1 Introduction

In this paper, we derive some regularity results for the best-Sobolev-constant function defined by

$$\begin{aligned} q\in [1,p^{\star }]\mapsto \lambda _{q}:=\inf \left\{ \mathcal {R} _{q}(u):u\in W_{0}^{1,p}(\Omega )\setminus \{0\}\right\} \end{aligned}$$
(1)

where \(\Omega \) is a bounded and smooth domain of \(\mathbb {R}^{N}\), \(N\ge 2,\, 1<p<N,\, p^{\star }:=\dfrac{Np}{N-p}\) and

$$\begin{aligned} \mathcal {R}_{q}(u):=\frac{\left\| \nabla u\right\| _{p}^{p}}{\left\| u\right\| _{q}^{p}};\text { }u\in W_{0}^{1,p}(\Omega )\setminus \{0\} \end{aligned}$$

is the Rayleigh quotient associated with the Sobolev immersion \(W_{0} ^{1,p}(\Omega )\hookrightarrow L^{q}(\Omega )\). (Here \(\left\| \cdot \right\| _{s}:=\left( {\int _{\Omega }}\left| \cdot \right| ^{s}\hbox {d}x\right) ^{\frac{1}{s}}\) denotes the usual norm of \(L^{s}(\Omega )\).)

It is well known that the immersion \(W_{0}^{1,p}(\Omega )\hookrightarrow L^{q}(\Omega )\) is continuous if \(1\le q\le p^{\star }\) and compact if \(1\le q<p^{\star }\). Hence, there exists \(u_{q}\in W_{0}^{1,p}(\Omega )\setminus \{0\}\) such that \(\mathcal {R}_{q}(u_{q})=\lambda _{q}\), if \(1\le q<p^{\star }\). Since \(\mathcal {R}_{q}\) is homogeneous the extremal function \(u_{q}\) associated with \(\lambda _{q}\) can be chosen such that \(\left\| u_{q}\right\| _{q}=1\). (From now on \(u_{q}\) will denote any \(L^{q}\)-normalized extremal function corresponding to \(\lambda _{q}\)).

It is straightforward to verify that such a normalized extremal function \(u_{q}\) is a weak solution of the Dirichlet problem

$$\begin{aligned} \left\{ \begin{array}{ll} -\Delta _{p}u = \lambda _{q}\left| u\right| ^{q-2}u &{} \quad \text {in }\Omega \\ u = 0 &{} \quad \text {on }\partial \Omega , \end{array} \right. \end{aligned}$$
(2)

for the \(p\)-Laplacian operator \(\Delta _{p}u:=\mathrm{div }(\left| \nabla u\right| ^{p-2}\nabla u)\). Hence, classical results imply that \(u_{q}\in C^{1,\alpha }(\overline{\Omega })\) for some \(0<\alpha <1\). Thus, \(u_{q}\in W_{0}^{1,p}(\Omega )\cap C^{1,\alpha }(\overline{\Omega })\) satisfies, for each \(q\in [1,p^{\star })\):

$$\begin{aligned} \left\| u_{q}\right\| _{q}=1\quad \text { and }\quad \mathcal {R}_{q} (u_{q})=\left\| \nabla u_{q}\right\| _{p}^{p}=\lambda _{q}. \end{aligned}$$
(3)

Therefore, the infimum in (1) is actually a minimum if \(1\le q<p^{\star }\). In the critical case, \(q=p^{\star }\), one has \(\lambda _{p^{\star }}=S^{p}\), where \(S\) is the well-known Sobolev constant (see [4, 20]) and the minimum is not reached if \(\Omega \) is a proper subset of \(\mathbb {R}^{N}\). We recall that \(S\) is explicitly given by

$$\begin{aligned} S:=\sqrt{\pi }N^{\frac{1}{p}}\left( \frac{N-p}{p-1}\right) ^{\frac{p-1}{p} }\left( \frac{\Gamma (N/p)\Gamma (1+N-N/p)}{\Gamma (1+N/2)\Gamma (N)}\right) ^{\frac{1}{N}} \end{aligned}$$
(4)

where \(\Gamma (t)=\int \nolimits _{0}^{\infty }s^{t-1}e^{-s}\hbox {d}s\) is the Gamma Function.

We remark that \(\lambda _{q}\) is simple if \(1\le q\le p\) (see [14]), which means that extremal functions associated with \(\lambda _{q}\) are scalar multiple one of the other. This property is still valid in the “super-linear” case \(p<q<p^{\star }\) if \(\Omega \) is a ball (see [1, 15]) or if \(p=2\) and \(2\le q\le 2+\epsilon \) (see [7]). However, for a general bounded \(N\)-dimensional domain, \(\lambda _{q}\) is not known to be simple in the super-linear case. In fact, \(\lambda _{q}\) is not simple if \(\Omega \) is an annulus and \(q\) is close enough to \(p^{\star }\) (see [18]).

Thus, if

$$\begin{aligned} E_{q}:=\left\{ u\in W_{0}^{1,p}(\Omega ):\left\| u\right\| _{q}=1\text { and }\left\| \nabla u\right\| _{p}=\root p \of {\lambda _{q}}\right\} \end{aligned}$$
(5)

denotes the set of the \(L^{q}\)-normalized extremal functions, it follows that \(E_{q}=\left\{ \pm u_{q}\right\} \) whenever \(\lambda _{q}\) is simple. Otherwise, \(E_{q}\) might be larger than \(\left\{ \pm u_{q}\right\} \) and the question of determining the size of \(E_{q} \) for a general domain in the “super-linear”case \(p<q<p^{\star }\) is still an open problem for which our results might be useful.

