surrounding fluid through a torsional balance equation. In general, this energy, ultimately captured by vortex shedding, plays a crucial role in generating the backward fluid momentum required for the body’s locomotion in the opposite direction.

For a better comprehension of the added-mass effects, we like to consider here, as a starting point, swimming in a pure inviscid fluid able to exchange only reactive forces without any release of vorticity, that we identify as a perfect fluid following Saffman (Reference Saffman1967). This problem has been studied by several authors, among others Childress (Reference Childress1981), Kelly (Reference Kelly1998), Kelly & Murray (Reference Kelly and Murray2000) and Kanso et al. (Reference Kanso, Marsden, Rowley and Melli-Huber2005). A similar problem was also studied by Miloh & Galper (Reference Miloh and Galper1993) and by Chambrion & Munnier (Reference Chambrion and Munnier2011) within the framework of geometric mechanics.

The aim of the present study, about swimming in a perfect fluid, is twofold. First, by considering only the reactive forces we can precisely evaluate the added-mass terms in the solution, either for flexible or rigid tails, which should be extended afterwards to include the release of vorticity. Hence, we intend to consider the perfect fluid solution as a valuable step to obtain a reliable extension of the model to include circulatory contributions. Second, the present ideal solutions are of fundamental interest per se, as they address the question posed by Saffman (Reference Saffman1967) regarding whether a fish-like body, initially at rest in an unbounded fluid, can achieve locomotion solely by undergoing periodic shape changes. The solution shown in the present paper can be quite significant for the case of homogeneous bodies. The hypothetical application for swimming in superfluids is just corroborating the above interest.

More specifically, in this paper, we apply the model to study the locomotion of a flat plate undergoing prescribed heaving motion and free to pitch about its leading edge. A torsional spring at the leading edge mimics the flexibility of the plate, influencing in an analogous way the overall performance (see Eldredge, Toomey & Medina Reference Eldredge, Toomey and Medina2010; Wan, Dong & Huang Reference Wan, Dong and Huang2012; Moore Reference Moore2015).

The displacement due to a full cycle of shape variation, giving rise to the body locomotion, is here obtained by the classical theoretical models frequently adopted in fluid mechanics. The same result may be seen as a geometric phase in the framework of geometric mechanics. This approach has been used to study body locomotion either for Stokes flow or for the pure potential flow of interest in the present paper. In fact, for both very low or very high values of the Reynolds number, although the physical reasons are completely different, the resulting linear equations allow us to exploit the methodology in a quite similar way to explain the locomotion in a fluid–body system with null external forces. Purcell (Reference Purcell1977), in his seminal paper, after discussing the scallop theorem, proposed a three-link body, with two prescribed degrees of freedom, to allow for self-propulsion in the absence of external forces. Many authors followed the same track, mostly for application to Stokes flow (e.g. see Childress & Dudley Reference Childress and Dudley2004), but also for application to pure potential flow in a perfect fluid (e.g. Radford Reference Radford1998, Mason Reference Mason2003; Melli, Rowley & Rufat Reference Melli, Rowley and Rufat2006; Ross Reference Ross2006). Some works considered a comparative treatment of both cases (e.g. Hatton & Choset Reference Hatton and Choset2010).

In the following we will keep on with our methodology, although accounting for several of the above applications, to have a better insight and useful suggestions for a deeper physical interpretation of the results. Initially, a fully prescribed heave and pitch motion is analysed just to confirm that a small body displacement can occur even if the mean force is zero, provided an appropriate phase shift exists between the two motions. Afterwards, we focus on the main purpose of the present work, i.e., the passive behaviour of a flexible tail in pure potential flow, which, in our opinion, has not yet received sufficient attention in either classical fluid dynamics or geometric mechanics. In the passive case the pitch motion, in terms of amplitude and phase, is not prescribed but rather is obtained by solving a torsional balance equation. This approach is shown to lead naturally to a proper phase shift once the optimal values of the ruling parameters, driven by resonance phenomena, are matched.

The paper is organised as follows: in § 2 we report the force balance for an isolated fluid–body system in an acyclic flow. We state the equations in terms of the fluid dynamic impulse and consider a two-dimensional plate to obtain the classical representation in terms of the added mass (see Batchelor Reference Batchelor1991; Newman Reference Newman2017). Once the harmonic expressions are defined to prescribe both heave and pitch motions of the tail, a first solution is obtained in § 3 to confirm that locomotion is possible in a perfect fluid even in the absence of mean forces. Section 4 is devoted to the study of the passive pitching motion: the expression of the torque balance equation and of the related fluid dynamic moment are used to derive the analytical solution in terms of pitch angle and phase; afterwards, the locomotion of the passive flapping plate is discussed together with the fundamental role of resonance. Finally some concluding remarks are presented.

2. Impulse equation and self-propulsion

Here, we adopt the approach used in our previous works, where more details are reported (see e.g. Paniccia et al. Reference Paniccia, Graziani, Lugni and Piva2021a , Reference Paniccia, Graziani, Lugni and Piva2021b ), following the formulation presented in Kanso (Reference Kanso2009). Considering the fluid–body system with $V_f$ and $V_b$ the fluid and body volumes, respectively, as an isolated system with no external forces acting upon it, and denoting $\boldsymbol{F}_b$ as the force acting on the body and $\boldsymbol{F}_{\!f}$ as the force acting on the fluid, the following relation can be established:

(2.1) \begin{equation} \;\;\;\, \boldsymbol{F}_b + \boldsymbol{F}_{\!f} = 0, \end{equation}

which expresses the total momentum conservation in integral form

(2.2) \begin{equation} \frac{d}{{\rm d}t} \left ( \int _{V_b} \rho _b \, \boldsymbol{U}_b\, {\rm d}V + \int _{V_f} \rho \, \boldsymbol{U}{\rm d}V \right ) = 0, \end{equation}

where $\boldsymbol{U}_b, \rho _b$ are the velocity and density at any point in the homogeneous body while $\boldsymbol{U}, \rho$ refer to the same quantities in the surrounding fluid. By introducing the velocity of the body’s centroid, $\boldsymbol{U}_\textit{cm}$ , the first integral in (2.2) gives

(2.3) \begin{equation} \frac{d}{{\rm d}t} \int _{V_b} \rho _b \, \boldsymbol{U}_b\, {\rm d}V = \boldsymbol{F}_b = m_b\, \frac {{\rm d} \boldsymbol{U}_\textit{cm} }{{\rm d}t}, \end{equation}

where $m_b$ is the total mass of the body. The second integral in (2.2) represents the time variation of the fluid’s momentum and can be rewritten in terms of the hydrodynamic impulse $\boldsymbol{P}$

(2.4) \begin{equation} \frac{d}{{\rm d}t} \int _{V_f} \rho \, \boldsymbol{U}\, {\rm d}V = \boldsymbol{F}_{\!f} = \rho \, \frac {{\rm d} \boldsymbol{P}}{{\rm d}t}. \end{equation}

In a pure potential flow, the impulse $\boldsymbol{P}$ is confined to its irrotational (acyclic) component, while vorticity-related contributions are not considered. By assuming the normal outward from the body, it is defined in terms of the velocity potential $\phi$ as

(2.5) \begin{equation} \boldsymbol{P} = \boldsymbol{P}_\phi = - \int _{S_b} \phi \boldsymbol{n}{\rm d}S. \end{equation}

Equation (2.4) can be written as

(2.6) \begin{equation} \boldsymbol{F}_{\!f} = - \rho \frac{d}{{\rm d}t} \int _{S_b} \phi\boldsymbol{n}{\rm d}S, \end{equation}

which aligns with the formulation by Saffman (Reference Saffman1992). To analyse the motion of the body, we directly employ the impulse equation by combining (2.3) and (2.4) and by eliminating the time derivative (for a null initial condition), as also discussed in Kanso (Reference Kanso2009) and Paniccia et al. (Reference Paniccia, Graziani, Lugni and Piva2021a )

(2.7) \begin{equation} m_b\, \boldsymbol{U}_\textit{cm} = - \rho \boldsymbol{P}. \end{equation}

Now we split the impulse $\boldsymbol{P}$ into a part, $\boldsymbol{P}_{LOC}$ , due to the body locomotion and a part, $\boldsymbol{P}_\textit{SH}$ , due to the body shape deformation. The former can be expressed through the added-mass matrix $\boldsymbol{M}$ (see also Appendix A) yielding

(2.8) \begin{align} \rho \boldsymbol{P}_\textit{LOC} = \boldsymbol{M}\boldsymbol{U}_\textit{cm}, \end{align}

and (2.7) becomes

(2.9) \begin{equation} (m_b + \boldsymbol{M})\, \boldsymbol{U}_\textit{cm} = - \rho \boldsymbol{P}_\textit{SH}, \end{equation}

which shows that, upon enforcing a periodic shape deformation given by a non-reciprocal motion of the body (as defined in Purcell Reference Purcell1977), we may have locomotion in the absence of mean forces or accelerations.

As previously anticipated, to analyse the self-propulsion of a fish, we model the tail as a heaving and pitching plate attached to a virtual body that contains all the mass of the system while it does not experience either applied forces or moments. This implies that: (i) the virtual body does not contribute to the impulse $\boldsymbol{P}$ in (2.7); (ii) the only source of propulsion is the oscillating tail; and (iii) the centre of mass of the system is assumed to move solely with velocity $U_X$ in the ground reference frame, as a result of the tail’s oscillations. To this aim the tail undergoes prescribed heave oscillations in the $Y$ -direction and pitch oscillations with angular velocity $\varOmega (t) \boldsymbol{e}_3$ (positive counterclockwise) around the centre of rotation located at its leading edge (hereinafter denoted as LE or $\boldsymbol{x}_o$ ). As a result we will obtain the locomotion of the whole system.

