Abstract
For the extended Rayleigh problem of hydrodynamics stability dealing with homogeneous shear flows with variable cross section, we have obtained a parabolic instability region. This improved parabolic instability region intersects with the semicircular instability region under certain condition. The validity of the result is illustrated with an example of basic flows. Furthermore, we have obtained a bound for the complex part of the phase velocity.
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1 Introduction
The concept of inviscid incompressible shear flows in sea straits with variable cross section was first initiated by Pratt et al. (2000), a well-structured mathematical analysis of this problem was developed in Deng et al. (2003). An extended Taylor–Goldstein problem with respect to the variable topography that is applicable to sea straits was obtained in Deng et al. (2003). In the aforementioned studies, the density could be either a variable or a constant. In case of the density being the variable, it leads to the extended version of the Taylor–Goldstein problem of hydrodynamic stability. Whereas, the extended Rayleigh problem of hydrodynamic stability is attained, when the density is constant. It was observed that in many ways the general analytical results on the above said problems are varied. Specifically, the role of the curvature of the basis flow velocity plays a vital place in the homogeneous case but not so in the stratified case.
In this paper, the extended Rayleigh problem is taken for the study. Several analytical results associated with this problem have already been obtained in Pratt et al. (2000), Ganesh and Subbiah (2013), Subbiah and Ganesh (2010), Dou and Ganesh (2014), Jafer and Godo (2017) and Deng et al. (2003). Specifically, Subbiah and Ganesh (2007) derived a parabolic instability and it intersects with the semicircular instability region of Deng et al. (2003) for a class of basic flows. The functions \( f \)(z) and \( g \)(z) were defined in Subbiah and Ganesh (2007). The semicircular instability region of Deng et al. (2003) is reduced in Subbiah and Ganesh (2007) for the flows satisfying the conditions like \(f(z) < 0\) or \(g(z) > 0\). In this paper, we obtained an improved parabolic instability region.
Banerjee et al. (1988) has proved the parabolic instability region for the Rayleigh problem. This was taken deeper to extended Rayleigh problem by Subbiah and Ganesh (2007). Reenapriya and Ganesh (2015) extended the work and derived a parabolic instability region with the condition that \(U_{0\mathrm{min}}>0\). The parabolic instability region referred in Subbiah and Ganesh (2007) is dependent on conditions like \(f(z) < 0 \) or \(g(z) > 0\). Reenapriya and Ganesh (2015) have obtained a parabolic instability region which is valid for \( U_{0\mathrm{min}}>0\). Therefore, it is essential to improve the parabolic instability region for the extended Rayleigh problem that has none of the conditions as given in Subbiah and Ganesh (2007), Reenapriya and Ganesh (2015). The new parabolic instability region is a generalized instability region for both the Rayleigh problem and the extended Rayleigh problem. Also, we derived a bounds for complex part of the phase velocity.
2 Extended Rayleigh problem (Fig. 1)
We consider a channel with variable topography aligned in the \( x \)-direction and \(b(z)=y_{L}-y_{R}\) be the width of the channel, where \(y= y_{L}\) and \(y=y_{R}\) are the lateral positions of the side walls. The channel contains an incompressible, inviscid, homogeneous fluid flow for which the density \(\rho _{0}\)(constant), Pressure \( P \) and velocity \( \overrightarrow{u}=(u, v, w)\) are governed by Euler’s equations such as
and
where \(\frac{\mathrm{d}}{\mathrm{d}t} =\frac{\partial }{\partial t}+ u\frac{\partial p}{\partial x}+w\frac{\partial }{\partial z}\) is the Eulerian derivative.
Integrating \(\nabla .\overrightarrow{u}=0,\) across the channel and applying the boundary conditions at the walls, we have
where \(T(z) = \frac{1}{b(z)} \frac{\mathrm{d}b(z)}{\mathrm{d}z} = \frac{b^{'}}{b}=\frac{\mathrm{d}(logz)}{\mathrm{d}z}\) is the topography.
Let the basic flow be given by the velocity (U(z), 0, 0) and Pressure \(P=P_{0}\) (constant)and the perturbed state is given by velocity field \((U_{0}(z)+u,v,w)\) and the Pressure \(P=P_{0}+P\).
After linearizing the equation of motions, we have
By applying the normal mode disturbances \((u,w,P,\rho )=({\hat{u}},{\hat{w}},{\hat{P}},{\hat{\rho }})e^{ik(x-ct)}\) in the above equations and omitting the hat sign we have
Eliminating all variables except w from the above equations we obtained the extended Rayleigh problem (cf. Deng et al. (2003)), given by
with boundary conditions
Here W is the complex eigen function(note we have used W(z) instead of \( w \)(z) for convention), \(k > 0\) is the wave number, \( c=c_{r}+ic_{i}\) is the complex phase velocity, \(U_{0}\) is the basic velocity profile, b(z) is the breadth function.
For unstable models \(c_{i}>0 \) and so \((U_{0}-c)^\frac{1}{2}\) is well defined.
Introducing the transformation \(W=(U_{0}-c)^{1/2}G\), we can get the equation satisfied by G to be
with boundary conditions
3 Instability regions
Theorem 3.1
The following integral relations are valid when the imaginary part of the complex phase velocity \(c_{i}\) is strictly greater than zero and by considering \( U_{0s}\) as an arbitrary real number.