Up to our knowledge, very little attention has been paid to the behavior of the function \(q\in [1,p^{\star }]\mapsto \lambda _{q}\) in the literature.

In [5] Benci and Cerami considered the function \((q,\mu )\in (2,2^{\star })\times [0,+\infty )\mapsto m(q,\mu )\) where

$$\begin{aligned} m(q,\mu ):=\inf \left\{ \left\| \nabla u\right\| _{2}^{2}+\mu \left\| u\right\| _{2}^{2}:u\in W_{0}^{1,2}(\Omega )\text { and }\left\| u\right\| _{q}=1\right\} . \end{aligned}$$
(6)

This minimizing problem is closely associated with Dirichlet problem

$$\begin{aligned} \left\{ \begin{array}{ll} -\Delta u+\mu u = \left| u\right| ^{q-2}u &{}\quad \text {in }\Omega \\ u = 0 &{}\quad \text {on }\partial \Omega . \end{array} \right. \end{aligned}$$
(7)

Benci and Cerami proved that for each fixed \(\mu \ge 0\) there exists \(q_{\mu }\in (2,2^{\star })\) such that (7) has at least \(\mathrm{cat }\Omega \) positive solutions whenever \(q_{\mu }\le q\le 2^{\star }\) (here \(\mathrm{cat }\Omega \) denotes the Lyusternik–Shnirel’man category of \(\overline{\Omega }\) in itself). In order to reach this remarkable multiplicity result they verified (see [5, Leema 4.1]) that for each \(\mu \ge 0\) fixed the function \(q\in (2,2^{\star })\mapsto m(q,\mu )\) is (left) continuous at \(q=2^{\star }\). We observe that for \(\mu =0\) (and \(p=2\)) this means that the function \(q\in [1,2^{\star }]\mapsto \lambda _{q}\) is (left) continuous at \(q=2^{\star }\). (We remark that Benci and Cerami [5] also proved in the same multiplicity result for all \(\mu \ge \mu _{q}\) where \(\mu _{q}\ge 0\) is obtained from each fixed \(q\in (2,2^{\star })\).)

With respect to \(p>1\), Huang proved in [13, Thm 2.1] that the function \(q\in [1,p^{\star }]\mapsto \lambda _{q}\) is continuous in the open interval \((1,p)\) and lower semi-continuous in the open interval \((p,p^{\star })\).

We have recently started, in [10], a study on the behavior of the function \(q\in [1,p^{\star }]\mapsto \lambda _{q}\) proving that it is decreasing, Lipschitz continuous in \([1,p^{\star }-\epsilon ]\) for each \(\epsilon >0\) and left-continuous at \(q=p^{\star }\), thus obtaining its absolute continuity in \([1,p^{\star }]\). Therefore, for almost all \(q\in [1,p^{\star }]\), the derivative \(\lambda _{q}^{\prime }\) of \(\lambda _{q}\) exists. Using a different method, these results were extended in [2], to allow \(q\in (0,1)\) and \(p\ge N\) as well (so, \(p^{\star }=\infty \) in this case).

In [9] we studied the asymptotic behavior, as \(q\rightarrow p\), of the positive solutions of the “resonant Lane–Emden problem”

$$\begin{aligned} \left\{ \begin{array}{ll} -\Delta _{p}u = \lambda _{p}\left| u\right| ^{q-2}u &{}\quad \text {in }\Omega \\ u = 0 &{}\quad \text {on }\partial \Omega \end{array} \right. \end{aligned}$$

and obtained, as a byproduct of our main result, the existence of \(\lambda _{p}^{\prime }\).

In the present paper, we give two characterizations of the existence of \(\lambda _{q}^{\prime }\) and prove a Hölder regularity result for \(\lambda _{q}\).

In Sect. 2, we first prove that the derivative \(\lambda _{q}^{\prime }\) exists if, and only if the functional

$$\begin{aligned} I_{q}(u):=\int \limits _{\Omega }\left| u\right| ^{q}\log \left| u\right| dx \end{aligned}$$
(8)

is constant on the set \(E_{q}\). It follows that \(I_{q}\) is constant on \(E_{q}\) for almost all \(q\in (p,p^{\star })\) which is a new and nontrivial property that, at least in principle, could be used to prove results on simplicity of \(\lambda _{q}\) for suitable domains or even to give estimates for the number of extremal functions associated with \(\lambda _{q}\).

Thereafter, still in Sect. 2, we prove that the existence of \(\lambda _{q}^{\prime }\) is also equivalent to the continuity of the function \(s\in [1,p^{\star }]\mapsto I_{s}(u_{s})\) at \(s=q\).

As consequence of these characterizations, we conclude that the function \(s\in [1,p^{\star }]\mapsto \lambda _{s}\) is continuously differentiable at \(s=q\) whenever \(\lambda _{q}\) is simple. Thus, for a general bounded \(\Omega \) and \(p>1\) one always has \(\lambda _{s}\in C^{1}([1,p])\). If \(p=2\) one also has \(\lambda _{s}\in C^{1}([1,2+\epsilon ])\), for some \(\epsilon >0\) and if \(p>1\) and \(\Omega \) is a ball then \(\lambda _{s}\in C^{1}([1,p^{\star }))\).

