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2015, No. 19, 1–15;

http://www.math.u-szeged.hu/ejqtde/

Nonoscillation of higher order half-linear differential equations

Ondˇrej Došlý

B

and Vojtˇech R ˚užiˇcka

Department of Mathematics and Statistics, Masaryk University, Kotláˇrská 2, CZ-611 37 Brno, Czech Republic

Received 7 November 2014, appeared 25 March 2015 Communicated by Michal Feˇckan

Abstract. We establish nonoscillation criteria for even order half-linear differential equations. The principal tool we use is the Wirtinger type inequality combined with various perturbation techniques. Our results extend nonoscillation criteria known for linear higher order differential equations.

Keywords: even-order half-linear differential equation, Wirtinger inequality, nonoscil- lation, half-linear Euler equation.

2010 Mathematics Subject Classification: 34C10.

1 Introduction

In this paper we deal with the even order half-linear differential equation

n k=0

(−1)krk(t)Φ y(k)(k)

=0 (1.1)

where Φ(y) = |y|p2y, p > 1, is the odd power function, rj are continuous functions, j = 0, . . . ,n, and rn(t) > 0 in the interval under consideration. The terminology half-linear equation was introduced by I. Bihari [3] and reflects the fact that the solution space of (1.1) is homogeneous, but not additive, i.e., it has just one half of the properties characterizing linearity. In the case n = 1, equation (1.1) reduces to the classical second order half-linear differential equation

− r1(t)Φ(x0)0+r0(t)Φ(x) =0 (1.2) whose oscillation theory is relatively deeply developed, see [1,16] and e.g. the recent papers [11,13,17,19,24,27,28].

The theory of (1.1) is much less developed and as far as we known only [16, Sec. 9.4] and the paper [25] deal with this problem. The reason is that we miss the so-called Reid’s round- about theorem in the higher order case, in particular, the Riccati technique is not available for

BCorresponding author. Email: dosly@math.muni.cz

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(1.1), in contrast to (1.2). Actually, necessary and sufficient conditions for (non)oscillation of (1.1) with p = 2, i.e., in the linear case, follow from the fact that this equation can be writ- ten as a linear Hamiltonian system (for which the Reid’s roundabout theorem is well known, [26, Chap. V., Theorem 6.3]) and this enables to present oscillation and spectral theory of (1.1) withp=2 as it is exhibited e.g. in the book [22], see also [20] and the references given therein.

The energy functional associated with (1.1) considered on the interval[T,∞)is Fn(y) =

Z

T

"

n k=0

rk(t)|y(k)|p

#

dt (1.3)

(equation (1.1) is the Euler–Lagrange equation of (1.3)). If there exists a nontrivial solution ˜y of (1.1) with two zeros of multiplicitynin[T,∞), i.e.,

(i)(t1) =0= y˜(i)(t2), i=0, . . . ,n−1, (1.4) for someT≤t1<t2, then we define the function

y(t) =

(y˜(t), t∈[t1,t2]

0 t∈[T,∞)\[t1,t2],

and obviously y ∈ W0n,p[T,∞) (the definition of this Sobolev space will be recalled later).

Multiplying (1.1) by y and integrating by parts over [T,∞) gives Fn(y) = 0. Hence, if we show thatFn(y)>0 for all nontrivial functions y∈W0n,p[T,∞), we eliminate the existence of a solution of (1.1) satisfying (1.4) for somet1,t2 ∈[T,∞).

The paper is organized as follows. In the next section we concentrate our attention on basic properties of the higher order half-linear Euler differential equation and on the so-called Wirtinger inequality which is the principal tool in our investigation. Section 3 is devoted to nonoscillation criteria for Euler type even order differential equation. Section 4 deals with nonoscillation criteria for general two-term 2nth order half-linear differential equations and in the last section we present some remarks and comments concerning possible further inves- tigation.