-
(i)
$$\begin{aligned}&\int (U_{0}-c_{r}) Q \mathrm{d}z+\frac{1}{2}\int b\left( \frac{U_{0}'}{b}\right) 'b |G|^{2} \mathrm{d}z +\int \frac{\frac{(U_{0}')^{2}}{4}}{|U_{0}-c|^{2}}(U_{0}-U_{0s})b |G|^{2} \mathrm{d}z \\&\quad -\,(c_{r}-U_{0s})\int \frac{\frac{(U_{0}')^{2}}{4}}{|U_{0}-c|^{2}} b |G|^{2} \mathrm{d}z =0, \end{aligned}$$
-
(ii)
$$\begin{aligned} -c_{i} \int Q \mathrm{d}z+c_{i}\int \frac{\frac{(U_{0}')^{2}}{4}}{|U_{0}-c|^{2}} b |G|^{2} \mathrm{d}z =0. \end{aligned}$$
Proof
Multiplying (3) by \((bG^{*})\), where * stands for complex conjugation; integrating over [0,D] and using (4), we get
Let \(Q=\frac{|(bG)'|^{2}}{b}+ k^{2}b|G|^{2}\) then the aforementioned equation becomes
The real part of the Eq. (6) is given by
Rewriting \((U_{0}-c_{r})\) as \((U_{0}-U_{0s})-(c_{r}-U_{0s})\), where \(U_{0s}\) is an arbitrary real number, we get
The imaginary part of the Eq. (6) is given by
Thus we arrive with the results of Theorem 3.1.
Theorem 3.2
For the existence of unstable mode, the following integral relation is true
Proof
The real part of Eq. (5) is given by
The imaginary part of Eq. (5) is given by
Multiplying the Eq. (10) by \(\left( \frac{c_{r}+U_{0s}}{c_{i}}\right) \) and subtracting from (9), we get
Multiplying the Eq. (10) by \(\left( \frac{U_{0\mathrm{max}}-U_{0\mathrm{min}}}{2c_{i}}\right) \) and adding the resultant with (9), we get
Since
dropping the term, we get
Hence the Theorem 3.2 is proved.
Theorem 3.3
An essential condition for the existence of unstable mode is
Proof
Substituting the Eq. (12) in (11), we get
Since
and using Rayleigh–Ritz inequality,
Substituting \( U_{0s}=\frac{U_{0\mathrm{max}}+U_{0\mathrm{min}}}{2}\) in the above equation we get
where
Theorem 3.4
If \(\lambda < \lambda _{c}\)
where
then the parabola
intersects the semicircle
Proof
The semi-circle given in Deng et al. (2003) is
Substituting (13) in (14), we get
It’s discriminant part is given by
Solving for \(\lambda ,\) we get
If \( \lambda <\lambda _{c}\), \(\lambda _{c}=(U_{0 \mathrm{min}}+3U_{0 \mathrm{max}})-2\sqrt{2U_{0 \mathrm{max}}(U_{0 \mathrm{max}}+U_{0\mathrm{min}})}\),
then the parabola will intersects the semicircle.
Remark
If \(U_{0}=constant\) then by semicircle theorem, the flow is stable. If \(U_{0}\ne constant\) and \(U_{0 \mathrm{min}}=0\), then the above instability region is valid. Moreover, if \(U_{0}\) changes its sign then \(\left| \frac{(3U_0 \mathrm{min}+U_{0 \mathrm{max}})}{2}\right| > 0\) and the region is valid. Now we shall illustrate the applicability of our results for an example of basic flow.
Example
\( U_{0}=z-\frac{1}{2}\), \(0\le z\le 1\). In this case \(U_{0 \mathrm{min}} = -\frac{1}{2}\), \(U_{0\mathrm{max}} = \frac{1}{2}\). Our result is valid for this case (Fig. 2).
Theorem 3.5
If \(c_{i}>0 \) then we have the integral relation
Proof
The extended Rayleigh problem is given by
with boundary conditions
Multiplying (15) by \( W^{*}\), integrating over [0, D] and using (16), we get
since \(\hbox {Re}\int TW'W^{*}\mathrm{d}z=-\frac{1}{2}\int T'\left| W\right| ^{2}\mathrm{d}z\) and taking real and imaginary part, we get
and
Multiplying (18) by \(\frac{c_{r}-U_{0s}}{c_{i}}\) and adding to (17),we get
Theorem 3.6
If \(c_{i}>0 \) then we have the following integral relation
Proof
Multiplying (1) by \([\frac{(bW^{*})'}{b}]'\) and integrating over [0,D] and using (2), we get
From (1),
Substituting (21) in (20), we get
Equating the real part, we get
Theorem 3.7
If \(T'\le 0\) and \(c_{r}=U_{0s}\) then bounds for \(c_{i}\) is given by
Proof
Multiplying (18) by \(\frac{\left( c_{r}-U_{0s}\right) }{c_{i}}2k^{2}\) and subtracting from (22), we get
Multiplying (19) by \(k^{2}\) and adding to (23), we get
If \( T'\le 0, c_{r}=U_{0S}\) and using Rayleigh -Ritz inequality, we get
Since
4 Concluding remarks
For the extended Rayleigh problem of hydrodynamic stability, we have obtained a parabolic instability region. The parabolic instability region is an unbounded region it will be important only if the parabolic instability region intersects the semicircular instability region. Hence, we have proved that the parabolic instability region which intersects the semicircular instability region under some conditions. We have illustrated the validity of our results for a basic flow. Unlike the previous parabolic instability regions, our new parabolic instability region does not depend on any conditions. When b = constant or \(T=0\), we can get the instability region for standard Rayleigh problem. Hence, our parabolic instability region is also true for standard Rayleigh problem. Also, we have derived a bound for the complex part of phase velocity.
References
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Communicated by Corina Giurgea.
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Reena Priya, K., Ganesh, V. An improved instability region for the extended Rayleigh problem of hydrodynamic stability. Comp. Appl. Math. 38, 79 (2019). https://doi.org/10.1007/s40314-019-0848-y
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DOI: https://doi.org/10.1007/s40314-019-0848-y