In order to obtain both characterizations of the differentiability, we first prove that

$$\begin{aligned} \lambda _{q}^{\prime }+\frac{p}{q}I_{q}(u_{q})\lambda _{q}=0 \end{aligned}$$

at each point \(q\in [1,p^{\star }]\) where the derivative \(\lambda _{q}^{\prime }\) exists. Thus, \(\lambda _{q}\) satisfies a simple linear and homogeneous ordinary differential equation in the Carathéodory sense (that is, almost everywhere). Then, we combine this fact with the absolute continuity of the function \(q\in [1,p^{\star }]\mapsto \lambda _{q}\) to obtain the following representation formula:

$$\begin{aligned} \lambda _{q}=\lambda _{1}\exp \left( -p\int \limits _{1}^{q}\frac{1}{s}\int \limits _{\Omega }\left| u_{s}\right| ^{s}\log \left| u_{s}\right| \hbox {d}x\hbox {d}s\right) ,\quad \text {for all }q\in [1,p^{\star }], \end{aligned}$$
(9)

where each extremal function \(u_{s} \) can be arbitrarily chosen in \(E_{s}\) for each \(s\in [1,p^{\star })\).

In Sect. 3, we prove a Hölder regularity at \(p^{\star }\) after deriving some estimates for \(I_{q}(u_{q})\). More precisely, we prove that \(\lambda _{q}\) is \(\alpha \)-Hölder continuous in the interval \([1,p^{\star }]\), for any \(0<\alpha <1\), under the additional hypothesis

$$\begin{aligned} \limsup _{q\rightarrow p^{\star }} (p^{\star }-q)\left\| u_{q}\right\| _{\infty }^{\gamma }<\infty \end{aligned}$$
(10)

for some \(\gamma >0\). This asymptotic behavior holds true, for instance, if \(\Omega \) is a ball and \(p>1\) and also if \(p=2\) and \(\Omega \) is an arbitrary bounded domain. Thus, at least in these two situations, our results guarantee that \(\lambda _{q}\) is \(\alpha \)-Hölder continuous for any \(0<\alpha <1\). However, we believe that (10) holds true for a general bounded and smooth domain, also if \(1<p\not =2\).

2 Characterizations of the differentiability

From now on \(E_{q}\) denotes the set of the \(L^{q}\)-normalized extremal functions, defined in (5), and \(I_{q}\) denotes the functional defined by (8).

Theorem 1

For each \(q\in [1,p^{\star })\), let \(u_{q}\) be arbitrarily chosen in \(E_{q}\). The following estimates hold for each \(q\in (1,p^{\star })\):

$$\begin{aligned} \limsup _{s\rightarrow q^{+}}\frac{\lambda _{q}-\lambda _{s}}{q-s}\le -\frac{p}{q}I_{q}(u_{q})\lambda _{q}\le \liminf \limits _{s\rightarrow q^{-}} \frac{\lambda _{q}-\lambda _{s}}{q-s}. \end{aligned}$$
(11)

Therefore, the function \(q\mapsto \lambda _{q}\) satisfies

$$\begin{aligned} \lambda _{q}^{\prime }+\frac{p}{q}I_{q}(u_{q})\lambda _{q}=0 \end{aligned}$$
(12)

at each point \(q\in (1,p^{\star })\) where its derivative \(\lambda _{q}^{\prime }\) exists.

Proof

Let \(q\in (1,p^{\star })\). Since \(\int _{\Omega }\left| u_{q}\right| ^{q}\hbox {d}x=1\) we have

$$\begin{aligned} \frac{\hbox {d}}{\hbox {d}s}\left[ \left( \int \limits _{\Omega }\left| u_{q}\right| ^{s}\hbox {d}x\right) ^{\frac{p}{s}}\right] _{s=q}&= \left( \int \limits _{\Omega }\left| u_{q}\right| ^{q}\hbox {d}x\right) ^{\frac{p}{q}}\left( \frac{\hbox {d}}{\hbox {d}s}\left[ \frac{p}{s}\log \left( \int \limits _{\Omega }\left| u_{q}\right| ^{s}\hbox {d}x\right) \right] _{s=q}\right) \\&= \frac{p}{q}I_{q}(u_{q}). \end{aligned}$$

It follows from (3) that

$$\begin{aligned} \lambda _{q}=\int \limits _{\Omega }\left| \nabla u_{q}\right| ^{p}\hbox {d}x\ge \lambda _{s}\left( \int \limits _{\Omega }\left| u_{q}\right| ^{s}\hbox {d}x\right) ^{\frac{p}{s}}. \end{aligned}$$

Therefore, the continuity of the function \(q\mapsto \lambda _{q}\) and L’Hôpital’s rule yield

$$\begin{aligned} \liminf \limits _{s\rightarrow q^{-}}\frac{\lambda _{q}-\lambda _{s}}{q-s}&\ge \liminf \limits _{s\rightarrow q^{-}}\lambda _{s}\frac{\left( \int \nolimits _{\Omega }\left| u_{q}\right| ^{s}\hbox {d}x\right) ^{\frac{p}{s}}-1}{q-s}\\&=-\lambda _{q}\lim \limits _{s\rightarrow q^{-}}\frac{\hbox {d}}{\hbox {d}s}\left[ \left( \int \limits _{\Omega }\left| u_{q}\right| ^{s}\hbox {d}x\right) ^{\frac{p}{s}}\right] _{s=q}=-\lambda _{q}\frac{p}{q}I_{q}(u_{q}). \end{aligned}$$

Analogously,

$$\begin{aligned} \limsup _{s\rightarrow q^{+}}\frac{\lambda _{q}-\lambda _{s}}{q-s}\le \limsup _{s\rightarrow q^{+}}\lambda _{s}\frac{\left( \int \nolimits _{\Omega }\left| u_{q}\right| ^{s}\hbox {d}x\right) ^{\frac{p}{s}}-1}{q-s}=-\lambda _{q}\frac{p}{q}I_{q}(u_{q}). \end{aligned}$$

\(\square \)

We remark that Theorem 1 is valid for any choice of the extremal function \(u_{q}\) in \(E_{q}\). Therefore, the following consequence is immediate.