2 Preliminaries and Euler equation

The higher order Euler type half-linear differential equation is the equation

(−1)n tαΦ(y(n))(n)+ (−1)n1βn1 tαpΦ(y(n1))(n1)+· · ·+β0tαnpΦ(y) =0, (2.1) where α, βi, i = 0, . . . ,n−1, are real constants. Moreover, it is supposed that α 6∈ {p−1, 2p−1, . . . ,np−1}(this restriction will be explained later).

The “classical” Euler second order half-linear differential equation is the equation

Φ(x0)0+ γ

tpΦ(x) =0. (2.2)

This equation and its various perturbations were studied in detail in [18] and also in [11,13,14,17,24,27]. It is known that the classical linear Sturmian oscillation theory extends almost verbatim to (1.2). Elbert [18] showed that (2.2) is oscillatory if and only if γ < −γp,

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γp := pp1p. In the critical caseγ =−γp, equation (1.2) has a solution x(t) = t

p1

p as can be verified by a direct computation.

Concerning equation (2.1), similarly to the linear case, we look for a solution in the form x(t) =tλ. Consider first the two-term equation

(−1)n tαΦ(x(n))(n)+γtαnpΦ(x) =0, (2.3) with α6∈ {p−1, . . . ,np−1}andγR. Substituting into (2.3) we find thatλmust be a root of the algebraic equationG(λ) +γ=0 with

G(λ) = (−1)nΦ λ(λ−1)· · ·(λ−n+1)(p−1)(λ−n) +α

· · ·(p−1)(λ−n) +α−n+1 . Next we show that the function G has a stationary point λ = npp1α. We have the equality Φ0(x) = (p−1)Φ(xx), therefore, by a direct calculation we obtain that for λ 6= j,n− αp1j, j=0, . . . ,n−1,

G0(λ) = (−1)n(p−1)G(λ) 1

λ+ 1

λ−1+· · ·+ 1

λ−(n−1)+ 1

(p−1)(λ−n) +α

+ 1

(p−1)(λ−n) +α−1+· · ·+ 1

(p−1)(λ−n) +α−(n−1)

. Because

1

λ−k =− 1

(p−1)(λ−n) +α−(n−1−k) for each k∈ {0, . . . ,n−1}, we have

G0(λ) =0.

Substituting the valueλ intoGgives the value of the so-calledcritical constantin the 2nth order Euler half-linear differential equation (2.3). We denote

γn,p,α :=G(λ) =

n j=1

|jp−1−α| p

p

.

The previous computation shows that the equation G(λ)−γn,p,α = 0 has a double root λ =

np1α

p .

The terminology critical constant is used by analogy with the linear case where its value is a “borderline” between oscillation and nonoscillation of equation (2.3) with p=2. In the half- linear case, we are able to prove only “one half” of conditions for an oscillation constant yet, namely that (2.3) is nonoscillatory forγ > −γn,p,α. The proof of an “oscillation counterpart”

resists our effort till now, nevertheless, it is a subject of the present investigation. More details about this problem are given in the last section.

Therefore, (2.3) withγ=−γn,p,α has a solutionx(t) =tλ. Note that linearly independent solutions cannot be computed explicitly even in the case n = 1 and α = 0 (i.e., for second order equation (2.2) withγ = −γp, because γp = γ1,p,0). Nevertheless, as shown in [18], any solution of (2.2) withγ=−γp, which is linearly independent of x(t) =tp

1

p is asymptotically equivalent to the function ˜x(t) =Ctp

1

p log2p t, 0 6= C∈ R. It is an open problem whether the function ˜x(t) =tnp

1α

p log2p t is also an “approximate” solution of the equation

(−1)n tαΦ(x(n))(n)γn,p,αtαnpΦ(x) =0, (2.4)

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since if p=2 in (2.4) then ˜x(t) =t2n21αlogt is a solution of this equation.

