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Oscillation criteria for a class of third-order Emden–Fowler delay dynamic equations with sublinear neutral terms on time scales
Advances in Difference Equations volume 2021, Article number: 53 (2021)
Abstract
In this paper, we study the oscillation of a class of third-order Emden–Fowler delay dynamic equations with sublinear neutral terms on time scales. By using Riccati transformation and integral inequality, we establish several new theorems to ensure that each solution of the equation oscillates or asymptotically approaches zero, and the results in the literature are supplemented and extended. Examples are given to illustrate our main results.
1 Introduction
In this paper, we are concerned with the oscillation and asymptotic behavior of the third-order Emden–Fowler delay dynamic equation with sublinear neutral terms of the form
on a time scale \(\mathbb{T}\).
Throughout this paper, the following assumptions are tacitly satisfied:
(\(A_{1}\)) \(a(t), b(t), p(t)\in C_{rd}^{1}(\mathbb{T,\mathbb{R}})\), and \(b^{\Delta }(t)\geq 0\), \(0< p(t)\leq p<1\),
(\(A_{2}\)) \(\alpha, \beta, \gamma \) are quotients of odd positive integers, where \(\beta \geq \gamma \), \(0<\alpha \leq 1\);
(\(A_{3}\)) \(\delta (t), \tau (t)\in C_{rd}^{1}(\mathbb{T,\mathbb{R}})\) such that \(\tau (t)\leq t\), \(\delta (t)\leq t\), \(\lim_{t \to +\infty }\tau (t)=\lim_{t \to +\infty }\delta (t)= \infty \).
(\(A_{4}\)) \(f\in C(\mathbb{T}\times \mathbb{R}, \mathbb{R})\) is assumed that \(uf(t,u)>0\) for \(u\neq 0\), \(t\in \mathbb{T}\), and there exists a function \(q(t)\in C_{rd}^{1}(\mathbb{T,\mathbb{R}})\) such that \(\frac{f(t,u)}{u^{\beta }}\geq q(t)\) for \(u\neq 0\), \(t\in \mathbb{T}\).
For the basic theory and notation of calculus on the time scale \(\mathbb{T}\), we can see, for instance, the monograph [1], which systematically gives the definition of delta (or nabla) differentiation, the basic algorithm, and the important properties, such as the following:
Assume that \(f: \mathbb{T}\rightarrow \mathbb{R}\) is a function, and let \(t\in \mathbb{T}^{k}\). We define \(f^{\Delta }(t)\) to be the number, provided it exists, with the property that, for any \(\epsilon >0\), there exists a neighborhood U of \(t, U=(t-\delta,t+\delta )\cap \mathbb{T}\) for some \(\delta >0\) such that
We call \(f^{\Delta }(t)\) the \(delta\) or \(Hilger\) derivative of f at t. We say that f is \(delta\) or \(Hilger\) differentiable, shortly differentiable, in \(\mathbb{T}^{k} \) if \(f^{\Delta }(t)\) exists for all \(t\in \mathbb{T}^{k}\). The function \(f^{\Delta }:\mathbb{T}\rightarrow \mathbb{R}\) is said to be the \(delta\) derivative or \(Hilger\) derivative, shortly derivative, of f in \(\mathbb{T}^{k}\), where \(\sigma (t)=\inf \{s\in \mathbb{T}:s>t\}\) is called the forward jump operator. The properties of the delta (Δ) derivative and the knowledge of nabla (∇) derivatives can be found in the monograph [1], which is omitted here.
Since we are interested in oscillation and asymptotic behavior of solutions to equation, we assume that the time scale \(\mathbb{T}\) is unbounded. In this paper, we only consider those solutions of Eq. (1.1) which satisfy \(\sup \{|x(t)|: t\in [\mathbb{T}, \infty )_{\mathbb{T}}\}>0\) and assume that such solutions exist. A solution of (1.1), which is nontrivial for all large t, is said to be oscillatory if it is neither eventually positive nor eventually negative. Otherwise, it is called nonoscillatory.