Corollary 2

Let \(q\in (1,p^{\star })\) be such that \(\lambda _{q}^{\prime }\) exists. Then the functional \(I_{q}\) is constant on \(E_{q}\).

In the sequel \(f:[1,p^{\star })\rightarrow \mathbb {R}\) denotes the function defined by

$$\begin{aligned} f(q):=\frac{p}{q}I_{q}(u_{q}) \end{aligned}$$

where, for each \(q\in [1,p^{\star })\), \(u_{q}\) is arbitrarily chosen in \(E_{q}\).

Now, we prove the representation formula (9) for the function \(q\in [1,p^{\star }]\mapsto \lambda _{q}\).

Theorem 3

It holds

$$\begin{aligned} \lambda _{q}=\lambda _{1}e^{-\int \nolimits _{1}^{q}f(s)\mathrm{d}s} \quad \mathrm{for \; all }\,\quad q\in [1,p^{\star }]. \end{aligned}$$
(13)

Proof

Since the function \(q\in [1,p^{\star }]\mapsto \lambda _{q}\) is absolutely continuous and its image is a closed interval \([a,b]\subset (0,\infty )\) we also have that the function \(q\in [1,p^{\star }]\mapsto \log \lambda _{q}\) is absolutely continuous. Therefore,

$$\begin{aligned} \log (\lambda _{q}/\lambda _{1})=\int \limits _{1}^{q}\left( \log \lambda _{s}\right) ^{\prime }\hbox {d}s=-\int \limits _{1}^{q}f(s)\hbox {d}s \quad \hbox {for all}\quad q\in [1,p^{\star }] \end{aligned}$$

where the last equality follows from (12). Now, (13) follows after exponentiation. \(\square \)

Since \(\lambda _{p^{\star }}=S^{p}\) we note from (13) that

$$\begin{aligned} \lambda _{q}=S^{p}\exp \left( p\int \limits _{q}^{p^{\star }}\frac{1}{s^{2}}\int \limits _{\Omega }\left| u_{s}\right| ^{s}\log \left| u_{s}\right| ^{s}\hbox {d}x\hbox {d}s\right) \text { for all }\quad q\in [1,p^{\star }]. \end{aligned}$$

(We recall that the Sobolev constant \(S\) is explicitly given by (4).)

The following result is an immediate consequence of (13). We leave its proof to the reader.

Corollary 4

Let \(q\in [1,p^{\star })\) be a point where \(f\) is continuous. Then the derivative \(\lambda _{q}^{\prime }\) exists and is given by the continuous expression \(\lambda _{q}^{\prime }=-\lambda _{q}f(q)\).

Proposition 5

Suppose that \(I_{q}\) is constant on \(E_{q}\) for some \(q\in [1,p^{\star })\). Then \(f\) is continuous at \(q\). In particular, \(f\) is continuous at each point \(q\) where \(\lambda _{q}^{\prime }\) exists.

Proof

Let \(q_{n}\rightarrow q\). Then \(\lambda _{q_{n}}\rightarrow \lambda _{q}\) and, up to subsequences, \(u_{q_{n}}\) converges in \(C^{1}(\overline{\Omega })\) to a function \(u\) satisfying (2) and such that \(\left\| u\right\| _{q}=1\). This last claim follows by combining the classical Hölder regularity result (see [17]) with the fact that \(\left\| u_{q_{n}}\right\| _{\infty }\) is bounded from above by a constant which is uniform with respect to \(n\) (see Lemma 11 in the next section).

Therefore, \(u\in E_{q}\) and thus

$$\begin{aligned} f(q_{n})\!=\!\frac{p}{q_{n}}\int \limits _{\Omega }\left| u_{q_{n}}\right| ^{q_{n} }\log \left| u_{q_{n}}\right| \hbox {d}x\rightarrow \frac{p}{q}\int \limits _{\Omega }\left| u_{q}\right| ^{q}\log \left| u_{q}\right| \hbox {d}x\!=\!\frac{p}{q}I_{q}(u)\!=\!\frac{p}{q}I_{q}(u_{q})=f(q), \end{aligned}$$

since \(I_{q}\) is constant on \(E_{q}\). \(\square \)

Corollary 6

The function \(q\mapsto \lambda _{q}\) is continuously differentiable in

  1. 1.

    \([1,p]\) if \(p>1\),

  2. 2.

    \([1,2+\epsilon ]\) (for some \(\epsilon >0\)) if \(p=2\),

  3. 3.

    \((p,p^{\star })\) if \(\Omega \) is ball.

Proof

Since \(I_{q}(u_{q})=I_{q}(\left| u_{q}\right| )\), this corollary follows from the fact that \(\lambda _{q}\) is simple in all of these cases. \(\square \)

Combining corollaries 2 and with Proposition 5 we obtain:

Theorem 7

The following assertions on a point \(q\in [1,p^{\star })\) are equivalent:

  1. 1.

    \(\lambda _{q}^{\prime }\) exists.

  2. 2.

    \(I_{q}\) is constant on \(E_{q}\).

  3. 3.

    The function \(s\in [1,p^{\star }]\mapsto I_{s}(u_{s})\) is continuous at \(s=q\).

We observe that the proof of Corollary also works for \(q=p^{\star }\) if the limit \(\lim \limits _{q\rightarrow p^{\star }}I_{q}(u_{q})\) exists. However, even the verification that \(I_{q}(u_{q})\) is finite at \(q=p^{\star }\) does not seem to be a simple task. One of the difficulties is that \(\left\| u_{q}\right\| _{\infty }\rightarrow \infty \) as \(q\rightarrow p^{\star }\). In fact, otherwise we reach a contradiction by applying a regularity result as in [21] and then making \(q\rightarrow p^{\star }\) in the equation \(-\Delta _{p}u_{q}=\lambda _{q}u_{q}^{q-1}\), thus obtaining a limit function \(u\in W_{0}^{1,p}(\Omega )\) that minimizes the Rayleigh quotient \(\mathcal {R}_{p^{\star }}(\Omega )\). Since \(\Omega \not =\mathbb {R}^{N}\), this is absurd.

In the next section, we derive some estimates for \(I_{q}(u_{q})\) and use them to prove that, under an additional (and natural) hypothesis on the behavior of \(\left\| u_{q}\right\| _{\infty }\) (as \(q\) tends to \(p^{\star }\)) the function \(q\mapsto I_{q}(u_{q})\) belongs to \(L^{r}([0,p^{\star }])\), for all \(r>1\). Unfortunately, the \(L^{r}\) bounds we obtain from these estimates are just linear with respect to \(r\) and thus not enough to prove that \(I_{q} (u_{q})\) stays bounded as \(q\rightarrow p^{\star }\).

3 Hölder regularity

In order to obtain the absolute continuity of the function \(\lambda _{q}\) in [10] we first prove that this function is Lipschitz continuous in each closed interval of the form \([1,p^{\star }-\epsilon ]\subset [1,p^{\star }]\). Of course, this fact guarantees that \(\lambda _{q}\) is Hölder continuous (with any exponent \(\alpha \in (0,1)\)) in \([1,p^{\star }-\epsilon ]\). However, as pointed out in the end of the previous section, the precise behavior of \(\lambda _{q}^{\prime }\) (or equivalently of \(I_{q}(u_{q})\)) as \(q\rightarrow p^{\star }\) seems difficult to determine, even when \(\Omega \) is a ball.

In this section we prove a Hölder regularity result for the function \(\lambda _{q}\) in \([1,p^{\star }] \) by estimating \(\big \Vert \lambda _{q}^{\prime }\big \Vert _{L^{r}([0,p^{\star }])}\) for any \(r>1\). Taking into account (12), we first need to estimate \(I_{q}(u_{q})\).

Lemma 8

The following estimates hold for each \(0\not \equiv u\in W_{0}^{1,p}\left( \Omega \right) \):

$$\begin{aligned} \frac{1}{q}\left\| u\right\| _{q}^{q}\log (\left| \Omega \right| ^{-1}\left\| u\right\| _{q}^{q})<I_{q}(u)\le \left\| u\right\| _{q}^{q}\left( \log \left\| u\right\| _{q}+\frac{\log \left\| u\right\| _{p^{\star }}^{p^{\star }}-\log \left\| u\right\| _{q}^{p^{\star }}}{p^{\star }-q}\right) , \end{aligned}$$
(14)

where \(\left| \Omega \right| :=\int \nolimits _{\Omega }\hbox {d}x\).

Proof

The continuous function \(\varphi :[0,\infty )\rightarrow \mathbb {R}\) defined by \(\varphi (\xi )=\xi \log \xi \), if \(\xi >0\) and \(\varphi (0)=0\) is strictly convex. Hence, for each \(u\not \equiv 0\) Jensen’s inequality yields

$$\begin{aligned} \frac{1}{\left| \Omega \right| }I_{q}(u)=\frac{1}{q\left| \Omega \right| }\int \limits _{\Omega }\varphi (\left| u\right| ^{q} )\hbox {d}x>\frac{1}{q}\varphi (\left| \Omega \right| ^{-1}\left\| u\right\| _{q}^{q})=\frac{1}{q\left| \Omega \right| }\left\| u\right\| _{q}^{q}\log (\left| \Omega \right| ^{-1}\left\| u\right\| _{q}^{q}). \end{aligned}$$

Thus,

$$\begin{aligned} I_{q}(u)>\left\| u\right\| _{q}^{q}\log \left| \Omega \right| ^{-\frac{1}{q}}. \end{aligned}$$

(Note that the equality in the Jensen’s inequality occurs only if \(u^{q} \equiv \int _{\Omega }\left| u\right| ^{q}\hbox {d}x\).)

Now, we prove the upper bound in (14) following [8]. Let \(t\in [q,p^{\star }]\). It follows from Hölder inequality that

$$\begin{aligned} \left\| u\right\| _{t}\le \left\| u\right\| _{q}^{\alpha (t)}\left\| u\right\| _{p^{\star }}^{1-\alpha (t)},\quad q\le t\le p^{\star } \end{aligned}$$

with

$$\begin{aligned} \alpha (t):=\frac{q}{t}\frac{p^{\star }-t}{p^{\star }-q}=\left( \frac{p^{\star } }{t}-1\right) \frac{q}{p^{\star }-q}. \end{aligned}$$

Thus,

$$\begin{aligned} \log \left\| u\right\| _{t}\le \alpha (t)\log \left\| u\right\| _{q}+(1-\alpha (t))\log \left\| u\right\| _{p^{\star }} \end{aligned}$$

and

$$\begin{aligned} g(t):=\log \left\| u\right\| _{t}+\alpha (t)(\log \left\| u\right\| _{p^{\star }}-\log \left\| u\right\| _{q})-\log \left\| u\right\| _{p^{\star }}\le 0. \end{aligned}$$

Since \(g(q)=0 \), we obtain

$$\begin{aligned} g^{\prime }(q)=\lim _{t\rightarrow q^{+}}\frac{g(t)}{t-q}\le 0. \end{aligned}$$

But

$$\begin{aligned} g^{\prime }(t)&=\left( \frac{1}{t}\log \int \limits _{\Omega }\left| u\right| ^{t}\hbox {d}x\right) ^{\prime }+\alpha ^{\prime }(t)(\log \left\| u\right\| _{p^{\star }}-\log \left\| u\right\| _{q})\\&=\frac{1}{t}\left( \left\| u\right\| _{t}^{-t}\int \limits _{\Omega }\left| u\right| ^{t}\log \left| u\right| \hbox {d}x-\log \left\| u\right\| _{t}\right) -\frac{qp^{\star }}{t^{2}(p^{\star }-q)} (\log \left\| u\right\| _{p^{\star }}-\log \left\| u\right\| _{q}) \end{aligned}$$

and thus,

$$\begin{aligned} g^{\prime }(q)=\frac{1}{q}\left( \left\| u\right\| _{q}^{-q}\int \limits _{\Omega }\left| u\right| ^{q}\log \left| u\right| \hbox {d}x-\log \left\| u\right\| _{q}\right) -\frac{p^{\star }}{q}\frac{\log \left\| u\right\| _{p^{\star }}-\log \left\| u\right\| _{q} }{p^{\star }-q}\le 0 \end{aligned}$$

implying that

$$\begin{aligned} I_{q}(u)=\int \limits _{\Omega }\left| u\right| ^{q}\log \left| u\right| \hbox {d}x\le \left\| u\right\| _{q}^{q}\left( \log \left\| u\right\| _{q}+\frac{\log \left\| u\right\| _{p^{\star }}^{p^{\star }}-\log \left\| u\right\| _{q}^{p^{\star }}}{p^{\star }-q}\right) . \end{aligned}$$

\(\square \)

Remark 9

We emphasize that the estimates in (14) become simpler to handle if \(\left| \Omega \right| \le 1=\left\| u\right\| _{q}\). In fact, under these conditions one has

$$\begin{aligned} 0<I_{q}(u)\le \frac{\log \left\| u\right\| _{p^{\star }}^{p^{\star }} }{p^{\star }-q}. \end{aligned}$$
(15)

We also note that a simple scaling argument gives

$$\begin{aligned} \lambda _{q}(\Omega _{1})=\lambda _{q}(\Omega )\left| \Omega \right| ^{\frac{p}{q}-\frac{p}{p^{\star }}} \end{aligned}$$
(16)

where \(\Omega _{1}:=\left\{ x\in \mathbb {R}^{N}:x\left| \Omega \right| ^{\frac{1}{N}}\in \Omega \right\} \) is such that \(\left| \Omega _{1}\right| =1\) and \(\lambda _{q}(D)\) is defined as in (1) with \(\Omega =D\).

It is also worth mentioning that \(\frac{\log \left\| u_{q}\right\| _{p^{\star }}^{p^{\star }}}{p^{\star }-q}\) becomes an indeterminate form of the type \(0/0\) as \(q\rightarrow p^{\star }\), since

$$\begin{aligned} \lim _{q\rightarrow p^{\star }}\left\| u_{q}\right\| _{p^{\star }}=1. \end{aligned}$$
(17)

Indeed, since \(1=\left\| u_{q}\right\| _{q}^{q}\le \left\| u_{q}\right\| _{p^{\star }}^{q}\left| \Omega \right| ^{1-\frac{q}{p\star }}\) one has

$$\begin{aligned} 1=\liminf _{q\rightarrow p^{\star }}\left| \Omega \right| ^{\frac{1}{p^{\star }}-\frac{1}{q}}\le \liminf _{q\rightarrow p^{\star }}\left\| u_{q}\right\| _{p^{\star }}. \end{aligned}$$

On the other hand, the inequality

$$\begin{aligned} \lambda _{p^{\star }}\left\| u_{q}\right\| _{p^{\star }}^{p}\le \left\| \nabla u_{q}\right\| _{p}^{p}=\lambda _{q} \end{aligned}$$

yields

$$\begin{aligned} \limsup _{q\rightarrow p^{\star }}\left\| u_{q}\right\| _{p^{\star }} \le \limsup _{q\rightarrow p^{\star }}\left( \frac{\lambda _{q}}{\lambda _{p^{\star }}}\right) ^{\frac{1}{p}}=1. \end{aligned}$$

Lemma 10

For each \(\beta >0\) and all \(1\le q<p^{\star }\) one has

$$\begin{aligned} I_{q}(u_{q})\le \log \left\| u_{q}\right\| _{\infty }\le \left| \Omega \right| ^{\frac{\beta }{q}}\beta ^{-1}\left\| u_{q}\right\| _{\infty }^{\beta }. \end{aligned}$$
(18)

Proof

The first inequality in (18) follows from (15) since

$$\begin{aligned} \log \left\| u_{q}\right\| _{p^{\star }}^{p^{\star }}\le \log \left( \left\| u_{q}\right\| _{\infty }^{p^{\star }-q}\int \limits _{\Omega }\left| u_{q}\right| ^{q}\hbox {d}x\right) =\log \left\| u_{q}\right\| _{\infty }^{p^{\star }-q}=(p^{\star }-q)\log \left\| u_{q}\right\| _{\infty }. \end{aligned}$$

Since \(\log (x)\le \beta ^{-1}x^{\beta }\) for all \(x\ge 1\) and \(1=\left\| u_{q}\right\| _{q}\le \left\| u_{q}\right\| _{\infty }\left| \Omega \right| ^{\frac{1}{q}}\) the second inequality follows. \(\square \)

Lemma 11

The following estimate holds

$$\begin{aligned} \log \left\| u_{q}\right\| _{\infty }\le \frac{C}{p^{\star }-q},\quad \mathrm{for}\ \mathrm{all }\quad 1\le q<p^{\star } \end{aligned}$$
(19)

where \(C\) is a positive constant which does not depend on \(q\).

Proof

By taking \(\sigma =q\) in Lemma 5 of Ercole [10] we obtain

$$\begin{aligned} \left\| u_{q}\right\| _{\infty }^{p^{\star }-q}\le K_{q}\left( \frac{\lambda _{q}}{\lambda _{p^{\star }}}\right) ^{\frac{N}{N-p}},\quad \mathrm{for}\ \mathrm{all }\quad 1\le q<p^{\star } \end{aligned}$$

where

$$\begin{aligned} K_{q}:=2^{\frac{N(p-1)+qp}{N-p}}\left( \frac{p+N(p-1)}{p}\right) ^{\frac{p^{\star }(N-1)}{N}}\le K_{p^{\star }},\quad 1\le q\le p^{\star }. \end{aligned}$$

Hence, (19) follows with

$$\begin{aligned} C:=\log \left( K_{p^{\star }}\max _{1\le q\le p^{\star }}\left( \frac{\lambda _{q}}{\lambda _{p^{\star }}}\right) ^{\frac{N}{N-p}}\right) . \end{aligned}$$

\(\square \)

Now, we are in position to prove a Hölder regularity result for the function \(q\mapsto \lambda _{q}\) by assuming that

$$\begin{aligned} \limsup _{q\rightarrow p^{\star }} (p^{\star }-q)\left\| u_{q}\right\| _{\infty }^{\gamma }<\infty \end{aligned}$$
(20)

for some constant \(\gamma >0\). Before proceeding, let us give some motivations for the assumption (20).

In [16] Knaap and Peletier proved the following asymptotic behavior for the case where \(\Omega \) is the ball centered at the origin:

$$\begin{aligned} \lim _{q\rightarrow p^{\star }}(p^{\star }-q)\left\| u_{q}\right\| _{\infty }^{p/(p-1)}=A_{N,p,\Omega } \end{aligned}$$
(21)

being \(A_{N,p,\Omega }\) a positive constant given explicitly in terms of \(N\), \(p\) and the volume of \(\Omega \). Of course, (21) implies (20) with \(\gamma =\frac{p}{p-1}\).

In the case where \(p=2\), the asymptotic behavior (21) for a ball had already been proved by Atkinson and Peletier in [3]. In [6], still with \(p=2\) and for a ball, Brezis and Peletier gave another proof of (21) and, among other important results, they conjectured that a similar asymptotic behavior should be true for a nonspherical bounded and smooth domain \(\Omega \) (keeping \(p=2\)). This conjecture was then proved, independently, by Rey in [19] and by Han in [12]. The regular part of the Green function of \(\Omega \) (associated with the Laplacian) played an essential role in the proofs presented in [12, 19]. Indeed, the proofs rely on the fact that, as \(q\) goes to \(2^{\star }\), the maximum points of \(u_{q}\) concentrate at a point \(x_{0}\in \Omega \) which is a critical point of the Robin function of \(\Omega \) (the diagonal of the regular part of the Green function). In the case where \(\Omega \) is a ball \(x_{0}\) is its center.

However, to the best of our knowledge in the case \(1<p\not =2\), the only result specifically related to the asymptotic behavior (21) is that by Knaap and Peletier in [16] for a ball. For a general bounded and smooth domain \(\Omega \), Garcia Azorero and Peral Alonso showed in [11] that \(u_{q}\) converges in the sense of measure to a multiple of the Dirac Delta Function concentrated at a point \(x_{0}\in \Omega \). Thus, they reproduced for \(1<p\not =2\) the concentration property known in the case \(p=2\). After [11] some works have dealt with the convergence of the family \(\left\{ u_{q}\right\} \) in the measures sense but, as far as we are aware, the generalization of (21) for a nonspherical bounded domains remains open if \(1<p\not =2\).

In the sequel, we show that the asymptotic behavior (20) combined with (15) imply that \(\lambda _{q}\in W^{1,r}([1,p^{\star }])\) for any \(r\ge 1\) and hence that \(\lambda _{q}\in C^{0,\alpha }([1,p^{\star }])\) for any \(0<\alpha <1\) (by taking \(\alpha :=1-\dfrac{1}{r}\)). Thus, for a ball and \(p>1\) and for a general bounded domain and \(p=2\) we get more regularity at \(p^{\star }\) than just absolute continuity.

We remark that \(\lambda _{q}\in W^{1,1}([1,p^{\star }])\) for a general bounded domain \(\Omega \) (because \(\lambda _{q}\) is absolutely continuous in the closed interval \([1,p^{\star }]\)).

Theorem 12

Assume that (20) happens for some \(\gamma >0\). The function \(q\mapsto \lambda _{q}\) belongs to the Sobolev space \(W^{1,r} ([1,p^{\star }])\) for any \(r>1\). Moreover,

$$\begin{aligned} \limsup _{r\rightarrow \infty }\left( r^{-1}\left\| \lambda _{q}^{\prime }\right\| _{L^{r}([1,p^{\star }])}\right) <\infty . \end{aligned}$$
(22)

Proof

By taking into account (16) we can assume, without loss of generality, that \(\left| \Omega \right| \le 1\). Hence,

$$\begin{aligned} 0<I_{q}(u_{q})\le \beta ^{-1}\left\| u_{q}\right\| _{\infty }^{\beta } \end{aligned}$$
(23)

for any \(\beta >0\), according to (18).

It follows from (12) that

$$\begin{aligned} \left\| \lambda _{q}^{\prime }\right\| _{L^{r}([1,p^{\star }])} \le \left\| \frac{p}{q}I_{q}(u_{q})\lambda _{q}\right\| _{L^{r} ([1,p^{\star }])}\le p\left( \max \limits _{1\le q\le p^{\star }}(\lambda _{q}/q)\right) \left\| I_{q}(u_{q})\right\| _{L^{r}([1,p^{\star }])}. \end{aligned}$$

Therefore, we just need to prove that \(\left\| I_{q}(u_{q})\right\| _{L^{r}([1,p^{\star }])}\) is finite.

The hypothesis (20) implies that there exists \(\overline{q} \in (1,p^{\star })\) such that

$$\begin{aligned} \left\| u_{q}\right\| _{\infty }\le c(p^{\star }-q)^{-\frac{1}{\gamma } }\quad \text { for all }\overline{q}\le q\le p^{\star } \end{aligned}$$

for some positive constant \(c\) (which may depend on \(\gamma \)).

Combining this with (23) yields

$$\begin{aligned} \int \limits _{\overline{q}}^{p^{\star }}\left| I_{q}(u_{q})\right| ^{r} \hbox {d}q\le \beta ^{-r}c^{\beta r}\int \limits _{\overline{q}}^{p^{\star }}(p^{\star }-q)^{-\frac{\beta r}{\gamma }}\hbox {d}q. \end{aligned}$$

Thus, by taking \(\beta :=\dfrac{\gamma }{2r}\) we obtain

$$\begin{aligned} \int \limits _{\overline{q}}^{p^{\star }}\left| I_{q}(u_{q})\right| ^{r} \hbox {d}q&\le \left( \frac{2r}{\gamma }\right) ^{r}c^{(\gamma /2)}\int \limits _{\overline{q} }^{p^{\star }}(p^{\star }-q)^{-\frac{1}{2}}\hbox {d}q\\&\le \left( \frac{2r}{\gamma }\right) ^{r}c^{(\gamma /2)}2(p^{\star }-\overline{q})^{\frac{1}{2}}\le k\left( \frac{2r}{\gamma }\right) ^{r}, \end{aligned}$$

where \(k:=c^{(\gamma /2)}2(p^{\star }-\overline{q})^{\frac{1}{2}}\).

On the other hand, it follows from Lemma 11 that

$$\begin{aligned} \int \limits _{1}^{\overline{q}}\left| I_{q}(u_{q})\right| ^{r}\hbox {d}q&\le \int \limits _{1}^{\overline{q}}\left( \log \left\| u_{q}\right\| _{\infty }\right) ^{r}\hbox {d}q\\&\le \int \limits _{1}^{\overline{q}}\left( \frac{C}{p^{\star }-q}\right) ^{r} \hbox {d}q\le \left( \frac{C}{p^{\star }-\overline{q}}\right) ^{r}(\overline{q}-1). \end{aligned}$$

Thus, we conclude that \(\lambda _{q}^{\prime }\in L^{r}([1,p^{\star }])\) and that

$$\begin{aligned} \int \limits _{1}^{p^{\star }}\left| I_{q}(u_{q})\right| ^{r}\hbox {d}q\le p\max \limits _{1\le q\le p^{\star }}(\lambda _{q}/q)\left[ k\left( \frac{2r}{\gamma }\right) ^{r}+\left( \frac{C}{p^{\star }-\overline{q}}\right) ^{r}(\overline{q}-1)\right] \le C_{1}C_{2}^{r}(1+r^{r}) \end{aligned}$$

for positive constants \(C_{1}\) and \(C_{2}\) which do not depend on \(r\). Hence we obtain (22). \(\square \)

The following corollary follows immediately.

Corollary 13

Suppose that \(p>1\) and \(\Omega \) is a ball or that \(p=2\) and \(\Omega \) is a general bounded and smooth domain. Then \(\lambda _{q}\in C^{0,\alpha }([1,p^{\star }])\) for any \(0<\alpha <1\).