Abstract
In this manuscript, based on the geometric singular perturbation theory, several new solitary wave solutions in a perturbed generalized Benjamin–Bona–Mahony (BBM) equation are detected by the explicit calculation of the associated Melnikov integrals. These solitary wave solutions are homoclinic to non-trivial steady states and have not been found before. We also determine the zeroth-order approximations to the speeds of these solitary waves explicitly. In the calculations of the Melnikov integrals, the explicit expressions of the unperturbed homoclinic orbits play an important role.
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Appendix
Appendix
1.1 The explicit expressions of homoclinic orbits for the unperturbed system (11)
Here, we only give the detailed derivation of the explicit expression of homoclinic orbit for the unperturbed system (11) when \(C\in (-\frac{4}{27}, 0)\). The other cases are similar and hence are omitted.
The homoclinic orbit in this case is determined by
where \(x=x_{3}\) is solved from \(x^3-x^2-C=0\), and \(x=x_{1}, x=x_{5}\) are determined by \(-\frac{1}{3}x^{3}+\frac{1}{4}x^{4}-Cx=h\) where \(-\frac{4}{27}<C<0\), \(h=u(x_{3})\).
If \(x>x_{3}\), let \(x-x_{3}=\frac{1}{u}>0\), we get
Then, setting \(x_{3}u+1-x_{1}u=v\) gives
Now let \(\sqrt{v}=w\), one obtains
i.e.,
where \(\sigma \) is a constant of integral.
Without loss of generality, let \(X_{5}(x_{5},0)\) be the initial point, that is, \(x(0)=x_{5}\), then
Denote
we obtain
Similarly, if \(x<x_{3}\), we can derive
1.2 The detailed calculations of the Melnikov integrals
Case 1 When \(C=0\).
In this case, the Melnikov integral is
where \(x(\tau )\) is given in (21).
Consider
we thus have
Here, \(x(\tau )=\frac{1}{\frac{3}{4}+\frac{\tau ^{2}}{6}}\), hence we have \(a=3/4\) and \(b=1/6\), and thus,
Case 2 When \(C=-\frac{2}{27}\).
The Melnikov integral is
in which
Denote \(\chi =\frac{\sqrt{6}}{3}\mathrm{sech}(\frac{\sqrt{3}}{3}\tau )\), then
Let
it follows from \(\mathrm{sech} p^{2}=1-\mathrm{tanh}p^{2}\) and \(d\mathrm{tanh}p=\mathrm{sech}p^{2}dp\) that
where \(p=\frac{\sqrt{3}}{3}\tau \), \(\eta =\sqrt{3}(\frac{\sqrt{6}}{3})^{k}\), which is equivalent to
where \(\mu =\mathrm{tanh}p\).
Let
which becomes
where \(\theta =\sin \gamma \). When \(m=0, 1, 2, 3, \cdots \), it can be calculated that
and when \(m=\frac{1}{2},\frac{3}{2},\frac{5}{2},\frac{7}{2}, \cdots \),
Obviously,
thus
and
which finally gives
Case 3 When \(C=-\frac{4}{27}\).
In this case, \(x(\tau )=\frac{2}{3}-\frac{1}{\frac{3}{4}+\frac{\tau ^{2}}{3}}\). Denote \(\chi (\tau )=\frac{1}{\frac{3}{4}+\frac{\tau ^{2}}{3}}\); direct calculation gives the Melnikov integral
By further calculation, we get
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Zhu, K., Wu, Y., Yu, Z. et al. New solitary wave solutions in a perturbed generalized BBM equation. Nonlinear Dyn 97, 2413–2423 (2019). https://doi.org/10.1007/s11071-019-05137-9
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DOI: https://doi.org/10.1007/s11071-019-05137-9