The theory of dynamic equations on time scales not only unifies the theory of differential equations and difference equations, but it also extends these classical cases to cases “in between”, e.g., \(\mathbb{T}=q^{\mathbb{N}_{0}}\), \(\mathbb{T}=h\mathbb{Z}\), and other different time scales, which have wide application value in quantum theory, mathematical, theoretical, and chemical physics and ecology. Therefore, the study of the properties of dynamic equations on time scales has become a hot topic. In the past 20 years, there have been a lot of research results on the oscillation of dynamic equations. As a matter of fact, Eq. (1.1) is a natural generalization of the half-linear/Emden–Fowler dynamic equation (including related differential equation) which arises in a variety of real world problems such as in the study of p-Laplace equations, non-Newtonian fluid theory, the turbulent flow of a polytrophic gas in a porous medium, and so on; see, e.g., the papers [2–5] for more details. In this paper, our main purpose is to study the oscillation and asymptotic behavior of Eq. (1.1). In order to enlighten the research ideas, we briefly review the following research progress and important results of this problem.
Agarwal et al. [6] investigated the oscillation of a certain class of second-order differential equations with a sublinear neutral term
where \(0<\alpha <1\) is a ratio of odd positive integers.
Dzurina et al. [3], Grace and Graef [7], and Tamilvanan et al. [8] established sufficient conditions for the oscillation of all solutions of a nonlinear differential equation
where α and β are ratios of odd positive integers.
Agarwal et al. [9] and Erbe et al. [10] established several Hille and Nehari type criteria for the third-order dynamic equation
Agarwal et al. [11, 12], Han et al. [13], and Li et al. [14] considered the oscillatory behavior of the third-order dynamic equation
where \(\gamma >0\) is the ratio of positive odd integers, and proved the following results.
Theorem 1.1
Assume that \(\int _{t_{0}}^{\infty }p(t)(h_{2}(\tau (t),t_{0}))^{\gamma }\Delta t= \infty \) holds. Furthermore, suppose that there exists a positive function \(\delta (t)\in C_{rd}^{1}(\mathbb{T}, \mathbb{R})\) such that
where \(0< k<1\), \(\zeta (t)=(\frac{h_{2}(\tau (t),t_{0})}{\sigma (t)})^{\gamma }\). Then every solution \(x(t)\) of Eq. (1.6) is either oscillatory or \(\lim_{t\to \infty } x(t)=0\).
Yang [15] studied the oscillatory and asymptotic behavior of third-order nonlinear variable delay dynamic equations
where \(y(t)=x(t)+B(t)g(x(\tau (t)))\), \(\phi (u)=|u|^{\lambda -1}u\), \(\lambda >0\) is the ratio of positive odd integers, and got the following results.
Theorem 1.2
If there exists a function \(\delta (t)\in C_{rd}^{1}(\mathbb{T}, \mathbb{R})\) such that
where \(\Psi (t)= \frac{k[1-\beta B(\delta (t))]h_{2}(\delta (t),t_{0})}{2a(\delta (t))\sigma (t)}\), then every solution \(x(t)\) of Eq. (1.8) is either oscillatory or \(\lim_{t\to \infty } x(t)=0\).
Grace [16] was concerned with new oscillation criteria for third-order nonlinear difference equations with a nonlinear non-positive neutral term of the form
where α, γ, and β are the ratios of positive odd integers.
Candan [17] was concerned with oscillation of the third-order nonlinear neutral dynamic equation
where \(\gamma \geq 1\) is a ratio of odd positive integers.
It would also be interesting to establish sufficient conditions for the oscillation and asymptotic behavior of solutions to Eq. (1.1) for the other ranges of the neutral coefficient \(p(t)\) such as (1.10). For this research issue, see, e.g., the papers [18, 19] for more details.