The impulses $\boldsymbol{P} =\{{P}_X,{P}_Y\}$ appearing in (2.7) are evaluated in the ground frame. In the following, we will see that it is more convenient to use the components in the body-fixed frame $\{{P}_x,{P}_y\}$ , expressed by using the rotation matrix which maps the ground to the body frame, following the approach presented in Eldredge (Reference Eldredge2019) and Limacher (Reference Limacher2021)

(2.10) \begin{equation} R(\theta ) = \quad \begin{bmatrix} \cos \theta & \sin \theta \\ -\sin \theta & \cos \theta \end{bmatrix}, \end{equation}

the angle $\theta$ being assumed positive anti-clockwise. It follows that

(2.11) \begin{equation} \begin{bmatrix} P_x \\ P_y \end{bmatrix} = R(\theta ) \begin{bmatrix} P_X \\ P_Y \end{bmatrix} = \begin{bmatrix} P_X\,\cos \theta + P_Y\,\sin \theta \\ -P_X\,\sin \theta + P_Y\,\cos \theta \end{bmatrix}. \end{equation}

By using the rotation matrix, (2.7) becomes, in the body frame,

(2.12) \begin{equation} \left \{ \begin{array}{l} m_b\,u_x = - \rho \,P_x ,\\ m_b\,u_y = - \rho \,P_y, \end{array} \right . \end{equation}

where the body mass $m_b$ is estimated as reported in Appendix B.

Let us consider a flat plate whose half-length is $b=c/2$ undergoing imposed harmonic heave and pitch motions $(\dot h\boldsymbol{e}_2; \dot \theta \,\boldsymbol{e}_3 = \varOmega\boldsymbol{e}_3)$ , while its rotation centre moves with locomotion velocity ( $u_x, u_y$ ) expressed in the body frame. The outgoing normal to the upper face is $\boldsymbol{n} = \{-\sin \theta ; \cos \theta \} \simeq \{- \theta ; 1\}$ . The velocity normal to the plate is

(2.13) \begin{equation} U_2 = u_y + \dot h \,\cos \theta \simeq u_y + \dot h. \end{equation}

The relevant details to obtain the expression of the impulses in (2.12) are reported in Appendix A. By using (2.13), the impulse $P_y$ expressed according to (A11) becomes

(2.14) \begin{equation} P_y = \pi \,b^2 \left [ u_y + \dot h + b \dot \theta \right ]. \end{equation}

By combining both the first (2.12) and (A11), we obtain $u_x=0$ . Finally, from the second equation in (2.12) and (2.14), the solution $u_y$ may be obtained

(2.15) \begin{equation} u_y = \frac {- \pi \,\rho \,b^2}{m_b + \pi \,\rho \,b^2} \left [ \dot h + b \dot \theta \right ]. \end{equation}

The self-propulsion speed of the whole body is evaluated in the ground frame through the velocity $\boldsymbol{U}_\textit{cm} = \{U_X , U_Y \}$ which is expressed as

(2.16) \begin{equation} \begin{bmatrix} U_X \\ U_Y \end{bmatrix} = R(\theta ) ^T \begin{bmatrix} u_x \\ u_y \end{bmatrix} = \begin{bmatrix} \,\,\, \cos \theta \,u_x - \sin \theta \,u_y \\ \sin \theta \,u_x + \cos \theta \,u_y \end{bmatrix}. \end{equation}

The locomotion velocity in the body frame is given by $u_x=0$ and $u_y$ by (2.15), so (2.16) gives

(2.17) \begin{equation} \begin{array}{l} U_X= \;\;\, \dfrac {\pi \rho b^2}{\left(m_b + \pi \rho b^2\right)} \left[ \dot \theta \, b + \dot h \right] \sin \theta \end{array}, \end{equation}

while the $U_Y$ component is neglected since we have assumed previously that the presence of the virtual body prevents its motion in the $Y$ direction. It is worth highlighting that the normal component of the velocity in the body frame gives the essential contribution to obtain locomotion in the inertial frame. With respect to energy considerations, we may notice that the kinetic energy injected into the fluid by the body’s deformation is essentially transferred to the locomotion kinetic energy (see Wu Reference Wu1971, Kanso Reference Kanso2009). Since no vorticity release is included in the model, the total kinetic energy shows a periodically oscillating behaviour with a constant mean value, hence no power is transferred to the fluid and wasted into the wake. Consistently, the Froude efficiency, given in the present case by the ratio of two equal and null quantities, looses most of its interest and is not considered in the following. For a detailed description of the energy transfer process see Appendix C.

The motion of the body’s centre of mass is obtained by solving $ {{{\rm d} X}/{ {\rm d}t}} = U_X$ and integrating in time to obtain the axial displacement for each time.

From Appendix A we may notice that, even if $P_x = 0$ , this results in $F_x \neq 0$ , so the force is not purely normal to the body but a tangential component arises due to the rotation of the normal vector. This aspect has been mentioned in Limacher (Reference Limacher2021) discussing the chord-wise component of the added-mass force.

By recalling (A9) and using $\dot \theta$ for $\varOmega$ , we obtain

(2.18) \begin{equation} \left \{ \begin{array}{l} F_x = \pi \rho b^2\,\dot \theta \left[ u_y + \dot h + b \dot \theta \right],\\[2mm] F_y = - \pi \rho b^2\,\left[ \dot {u}_y + \ddot h + b \ddot \theta \right] ,\\[2mm] \end{array} \right . \end{equation}

where the expression of $F_y$ may be compared with the lift reported in Theodorsen (Reference Theodorsen1935). Let us underline that, by the theory of Theodorsen, we are able to compute separately the finite integral contributions given by the purely potential flow in terms of added-mass coefficients. By using the transpose of the rotation matrix (2.10) the forces in the ground and body reference frames are related by

(2.19) \begin{equation} \begin{bmatrix} F_X \\ F_Y \end{bmatrix} = \begin{bmatrix} \,\,\, \cos \theta \,F_x - \sin \theta \,F_y \\ \sin \theta \,F_x + \cos \theta \,F_y \end{bmatrix} \simeq \begin{bmatrix} \,\, \,F_x - \theta \,F_y \\ \theta \,F_x + \,F_y \end{bmatrix}. \end{equation}

The development of the forces during one period, both in the ground and in the body-fixed frame, is displayed in figure 2 for $h_o = 0.1$ and $\theta _o = 10^\circ$ . By evaluating the average values over one period we obtain $\overline {F_X} =0$ , $\overline {F_Y} =0$ , $\overline {F_y} =0$ while $\overline {F_x} \neq 0$ (represented by the dashed line in the same figure).

It should be noted that the forces described above arise solely from the flapping tail, with the added-mass contribution of the virtual body excluded from the balance.

Figure 2. Time behaviour of (a) $F_X$ and $F_Y$ in the ground frame; (b) $F_x$ and $F_y$ in the body-fixed frame (the dashed line shows the mean value of $F_x$ ) for $h_o=0.1$ and $\theta _o = 10^\circ$ .

3. Locomotion for prescribed heave and pitch

As a starting point, we evaluate the motion of the body which results from prescribed heave and pitch motions. The relevant parameters appearing in what follows are: the plate thickness $s^\ast$ , its length $c^\ast =2\,b^\ast$ and the densities of the fluid $\rho ^\ast$ and body $\rho ^\ast _b$ . While dimensional quantities were used up to this point, we will now distinguish between dimensional values, denoted with an asterisk ( $^\ast$ ), and their corresponding non-dimensional counterparts, which will be written without the asterisk. We define the amplitudes of the pitch and heave motions as $\theta _o$ and $h_o^\ast$ , respectively, while the phase angle between them is denoted as $\phi$ and the oscillation frequency is $\omega ^\ast = 2 \pi f^\ast$ . The motion of the plate is then given by

(3.1) \begin{equation} \left \{ \begin{array}{l} \theta = \theta _o \,\sin \left(\omega ^\ast \,t^\ast + \phi \right) ,\\[2mm] h^\ast = h_o^\ast \,\sin \left(\omega ^\ast \,t^\ast \right). \end{array} \right . \end{equation}

To determine the mean locomotion speed, $\overline {U^\ast _X}$ , we evaluate the average velocity over one period using (2.17). Noting that all cross-terms between heave and pitch contributions have a zero mean value, the only remaining term is $\overline {\theta \dot h^\ast } = (1/2) \omega ^\ast \theta _o h_o^\ast sin(\phi )$ , leading to

(3.2) \begin{equation} \overline {U^\ast _X} = \frac {1}{2} \frac {\pi \rho ^\ast {b^\ast }^2}{\left(m_b^\ast + \pi \rho ^\ast {b^\ast }^2\right)} \theta _o \omega ^\ast h_o^\ast \sin (\phi ). \end{equation}

From (3.2) we observe two key results: (i) the sign and magnitude of the mean locomotion velocity are directly controlled by $\sin \phi$ , the maximum locomotion (i.e. negative velocity) occurring for $\phi = -\pi /2$ , which means that the pitch motion lags the heave motion by a quarter period, in agreement with previous findings (Quinn, Lauder & Smits Reference Quinn, Lauder and Smits2015; Van Buren, Floryan & Smits Reference Van Buren, Floryan and Smits2018); (ii) no motion occurs when heave and pitch are in phase. Additionally, both heave and pitch must be present for locomotion. If either is absent, the body remains stationary.