Now we recall the definition of the Sobolev space, consisting of functions with a compact support. We denote forT∈R

W0n,p[T,∞) =

y: [T,∞)→R|y(n1) ∈ AC[T,∞), y(n) ∈ Lp(T,∞), y(i)(T) =0 fori=0, 1, . . . ,n−1 and there exists T1> T such thaty(t) =0 fort ≥T1

,

whereAC[T,∞)is the set of absolutely continuous functions with the domain[T,∞).

We finish this section with a half-linear version of the classical Wirtinger inequality, which we use in the next sections. Its proof in the formulation presented here can be found in [7].

Lemma 2.1. Let M be a positive continuously differentiable function for which M0(t) 6= 0in[T,∞) and let y∈W01,p[T,∞). Then

Z

T

|M0(t)||y|pdt≤ pp Z

T

Mp

|M0(t)|p1|y0|pdt. (2.5)

3 Euler equation

Following the linear terminology, we say that (1.1) is nonoscillatoryif there exists T ∈ Rsuch that no solution of this equation has two or more zeros of multiplicity n in [T,∞). In the opposite case, i.e., when for everyT∈Rthere exists a nontrivial solution of (1.1) with at least two zeros of multiplicitynin[T,∞), then (1.1) is said to beoscillatory.

We start this section with a variational lemma which plays the fundamental role in our treatment, for its proof (whose outline we have already presented below (1.3)) see [16, Sec. 9.4].

Lemma 3.1. Equation(1.1)is nonoscillatory if there exists T∈Rsuch that Fn(y)>0

for every06≡y∈W0n,p[T,∞).

The first statement of this section is a nonoscillation criterion which is essentially proved in [16, Theorem 9.4.5]. This criterion is formulated in [16] for the equation

(−1)n Φ(x(n))(n)+ γ

tnpΦ(x) =0, (3.1)

but a small modification of the proof (via Wirtinger inequality) shows that it can be extended to a more general equation (2.3).

Theorem 3.2. Suppose thatα6∈ {p−1, . . . ,np−1}. If γn,p,α+γ>0, γn,p,α =

n j=1

|jp−1−α| p

p

, then(2.3)is nonoscillatory.

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Proof. The proof is based on the application of the inequality Z

T tα|y(n)|pdt≥γn,p,α

Z

T tαnp|y|pdt (3.2)

for y ∈ W0n,p[T,∞), which is obtained by repeated application of the following Wirtinger inequality

Z

T tβ|x0|pdt≥

|p−1−β| p

pZ

T tβp|x|pdt, x∈W01,p[T,∞) (3.3) forβ=α,α−p,α−2p, . . . ,α−(n−1)pand forx0 =y(n),y(n1), . . . ,y0respectively. Inequality (3.3) follows from inequality (2.5) in Lemma 2.1 by taking M(t) = (|p−1−β|)p1tβp+1 for β6= p−1. Then for anyy∈W0n,p[T,∞)such thaty6≡0 we have

Fn(y) =

Z

T tα|y(n)|pdt+γ Z

T tαnp|y|pdt

≥(γn,p,α+γ)

Z

T tαnp|y|pdt>0, what we needed to prove, due to Lemma3.1.

Note that the same statement (forα = 0) is proved via the weighted Hardy inequality in [25], we will mention this result later in our paper.

Now we turn our attention to the “full term” 2nth order Euler differential equation.

(−1)n tαΦ(y(n))(n)+ (−1)n1βn1 tαpΦ(y(n1))(n1)+· · ·+β0tαnpΦ(y) =0, (3.4) with α6∈ {p−1, 2p−1, . . . ,np−1}.

Theorem 3.3. Suppose that α6∈ {p−1, . . . ,np−1}and

n1 k

=0

nk

j=1

|(k+j)p−1−α| p

p

βnk+β0 >0, βn :=1, then equation(3.4)is nonoscillatory.

Proof. We apply the Wirtinger inequality to each term (except that one fork =n) in the energy functional

Fn(y) =

Z

T

n k=0

tαkp|y(nk)|p

! dt.