It is not difficult to see that the results on the oscillation of delay dynamic (differential/difference) equations with sublinear neutral terms are mainly concentrated in the second order (see [3, 6–8] and the references cited therein), but the results of the third order are relatively lower [16, 20]. Numerous researchers have studied the special case of Eq. (1.1), see, e.g., Ref [9–30]. Inspired by the above papers, in this paper, by employing the Riccati transformation and some integral inequality, we present sufficient conditions to ensure that every solution of Eq. (1.1) is oscillatory or asymptotically converges to zero. Our results improve and generalize the results of the papers [13, 15].
2 Preliminaries
Before proving the main theorems, we need some useful lemmas which will be used later.
In [1], p. 190, Taylor’s monomials \({h_{n}(t,s)}_{n=0}^{\infty }\) are defined recursively by
It follows from [1] that \(h_{1}(t,s)=t-s\) for any time-scale, but simple formulas in general do not hold for \(n\geq 2\).
Lemma 2.1
([10])
If u satisfies \(u(t)>0, u^{\Delta }(t)>0, u^{\Delta \Delta }(t)>0, u^{\Delta \Delta \Delta }(t)<0, t \in [ t_{0},\infty )_{\mathbb{T}}\), then
Lemma 2.2
([10])
Set the following conditions to be established:
(1) \(u\in C_{rd}^{2}(\mathbb{I}, \mathbb{R})\), where \(\mathbb{I}=[t_{0}, \infty )_{\mathbb{T}}\),
(2) \(u(t)>0, u^{\Delta }(t)>0\), and \(u^{\Delta \Delta }(t)<0\), \(t\in \mathbb{I}\).
Then, for any \(k\in (0,1)\), there exists \(t_{1}\in \mathbb{I}\) such that, while \(t\in \mathbb{I}\) and \(t\geq t_{1}\),
Lemma 2.3
Keller’s chain rule
where \(z(t)\) is Δ-differentiable and eventually positive or eventually negative.
Its proof is not difficult from the monograph [1, Theorem 2.57], and so it is omitted here.
Lemma 2.4
Assume that \(A\geq 0\), \(B>0\), and \(\gamma >0\) are arbitrary real numbers. Then, for all \(X\geq 0\),
Proof
Let \(g(X)=AX-BX^{\frac{\gamma +1}{\gamma }}, X\in [0,\infty )\), \(A\geq 0\), \(B>0\), and \(\gamma >0\) be arbitrary real numbers and
We can obtain \(X^{*}= (\frac{A\gamma }{B(\gamma +1)} )^{\gamma }\), the unique solution to (2.5). It is clear that \(g'(X)>0\) for all \(X< X^{*}\) and \(g'(X)<0\) for all \(X>X^{*}\). Then \(g(X)\) attains its maximum value on \([0,\infty )\) at \(X^{*}\), and
Thus (2.4) holds, this completes the proof of the lemma.
It is obvious that Lemma 2.4 is an improvement of Lemma 2.3 in [31] about the constant \(\gamma >0\), which must be a ratio of two positive odd integers is no longer suitable for Eq. (1.1). □
3 Main results
Theorem 3.1
Assume that (1.2) holds. If there exists a positive function \(\eta (t)\in C_{rd}^{1}(\mathbb{T}, \mathbb{R})\) such that, for any constants \(L\in (0,1)\), \(M\in (0,1]\) (if \(\alpha =1\) have \(M=1\)), and sufficiently large \(t_{1}\geq t_{0}>0\),
and
hold, where
then every solution \(x(t)\) of Eq. (1.1) is either oscillatory or \(\lim_{t\to \infty } x(t)=0\).
Proof
Assume to the contrary that \(x(t)\) is an eventually positive solution of Eq. (1.1), that is, there exists \(t_{1}>t_{0}\) such that \(x(t)>0, x(\tau (t))>0, x(\delta (t))>0\) for all \(t\in [t_{1}, \infty )_{\mathbb{T}}\), \(t_{1}\in [t_{0},\infty )_{\mathbb{T}}\). Then \(z(t)\) has two possible cases:
(I) \(z(t)>0,z^{\Delta }(t)>0,(a(t)z^{\Delta }(t))^{\Delta }>0,(b(t)((a(t)z^{ \Delta }(t))^{\Delta })^{\gamma })^{\Delta }<0\);
(II) \(z(t)>0,z^{\Delta }(t)<0,(a(t)z^{\Delta }(t))^{\Delta }>0,(b(t)((a(t)z^{ \Delta }(t))^{\Delta })^{\gamma })^{\Delta }<0\).