By using $\omega ^\ast = 2\,\pi \,f^\ast$ and $h_o^\ast = b^\ast \, h_o$ , the average locomotion speed (3.2) can be expressed in terms of the reduced speed or the ‘stride length’, i.e. the non-dimensional locomotion velocity (based on the reference velocity $V^\ast _R = b^\ast f^\ast$ ) or the travelling distance measured in body lengths per second

(3.3) \begin{equation} U = \frac {\overline {U^\ast _X}}{b^\ast f^\ast } = \frac {\pi ^2 \rho ^\ast {b^\ast }^2}{\left(m_b^\ast + \pi \rho ^\ast {b^\ast }^2\right)} \theta _o h_o \sin (\phi ). \end{equation}

Figure 3. Time evolution of the $X$ -component of impulse, velocity and displacement for heave and pitch ( $h_o = 0.1$ ; $\theta = 10^\circ$ ; $\phi = -\pi /2$ ). The horizontal dashed line represents the mean value of $U_X$ .

Figure 3 illustrates the time evolution of impulse, velocity and displacement in the $X$ -direction for $h_o = 0.1$ and $\theta _0 = 10^\circ$ with a phase shift $\phi = -\pi /2$ . The dashed line in the figure represents the mean velocity calculated from (3.2). According to the analytical expression of the mean locomotion velocity (3.2), leftward motion occurs for negative phase angles. Figure 4 shows the solution in terms of $X$ -displacement in the ground frame as the phase shift between heave and pitch is varied from $0$ to $-\pi$ . In particular, we notice that the maximum displacement at the end of the cycle increases monotonically as $\phi$ approaches $-\pi /2$ , with smaller and equal values for symmetric variations of $\phi$ about $- \pi /2$ .

Figure 4. Temporal evolution of $X$ displacement for heave ( $h_o =0.1$ ) and pitch ( $\theta = 10^\circ$ ) with several values of the phase shift.

In previous studies (Paniccia et al. Reference Paniccia, Padovani, Graziani and Piva2021c , Reference Paniccia, Padovani, Graziani and Piva2023), it was shown that an appropriate phase shift can generate a travelling wave with an approximate phase velocity, $c=\omega ^\ast h_o^\ast /\theta _o$ , which reproduces a behaviour similar to undulatory swimming by creating a certain dissymmetry in the resulting motion. However, in the present case of a purely reactive solution, the resulting locomotion is significantly lower than the above defined $c$ , showing a poor performance in the absence of vortex shedding.

4. Locomotion of a passive flapping plate

In this section, we analyse the fluid dynamic moment acting on a flapping plate and derive the torque balance equation, which governs the evolution of passive pitch. To represent in an efficient way a flexible plate, we will assume that the pitching motion of the plate is not prescribed but results from a torque balance involving a torsional spring at the LE (see also Toomey & Eldredge Reference Toomey and Eldredge2008; Vanella et al. Reference Vanella, Fitzgerald, Preidikman, Balaras and Balachandran2009; Eldredge et al. Reference Eldredge, Toomey and Medina2010; Spagnolie et al. Reference Spagnolie, Moret, Shelley and Zhang2010; Zhang, Liu & Lu Reference Zhang, Liu and Lu2010; Moore Reference Moore2014; Hang et al. Reference Hang, Heydari, Costello and Kanso2022). To solve the torque balance, we must evaluate the hydrodynamic moment exerted by the surrounding fluid on the rigid body, which moves in an arbitrary manner in an unbounded fluid. For purely potential flow, only the reactive contribution is considered in the expression of the moment, while the circulatory contribution is omitted.

4.1. Fluid dynamic moment, torque balance and pitch solution

We start from the classical added-mass formulation as reported in Newman (Reference Newman2017), with an opposite sign convention due to the outward normal vector from the body into the fluid. We consider a two-dimensional flow field and use the position vector $r^\prime$ from the rotation centre at the LE of the plate. All the relevant details are reported in Appendix A.

The motion of the flat plate can be described in the body system as the superposition of the locomotion velocity components ( $u_x$ , $u_y$ ) and the prescribed heaving motion $\dot h$

(4.1) \begin{equation} U_1 = u_x + \dot h \sin \theta \simeq u_x + \dot h \theta \quad U_2 = u_y + \dot h \cos \theta \simeq u_y + \dot h. \end{equation}

By combining with (A17), removing quadratic terms and considering that $u_x = 0$ for a flat plate, we obtain

(4.2) \begin{equation} M_3 = - \pi \rho b^3 \!\left [\dot u_y + \ddot h + \frac {9}{8} b {\ddot \theta } \right ] ,\end{equation}

where the angular acceleration causes a moment which may be thought of as due to a virtual moment of inertia $ (9/8) \rho \pi b^4$ . By time differentiating (2.15) and combining with (4.2) we obtain

(4.3) \begin{equation} M_3 = -\pi \rho b^3 \!\left \{ \frac {m_b}{m_b + \pi \rho b^2} \ddot h + \left [ \frac {m_b}{m_b + \pi \rho b^2} + \frac {1}{8}\right ] b {\ddot \theta } \right \}. \end{equation}

Now we consider a thin foil undergoing prescribed heaving motion with a torsional spring at its LE. This set-up has been widely used in the literature as an effective model for plate flexibility due to fluid–body interaction, (see e.g. Moore Reference Moore2014). Since pitching motion is not prescribed, it must be determined by solving a torsional balance equation that accounts for the fluid dynamic moment, spring restoring torque and body inertia effects.

The goal is to analyse the combined effect of forced heaving and passive pitching motion in a perfect fluid to determine to what extent self-propulsion occurs. Although approximate, this model provides some insight into the body’s locomotion mechanism. A more generalised approach including the wake dynamics is addressed in an ongoing work.

A time-harmonic heaving motion, with non-dimensional amplitude $h_o ={h_o^\ast }/{b^\ast }$ , is imposed at the LE of the plate. In response to this driving motion, a torsional spring with rotational stiffness $k^\ast$ at the LE allows the plate to pitch passively with an assumed harmonic motion $\theta = {\theta _o} e^{i\,(\omega ^\ast \,t^\ast + \phi )}$ . The pitching motion of the plate (amplitude and phase) is not prescribed but rather is evaluated by balancing the angular moments due to the fluid (see 4.3), to the spring and to the body’s inertia.

The torque balance equation governing the passive flapping motion is derived in detail in Appendix B. Below, we only report its dimensionless form and the solution in terms of pitch amplitude and phase shift between heave and pitch

(4.4) \begin{equation} \frac {16}{3} R\,\ddot \theta + C \dot \theta + K\, \theta = {M_f} + {M_i} ,\end{equation}

where $R$ is the body–fluid mass ratio, $C$ and $K$ are the dimensionless spring damping and stiffness coefficients, respectively, $M_f$ is the dimensionless form of the fluid dynamic moment given by $M_3$ in (4.3) while $M_i$ is the inertial torque due to the forced heaving.

In the torsional balance (4.4), the terms related to $\dot \theta$ may introduce a non-zero phase shift between heave and pitch which is required to obtain $\theta \ne 0$ and hence locomotion. The $\dot \theta$ term clearly appears in the spring damping while, concerning the fluid dynamic moment $M_f$ , its presence would be associated with the circulatory component and vortex shedding.

Consistently, in the present purely reactive solution, this term is missing in the fluid dynamic moment, so the spring damping remains the only contributor to phase shift (see the second expression in (4.5) below).

Once the harmonic expressions for heave and pitch are considered and by using standard harmonic analysis, the solution for the passive pitch motion is obtained in terms of $\theta _o$ and $\phi$

(4.5) \begin{equation} \left \{ \begin{split} &\theta _o = \frac {\textit{BB}\,h_o}{\sqrt {\textit{AA}^2 + 4 \pi ^2 C^2}}, \\ &\tan(\phi ) = \frac {- 2 \pi C }{\textit{AA}} .\end{split} \right . \end{equation}

This solution is expressed in terms of the coefficients provided in Appendix B: $\textit{BB}$ , which depends on the mass ratio $R$ , and $AA$ , which is function of the mass ratio as well as of the spring stiffness $K$ . For the reader’s convenience, we report below their expressions

(4.6) \begin{align} \textit{BB} & = 16\,\pi ^2\,R \left [\frac {4\,R + 2\,\pi }{4\,R + \pi } \right ] \quad \quad R = \frac {s^\ast \,\rho ^\ast _b}{c^\ast \,\rho ^\ast },\end{align}
(4.7) \begin{align} \textit{AA} & = -4 \pi ^2 \left [ \frac {16}{3} R + \frac {\pi }{4} \left ( \frac {36\,R + \pi }{8\,R + 2\,\pi } \right ) \right ] + K = -4 \pi ^2 A_1 + K.\end{align}

Figure 5. Behaviour of the mean self-propulsion speed $U_s$ as a function of $K$ ( $h_o =0.1$ ) for different values of the spring damping coefficient $C$ : $C=0.1, 0.2, 0.5$ (a); $C=1, 2, 10.$ (b).

As clearly appears from (4.5), no pitch may occur without heave, i.e. if we have $h_o=0$ it follows also that $\theta _o=0$ . Moreover, the solution gives $\phi =\pm \pi /2$ for $AA=0$ , i.e., for a given relation between the mass ratio and the spring stiffness, which, as shown below, is related to the resonance frequency. In this condition the larger energy transfer is obtained, maximising locomotion, which still remains quite small.