We obtain for any y∈W0n,p[T,∞)and fork =0, . . . ,n−1 Z

T tαpk|y(nk)|pdt≥

nk

j=1

|(k+j)p−1α| p

pZ

T tαnp|y|pdt.

Then we have Fn(y)≥

"

n1 k

=0

nk

j=1

|(k+j)p−1−α| p

p

βnk+β0

# Z

T tαnp|y|pdt>0 for any nontrivialy∈W0n,p[T,∞).

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Remark 3.4. The reason why the caseα∈ {p−1, . . . ,np−1}we needed to exclude from the previous considerations is the following. For α = p−1 the Wirtinger inequality takes the form

Z

T tp1|y0|pdt≥

p−1 p

pZ

T

1

tlogpt|y|pdt, (3.5) so, a logarithmic term appears. This more difficult case is treated in the next part of this section.

We start with an auxiliary statement.

Lemma 3.5. Letα= jp−1for some j∈ {1, . . . ,n}. Then, we have for any y ∈W0n,p[T,∞)

Z

T

tα|y(n)|pdt≥ [(n−j)!(j−1)!]p γnpj1

Z

T

1+O(log1t) t(nj)p+1logpt|y|pdt.

Proof. First we make some auxiliary computations. Integration by parts gives forl∈Nandq the conjugate exponent ofp, i.e., 1p +1q =1,

Z

tlq1logqt dt= t

lq

lq logqt−1 l

Z

tlq1logq1t dt

= t

lq

lq logqth

1+O(log1t)i

ast→∞. This integral we use in establishing the inequality forz∈W01,p[T,∞)

Z

T

|z0|p

tl p+1logptdt≥ (l+1)p γp

Z

T

1+O(log1t)

t(l+1)p+1logpt|z|pdt. (3.6) We prove (3.6) as follows. Letr(t)>0 be a continuous function withR

r1q(t)dt=∞, then we have the inequality

Z

T r(t)|y0|pdt≥γp Z

T

r1q(t) Rt

T0r1q(s)dsp|y|pdt, T0 <T, (3.7) which follows from (3.3) with β = 0. Indeed, lets = Rt

T0r1q(τ)dτ, i.e., dtd = r1q(t)dsd, then (3.7) is the same as

Z

S

|y˙|pds≥γp Z

S

|y|p

sp ds, ˙= d

ds, S=

Z T

T0

r1q(τ)dτ.

Forr(t) =tl p1logptwe haver1q(t) =t(l+1)q1logqt, hence Z t

r1q(s)ds= t

(l+1)q

(l+1)qlogqt

1+O(log1t) ast→∞. Therefore

r1q(t) Rt

r1q(s)dsp =t(l+1)q1logqt t(l+1)q (l+1)qlogqt

!p

1+O(log1t)p

= (l+1)p γp

1 t(l+1)p+1logpt

1+O(log1t).

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Substituting these computations into (3.7) we obtain (3.6).

Lety∈W0n,p[T,∞). Applying inequalities (3.5) and (3.6), we obtain Z

T tα|y(n)|pdt=

Z

T tjp1|y(n)|pdt≥[(j−1)!]p

Z

T tp1|y(nj+1)|pdt

≥[(j−1)!]pγp

Z

T

1

tlogpt|y(nj)|pdt

≥ [(n−j)!(j−1)!]p γnpj1

Z

T

1+O(log1t) t(nj)p+1logpt|y|pdt.

The proof is complete.

Now we are ready to deal with the caseα∈ {p−1, 2p−1, . . . ,np−1}. Theorem 3.6. Letα=jp−1for some j ∈ {1, . . . ,n}and consider the equation

(−1)n tjp1Φ(y(n))(n)+

j1 i

=1

(−1)niβni

t(ji)p1Φ(y(ni)(ni)

+

nj1

i=0

(−1)njiβnji Φ(y(nji) tip+1logpt

!(nji)

+β0 Φ(y)

t(nj)p+1logpt =0.