If case (I) holds, then \(z(t)>0, z(\tau (t))>0, z(\delta (t))>0\) for all \(t>t_{1}\). Furthermore, in view of the fact that \(z(t)\) is monotonically increasing on \([t_{1},\infty )_{\mathbb{T}}\), there exists a positive constant \(M_{0}\) such that \(z(t)>M_{0}\), where \(M_{0}=\min \{z(t_{1}),1\}\in (0,1]\). According to the definition of \(z(t)\), we can easily get
From Eq. (1.1) and the above inequality, we have
Define the generalized Riccati transformation
Letting \(u(t)=a(t)z^{\Delta }(t)\), the above formula can be abbreviated as
Obviously \(\omega (t)>0\) for \(t\geq t_{1}\), and by the product rule and the quotient rule on time scales, we have
From (3.4), (3.6), and the definition of \(\omega (t)\), we can obtain
where
In view of the fact that \((b(t)(u^{\Delta }(t))^{\gamma })^{\Delta }\leq 0\), we have
Also \(b^{\Delta }(t)>0\), then, it is not hard for us to get \(u^{\Delta \Delta }(t)<0\) for \(t\geq t_{1}\). Further, we have
If \(\gamma >1\), by (3.9), we can get
where
Since \(z(t)\) is monotonically increasing on \([t_{1},\infty )_{\mathbb{T}}\), we get \(z(t_{1})< z(\tau (t))\) for \(t\geq t_{1}\). Also, since the definition of \(M_{0}\) and \(\beta \geq \gamma \), we have
and
In addition, since (3.8), we can easily get \(u(t)\), which satisfies Lemma 2.2, then there exists a constant \(k\in (0,1)\) such that
When letting \(\nu (t)=\int _{t_{1}}^{t} a(s)z^{\Delta }(s)\Delta s\), we can see that it satisfies Lemma 2.1. So there exists some \(t_{l}\in [t_{1}, \infty )_{\mathbb{T}}\) such that
for any \(t\in [t_{1}, \infty )_{\mathbb{T}}\) and for any \(l\in (0,1)\). Meanwhile, we can easily deduce \(a(t)z(t)>\int _{t_{1}}^{t} a(s)z^{\Delta }(s)\Delta s\), so
and then
for all \(t\geq t_{1}\). Substituting the above formula into (3.10), we conclude that
where \(L=M_{0}^{\beta -\gamma }(kl)^{\gamma }\in (0,1)\). Apply inequality (2.4) to \(P(t)\) with
which yields
Substituting the above formula into (3.15), we have
for all \(t\geq t_{1}\). Similarly, if \(0<\gamma <1\), it is easy for us to get (3.17). From inequality (3.17), we have
Integrating the above inequality from sufficiently large \(t_{1}\) to \(t\geq t_{1}\), we have
Take the limsup on both sides of the above inequality as \(t\rightarrow \infty \), which contradicts (3.1).
If case (II) holds, by \(z(t)>0\) and \(z^{\Delta }(t)<0\), we know that \(z(t)\) is decreasing and \(\lim_{t \to +\infty } z(t)=l\geq 0\). We assert that \(l=0\). If not, then \(l>0\). By the definition of limit, we pick \(0<\varepsilon <l^{2-\alpha }(1-p)/(\alpha p)\) and large enough \(t_{2}\in [t_{1},\infty )_{\mathbb{T}}\) such that \(l\leq z(t)\leq l+\varepsilon \) for all \(t\in [t_{2},\infty )_{\mathbb{T}}\). So that
where \(k=\frac{l-p(l+\varepsilon )^{\alpha }}{l+\varepsilon }>0\), and thus
Substituting it into Eq. (1.1), we obtain
Integrating the above formula from sufficiently large \(t\geq t_{2}\) to ∞ and noting that \(z^{\beta }(\tau (t))\geq l^{\beta }\), we have
and then
Integrating the above inequality from sufficiently large t to ∞, we have
Integrating the last inequality again from t to ∞, we can obtain
which contradicts (3.2), hence \(l=0\). The proof is completed. □
Corollary 3.2
The conclusion of Theorem 3.1remains intact if assumption (3.1) is replaced with two conditions
and
Remark 3.3
Obviously, the result of Theorem 3.1 is more extensive. When the corresponding coefficients of Eq. (1.1) are equal to those of Eq. (1.6) and Eq. (1.8), Eq. (1.1) can be simplified into Eq. (1.6) or (1.8). In this case, Theorem 1.1 or Theorem 1.2 can be completely included.
Remark 3.4
From Theorem 3.1, we can obtain different conditions for oscillation of Eq. (1.1) with different choices of \(\eta (t)\). For example, \(\eta (t)=t\) or \(\eta (t)=1\). Now, letting us consider \(\eta (t)=1\), we have the following corollary.
Corollary 3.5
Assume that (1.2) holds. If, for sufficiently large \(t_{1}\geq t_{0}>0\),
holds, where \(Q_{1}(t)=q(t) (1-\frac{p(\tau (t))}{M^{1-\alpha }} )^{ \beta }\), and M is the same as in Theorem 3.1, then every solution \(x(t)\) of Eq. (1.1) is either oscillatory or \(\lim_{t\to \infty } x(t)=0\).
The following theorem gives the Philos-type oscillation criterion for Eq. (1.1). First, let us introduce now the class of functions \(\mathfrak{H}\) which will be extensively used in the sequel.
Let \(\mathbb{D}=:\{(t,s):t\geq s \geq t_{0}\}\) and \(\mathbb{D}_{0}=:\{(t,s):t> s \geq t_{0}\}\). The function \(H\in C(\mathbb{D},\mathbb{R})\) is said to belong to the class \(\mathfrak{H}\) if it satisfies the following conditions:
\((H_{1})\) \(H(t,t)=0, t\in \mathbb{D}, H(t,s)>0, t\in \mathbb{D}_{0}\);
\((H_{2})\) \(H^{\Delta s}(t,t)=0, t\in \mathbb{D}, H^{\Delta s}(t,s) \leq 0, t\in \mathbb{D}_{0}\).
Theorem 3.6
Assume that (1.2) holds. Furthermore, suppose that there exist two positive functions \(\eta (t)\in C_{rd}^{1}(\mathbb{T}, \mathbb{R})\) and \(h(t,s)\in C_{rd}(\mathbb{D},\mathbb{R})\) satisfying conditions \((H_{1})\), \((H_{2})\), and
If, for sufficiently large \(t_{1}\geq t_{0}>0\),
holds, where \(K_{1}(t)=H(\sigma (t),\sigma (s))K(s)\) and \(K(t)\) is defined by \(( 3.1)\), then every solution \(x(t)\) of Eq. (1.1) is either oscillatory or \(\lim_{t\to \infty } x(t)=0\).
Proof
Assume to the contrary that \(x(t)\) is an eventually positive solution of Eq. (1.1), that is, there exists \(t_{1}>t_{0}\) such that \(x(t)>0, x(\tau (t))>0, x(\delta (t))>0\) for all \(t\in [t_{1}, \infty )_{\mathbb{T}}\). Then \(z(t)\) satisfies case (I) or (II). If case (I) holds, we process as in the proof of Theorem 3.1 and get (3.15) as follows:
Multiplying both sides of (3.23), with t replaced with s, by \(H(\sigma (t),\sigma (s))\), integrating with respect to s from \(t_{1}\) to \(t\geq t_{1}\), we have
Integrating by parts, we obtain
Using conditions \((H_{1})\)–\((H_{3})\) and inequality (2.4), we deduce that
this implies that
which contradicts condition (3.22).