4.2. Swimming speed and natural frequency

Once the pitch angle and phase have been evaluated through (4.5), then the mean locomotion speed $U_s = \overline {U_X}$ may be evaluated. By using the above introduced non-dimensional quantities, the first in (3.2) gives

(4.8) \begin{equation} U_s = \frac {\overline {U_X^\ast }}{b^\ast f^\ast } = \pi (1-\textit{CC}) \theta _o h_o \sin (\phi ) =\frac {\pi ^2}{4\,R + \pi }\, \theta _o h_o \sin (\phi ), \end{equation}

where the coefficient $\textit{CC}$ , depending on the mass ratio only, is reported in (B7) in Appendix B.

The above reported solution shows that: (i) no self-propulsion occurs unless pitch and heave are simultaneously present; (ii) a non-zero phase shift is required for the generation of net locomotion; and (iii) to achieve maximum velocity, $\phi \simeq \pm \pi /2$ is required. In the figures we present results for $U_s$ , $\theta _o$ and $\phi$ as functions of the spring stiffness $K$ for several values of the spring damping $C$ from 0.1 to 10. All the plots are drawn for a given value of $C$ , as a function of ${k^\ast }/{{f^\ast }^2}$ or $K$ in dimensionless form, to ensure that all solutions collapse onto a single curve (see also Zhong et al. Reference Zhong, Zhu, Fish, Kerr, Downs, Bart-Smith and Quinn2021). From figure 5 we may notice several results: first, the locomotion speed peaks at a specific value of $K$ and, second, the maximum value of the locomotion velocity increases as the spring damping decreases. This peak is likely a result of resonance effects, as discussed below.

Figure 6. Pitch amplitude $\theta _o$ as a function of $K$ ( $h_o =0.1$ ) for $C=0.1, 0.2, 0.5$ (a); $C=1, 2, 10.$ (b).

Figure 7. Phase angle variation as a function of $K$ ( $h_o =0.1$ ): (a) $C=0.1, 0.2, 0.5$ ; (b) $C=1, 2, 10$ .

The values of the pitch amplitude $\theta _o$ are reported in figure 6 as a function of $K$ for several values of $C$ . We notice both a peak at the same value of $K$ as for the locomotion speed and a reduction in the amplitude for increasing $C$ . Moreover, for $C$ larger than one, the pitch amplitude quickly falls to very small values. On the contrary, for the smallest $C$ it follows that $\theta _o$ exceeds the small-angle approximation, although a similar trend persists.

A comparison between active and passive motion reveals key differences. In the former case, the solution is given by (3.3) and shows a linear dependence of the velocity on both the amplitudes of heave $h_o$ and pitch $\theta _o$ . On the other hand, in the passive case the pitch amplitude is not prescribed but is evaluated from the torsional balance. Equation (4.5) shows that $\theta _o$ is linearly dependent on $h_o$ , leading to $U_s \propto h_o^2$ . Both the physical coefficients of the spring balance, $C$ and $K$ , can also significantly affect the resulting pitch amplitude. Thus, we may argue that, to achieve optimal locomotion, these physical parameters should be tuned consistently to achieve the proper pitch amplitude.

The variation of the phase angle $\phi$ between pitch and heave is plotted in figure 7 as a function of $K$ for the previously considered values of $C$ . Notably, a steep change in $\phi$ occurs near the peak values of both $U_s$ and $\theta _o$ . Specifically, by observing the peak values in figures 5 and 6 and by comparing with figure 7, we notice that, when $U_s$ and $\theta _o$ reach their maximum values, it follows always that $\phi = -\pi /2$ . In fact, from the second of (4.5), we notice that $\phi = \pm \pi /2$ for $AA=0$ or, due to (4.7), $K = 4\,\pi ^2\,A_1$ . By using the non-dimensional spring stiffness defined in (B4), the peak frequency occurs for

(4.9) \begin{equation} \frac {k^\ast }{{f^\ast }^2} = K \,\rho ^\ast \,{b^\ast }^4 = \rho ^\ast \,{b^\ast }^4\,4\,\pi ^2\,A_1 ,\end{equation}

where $A_1$ depends on the mass ratio only, and its expression is reported in Appendix B.

Figure 8. (a) Variation of $\theta _o$ and $\phi$ as a function of frequency; (b) self-propulsion velocity ( $h_o =0.1, k=4000, C=1$ ).

At the peak condition, i.e. for $AA=0$ , the torque balance equation shrinks to (see (B12))

(4.10) \begin{align} C\, \dot \theta = \textit{BB}\, h ,\end{align}

while the first expression in (4.5) yields

(4.11) \begin{align} \theta _o = \frac{\textit{BB}}{ 2 \pi C}\,h_o. \end{align}

Since the coefficient ${\textit{BB}}$ , defined in (4.6), is only function of the ratio between the body and the fluid mass, the pitch amplitude value increases without limits for vanishing spring damping $C$ . Then, from (4.8), the self-propulsion speed is expressed as

(4.12) \begin{align} U_s =- 16\,\pi ^3 \frac {R\,(2\,R + \pi )}{C\,(4\,R + \pi )^2} h_o^2 ,\end{align}

which also shows both the increase of the peak locomotion velocity for decreasing $C$ and the relevance of $h_o$ .

The pitch amplitude and phase and the opposite of the mean self-propulsion speed, $-U=-\overline {U_X^\ast }$ , for $C=1$ and $k=4000$ , are shown, as functions of the oscillation frequency, in figures 8(a) and 8(b), respectively. The values of $\theta _o$ and $\phi$ for some selected frequencies are used in figure 9 to represent the corresponding stroke loop in the shape space (i.e. where the variables $h$ and $\theta$ , which describe the shape of the body, are the independent variables). We notice that the area of each curve increases with the mean self-propulsion speed, while its orientation is only related to the phase angle. For vanishing $\phi$ , a reciprocal motion is obtained, which gives null locomotion. On the contrary, the curve with the largest area in the shape space corresponds to the maximum locomotion speed and to a phase shift $-\pi /2$ . These results confirm the observations of other authors (see e.g. Ross Reference Ross2006, Hatton & Choset Reference Hatton and Choset2010).

Figure 9. Stroke loops in the shape space for the frequencies selected in figure 8 ( $h_o =0.1, k=4000, C=1$ ).

Several solutions reported above for the passive swimming plate display a peaky behaviour which resembles that of the amplification factor of a forced harmonic oscillator with damping.

The peak frequency given by (4.9) is related to the natural oscillation frequency defined by (B19). From this expression we obtain $ {k^\ast }/{{f^\ast _N}^2} = 4 \pi ^2 \rho ^\ast {b^\ast }^4 A_1$ , as given by (4.9), confirming that the peak locomotion speed occurs at the natural frequency with a clear connection to resonance phenomena (see Beal et al. Reference Beal, Hover, Triantafyllou, Liao and Lauder2006, Michelin & Smith Reference Michelin and Smith2009, Alben et al. Reference Alben, Witt, Baker, Anderson and Lauder2012, Moore Reference Moore2014, Paraz, Schouveiler & Eloy Reference Paraz, Schouveiler and Eloy2016, Lopez-Tello, Fernandez-Feria & Sanmiguel-Rojas Reference Lopez-Tello, Fernandez-Feria and Sanmiguel-Rojas2023). The damping term was not accounted for in the above evaluation of the natural frequency, since it has a negligible effect.

5. Concluding remarks

The results presented in this paper provide a further contribution to clarify the question raised by Saffman more than 50 years ago regarding swimming in a perfect fluid. Namely, if we consider a deformable body in a quiescent perfect fluid, we find that a self-propulsion may occur through the exchange of reactive forces with the surrounding fluid, without any generation or release of vorticity, provided that a proper deformation is prescribed. Our study focuses on fish locomotion driven by a tail flapping, while the main body contributes only inertial effects, as no resistive forces are considered. This oscillatory swimming model is representative of tuna or other species within the broader class of carangiform fish. Similar configurations can be effectively analysed using a simplified model consisting of a virtual body with an oscillating tail attached to its end to generate the propulsion for the entire fish. This approximation provides a direct answer to the fundamental question of whether a fish can achieve locomotion solely through appropriate body deformation, without the release of vorticity.

To investigate this phenomenon, we adopted an impulse-based mathematical model that considers only added-mass forces in a purely potential flow. As a preliminary case, we analysed active oscillations in which heave and pitch motions are fully prescribed. A flat plate was used as the geometric model for the tail, allowing analytical solutions to provide global results without caring about singular behaviour at the plate’s sharp edges in the absence of viscosity The results confirm that self-propulsion is generated by the flapping tail, provided a phase shift between heave and pitch is established, and, if one of these motions is prevented, no self-propulsion takes place. Even in this relatively simple case, despite several results already available in the literature, the topic of locomotion in a perfect fluid still raises some perplexities. We hope that our findings for a simple fish-like configuration may help to further clarify this issue.

The aim of the paper is to consider more realistic configurations accounting for the flexibility of the tail. In this case, the pitch amplitude and phase lag are no longer prescribed, but instead emerge from fluid–structure interaction. Within this framework, the tail motion is passive and requires an additional torque balance equation to capture its flexibility, which we model as being concentrated at the LE via a torsional spring. Notice that a localised torsional spring with tuneable stiffness is considered one of the most effective approaches for assessing the role of flexibility in the passive tail dynamics. A more detailed analysis was required to balance all torques acting about the rotation centre, located at the peduncle that connects the tail to the main body. Structural damping must also be taken into account, in addition to fluid–structure interaction. In this context, the phase shift, previously shown to be essential for locomotion, emerges as a result of structural damping, which may become negligible in a complete solution where damping due to vortex shedding dominates.