(3.8)

If

L:= [(j−1)!(n−j)!]p γnpj1

+

j1 i

=1

βni

[(j−i−1)!(n−j)!]p γnpj1

+

nj1 i

=0

βnji[(i+1)· · ·(n−j)]p γnpji

+β0>0

(3.9)

then equation(3.8)is nonoscillatory.

Proof. The energy functional corresponding to (3.8) is Fn(y) =

Z

T

"

tjp1|y(n)|p+

j1 i

=1

βnit(ji)p1|y(ni)|p

+

nj1 i

=0

βnji|y(nji)|p

tip+1logpt +β0 |y|p t(nj)p+1logpt

# dt

The first term in the integral is estimated in Lemma3.5. Concerning the terms under summa- tion signs, fori=0, . . . ,j−1

Z

T t(ji)p1|y(ni)|pdt≥ [(j−i−1)!(n−j)!]p γnpj1

Z

T

1+O(log1t) t(nj)p+1logpt|y|pdt and fori=0, . . . ,n−j−1

Z

T

|y(nji)|p

tip+1logptdt≥ [(i+1). . .(n−j)]p γnpji

Z

T

1+O(log1t) t(nj)p+1logpt|y|pdt.

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Substituting these computations intoFn(y), we have Fn(y) =

Z

T

|y|p

t(nj)p+1logpt dt

×

"

L+

Z

T

O(log1t)

t(nj)p+1logpt|y|pdt

!Z

T

|y|p

t(nj)p+1logpt dt 1#

.

Since the second term in the bracket tends to zero as T → ∞, we have Fn(y;T,∞) > 0 for T sufficiently large if (3.9) holds, which means that equation (3.8) is nonocillatory by Lemma3.1.

4 General nonoscillation criteria

We start with two nonoscillation criteria from [25] (proved in [25] via the weighted Hardy in- equality) which we later compare with our results. Both criteria are contained in the following theorem.

Theorem 4.1. Suppose that c(t)≤0for large t and q is the conjugate exponent of p, i.e., 1p+ 1q =1.

If one of the following conditions

Tliminf

t>T

Z t

T r1q(s)ds

p1Z

t c(s)(s−T)(n1)pds>−[(n−1)!]p

p−1 γp (4.1) or

Tliminf

t>T

Z t

T r1q(s)ds

1Z t

T c(s)(s−T)(n1)p Z s

T r1q(u)du p

ds>−γp[(n−1)!]p, (4.2) holds, then the two-term differential equation

(−1)n r(t)Φ(y(n))(n)+c(t)Φ(y) =0 (4.3) is nonoscillatory.

In the next theorem we present a Hille–Nehari type nonoscillation criterion for (4.3) with r(t) = tα. This criterion extends the linear result given in [10]. We will need the following auxiliary statement, its proof can be found e.g. in [6].

Lemma 4.2. Let m∈ {0, . . . ,n−1}, then we have y(n)=

(1 t

tm+1y tm

0(m))(nm1)

. Theorem 4.3. Suppose that α 6∈ {p−1, . . . ,np−1}, R

c(t)t(nj)pdt > −∞, where c(t) = min{0,c(t)}is the negative part of c, and

lim inf

t tjp1α Z

t c(s)s(nj)pds> − γn,p,α

|jp−1−α| (4.4)

for some j∈ {1, . . . ,n}. Then the equation

(−1)n tαΦ(x(n))(n)+c(t)Φ(x) =0, (4.5) is nonoscillatory.