If case (II) holds, then clearly \(\lim_{t\to \infty } x(t)=0\). The proof is completed. □
Remark 3.7
From Theorem 3.6, we can obtain different conditions for oscillation of all solutions of Eq. (1.1) with different choices of \(\eta (t)\) and \(H(t,s)\). For example, \(H(t,s)=(t-s)^{m} \) or \(H(t,s)=(\ln \frac{t+1}{s+1})^{m}\). Now, let us consider the function \(H(t,s)\) defined by
Hence we have the following Kamenev-type oscillation criterion for Eq. (1.1).
Corollary 3.8
Assume that (1.2) holds. Furthermore, suppose that there exist a positive function \(\eta (t)\in C_{rd}^{1}(\mathbb{T}, \mathbb{R})\) and a constant \(m\geq 1\) such that, for all sufficiently large \(t_{1}\geq t_{0}>0\),
holds, where \(K(t)\) is defined by \(( 3.1)\). Then every solution \(x(t)\) of Eq. (1.1) is either oscillatory or \(\lim_{t\to \infty } x(t)=0\).
Corollary 3.9
Assume that (1.2) holds. Furthermore, suppose that there exist two positive functions \(\eta (t)\in C_{rd}^{1}(\mathbb{T}, \mathbb{R})\) and \(r(t,s)\in C_{rd}(\mathbb{D},\mathbb{R})\) satisfying conditions \((H_{1})\), \((H_{2})\), and
If, for all sufficiently large \(t_{1}\geq t_{0}>0\),
holds, where \(K_{1}(t)\) is defined by \(( 3.22)\), then every solution \(x(t)\) of Eq. (1.1) is either oscillatory or \(\lim_{t\to \infty } x(t)=0\).
4 Application
In this section, we give an example to illustrate our main results of this paper.
Example 4.1
Consider a third-order neutral dynamic equation
where \(\lambda >0\) is a constant.
Here,
According to [1], when \(\mathbb{T}=\overline{2^{Z}}\),
Letting \(\eta (t)=1\), it is clear that conditions \((A_{1})\)–\((A_{4})\) and (1.2) hold. Next, we will prove that (3.21) is satisfied. It is the key to prove that the following
is true. Since, for any fixed \(M\in (0,1]\), we have
And obviously, when \(t>M^{-\frac{2}{3}}\), \(1-M^{-\frac{2}{3}}t^{-1}\geq \frac{1}{2} \) always holds. Therefore when \(4= t_{1}>2M^{-\frac{2}{3}}=t_{0}\), we have
holds and (4.2) is true. Thus, by Corollary 3.5, we know that every solution \(x(t)\) of (4.1) is either oscillatory or \(\lim_{t\to \infty } x(t)=0\).
Remark 4.2
As fairly noticed by the referees, it would be of interest to study Eq. (1.1) with nabla (∇) derivative or mixed delta (Δ)-nabla (∇) derivatives.
5 Conclusions
In this paper, we consider the oscillation and asymptotic behavior of a class of third-order Emden–Fowler delay dynamic equations with sublinear neutral terms on time scales. Under the conditions of \((A_{1})\)–\((A_{4})\), the above theorems and related corollaries are obtained, and the correctness of the conclusion is verified by an example.
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Acknowledgements
The authors would like to thank the referees for their useful suggestions.
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This project is supported by the National Sciences Foundation of China (11701528 and 11647034).
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Zhang, Z., Feng, R. Oscillation criteria for a class of third-order Emden–Fowler delay dynamic equations with sublinear neutral terms on time scales. Adv Differ Equ 2021, 53 (2021). https://doi.org/10.1186/s13662-021-03212-3
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DOI: https://doi.org/10.1186/s13662-021-03212-3
Keywords
- Time scale
- Oscillation
- Third-order
- Sublinear neutral term
- Emden–Fowler delay dynamic equation