The solution for the flexible tail reveals the key result: a unique relationship between stride length and non-dimensional stiffness. This relationship displays a characteristic growth pattern at a specific value of non-dimensional stiffness, corresponding to the natural frequency of the tail foil in an otherwise quiescent fluid.

To maintain an optimal stride length, a fish swimming at a given frequency must adjust its stiffness through muscular action in the peduncle region. Alternatively, for a fixed stiffness, the fish must tune its swimming frequency to maximise performance. This result closely mirrors self-propulsion mechanisms observed in nature. In essence, the fish must fine tune its physical parameters to achieve a stride length that aligns with the resonance region.

Finally, extending this study to more realistic conditions – including circulatory forces and vorticity shedding, for instance, by means of a Kutta condition – will be greatly facilitated by our current approach. The proposed methodology ensures precise control over the critical components of the solution associated with pure inertial terms. In contrast, the inclusion of vortical impulse and vorticity release tends to dominate the resulting dynamics, potentially obscuring the more subtle aspects addressed in this paper. A further deepening on this matter is firmly envisaged by the authors to strengthen the above conceptual points.

Acknowledgements

The research of G.G. was founded by Sapienza University of Rome through the research grant ‘Progetti di Ricerca 2023 N.RP123188E86CE50C’. This work was produced externally to Leonardo S.p.A. and does not involve any proprietary data, information or projects. We also thank the anonymous referee for the many helpful remarks.

Declaration of interests

The authors report no conflict of interest.

Author contributions

All authors contributed equally to this work.

Appendix A. Forces and moment

According to Newman (Reference Newman2017), we may express the forces acting on the body within an acyclic potential flow. Let us denote the translation velocity of LE as $\boldsymbol{U}_o (t)=\{U_1 \boldsymbol{e}_1; U_2 \boldsymbol{e}_2; \}$ or, by defining $\boldsymbol{r}$ the radius vector with origin in LE, $\boldsymbol{V}_B = \boldsymbol{U}_o + \varOmega \,\boldsymbol{e}_3 \times \boldsymbol{r}$ .

The potential $\phi$ satisfies Laplace’s equation with the boundary condition on the body contour

(A1) \begin{equation} \frac {\partial \phi } {\partial n} = \boldsymbol{V}_B \boldsymbol{\cdot }\boldsymbol{n} = \boldsymbol{U}_o \boldsymbol{\cdot }\boldsymbol{n} + \varOmega \, (\boldsymbol{r} \times \boldsymbol{n}) \boldsymbol{\cdot }\boldsymbol{e}_3. \end{equation}

We split the potential into the basis potentials $\phi = \phi _i\,U_i$ with $i=1,2,3$ . Here, $\phi _i$ represents the velocity potential due to a body motion with unit velocity $U_i$ in the ith mode (linear $U_i = \boldsymbol{U}(t)$ for i = 1,2 or angular for $U_3 = \varOmega (t) \boldsymbol{e_3}$ ). These basis motions and their time derivatives ( $U_i$ and $\dot {U_i}$ ) are considered in the body frame

(A2) \begin{equation} \phi = U_1\,\phi _1 + U_2\,\phi _2 + U_3\,\phi _3 = U_i\,\phi _i \quad i=1,2,3. \end{equation}

By substituting (A2) into (A1) it follows that

(A3) \begin{equation} U_1\,\frac {\partial \phi _1}{\partial n} + U_2\,\frac {\partial \phi _2}{\partial n} + U_3\,\frac {\partial \phi _3}{\partial n} = U_1\,n_1 + U_2\,n_2 + U_3\,(\boldsymbol{r} \times \boldsymbol{n})_3. \end{equation}

Each one of the potentials $\phi _i$ satisfies Laplace’s equation, the vanishing condition at infinity and the condition on the body contour

(A4) \begin{equation} \frac {\partial \phi _1} {\partial n} = n_1 \quad \frac {\partial \phi _2} {\partial n} = n_2 \quad \frac {\partial \phi _3} {\partial n} = (\boldsymbol{r} \times \boldsymbol{n})_3. \end{equation}

In the body-fixed reference frame, the potentials $\phi _i$ depend only on the geometry of the body (through the normal $\boldsymbol{n}$ ) and not on time or the velocities $U_i$ . In the ground frame, the force acting on the body, by substituting (A2) into (2.6), is expressed as

(A5) \begin{equation} \boldsymbol{F_{b}} = \rho \frac{d}{{\rm d}t} \left ( U_i(t) \int _{S_b }\phi _i {\boldsymbol{n}} \,{\rm d}S \right ) ,\end{equation}

where the integral depends on time due to the variation of $\boldsymbol{n}$ caused by the rotation of the body: ${{\rm d} \boldsymbol{n}}/{{\rm d}t} = \boldsymbol{\varOmega } \times \boldsymbol{n}$ . From (A5), the force components in the body frame, expressed in index form, are

(A6) \begin{equation} F_j = \rho \, \dot {U_i}(t) \int _{S_b }\phi _i n_j \,{\rm d}S + \rho \, \epsilon _{j3l} {U_i} \varOmega \int _{S_b }\phi _i n_l \,{\rm d}S \quad i,l = 1,2,3 \quad j=1,2 ,\end{equation}

where $\epsilon _{ijk}$ is the permutation tensor. By considering the boundary conditions (A4), the above appearing integrals may be evaluated as

(A7) \begin{equation} \rho \int _{S_b }\phi _i n_j \,{\rm d}S = \rho \int _{S_b }\phi _i \frac {\partial \phi _j} {\partial n} \,{\rm d}S = - m_{j\,i} ,\end{equation}

where $m_\textit{ji}$ are the components of the added-mass tensor whose values depend solely on the geometry of the body. When considering a flat plate with length $2\,b$ (zero thickness) pitching about its LE, the only non-zero added-mass coefficients (including also $m_{3\,3}$ appearing in the following) are

(A8) \begin{align} m_{2\,2} = \rho \pi b^2 \quad m_{2\,3} = \rho \pi b^3 \quad m_{3\,3} = \frac {9}{8} \pi \rho b^4. \end{align}

According to (A6), by using $F_x$ and $F_y$ instead of $F_1$ and $F_2$ , the force components in the body-fixed frame may be written as

(A9) \begin{equation} \left \{ \begin{array}{l} F_x = \varOmega ( m_{2\,1} U_1 + m_{2\,2} U_2 + m_{2\,3} \varOmega ) = \rho \pi b^2 \,\varOmega ( U_2 + b\,\varOmega ),\\[3mm] F_y = -( m_{2\,1} \dot {U}_1 + m_{2\,2} \dot {U}_2 + m_{2\,3} \dot {\varOmega }) = -\rho \pi b^2 (\dot {U}_2 + b\, \dot {\varOmega }). \end{array} \right . \end{equation}

Similarly, by using the basis potentials, the impulse components can be expressed as

(A10) \begin{equation} \left \{ \begin{array}{l} \rho P_x = -\rho \int _{S_b }\phi n_x \,{\rm d}S = -\rho \int _{S_b }U_i\,\phi _i n_x \,{\rm d}S = m_{1\,1} U_1 + m_{1\,2} U_2 + m_{1\,3} \varOmega ,\\[3mm] \rho P_y = -\rho \int _{S_b }\phi n_y \,{\rm d}S = -\rho \int _{S_b }U_i\,\phi _i n_y \,{\rm d}S = m_{2\,1} U_1 + m_{2\,2} U_2 + m_{2\,3} \varOmega .\end{array} \right . \end{equation}

It follows for the flat plate

(A11) \begin{equation} \left \{ \begin{array}{l} P_x = 0 ,\\[3mm] P_y = \pi b^2 ({U}_2 + b\, {\varOmega }). \end{array} \right . \end{equation}

Finally, the forces can be expressed in terms of the impulses as

(A12) \begin{equation} \left \{ \begin{array}{l} F_x = \rho \dfrac{d}{{\rm d}t} \int _{S_b }\phi n_x \,{\rm d}S - \rho \varOmega \int _{S_b }\phi n_y \,{\rm d}S = \rho \varOmega \,P_y ,\\[3mm] F_y = \rho \dfrac{d}{{\rm d}t} \int _{S_b }\phi n_y \,{\rm d}S + \rho \varOmega \int _{S_b }\phi n_x \,{\rm d}S = - \rho \frac {{\rm d} P_y}{{\rm d}t} .\end{array} \right . \end{equation}

By following the same approach as above, the fluid dynamic moment is given by

(A13) \begin{align} M_j = \rho {\dot U}_i \int \phi _i\, (\boldsymbol{r^\prime } \times \boldsymbol{n})_j \,{\rm d}S + \rho \epsilon _{jkl} \,U_i\,U_k \int \phi _i n_l\,{\rm d}S \;\; \quad i=1,2,3. \end{align}

The boundary condition on the body contour is expressed as in (A1) with $\boldsymbol{r^\prime }$ instead of $\boldsymbol{r}$ , while each one of the basis potentials $\phi _i$ satisfies the condition (A4). In the present two-dimensional solution, the only non-vanishing component of the moment is $M_3$ , which follows from (A13)

(A14) \begin{equation} M_3 = \rho \left ( {\dot U}_i \int \phi _i\, (\boldsymbol{r^\prime } \times \boldsymbol{n})_3 \,{\rm d}S + U_i\,U_1 \int \phi _i n_2\,{\rm d}S - U_i\,U_2 \int \phi _i n_1\,{\rm d}S \right ) \,\,\, i=1,2,3. \end{equation}

By using (A7) and introducing further components of the added-mass matrix

(A15) \begin{equation} \rho \int \phi _i\, (\boldsymbol{r^\prime } \times \boldsymbol{n})_3 \,{\rm d}S = \rho \int _{S_b }\phi _i \frac {\partial \phi _3} {\partial n} \,{\rm d}S = - m_{3\,i} \quad i=1,2,3. \end{equation}

Equation (A14) gives, writing $\varOmega$ for $U_3$ ,

(A16) \begin{align} M_3= & -{\dot U}_1 m_{13} - {\dot U}_2 m_{23} - {\dot \varOmega } m_{33} - U_1^2 m_{12} - U_2 U_1 m_{22} - \varOmega U_1 m_{32}\nonumber\\ & + U_1\,U_2 m_{11} + U_2^2 m_{21} + \varOmega \,U_2 m_{31} ,\end{align}

which, for the flate plate, can be simplified into

(A17) \begin{align} M_3 & = -{\dot U}_2 m_{23} - {\dot \varOmega } m_{33} - U_2 U_1 m_{22} - \varOmega U_1 m_{32}\nonumber\\ &= - \pi \rho b^2 \!\left [b\,{\dot U}_2 + \frac {9}{8} b^2 {\dot \varOmega } + U_2 U_1 + b\,\varOmega U_1 \right ] ,\end{align}

where $m_{23}$ and $m_{33}$ relate fluid inertia to heave and pitch, while $m_{22}$ and $m_{32}$ introduce nonlinear effects due to added-mass coupling. Let us recall that $U_1$ and $U_2$ are the LE translation velocities in the body frame of reference.

Appendix B. Non-dimensional torque balance equation and pitch solution

We consider a thin flat plate with thickness $s^\ast$ , length $c^\ast$ and density $\rho ^\ast _b$ . The semi-chord $b^\ast =c^\ast /2$ is chosen as the reference length. The total mass of the plate is given by $m^\ast _p = \rho ^\ast _b \,s^\ast \,c^\ast$ . As previously defined, dimensional quantities are denoted with an asterisk $(^\ast )$ , while dimensionless variables appear without one. We introduce the following non-dimensional quantities $x, h, t$ , among others. Specifically we define $x = x^\ast /b^\ast$ , $h = h^\ast /b^\ast$ and $t =t^\ast /T^\ast$ .

In order to estimate the mass of the body, we assume, as previously defined in Paniccia et al. (Reference Paniccia, Padovani, Graziani and Piva2021c ), that the length of the total body (virtual + tail) is $L^\ast$ ; that the length of the tail is $c^\ast =L^\ast /7$ ; and that the virtual body may be represented by an elliptical shape with chord $c^\ast _b= ({6}/{7})\,L^\ast =6\,c^\ast$ , $4\,\%$ thickness with $s^\ast _b=0.04\,c^\ast _b=0.24\,c^\ast$ . So the area of the virtual body is $V^\ast _b = \pi ({c^\ast _b\,s^\ast _b}/{4})=0.36 \pi {c^\ast }^2$ and $m^\ast _b = \rho ^\ast _b V^\ast _b$ .

The equation governing passive flapping motion, in its dimensional form, is

(B1) \begin{equation} I^\ast \, \ddot \theta ^\ast + C^\ast \,\dot \theta ^\ast + k^\ast \, \theta ^\ast = M^\ast _f + M^\ast _i ,\end{equation}

where $\theta$ has been defined in (3.1). The moment of inertia about the LE is $I^\ast = ({8}/{3}) \rho ^\ast _b s^\ast \,{b^\ast }^3$ while $C^\ast$ and $k^\ast$ represent the structural damping coefficient and the torsional stiffness of the spring, respectively. Here, $M_f^\ast$ is the fluid dynamic moment acting on the foil’s LE and $M_i^\ast$ is the inertial torque caused by the vertical acceleration of the LE. (i.e. the pitching pivot point) during flapping.

To obtain the non-dimensional form of (B1) we divide all terms by $\rho {b^\ast }^2 {V_R^\ast }^2$ , where $V^\ast _R = b^\ast f^\ast$ is the reference velocity.

The non-dimensionalised inertia term becomes

(B2) \begin{equation} \frac {I^\ast \,\ddot \theta ^\ast }{\rho {b^\ast }^4 {f^\ast }^2} = \frac {8}{3} \frac {\rho ^\ast _b s^\ast \,{b^\ast }^3 \ddot \theta ^\ast }{\rho {b^\ast }^4 {f^\ast }^2} = \frac {16}{3} \frac {\rho ^\ast _b \,s^\ast }{\rho ^\ast c^\ast } \ddot \theta = \frac {16}{3} R \ddot \theta ,\end{equation}

where $R = {s^\ast \,\rho ^\ast _b}/{c^\ast \,\rho ^\ast }$ is the ratio of body to fluid inertia. Similarly, the non-dimensional damping term is

(B3) \begin{equation} \frac {C^\ast \,\dot \theta ^\ast }{\rho ^\ast {b^\ast }^4 {f^\ast }^2} = \frac {C^\ast \,f^\ast \,\dot \theta }{\rho ^\ast {b^\ast }^4 {f^\ast }^2} = C \dot \theta \quad {\textrm {where}} \quad C = \frac {C^\ast }{\rho ^\ast {b^\ast }^4 f^\ast }. \end{equation}

The coefficient of the spring restoring torque is expressed as

(B4) \begin{equation} \frac {k^\ast }{\rho ^\ast {b^\ast }^4 {f^\ast }^2} = K. \end{equation}

In this form, according to (B4), the spring effect, through $K$ , appears to be related to the ratio $k^\ast /{f^\ast }^2$ . The inertial moment due to the forced heaving motion of the body, $M_i^\ast = - m^\ast _p b^\ast \ddot h^\ast$ , may be expressed in non-dimensional form as

(B5) \begin{equation} M_i = \frac {M_i^\ast }{\rho ^\ast {b^\ast }^4 {f^\ast }^2} = 8 \pi ^2 \frac {\rho ^\ast _b \,s^\ast }{\rho ^\ast \,b^\ast } h = 16 \pi ^2 R \,h. \end{equation}

The corresponding expression of the fluid dynamic moment is obtained by introducing in (4.3) the above defined non-dimensional quantities

(B6) \begin{equation} M_f = \frac {M_f^\ast }{\rho \,{b^\ast }^4\,{f^\ast }^2} = -\pi \left \{ \textit{CC}\,\ddot h + \left [ \textit{CC} + \frac {1}{8}\right ] {\ddot \theta } \right \} ,\end{equation}

where the non-dimensional coefficient $\textit{CC}$ is defined as

(B7) \begin{equation} \textit{CC}= \frac {m^\ast _p}{m^\ast _p + \pi \,\rho ^\ast \,{b^\ast }^2} =\frac {1}{1 + \frac {\pi }{4} \frac {\rho ^\ast \,c^\ast }{\rho ^\ast _b\,s^\ast }} = \frac {4\,R}{4\,R + \pi }. \end{equation}

The final non-dimensional form of the torque balance (B1) is

(B8) \begin{equation} \frac {16}{3} R\,\ddot \theta + C \dot \theta + K\, \theta = {M_f} + {M_i} ,\end{equation}

which can be recast, by using the above reported expressions for $M_i$ and $M_f$ , as

(B9) \begin{equation} \left [ \frac {16}{3} R\, + \pi \left ( \textit{CC} + \frac {1}{8}\right ) \right ] \ddot \theta + C \dot \theta + K\, \theta = -\pi \textit{CC}\,\ddot h + 16 \pi ^2 R \,h ,\end{equation}

or restated in a more concise form as

(B10) \begin{equation} A_1\, \ddot \theta + C \dot \theta + K\, \theta = -\pi \textit{CC}\,\ddot h + 16 \pi ^2 R \,h ,\end{equation}

where

(B11) \begin{equation} A_1 = \left [ \frac {16}{3} R\, + \pi \left ( \textit{CC} + \frac {1}{8}\right ) \right ]. \end{equation}

Equation (B10) can be rearranged, by using the harmonic expressions for $\ddot \theta$ and $\ddot h$ and by defining two further non-dimensional coefficients $AA$ and $BB$ , as

(B12) \begin{equation} AA\,\theta + C \dot \theta = \textit{BB}\,h ,\end{equation}

where

(B13) \begin{align} \textit{AA} & = -4 \pi ^2 A_1\, + K = - \frac {64}{3} \pi ^2 R\, + K\, - \pi ^3 \left ( \frac {36\,R + \pi }{8\,R + 2\,\pi } \right ) ,\end{align}
(B14) \begin{align} \textit{BB} & = 4\,\pi ^3 \textit{CC}\, + 16\,\pi ^2 R = 16\,\pi ^2\,R \left [\frac {4\,R + 2\,\pi }{4\,R + \pi } \right ].\end{align}

Finally, by using standard manipulations, the solution for the passive pitch motion is obtained in terms of $\theta _o$ and $\phi$

(B15) \begin{equation} \left \{ \begin{split} &\theta _o = \frac {\textit{BB}\,h_o}{\sqrt {\textit{AA}^2 + 4 \pi ^2 C^2}} ,\\[3pt] &\tan(\phi ) = \frac {- 2 \pi C }{\textit{AA}}. \end{split} \right . \end{equation}

Equation (B15) allows for several observations: (i) the phase angle increases with $C$ and reaches its maximum when $AA=0$ ; (ii) the pitch amplitude vanishes for $BB=0$ , i.e. for a massless body, and is otherwise inversely related to $C$ .

The passive flapping motion is described by (B1), which corresponds to a damped system with harmonic forcing. Therefore, a natural frequency may be evaluated which is related to a resonant behaviour. We have expressed the fluid dynamic torque in (4.3) which is here restated in a more concise form as

(B16) \begin{equation} M_f^\ast = M^\ast _h \ddot h^\ast + M^\ast _\theta \ddot \theta ^\ast ,\end{equation}

where

(B17) \begin{equation} M^\ast _h = -\pi \rho ^\ast {b^\ast }^3 \textit{CC} \quad M^\ast _\theta = -\pi \rho ^\ast {b^\ast }^4 \left [ \textit{CC} + \frac {1}{8}\right ] ,\end{equation}

and $\textit{CC}$ is defined in (B7).

Let us assume no heave forcing (i.e. $M^\ast _h=0$ ) and $M_i^\ast =0$ . Now (B1), by developing time derivatives, becomes

(B18) \begin{equation} - {\omega ^\ast }^2 (I^\ast - M^\ast _\theta ) + i\, \omega ^\ast C^\ast + k^\ast = 0. \end{equation}

The undamped natural frequency of torsional vibration in vacuum depends on the spring stiffness $k^\ast$ as well as on the moment of inertia about the LE $I^\ast$ : $\omega ^\ast _v= \sqrt {{k^\ast }/{I^\ast }}$ The presence of the fluid modifies this frequency and from (B18) we obtain

(B19) \begin{equation} \omega ^\ast _N =\sqrt {\frac {k^\ast }{I^\ast - M^\ast _\theta }} =\sqrt {\frac {k^\ast }{ \rho ^\ast {b^\ast }^4 A_1}}. \end{equation}

Appendix C. Kinetic energy

The kinetic energy ( $T$ ) of the isolated fluid–body system may be expressed through the sum of the kinetic energy of the body and of the fluid

(C1) \begin{equation} T_{body} = \frac {1}{2} m_b (u_y + \dot h)^2 + \frac {1}{2} I_{zz} {\dot \theta }^2. \end{equation}

The kinetic energy of the fluid may be expressed in terms of the added mass and of the base velocities (see e.g. Childress Reference Childress1981; Newman Reference Newman2017)

(C2) \begin{equation} T_{fluid} = \frac {1}{2} m_{ij} U_i U_j = \frac {1}{2} \left [ m_{22}(u_y + \dot h)^2 + m_{33}\,{\dot \theta }^2 +2\,m_{23}(u_y + \dot h) \dot \theta \right ] ,\end{equation}

which may be added to give

(C3) \begin{equation} T = \frac {1}{2} \left [ (m_b + m_{22}) (u_y + {\dot h})^2 + (I_{zz} + m_{33}) \dot \theta ^2 \right ] + m_{23}(u_y +\dot h ) \dot \theta. \end{equation}

As discussed in Kanso (Reference Kanso2009), the total kinetic energy could be split into three contributions: one related to the shape deformation ( $\dot h$ and $\dot \theta$ ), one related to the body locomotion ( $u_y$ ) and the remaining one acting as a coupling effect between both of them. In her case of a massless body it can be shown that most of the energy input into the fluid by the deformation is transformed in locomotion energy.

Figure 10. Time behaviour of total kinetic energy $T=T_{body}+T_{fluid}$ and partial contributions $T_{body}$ , $T_{fluid}$ for $m_b \neq 0$ , $h_o=0.1$ , $\theta _o=10^{\circ}$ , $\phi =-90^{\circ}$ .

Figure 11. Time behaviour of the separate contributions to the total kinetic energy appearing in (C3) for $m_b \neq 0$ , $h_o=0.1$ , $\theta _o=10^{\circ}$ , $\phi =-90^{\circ}$ . Here, $T_1 = (1/2) (m_b + m_{22}) (u_y + {\dot h})^2$ , $T_2 = (1/2) (I_{zz} + (9/8) m_{22} b^2) \dot \theta ^2$ , $T_3 = b \dot \theta m_{22}(u_y +\dot h )$ .

Here, we consider how the overall energy of the fluid is distributed between that of the fluid, $T_{fluid}$ given by (C2), and that of the body’s motion, $T_{body}$ given by (C1). When the surface of the body is periodically deformed due to the effect of some internal mechanism, the momentum of the body+fluid system changes and both these contributions are periodically oscillating in time. In the absence of shed vorticity, no energy is transferred to the wake, hence the total energy displays periodic oscillations with a constant non-zero mean value. On the contrary, in the presence of wake release, the mean value of the total energy increases with time. Each one of the above reported expressions is shown in figure 10 during one cycle.

In figure 11 we show the behaviour during one cycle of each one of the three parts of the total kinetic energy appearing in (C3). We notice that the first two terms are always positive, while the third one, representing the coupling between heave and pitch, has a negative mean value.

References

Akoz, E. & Moored, K.W. 2018 Unsteady propulsion by an intermittent swimming gait. J. Fluid Mech. 834, 149172.CrossRefGoogle Scholar
Alben, S., Witt, C., Baker, T.V., Anderson, E. & Lauder, G.V. 2012 Dynamics of freely swimming flexible foils. Phys. Fluids 24, 051901.10.1063/1.4709477CrossRefGoogle Scholar
Batchelor, G.K. 1991 An Introduction to Fluid Dynamics Cambridge University Press Google Scholar
Beal, D.N., Hover, F.S., Triantafyllou, M.S., Liao, J.C. & Lauder, G.V. 2006 Passive propulsion in vortex wakes. J. Fluid Mech. 549, 385402.10.1017/S0022112005007925CrossRefGoogle Scholar
Chambrion, T. & Munnier, A. 2011 Locomotion and control of a self-propelled shape-changing body in a fluid. J. Nonlinear Sci. 21, 325385.10.1007/s00332-010-9084-8CrossRefGoogle Scholar
Childress, S. 1981 Mechanics of Swimming and Flying. Cambridge University Press, Cambridge, USA.10.1017/CBO9780511569593CrossRefGoogle Scholar
Childress, S. & Dudley, R. 2004 Transition from ciliary to flapping mode in a swimming mollusc: flapping flight as a bifurcation in $Re_\omega$ . J. Fluid Mech. 498, 257288.CrossRefGoogle Scholar
Eldredge, J.D. 2019 Mathematical Modeling of Unsteady Inviscid Flows, vol. 50. Springer Intern. Publ., Cham, Switzerland.10.1007/978-3-030-18319-6CrossRefGoogle Scholar
Eldredge, J.D., Toomey, J. & Medina, A. 2010 On the roles of chord-wise flexibility in a flapping wing with hovering kinematics. J. Fluid Mech. 659, 94115.10.1017/S0022112010002363CrossRefGoogle Scholar
Hang, H., Heydari, S., Costello, J.H. & Kanso, E. 2022 Active tail flexion in concert with passive hydrodynamic forces improves swimming speed and efficiency. J. Fluid Mech. 932, A35.10.1017/jfm.2021.984CrossRefGoogle Scholar
Hatton, R.L. & Choset, H. 2010 Connection vector fields and optimized coordinates for swimming systems at low Reynolds numbers. In Proc. ASME 2010 Dynamic Systems and Control Confer. (DSCC 2010), ASME pp. 18.Google Scholar
Kanso, E. 2009 Swimming due to transverse shape deformations. J. Fluid Mech. 631, 127148.10.1017/S0022112009006806CrossRefGoogle Scholar
Kanso, E., Marsden, J.E., Rowley, C.W. & Melli-Huber, J.B. 2005 Locomotion of articulated bodies in a perfect fluid. J. Nonlinear Sci. 15, 255289.CrossRefGoogle Scholar
Kelly, S.D. & Murray, R.M. 2000 Modelling efficient pisciform swimming for control. Int. J. Robust Nonlinear Control 10, 217241.3.0.CO;2-X>CrossRefGoogle Scholar
Kelly, S.D. 1998 The mechanics and control of robotic locomotion with applications to aquatic vehicles PhD thesis. California Institute of Technology.Google Scholar
Lighthill, J. 1960 Note on the swimming of slender fish. J. Fluid Mech. 9 (2), 305317.10.1017/S0022112060001110CrossRefGoogle Scholar
Lighthill, J. 1969 Hydromechanics of aquatic animal propulsion: a survey. Annu. Rev. Fluid Mech. 1, 413446.10.1146/annurev.fl.01.010169.002213CrossRefGoogle Scholar
Limacher, E.J. 2019 Added mass and vortical impulse: theory and experiment PhD thesis. University of Calgary.Google Scholar
Limacher, E.J. 2021 Added-mass force on elliptic airfoils. J. Fluid Mech. 926, R2.10.1017/jfm.2021.741CrossRefGoogle Scholar
Lopez-Tello, P.E., Fernandez-Feria, R. & Sanmiguel-Rojas, E. 2023 Efficient self-propelled locomotion by an elastically supported rigid foil actuated by a torque. Appl. Mathem. Modell. 116, 236253.10.1016/j.apm.2022.11.007CrossRefGoogle Scholar
Mason, R. 2003 Fluid locomotion and trajectory planning for shape-changing robots PhD thesis. California Institute of Technology.Google Scholar
Melli, J.B., Rowley, C.W. & Rufat, D.S. 2006 Motion planning for an articulated body in a perfect planar fluid. SIAM J. Appl. Dyn. Syst. 5, 650669.10.1137/060649884CrossRefGoogle Scholar
Michelin, S. & Smith, S.G.L. 2009 Resonance and propulsion performance of a heaving flexible wing. Phys. Fluids 21, 071902.10.1063/1.3177356CrossRefGoogle Scholar
Miloh, T. & Galper, A. 1993 Self-propulsion of general deformable shapes in a perfect fluid. Proc. R. Soc. Lond. A 442, 273299.Google Scholar
Moore, M.N.J. 2014 Analytical results on the role of flexibility in flapping propulsion. J. Fluid Mech. 757, 559612.10.1017/jfm.2014.533CrossRefGoogle Scholar
Moore, M.N.J. 2015 Torsional spring is the optimal flexibility arrangement for thrust production of a flapping wing. Phys. Fluids 27, 091701.CrossRefGoogle Scholar
Moored, K.W. & Quinn, D.B. 2019 Inviscid scaling laws of a self-propelled pitching airfoil. AIAA J. 57 (9), 36863700.10.2514/1.J056634CrossRefGoogle Scholar
Newman, J.N. 2017 Marine Hydrodynamics. MIT Press, Cambridge, USA.Google Scholar
Paniccia, D., Graziani, G., Lugni, C. & Piva, R. 2021a On the role of added mass and vorticity release for self propelled aquatic locomotion. J. Fluid Mech. 918, A45.CrossRefGoogle Scholar
Paniccia, D., Graziani, G., Lugni, C. & Piva, R. 2021b The relevance of recoil and free swimming in aquatic locomotion. J. Fluids Struct. 103, 103290.10.1016/j.jfluidstructs.2021.103290CrossRefGoogle Scholar
Paniccia, D., Graziani, G., Lugni, C. & Piva, R. 2022 The fish ability to accelerate and suddenly turn in fast maneuvers. Sci. Rep. 12, 4946.10.1038/s41598-022-08923-5CrossRefGoogle ScholarPubMed
Paniccia, D., Padovani, L., Graziani, G. & Piva, R. 2021c The performance of a flapping foil for a self-propelled fishlike body. Sci. Rep. 11, 22297.10.1038/s41598-021-01730-4CrossRefGoogle ScholarPubMed
Paniccia, D., Padovani, L., Graziani, G. & Piva, R. 2023 Locomotion performance for oscillatory swimming in free mode. Bioinspir. Biomim. 18, 015004.10.1088/1748-3190/ac9fb4CrossRefGoogle Scholar
Paraz, F., Schouveiler, L. & Eloy, C. 2016 Thrust generation by a heaving flexible foil: resonance nonlinearities and optimality. Phys. Fluids 28, 011903.10.1063/1.4939499CrossRefGoogle Scholar
Purcell, E.M. 1977 Life at low Reynolds number. Am. J. Phy. 45 (1), 311.10.1119/1.10903CrossRefGoogle Scholar
Quinn, D.B. & Lauder, G.V. 2022 Tunable stiffness in fish robotics: mechanisms and advantages. Bioinspir. Biomim. 17, 011002.10.1088/1748-3190/ac3ca5CrossRefGoogle Scholar
Quinn, D.B., Lauder, G.V. & Smits, A.J. 2015 Maximizing the efficiency of a flexible propulsor using experimental optimization. J. Fluid Mech. 767, 430448.10.1017/jfm.2015.35CrossRefGoogle Scholar
Radford, J.E. 1998 Symmetry reduction and swimming in a perfect fluid PhD thesis. California Institute of Technology.Google Scholar
Ross, S.D. 2006 Optimal flapping strokes for self-propulsion in a perfect fluid. In Proc. American Control Confer. IEEE, ThC18.3, pp. 41184122 10.1109/ACC.2006.1657364CrossRefGoogle Scholar
Saffman, P.G. 1967 The self-propulsion of a deformable body in a perfect fluid. J. Fluid Mech. 28 (2), 385389.10.1017/S0022112067002149CrossRefGoogle Scholar
Saffman, P.G. 1992 Vortex Dynamics Cambridge University Press.Google Scholar
Smits, A.J. 2019 Undulatory and oscillatory swimming. J. Fluid Mech. 874, 170.10.1017/jfm.2019.284CrossRefGoogle Scholar
Spagnolie, S.E., Moret, L., Shelley, M.J. & Zhang, J. 2010 Surprising behaviors in flapping locomotion with passive pitching. Phys. Fluids 22 (4), 041903.10.1063/1.3383215CrossRefGoogle Scholar
Theodorsen, T. 1935 General theory of aerodynamic instability and the mechanism of flutter. Tech. Rep.Google Scholar
Toomey, J. & Eldredge, J. 2008 Numerical and experimental study of the fluid dynamics of a flapping wing with low order flexibility. Phys. Fluids 20 (7), 073603.10.1063/1.2956372CrossRefGoogle Scholar
Van Buren, T., Floryan, D. & Smits, A.J. 2018 Scaling and performance of simultaneously heaving and pitching foils. AIAA J. 57 (9), 112.Google Scholar
Vanella, M., Fitzgerald, T., Preidikman, S., Balaras, E. & Balachandran, B. 2009 Flapping wing structural deformation and thrust correlation study with flexible membrane wings. J. Exper. Biol. 212 (1), 95105.10.1242/jeb.016428CrossRefGoogle Scholar
Wan, H., Dong, H. & Huang, G.P. 2012 Hovering hinge-connected flapping plate with passive deflection. AIAA J. 50 (9), 20202026.10.2514/1.J051375CrossRefGoogle Scholar
Wu, T.Y. 1971 Hydromechanics of swimming propulsion. Part 1: swimming of 2D flexible plate at variable forward speed inviscid fluid. J. Fluid Mech. 46, 337355.10.1017/S0022112071000570CrossRefGoogle Scholar
Wu, T.Y. 1961 Swimming of a waving plate. J. Fluid Mech. 10 (3), 321344.10.1017/S0022112061000949CrossRefGoogle Scholar
Zhang, J., Liu, N.S. & Lu, X.Y. 2010 Locomotion of a passively flapping flat plate. J. Fluid Mech. 659, 4368.10.1017/S0022112010002387CrossRefGoogle Scholar
Zhong, Q., Zhu, J., Fish, F.E., Kerr, S.J., Downs, A.M., Bart-Smith, H. & Quinn, D.B. 2021 Tunable stiffness enables fast and efficient swimming in fish-like robots. Sci. Robot. 6, eabe4088.10.1126/scirobotics.abe4088CrossRefGoogle ScholarPubMed
Figure 0

Figure 1. Sketch of the virtual body with the flat plate attached through a torsional spring. The ground frame ($X\!-\!Y$) and the body-fixed one ($x\!-\!y$) are shown.

Figure 1

Figure 2. Time behaviour of (a) $F_X$ and $F_Y$ in the ground frame; (b) $F_x$ and $F_y$ in the body-fixed frame (the dashed line shows the mean value of $F_x$) for $h_o=0.1$ and $\theta _o = 10^\circ$.

Figure 2

Figure 3. Time evolution of the $X$-component of impulse, velocity and displacement for heave and pitch ($h_o = 0.1$; $\theta = 10^\circ$; $\phi = -\pi /2$). The horizontal dashed line represents the mean value of $U_X$.

Figure 3

Figure 4. Temporal evolution of $X$ displacement for heave ($h_o =0.1$) and pitch ($\theta = 10^\circ$) with several values of the phase shift.

Figure 4

Figure 5. Behaviour of the mean self-propulsion speed $U_s$ as a function of $K$ ($h_o =0.1$) for different values of the spring damping coefficient $C$: $C=0.1, 0.2, 0.5$ (a); $C=1, 2, 10.$ (b).

Figure 5

Figure 6. Pitch amplitude $\theta _o$ as a function of $K$ ($h_o =0.1$) for $C=0.1, 0.2, 0.5$ (a); $C=1, 2, 10.$ (b).

Figure 6

Figure 7. Phase angle variation as a function of $K$ ($h_o =0.1$): (a) $C=0.1, 0.2, 0.5$; (b) $C=1, 2, 10$.

Figure 7

Figure 8. (a) Variation of $\theta _o$ and $\phi$ as a function of frequency; (b) self-propulsion velocity ($h_o =0.1, k=4000, C=1$).

Figure 8

Figure 9. Stroke loops in the shape space for the frequencies selected in figure 8 ($h_o =0.1, k=4000, C=1$).

Figure 9

Figure 10. Time behaviour of total kinetic energy $T=T_{body}+T_{fluid}$ and partial contributions $T_{body}$, $T_{fluid}$ for $m_b \neq 0$, $h_o=0.1$, $\theta _o=10^{\circ}$, $\phi =-90^{\circ}$.

Figure 10

Figure 11. Time behaviour of the separate contributions to the total kinetic energy appearing in (C3) for $m_b \neq 0$, $h_o=0.1$, $\theta _o=10^{\circ}$, $\phi =-90^{\circ}$. Here, $T_1 = (1/2) (m_b + m_{22}) (u_y + {\dot h})^2$, $T_2 = (1/2) (I_{zz} + (9/8) m_{22} b^2) \dot \theta ^2$, $T_3 = b \dot \theta m_{22}(u_y +\dot h )$.