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Proof. LetT∈ Rbe so large, that the limited expression in (4.4) is greater than

γn,p,α

|jp−1−α|+ε=:K,

where ε > 0 is sufficiently small. Then for any 0 6≡ y ∈ W0n,p[T,∞) we have with z = y/tnj (using the inequality∫abf g≤ ∫ab|f|p1/pab|g|q1/qbetween the fourth and fifth line and (3.3) (with β = α−(j−1)p and x0 = z0) between the fifth and sixth line in the next computation)

Z

T c(t)|y|pdt≥

Z

T c(t)t(nj)p

y tnj

pdt= p Z

T c(t)t(nj)p Z t

T Φ(z)z0ds

dt

= p Z

T Φ(z)z0 1

tjp1αtjp1α Z

t c(s)s(nj)pds

dt

≥ p Z

T

|Φ(z)| |z0|

tjp1α tjp1α Z

t c(s)s(nj)pds

dt

> pK

Z

T

|Φ(z)|

tjp

α q

· |z0| tjp

α

q +jp1α

dt= pK Z

T

|Φ(z)|

tjp

α q

· |z0| t

(j1)pα q

dt

≥ pK Z

T

|z|p tjpα dt

1qZ

T

|z0|p t(j1)pα dt

1p

≥ pK

p

|jp−1−α|

pq Z

T

|z0|p t(j1)pα dt

1q Z

T

|z0|p t(j1)pα dt

1p

= pK

p

|jp−1−α|

p1Z

T

|z0|p t(j1)pα dt.

In the previous computation, we have used the equality |z(t)|p = pRt

TΦ(z(s))z0(s)ds, which follows from the formula |z|p0 = (z)z0 and from the definition of z (z(T) =0). We have also used the relation|Φ(z)|q=|z|p.

Now, we apply Lemma4.2withm=n−j, i.e.,n−m−1= j−1, and we denote v= 1

t

tnj+1 y tnj

0(nj)

, u=tnj+1 y tnj

0

.

Then, using Wirtinger inequality (3.2) (in a slightly modified form), we get fory∈W0n,p[T,∞)

Z

T tα|y(n)|p =

Z

T tα

(1 t

tnj+1 y tnj

0(nj))(j1)

p

dt

=

Z

T tα|v(j1)|pdt≥

j1

i=1

|ip−1−α| p

pZ

T tα−(j1)p|v|pdt

=

j1

i=1

|ip−1−α| p

pZ

T tα−(j1)p 1 tu(nj)

p

dt

j1

i=1

|ip−1−α| p

p n i=

j+1

|ip−1−α| p

pZ

T tαnp

tnj+1 y tnj

0

p

dt

=

j1

i=1

|ip−1−α| p

p n i=

j+1

|ip−1−α| p

pZ

T tα−(j1)p|z0|pdt.

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Summarizing the previous computations Z

T tα|y(n)|pdt+

Z

T c(t)|y|pdt

"

n i=1,i6=j

|ip−1−α| p

p

+pK

p

|jp−1−α| p1#

Z

T tα−(j1)p

y tnj

0

p

dt

= p

p

|jp−1−α|

p1"

1

|jp−1−α|

n i=1

|ip−1α| p

p

+K

#

×

Z

T tα−(j1)p

y tnj

0

p

dt

= p

p

|jp−1−α| p1

γn,p,α

|jp−1−α|+K Z

T tα−(j1)p

y tnj

0

p

dt.

Now, according to the definition of the constantKwe see that the energy functional corre- sponding to (4.5) is positive for largeT and hence (4.5) is nonoscillatory.

Next we prove a statement which relates nonoscillatory behavior of a two-term 2nth order half-linear differential equation to nonoscillation of a certain second order half-linear equation.

It also presents a simpler proof of the previous theorem withj=n.

Theorem 4.4. Consider equation(4.5) withα6∈ {p−1, . . . ,np−1}. If the second order differential equation

− tα−(n1)pΦ(x0)0+ c(t)

γn1,p,αΦ(x) =0 (4.6)

is nonoscillatory, γn1,p,α = nj=11|jpp1α|p, c(t) =min{0,c(t)}, then(4.5) is also nonoscilla- tory. In particular, ifα<np−1andR

c(t)dt>−, equation(4.5)is nonoscillatory provided lim inf

t tnp1α Z

t c(s)ds>− γn,p,α

np−1−α. (4.7)

Proof. Using the Wirtinger inequality (as in (3.2)) we can estimate the energy functional in (4.5) as follows

Z

T tα|y(n)|pdt+

Z

T c(t)|y|pdt≥γn1,p,α

Z

T tα−(n1)p|y0|pdt+

Z

T c(t)|y|pdt

=γn1,p,α

Z

T tα−(n1)p|y0|pdt+ 1 γn1,p,α

Z

T c(t)|y|pdt

. The expression in brackets on the second line of the previous computation is the energy functional of (4.6) and it is positive if this equation is nonoscillatory and Tis sufficiently large by [16, Theorem 2.1.1]. To prove the second statement of theorem, we apply the Hille–Nehari type nonoscillation criterion to (4.6). This criterion says (see, e.g., [16, Theorem 2.1.2]) that equation (1.2) with r1 satisfyingR

r11q(t)dt = andR

0 (r0)(t)> − (where(r0)(t) = min{0,r0(t)}) is nonoscillatory provided

lim inf

t

Z t

r11q(s)ds

p1Z

t

(r0)(s)ds>−1 p

p−1 p

p1

. (4.8)

(11)

Hence, forr1(t) =tα−(n1)p, we have Z t

0 r11q(s)ds p1

= t

α(1q)+q(n1)+1

α(1−q) +q(n−1) +1

!p1

= t

np1α

np1α p1

p1. andR

r11q(t)dt=, sinceα<np−1. Then (4.8) reads lim inf

t

tnp1α np1α

p1

p1

Z

t

(r0)(s)ds>−1 p

p−1 p

p1

which is just (4.7) with γc(t)

n1,p,α instead of(r0)(t).

Remark 4.5. Obviously, Theorem4.4applied to Euler type equation (2.3) gives Theorem3.2.

Remark 4.6. Let us have a look at Theorem 4.1withr(t) = tα,α6∈ {p−1, 2p−1, . . . ,np−1} andc(t)≤ 0 for large t. Thenr1q(t) = tα(1q) and forα< p−1 (the caseα > p−1 is more complicated) we have

Z t

0

r1q(s)ds= t

α(1q)+1

α(1−q) +1,

Z t

0

r1q(s)ds p1

= t

p1α

p1α p1

p1, Z t

0 r1q(s)ds p

= t

p

p1α p1

p,

Z t

0 r1q(s)ds 1

= [1−(q−1)α]tα(q1)−1.

Hence, (4.1) takes the form lim inf

t tp1α Z

t c(s)(s−T)(n1)pds>−

p−1−α p−1

p1

·

p−1 p

p

·[(n−1)!]p p−1

=− 1

p−1−α

p−1α p

p

[(n−1)!]p.

(4.9)

This condition ismore restrictivethan (4.4) with j=1. Indeed, forα< p−1 we have

γn,p,α p−1−α

=− 1

p−1−α

p−1−α p

p

2−α+1 p

p

· · ·

n− α+1 p

p

<− 1

p−1−α

p−1−α p

p

[(n−1)!]p since α+p1 < 1. The difference in terms R

t c(s)s(n1)pds and R

t c(s)(s−T)(n1)pds in (4.4) (with j= 1) and (4.9), respectively, is not important since limss−(n1)p·(s−T)(n1)p =1.

Concerning (4.2), similarly as for (4.1) we obtain lim inf

t tα(q1)−1 Z t

0 c(s)snpds>−[(n−1)!]p

p−1−α p

p

p−1 p−1−α.

This condition is not covered by results presented in this paper and a subject of the present investigation is to “insert” this criterion into a general framework of even-order half-linear oscillation theory.

Hivatkozások

KAPCSOLÓDÓ DOKUMENTUMOK

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Keywords: oscillation, asymptotic behavior, neutral differential equations, nonlinear, higher order, eventually positive solution.. 2010 Mathematics Subject Classification: