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very $0<\rho<\hat\rho_1=\hat\rho_1(\Omega,p)$ problem \eqref{eq:main_prob_U} admits a solution which is a local minimum of the energy ${\mathcal{E}}$ on ${\mathcal{M}}_\rho$. In particular, $U$ is positive, has Morse index one and the associated solitary w
ave is orbitally stable. Furthermore, for every Lipschitz $\Omega$, \begin{itemize} \item $\displaystyle 1<p<1+\frac{4}{N} \implies \hat\rho_1\left(\Omega,p\right) = +\infty$, \item $\displaystyle p=1+\frac{4}{N} \implies \hat\rho_1\left(\Omega,p\right) \
geq \|Z_{N,p}\|^2_{L^2({\mathbb{R}}^N)}$, \item $\displaystyle 1+\frac{4}{N}<p<2^*-1 \implies \hat\rho_1\left(\Omega,p\right) \geq D_{N,p} \lambda_1(\Omega)^{\frac{2}{p-1}-\frac{N}{2}}$, \end{itemize} where the universal constant $D_{N,p}$ is explicitly w
ritten in terms of $N$ and $p$ in Section \ref{sec:1const}. \end{theorem} \begin{remark}\label{rem:introGS} Of course, in the subcritical and critical cases, $c_1$ is actually a global minimum. Furthermore, the lower bound for the supercritical case agrees
with that of the critical one since, as shown in Section \ref{sec:1const}, $D_{N,1+4/N} = \|Z_{N,p}\|^2_{L^2({\mathbb{R}}^N)}$ (and $\lambda_1(\Omega)$ is raised to the $0^{\text{th}}$-power). Notice that the estimate for the supercritical case is new al
so in the case $\Omega=B_1$. \end{remark} We observe that the exponent of $\lambda_1(\Omega)$ in the supercritical threshold is negative, therefore such threshold decreases with the size of $\Omega$. Once the first thresholds have been estimated, we turn
to the higher ones: by exploiting the relations between $M_{\alpha,k}$ and $c_k$, we can show that the thresholds obtained for Morse index one--solutions in Theorem \ref{thm:intro_GS} can be increased, by considering higher Morse index--solutions, at least
for some exponent. \begin{proposition}\label{thm:intro_3>1} For every $\Omega$ and $1<p<2^*-1$, \[ \hat\rho_3\left(\Omega,p\right) \geq 2 \cdot D_{N,p} \lambda_3(\Omega)^{\frac{2}{p-1}-\frac{N}{2}}. \] \end{proposition} \begin{remark} In the critical case
, the lower bound for $\hat\rho_3$ provided by Proposition \ref{thm:intro_3>1} is twice that for $\hat\rho_1$ obtained in Theorem \ref{thm:intro_GS}. By continuity, the estimate for $\hat\rho_3$ is larger than that for $\hat\rho_1$ also when $p$ is supercr
itical, but not too large. To quantify such assertion, we can use Yang's inequality \cite{MR1894540,MR2262780}, which implies that for every $\Omega$ it holds \[ \lambda_3(\Omega)\leq \left(1+\frac{N}{4}\right)2^{2/N} \lambda_1(\Omega). \] We deduce that $
2 \cdot D_{N,p} \lambda_3(\Omega)^{\frac{2}{p-1}-\frac{N}{2}} \geq D_{N,p} \lambda_1(\Omega)^{\frac{2}{p-1}-\frac{N}{2}}$ whenever \[ p\leq 1+\frac{4}{N} + \frac{8}{N^2\log_2\left(1+\frac{4}{N}\right)}. \] In particular, the physically relevant case $N=3$
, $p=3$ is covered. Furthermore, if $N\geq 7$, the above condition holds for every $p<2^*-1$. \end{remark} Beyond existence results for \eqref{eq:main_prob_U}, also multiplicity results can be achieved. A first general consideration, with this respect, is
that Theorem \ref{thm:genus_1constr} holds true also when using the standard Krasnoselskii genus instead of $\gamma$; this allows to obtain critical points having Morse index bounded from below (see \cite{MR968487,MR954951,MR991264}), and therefore to obta
in infinitely many solutions, at least when $\rho$ is less than some threshold. More specifically, we can also prove the existence of a second solution in the supercritical case, thus extending to any $\Omega$ the multiplicity result obtained in \cite{MR33
18740} for the ball. Indeed, on the one hand, in the supercritical case ${\mathcal{E}}_\mu$ is unbounded from below; on the other hand the solution obtained in Theorem \ref{thm:genus_1constr}, for $k=1$, is a local minimum. Thus the Mountain Pass Theorem \
cite{MR0370183} applies on $\mathcal{M}$, and a second solution can be found for $\mu<\hat\mu_1$, see Proposition \ref{mpcritlev} for further details (and also Remark \ref{rem:further_crit_lev} for an analogous construction for $k\ge2$). To conclude thi
s introduction, let us mention that the explicit lower bounds obtained in Theorem \ref{thm:intro_GS} can be easily applied in order to gain much more information also in the case of special domains, as those considered in Remark \ref{rem:specialdomains}. F
or instance, we can prove then following. \begin{theorem}\label{pro:symm} Let $\Omega=B$ be a ball in ${\mathbb{R}}^N$. Then \[ p<1+\frac{4}{N-1} \quad\implies\quad \text{\eqref{eq:main_prob_U} admits a solution for every }\rho>0. \] An analogous result ho
lds when $\Omega=R$ is a rectangle, without further restrictions on $p<2^*-1$. \end{theorem} Therefore our starting problem in $\Omega=B$ can be solved for any mass value also in the critical and supercritical regime, at least for $p$ smaller than this fur
ther critical exponent $1+4/(N-1) > 1+ 4/N$. Of course, higher masses require higher Morse index--solutions. In particular, since by \cite{MR3318740} we know that ${\mathfrak{A}}_1(B,1+4/N) = (0,\|Z_{N,p}\|_{L^2})$, we have that for larger masses, even tho
ugh no positive solution exists, nodal solutions with higher Morse index can be obtained: in such cases \eqref{eq:main_prob_U} admits \emph{nodal ground states with higher Morse index}. The paper is structured as follows: in Section \ref{sec:blow-up} we p
erform a blow-up analysis of solutions with bounded Morse index, in order to prove Theorem \ref{thm:bbd_index}; Section \ref{sec:2const} is devoted to the analysis of the variational problem with two constraints \eqref{maxmin} and to the proof of Theorem \
ref{thm:genus_2constr}; that of Theorems \ref{thm:genus_1constr}, \ref{thm:intro_GS} and Proposition \ref{thm:intro_3>1} is developed in Section \ref{sec:1const}, by means of the variational problem with one constraint \eqref{infsuplev}; finally, Section \
ref{sec:symm} contains the proof of Theorem \ref{pro:symm}. \textbf{Notation.} We use the standard notation $\{\varphi_k\}_{k\geq1}$ for a basis of eigenfunctions of the Dirichlet laplacian in $\Omega$, orthogonal in $H^1_0(\Omega)$ and orthonormal in $
L^2(\Omega)$. Such functions are ordered in such a way that the corresponding eigenvalues $\lambda_k(\Omega)$ satisfy \[ 0<\lambda_1(\Omega)<\lambda_2(\Omega)\leq\lambda_3(\Omega)\leq\dots, \] and $\varphi_1$ is chosen to be positive on $\Omega$. $C_{N,p}$
denotes the universal constant in the Gagliardo-Nirenberg inequality \eqref{sobest}, which is achieved (uniquely, up to translations and dilations) by the positive, radially symmetric function $Z_{N,p}\in H^1({\mathbb{R}}^N)$, with \[ \|Z_{N,p}\|^2_{L^2({
\mathbb{R}}^N)}=\left(\frac{p+1}{2C_{N,p}}\right)^{N/2}. \] Finally, $C$ denotes every (positive) constant we need not to specify, whose value may change also within the same formula. \section{Blow-up analysis of solutions with bounded Morse index}\label{
sec:blow-up} Throughout this section we will deal with a sequence $\{(u_n,\mu_n,\lambda_n)\}_n \subset H^1_0(\Omega)\times{\mathbb{R}}^+\times{\mathbb{R}}$ satisfying \begin{equation}\label{eq:auxiliary_n} -\Delta u_n+\lambda_n u_n=\mu_n |u_n|^{p-1}u_n,\q
quad\int_\Omega u_n^2\, dx=1,\qquad \int_\Omega |\nabla u_n|^2\, dx=:\alpha_n. \end{equation} To start with, we recall the following result (actually, in \cite{MR3318740}, the result is stated for positive solution, but the proof does not require such assu
mption). \begin{lemma}[{\cite[Lemma 2.5]{MR3318740}}]\label{lemma:case_alpha_n_bounded} Take a sequence $\{(u_n,\mu_n,\lambda_n)\}_n$ as in \eqref{eq:auxiliary_n}. Then \[ \{\alpha_n\}_n \text{ bounded} \qquad\implies\qquad \{\lambda_n\}_n,\,\{\mu_n\}_n\te
xt{ bounded}. \] \end{lemma} Next we turn to the study of sequences having arbitrarily large $H^1_0$-norm. In particular, we will focus on sequences of solutions having a common upper bound on the Morse index \[ m(u_n) = \max\left\{k : \begin{array}{l} \ex
ists V\subset H^1_0(\Omega),\,\dim(V)= k:\forall v\in V\setminus\{0\}\smallskip\\ \displaystyle\int_\Omega |\nabla v|^2 + \lambda_n v^2 - p\mu_n|u_n|^{p-1}v^2\,dx<0 \end{array} \right\}. \] Throughout this section we will assume that \begin{equation}\label
{eq:mainass_secMorse} \text{the sequence }\{(u_n,\mu_n,\lambda_n)\}_n\text{ satisfies \eqref{eq:auxiliary_n}, with }\alpha_n\to+\infty\text{ and }m(u_n)\leq \bar k, \end{equation} for some $\bar k\in{\mathbb{N}}$ not depending on $n$. \begin{lemma}\label{l
em:lambda_bdd_below} Let \eqref{eq:mainass_secMorse} hold. Then \( \lambda_n \geq -\lambda_{\bar k}(\Omega). \) \end{lemma} \begin{proof} Assume, to the contrary, that for some $n$ it holds $\lambda_n < -\lambda_{\bar k}(\Omega)$. For any real $t_1,\dots t
_{\bar k}$ we define \[ \phi := \sum_{h=1}^{\bar k} t_h \varphi_h. \] By denoting $J_{\lambda,\mu}(u)={\mathcal{E}}_\mu(u)+\frac{\lambda}{2}\|u\|_{L^2}^2$, so that Morse index properties can be written in terms of $J''_{\lambda,\mu}$, we have \[ \begin{spl
it} J''_{\lambda_n,\mu_n}(u_n)[u_n,\phi] &= -(p-1)\mu_n\int_\Omega |u_n|^{p-1}u_n\phi,\\ J''_{\lambda_n,\mu_n}(u_n)[\phi,\phi] &= \sum_{h=1}^{\bar k} t_h^2 \int_\Omega \bigl (|\nabla \varphi_h| + \lambda_n \varphi_h^2\bigr )\,dx - p\mu_n\int_\Omega |u_n
|^{p-1}\phi^2\,dx \\ &\leq \sum_{h=1}^{\bar k} t_h^2(\lambda_{h}(\Omega) + \lambda_n) - (p-1)\mu_n\int_\Omega |u_n|^{p-1}\phi^2\,dx \leq - (p-1)\mu_n\int_\Omega |u_n|^{p-1}\phi^2\,dx, \end{split} \] where equality holds if and only if $t_1=\dots=t_{\ba
r k}=0$. As a consequence \begin{multline*} J''_{\lambda_n,\mu_n}(u_n)[t_0 u_n+ \phi, t_0 u_n + \phi] \leq -t_0^2 (p-1)\mu_n\int_\Omega |u_n|^{p-1}u_n^2 \\ - 2t_0(p-1)\mu_n\int_\Omega |u_n|^{p-1}u_n\phi \,dx - (p-1)\mu_n\int_\Omega |u_n|^{p-1}\phi^2\,dx.
\end{multline*} We deduce that $J''_{\lambda_n,\mu_n}(u_n)$ is negative definite on $\spann\{u_n, \varphi_1,\dots,\varphi_{\bar k}\}$, in contradiction with the bound on the Morse index (note that $u_n$ cannot be a linear combination of a finite number of
eigenfunctions, otherwise using the equations we would obtain that such eigenfunctions are linearly dependent). \end{proof} \begin{lemma} \label{localblow} Let \eqref{eq:mainass_secMorse} hold. Then $\lambda_n\to +\infty$. \end{lemma} \begin{proof} By Lem
ma \ref{lem:lambda_bdd_below} we have that $\lambda_n$ is bounded below. As a consequence, we can use H\"{o}lder inequality with $\|u_n\|_{L^2}=1$ and \eqref{eq:auxiliary_n} to write \[ \mu_n\,\|u_n\|^{p-1}_{L^{\infty}}\ge \mu_n \,\|u_n\|^{p+1}_{L^{p+1}}=\
alpha_n+\lambda_n \rightarrow +\infty. \] Let us define \begin{equation} \label{equn} U_n: =\mu_n^{\frac{1}{p-1}}\,u_n, \quad\text{ so that } -\Delta U_n+\lambda_n U_n=|U_n|^{p-1}U_n\quad \text{in}\,\,\Omega,\quad U|_{\partial\Omega}=0. \end{equation} Pick
$P_n\in\Omega$ such that $|U_n(P_n)|=\|U_n\|_{L^{\infty}(\Omega)}$ and set \begin{equation} \label{tildepsn} \tilde\varepsilon_n: =|U_n(P_n)|^{-\frac{p-1}{2}}=\frac{1}{\sqrt{\mu_n\,\|u_n\|^{p-1}_{L^{\infty}}}}\longrightarrow 0 \end{equation} Hence, $|U_n(
P_n)|\to+\infty$; moreover, as $P_n$ is a point of positive maximum or of negative minimum, we have \begin{equation} \nonumber 0\le \frac{-\Delta U_n(P_n)}{U_n(P_n)}=|U_n(P_n)|^{p-1}-\lambda_n\,. \end{equation} Thus $\lambda_n|U_n(P_n)|^{1-p}\le 1$, and si
nce $\lambda_n$ is bounded from below, we conclude \begin{equation} \label{limtildelam} \frac{\lambda_n}{|U_n(P_n)|^{p-1}}\longrightarrow \tilde\lambda\in [0,1]. \end{equation} Now, we are left to prove that $\tilde\lambda>0$. Let us define \begin{equation
} \label{tildeVn} \tilde V_n(y)=\tilde\varepsilon_n^{\frac{2}{p-1}}\, U_n(\tilde\varepsilon_n\,y+P_n),\quad\quad y\in \tilde\Omega_n :=\big (\Omega-P_n\big )/\tilde\varepsilon_n, \end{equation} and let $d_n := d(P_n,\partial\Omega)$; we have, up to subsequ
ences, \[ \frac{\tilde\varepsilon_n}{d_n}\longrightarrow L\in [0,+\infty] \qquad\text{and}\qquad \tilde\Omega_n\rightarrow\left\{ \begin{array}{ll} {\mathbb{R}}^n, & \text{if $L=0$;} \\ H, & \text{if $L>0
$,} \end{array} \right. \] where $H$ is a half-space such that $0\in \overline H$ and $d(0,\partial H)=1/L$. The function $\tilde V_n$ satisfies \begin{equation} \nonumber \left\{ \begin{array}{ll} -\Delta \tilde V_n+\la
mbda_n\,\tilde \varepsilon_n^2\,\tilde V_n=|\tilde V_n|^{p-1}\tilde V_n, & \hbox{in}\,\, \tilde\Omega_n;\\ |\tilde V_n|\le |\tilde V_n(0)|=1, & \hbox{in}\,\, \tilde\Omega_n;\\ \tilde V_n=0, & \hbox{on}\,\, \partial\tilde \Omega_n. \end{array} \ri
ght. \end{equation} From \eqref{tildepsn} and \eqref{limtildelam} we get $\tilde\varepsilon_n^2\,\lambda_n\rightarrow \tilde\lambda$; hence, by elliptic regularity and up to a further subsequence, $\tilde V_n\rightarrow \tilde V$ in $\mathcal{C}^1_{{\mathr
m{loc}}}(\overline H)$ where $\tilde V$ solves \begin{equation} \label{limprob1} \left\{ \begin{array}{ll} -\Delta \tilde V+\tilde\lambda\,\tilde V=|\tilde V|^{p-1}\tilde V, & \hbox{in}\,\, H;\\ |\tilde V|\le |\tilde V(0)|=1, & \hbox{in}\,\, H;\\
\tilde V=0, & \hbox{on}\,\, \partial H. \end{array} \right. \end{equation} Since $\sup_n m(U_n)\leq \bar k$ (as a solution to \eqref{equn}), one can show as in Theorem $3.1$ of \cite{MR2825606} that $m(\tilde V)\leq \bar k$. In particular, $\tilde V
$ is stable outside a compact set (see Definition $2.1$ in \cite{MR2825606}) so that, by Theorem $2.3$ and Remark $2.4$ of \cite{MR2825606}, we have $$\tilde V(x)\rightarrow 0 \quad\quad \text{as} \quad\quad |x|\rightarrow +\infty.$$ Moreover, since $\til
de V$ is not trivial, we also have that $\tilde\lambda>0$. For, if $\tilde\lambda=0$ the function $\tilde V$ would be a solution of the Lane-Emden equation $-\Delta u=|u|^{p-1}u$ either in ${\mathbb{R}}^n$ or in $H$. In both cases, $\tilde V$ would contra
dict Theorems $2$ and $9$ of \cite{MR2322150}, being non trivial and stable outside a compact set. Thus, $\tilde\lambda >0$ and by \eqref{limtildelam} we conclude $\lambda_n\rightarrow +\infty$. \end{proof} \begin{remark}\label{rem4} We stress that the sca
ling argument in Lemma \ref{localblow}, leading to the limit problem \eqref{limprob1} (with $\tilde\lambda>0$), can be repeated also near points of \emph{local} extremum. More precisely, let $Q_n$ be such that $|U_n(Q_n)|\to +\infty$ and $$ |U_n(Q_n)|=\max
_{\Omega\cap B_{R_n\tilde\varepsilon_n}(Q_n)}U_n, $$ for some $R_n\to +\infty$. Then the above procedure can be repeated by replacing $P_n$ with $Q_n$ in definition \eqref{tildepsn}. \end{remark} The local description of the asymptotic behaviour of the so
lutions $U_n$ to \eqref{equn} with bounded Morse index can be carried out more conveniently by defining the sequence (see \cite[Theorem $3.1$]{MR2825606}) \begin{equation} \label{defVn} V_n(y)=\varepsilon_n^{\frac{2}{p-1}}\, U_n(\varepsilon_n\,y+P_n),\quad
y\in \Omega_n :=\frac{\Omega-P_n}{\varepsilon_n}, \end{equation} where $P_n$ is defined before \eqref{tildepsn}, and $\varepsilon_n=\frac{1}{\sqrt{\lambda_n}}\to 0$. Then, $V_n$ satisfies \begin{equation} \nonumber \left\{ \begin{array}{ll} -\Delta
V_n+ V_n=| V_n|^{p-1} V_n, & \hbox{in}\,\,\Omega_n;\\ |V_n|\le | V_n(0)|=\big ({\varepsilon_n/\tilde\varepsilon_n}\big )^{\frac{2}{p-1}}\rightarrow \tilde\lambda^{-\frac{1}{p-1}}, & \hbox{in}\,\, \Omega_n;\\ V_n=0, & \hbox{on}\,\, \partial\Omega_n.
\end{array} \right. \end{equation} As before, we have (up to a subsequence) $V_n\rightarrow V$ in $\mathcal{C}^1_{\mathrm{loc}}(\overline H)$ where $H$ is either ${\mathbb{R}}^N$ or a half space and $V$ solves \begin{equation} \label{limprob2} \left\{
\begin{array}{ll} -\Delta V+ V=| V|^{p-1} V, & \hbox{in}\,\, H;\\ |V|\le | V(0)|=\tilde\lambda^{-\frac{1}{p-1}}, & \hbox{in}\,\, H;\\ V=0, & \hbox{on}\,\, \partial H. \end{array} \right. \end{equation} By recalling the discussion followin
g \eqref{limprob1} we also have $m(V)<+\infty$. We collect some well known property of such a $V$ in the following result. \begin{theorem}[\cite{MR688279,MR2825606,MR2322150,MR2785899}]\label{thm:unif_est_Farina} Let $V$ be a classical solution to \eqref{l
improb2} such that $m(V)\leq\bar k$. Then: \begin{enumerate} \item $H={\mathbb{R}}^N$; \item $V(x)\to 0$ as $|x|\rightarrow +\infty$, $V \in H^1({\mathbb{R}}^N)\cap L^{p+1}({\mathbb{R}}^N)$; \item there exist $C$ only depending on $\bar k$ (and not on $
V$) such that \[ \|V\|_{L^{\infty}} + \|\nabla V\|_{L^{\infty}}<C. \] \end{enumerate} \end{theorem} \begin{proof} Claim 2 follows from Theorem 2.3 and Remark 2.4 of \cite{MR2825606}, see also \cite[Remark 1.4]{MR688279}. As a consequence, Theorem 1.1 of
\cite[Remark 1.4]{MR688279} readily applies, providing claim 1 ($V$ is not trivial as $V(0)>0$). On the other hand, the $L^\infty$ estimates in claim 3. are proved in Theorem 1.9 of \cite{MR2785899}. \end{proof} \begin{corollary} \label{distpnbound} If th
e sequence $\{U_n\}$ of solutions to \eqref{equn} has uniformly bounded Morse index, and if $P_n\in\Omega$ is such that $|U_n(P_n)|=\|U_n\|_{L^{\infty}(\Omega)}\to+\infty$, then $$ \sqrt{\lambda_n}\,d(P_n,\partial\Omega)\rightarrow +\infty,\qquad\text{whe
re }\frac{\lambda_n}{|U_n(P_n)|^{p-1}}\to\tilde\lambda\in(0,1]. $$ \end{corollary} \begin{remark} Recall that $Z_{N,p}$, the unique positive solution to $-\Delta u+ u=| u|^{p-1} u$ in ${\mathbb{R}}^N$, has Morse index $1$ \cite{MR969899}; then, if $V$ sol
ves \eqref{limprob2} in ${\mathbb{R}}^N$ and $1<m(V)<+\infty$, then $V$ is necessarily sign-changing. \end{remark} Following the same pattern as in \cite{MR2825606}, we now analyze the global behaviour of a sequence $\{U_n\}$ of solutions to \eqref{equn}
for $\lambda_n\to +\infty$, assuming that \( \lim_{n\to +\infty} m(U_n)\leq\bar k<\infty. \) By the previous discussion, if $P^1_n$ is a sequence of points such that $|U_n(P^1_n)|=\|U_n\|_{L^{\infty}(\Omega)}$, we have $|U_n(P^1_n)|\rightarrow +\infty$ an
d ${\lambda_n}\,d(P^1_n,\partial\Omega)^2\rightarrow +\infty$. We now look for other possible sequences of (local) extremum points $P^i_n$, $i=2,3,..$, along which $|U_n|$ goes to infinity. For any $R>0$, consider the quantity \begin{equation} \nonumber h_
1(R)=\limsup_{n\to +\infty} \Bigl (\lambda_n^{-\frac{1}{p-1}}\max_{|x-P^1_n|\ge R\,\lambda_n^{-1/2}} |U_n(x)| \Bigr ). \end{equation} We will prove that if $h_1(R)$ is \emph{not vanishing} for large $R$, then there exists a 'blow-up' sequence $P^2_n$ for $
u_n$, 'disjoint' from $P^1_n$. Indeed, let us suppose that \begin{equation} \nonumber \limsup_{R\to +\infty} h_1(R)=4\delta>0. \end{equation} Hence, up to a subsequence and for arbitrarily large $R$, we have \begin{equation} \label{ass1} \lambda_n^{-\frac{
1}{p-1}}\max_{|x-P^1_n|\ge R\,\lambda_n^{-1/2}} |U_n(x)| \ge 2\delta. \end{equation} Since $U_n$ vanishes on $\partial\Omega$, there exists $P^2_n\in\Omega\backslash B_{R\,\lambda_n^{-1/2}}(P_n^1)$ such that \begin{equation} \label{pn2} |U_n(P_n^2)|=\max_{
|x-P^1_n|\ge R\,\lambda_n^{-1/2}}|U_n(x)|. \end{equation} Clearly, assumption \eqref{ass1} implies that $|U_n(P_n^2)|\rightarrow +\infty$. We first prove that the sequences $P_n^1$ and $P_n^2$ are far away each other. \begin{lemma} \label{disj} Take $R$ su
ch that \eqref{ass1} holds, and let $P_n^2$ be defined as in \eqref{pn2}; then \begin{equation} \label{limp1p2} \lambda_n^{1/2}|P_n^2-P^1_n|\rightarrow +\infty \end{equation} as $n\to \infty$. \end{lemma} \begin{proof} Assuming the contrary one would get,
up to a subsequence \[ \lambda_n^{1/2}|P_n^2-P^1_n|\rightarrow R'\ge R. \] Let us now recall that by \eqref{defVn} and the subsequent discussion, we have: \begin{equation} \label{limblowseq} \lambda_n^{-\frac{1}{p-1}}\, U_n(\lambda_n^{-1/2}\,y+P^1_n) =: V^
1_n(y)\rightarrow V(y)\quad \textrm{in} \,\, \mathcal{C}^1_{{\mathrm{loc}}}({\mathbb{R}}^N) \end{equation} as $n\to +\infty$. Then, up to subsequences, \begin{equation} \nonumber \lambda_n^{-\frac{1}{p-1}}\,|U_n(P_n^2)|=\big |V^1_n\bigr(\lambda_n^{1/2}(P_n
^2-P^1_n)\bigl)\big| \rightarrow \big |V(y')\big |,\quad |y'|=R'\ge R. \end{equation} Since $V$ is vanishing for $|y|\to +\infty$, one can choose $R$ such that $|V(y)|\le\delta$ for every $ |y|\ge R$. But this contradicts \eqref{ass1}. \end{proof} Furtherm
ore, we also have that the blow-up points stay far away from the boundary. \begin{lemma} \label{distbd} Assume \eqref{ass1} and let $P_n^2$ be defined as in \eqref{pn2}; then \begin{equation} \label{distp2nbound} \sqrt{\lambda_n}\,d(P^2_n,\partial\Omega)\r
ightarrow +\infty \end{equation} as $n\to \infty$. Moreover, \begin{equation} \label{maxp2nball} |U_n(P_n^2)|=\max_{\Omega\cap B_{R_n\lambda^{-1/2}_n}(P^2_n)}|U_n| \end{equation} for some $R_n\to +\infty$. \end{lemma} \begin{proof} Let us set \begin{equati
on} \nonumber \tilde\varepsilon^2_n: =|U_n(P^2_n)|^{-\frac{p-1}{2}}\quad \mathrm{and} \quad R_n^{(2)}:=\frac{1}{2}\,\frac{|P_n^2-P_n^1|}{\tilde\varepsilon^2_n}. \end{equation} Clearly, $\tilde\varepsilon^2_n\rightarrow 0$; moreover, by \eqref{ass1} and \eq
ref{pn2}, $\tilde\varepsilon^2_n\le (2\delta)^{-\frac{p-1}{2}}\lambda_n^{-1/2}$, so that $$R^{(2)}_n\ge \frac{(2\delta)^{\frac{p-1}{2}}}{2}\,\lambda_n^{1/2}\,{|P_n^2-P_n^1|} \rightarrow +\infty, $$ as $n\to +\infty$ by Lemma \ref{disj}. We claim that this
implies \begin{equation} \label{maxp2n} |U_n(P_n^2)|=\max_{\Omega\cap B_{R^{(2)}_n\tilde\varepsilon^2_n}(P^2_n)}| U_n|. \end{equation} For, if $x\in B_{R^{(2)}_n\tilde\varepsilon^2_n}(P^2_n)$, by \eqref{limp1p2} we would have $$|x-P^1_n|\ge |P^2_n-P^1_n|-
|x-P^2_n|\ge \frac{1}{2}\,|P^2_n-P^1_n|\ge R\,\lambda_n^{-1/2},$$ for arbitrarily large $R$. This means that $$\Omega\cap B_{R^{(2)}_n\tilde\varepsilon^2_n}(P^2_n)\subset \Omega\backslash B_{R\,\lambda_n^{-1/2}}(P^1_n).$$ Then, the claim follows. Now, by r
ecalling Remark \ref{rem4}, we can apply to $U_n$ satisfying \eqref{maxp2n} the same scaling arguments as in the proof of Lemma \ref{localblow}, so that we conclude $$ 0< \lim_{n\to +\infty}\tilde\varepsilon_n^2\,\sqrt{\lambda_n}. $$ Hence, \eqref{maxp2nb
all} holds by defining $R_n=R^{(2)}_n\tilde\varepsilon_n^2\,\sqrt{\lambda_n}$, and \eqref{distp2nbound} follows by Corollary \ref{distpnbound}. \end{proof} We can now iterate the previous arguments: let us define, for $k\ge 1$, \begin{equation} \label{d
efhn} h_k(R)=\limsup_{n\to +\infty} \Bigl (\lambda_n^{-\frac{1}{p-1}}\max_{d_{n,k}(x)\ge R\,\lambda_n^{-1/2}} |U_n(x)| \Bigr ), \end{equation} where $$d_{n,k}(x): =\min\{|x-P^i_n|\,:\, i=1,...,k\}$$ and the sequences $P^i_n$ are such that \begin{equation}
\nonumber \sqrt{\lambda_n}\,d(P^i_n,\partial\Omega)\rightarrow +\infty;\quad \lambda_n^{1/2}|P_n^i-P^j_n|\rightarrow +\infty,\quad\quad i,j=1,...,k,\quad i\neq j \end{equation} as $n\to +\infty$. Assume that $$\limsup_{n\to +\infty} h_k(R)=4\delta>0.$$ As
before, up to a subsequence and for arbitrarily large $R$, we have \begin{equation} \label{assk} \lambda_n^{-\frac{1}{p-1}}\max_{d_{n,k}(x)\ge R\,\lambda_n^{-1/2}} |U_n(x)| \ge 2\delta \end{equation} and there exist $P^{k+1}_n$ so that \begin{equation} \no
number |U_n(P_n^{k+1})|=\max_{d_{n,k}(x)\ge R\,\lambda_n^{-1/2}}|U_n(x)| \end{equation} with $\lim_{n\to +\infty}|U_n(P_n^{k+1})|=+\infty$. Moreover, as in Lemma \ref{disj} we deduce that, for every $i=1,...,k$ \begin{equation} \label{limblowseqi} \lambda_
n^{-\frac{1}{p-1}}\,U_n(\lambda_n^{-1/2}\,y+P^i_n): = V^i_n(y)\rightarrow V^i(y)\quad \textrm{in} \,\, \mathcal{C}^1_{{\mathrm{loc}}}({\mathbb{R}}^N) \end{equation} as $n\to +\infty$; hence, by \eqref{assk} and again from the vanishing of $V$ at infinity,
we conclude that \begin{equation} \lambda_n^{1/2}|P_n^{k+1}-P^i_n|\rightarrow +\infty \end{equation} as $n\to \infty$, for every $i=1,...,k$. Setting now \begin{equation} \nonumber \tilde\varepsilon^{k+1}_n: =|U_n(P^{k+1}_n)|^{-\frac{p-1}{2}}\quad \mathrm{
and} \quad R_n^{(k+1)}:=\frac{1}{2}\,\frac{d_{n,k}(P^{k+1}_n)}{\tilde\varepsilon^{k+1}_n} \end{equation} we still have $\tilde\varepsilon^{k+1}_n\to 0$ and, by \eqref{assk}, $R_n^{(k+1)} \to +\infty$ as $n\to \infty$ (see Lemma \ref{distbd}). Then, by th
e same arguments as in Lemma \ref{distbd}, we get \begin{equation} \label{maxpkn} |U_n(P_n^{k+1})|=\max_{\Omega\cap B_{R^{(k+1)}_n\tilde\varepsilon^{k+1}_n}(P^{k+1}_n)} |u_n|\,, \end{equation} and furthermore $$ \lim_{n\to +\infty}\tilde\varepsilon_n^{k+1}
\,\sqrt{\lambda_n}>0\,,$$ so that by defining $R_n=:R^{(k+1)}_n\tilde\varepsilon_n^{k+1}\,\sqrt{\lambda_n}\rightarrow +\infty$ we have \begin{equation} \label{maxpknball} |U_n(P_n^{k+1})|=\max_{\Omega\cap B_{R_n\lambda^{-1/2}_n}(P^{k+1}_n)}| U_n|. \end{equ
ation} Now, by the same arguments as in \cite{MR2825606}, it turns out that the iterative procedure must stop after \emph{at most} $\bar k-1$ steps, where $\bar k =\lim_{n\to +\infty} m(u_n)$. Thus, we have proved: \begin{proposition} \label{glob1} Let $\{
U_n\}_n$ be a solution sequence to \eqref{equn} such that $\lambda_n\to+\infty$ and $m(U_n)\leq\bar k$. Then, up to a subsequence, there exist $P_n^1,...,P_n^k$, with $k\le \bar k$ such that \begin{equation} \label{limpin} \sqrt{\lambda_n}\,d(P^i_n,\partia
l\Omega)\rightarrow +\infty;\quad \lambda_n^{1/2}|P_n^i-P^j_n|\rightarrow +\infty,\quad\quad i,j=1,...,k,\quad i\neq j \end{equation} as $n\to +\infty$ and \begin{equation} \nonumber |U_n(P_n^{i})|=\max_{\Omega\cap B_{R_n\lambda^{-1/2}_n}(P^{i}_n)}|U_n|,\q
uad i=1,...,k, \end{equation} for some $R_n\to +\infty$ as $n\to +\infty$. Finally, \begin{equation} \label{limhr0} \lim_{R\to +\infty} h_k(R)=0 \end{equation} where $h_k(R)$ is given by \eqref{defhn}. \end{proposition} We now show that the sequence $U_n$
decays exponentially away from the blow-up points. \begin{proposition} \label{glob2} Let $\{U_n\}_n$ satisfy the assumptions of Proposition \ref{glob1}. Then, there exist $P_n^1,...,P_n^k$ and positive constants $C$, $\gamma$, such that \begin{equation} \l
abel{stimglob} |U_n(x)|\le C\lambda^{\frac{1}{p-1}}_n \sum_{i=1}^ke^{-\gamma\sqrt{\lambda_n}|x-P_n^i|}\,,\quad\quad \forall \,x\in\Omega,\quad n\in{\mathbb{N}}\,. \end{equation} \end{proposition} \begin{proof} By \eqref{limhr0}, for large $R>0$ and $n>n_0(
R)$ it holds \begin{equation} \nonumber \lambda_n^{-\frac{1}{p-1}}\max_{d_{n,k}(x)\ge R\,\lambda_n^{-1/2}} |U_n(x)| \le \Bigr (\frac{1}{2p} \Bigl )^{\frac{1}{p-1} } \end{equation} Then, for $n>n_0(R)$ and for $x\in \{d_{n,k}(x)\ge R\,\lambda_n^{-1/2}\}$,
we have \begin{equation} \nonumber a_n(x): = \lambda_n-p |U_n(x)|^{p-1}\ge \lambda_n-\frac{\lambda_n}{2}=\frac{\lambda_n}{2} \end{equation} We stress that the linear operator \begin{equation} \nonumber L_n: =-\Delta + a_n(x) \end{equation} comes from the l
inearization of equation \eqref{equn} at $U_n$; let us compute this operator on the functions $$\phi^i_n(x)=e^{-\gamma\sqrt{\lambda_n}\,|x-P^i_n|}\,,\quad\quad \gamma>0,\quad\quad i=1,...,k$$ in $\{d_{n,k}(x)\ge R\,\lambda_n^{-1/2}\}$. We obtain: $$L_n \ph
i^i_n(x)=\lambda_n\phi^i_n(x)\Bigr [-\gamma^2+(N-1)\frac{\gamma}{\sqrt{\lambda_n}\,|x-P^i_n|} +\frac{a_n(x)}{\lambda_n}\Bigl ]\ge \lambda_n\phi^i_n(x)\bigr [-\gamma^2+1/2\bigl ]\ge 0$$ for $n$ large, provided $0<\gamma\le 1/\sqrt 2$. Moreover, for $|x-P^i_
n|=R\lambda_n^{-1/2}$, $ i=1,...,k,$ and $R$ large we have $$ e^{\gamma R}\phi^i_n(x)-\lambda_n^{-\frac{1}{p-1}}|U_n(x)|= 1-\lambda_n^{-\frac{1}{p-1}}|U_n(x)|>0 $$ as $n\to +\infty$, by \eqref{limblowseq}. Note further that $$\{x:d_{n,k}(x)= R\,\lambda_n^{
-1/2}\} = \bigcup_{i=1}^k \partial B_{R\,\lambda_n^{-1/2}}(P_n^i) \subset \Omega$$ for large enough $n$. Then, by defining \begin{equation} \nonumber \phi_n: = e^{\gamma R}\lambda_n^{\frac{1}{p-1}}\sum_{i=1}^k \,\phi^i_n \end{equation} we have $$\phi_n(x)-
|U_n(x)|\ge 0\quad\quad \mathrm{on}\quad\quad\{d_{n,k}(x)= R\,\lambda_n^{-1/2}\}\cup\partial\Omega$$ and \begin{equation} \nonumber L_n(\phi_n-|U_n|)\ge -L_n\,|U_n|=\Delta \,|U_n|-\lambda_n\,|U_n|+p|U_n|^p\ge (p-1)\,|U_n|^p\ge 0 \end{equation} in $\Omega\b
ackslash \{d_{n,k}(x)\le R\,\lambda_n^{-1/2}\}$. Then (for $R$ large and $n\ge n_0(R)$) we obtain $|U_n|\le \phi_n$ in the same set, by the minimum principle. Moreover, since by \eqref{limtildelam} $$|U_n(x)|\le\|U_n\|_{L^{\infty}(\Omega)}=|U_n(P^1_n)|\le
C \lambda_n^{\frac{1}{p-1}}$$ for some $C>0$, we also have, in $\{d_{n,k}(x)\le R\,\lambda_n^{-1/2}\}$, $$ |U_n(x)|\le\|U_n(x)\|_{L^{\infty}(\Omega)}=|U_n(P^1_n)|\le C e^{\gamma R}\lambda_n^{\frac{1}{p-1}}\sum_{i=1}^k e^{-\gamma\sqrt{\lambda_n}|x-P_n^i
|}. $$ Then, possibly by choosing a larger $C$, estimate \eqref{stimglob} follows for every $n$. \end{proof} We now exploit the previous results to show that suitable rescalings of the solutions to \eqref{eq:auxiliary_n} converge (locally) to some bounded
solution $V$ of \begin{equation} \label{eqV} -\Delta V+ V=| V|^{p-1} V \end{equation} in ${\mathbb{R}}^N$. \begin{lemma} \label{lemlim1} Let \eqref{eq:mainass_secMorse} hold. Then $|u_n|$ admits $k\le \bar k$ local maxima $P_n^1,...,P_n^k$ in $\Omega$ su
ch that, defining \begin{equation} u_{i,n}(x)= \Bigl ( \frac{\mu_n}{\lambda_n}\Bigr )^{\frac{1}{p-1}}u_n \bigr (\frac{x} {\sqrt {\lambda_n}}+P_n^i\bigl ),\quad\quad x\in \Omega_{n,i}:=\sqrt{\lambda_n}\bigr (\Omega-P_n^i \bigl ), \end{equation} it results,
up to a subsequence, \begin{equation} u_{i,n}(x)\rightarrow V_i\quad\quad \mathrm{in}\,\,\mathcal{C}^1_{{\mathrm{loc}}}({\mathbb{R}}^n)\quad \mathrm{as}\,\,n\to +\infty,\quad \forall\,\,i=1,2,...,k, \end{equation} where $V_i$ is a bounded solution of \eqre
f{eqV} with $m(V_i)\le \bar{k}$. \noindent As a consequence, for every $q\ge 1$, \begin{equation} \label{convlq} \Bigl ( \frac{\mu_n}{\lambda_n}\Bigr )^{\frac{q}{p-1}}\lambda_n^{N/2}\int_{\Omega} |u_n|^q \,dx\rightarrow \sum_{i=1}^{k}\int_{{\mathbb{R}}^n}
|V_i|^q\,dx\quad\quad \mathrm{as}\,\, n\to +\infty. \end{equation} \end{lemma} \begin{proof} By Lemma \ref{localblow} we have $\lambda_n\to +\infty$; then, the first part of the lemma follows by definition \eqref{equn}, by \eqref{limblowseqi} and by Propos
ition \ref{glob1}; by the same proposition and by Proposition \ref{glob2} we also have that the local maxima $P^i_n$ satisfies \eqref{limpin} and that the pointwise estimate \begin{equation} \label{stimglobvn} |u_n(x)|\le C\Bigl (\frac{\lambda_n}{\mu_n}\Bi
gr )^{\frac{1}{p-1}} \sum_{i=1}^ke^{-\gamma\sqrt{\lambda_n}|x-P_n^i|}\,,\quad\quad \forall \,x\in\Omega,\quad n\in{\mathbb{N}}\,. \end{equation} holds. Let us fix $R>0$ and set $r_n=R/\sqrt{\lambda_n}$; for large enough $n$, \eqref{limpin} implies $$B_{r_n
}(P^i_n)\subset \Omega,\quad\quad B_{r_n}(P^i_n)\cap B_{r_n}(P^j_n)=\emptyset, \quad i\neq j.$$ Then we obtain \[ \begin{array}{cl} &\left |\left ( \frac{\mu_n}{\lambda_n}\right)^{\frac{q}{p-1}}\lambda_n^{N/2}\int_{\Omega} |u_n|^q \,dx- \sum_{j=1}^{k}\int_
{B_R(0)}|u_{j,n}|^q\,dx\,\,\right | \smallskip\\& =\left ( \frac{\mu_n}{\lambda_n}\right )^{\frac{q}{p-1}}\lambda_n^{N/2}\left |\int_{\Omega} |u_n|^q \,dx- \sum_{j=1}^{k}\int_{B_{r_n}(P^j_n)}|u_{n}|^q\,dx\,\,\right | \smallskip\\ &=\left ( \frac{\mu_n}{\la
mbda_n}\right )^{\frac{q}{p-1}}\lambda_n^{N/2} \int_{\Omega\backslash \bigcup_{j=1}^k\,B_{r_n}(P^j_n)} |u_n|^q \,dx \le C^q\lambda_n^{N/2} \int_{\Omega\backslash \bigcup_{j=1}^k\,B_{r_n}(P^j_n)} \left |\sum_{i=1}^ke^{-\gamma\sqrt{\lambda_n}|x-P_n^i|}\right
|^q \,dx \smallskip\\ &\le C^qk^{q-1}\lambda_n^{N/2} \sum_{i=1}^k \int_{\Omega\backslash \bigcup_{j=1}^k\,B_{r_n}(P^j_n)} e^{-q\gamma\sqrt{\lambda_n}|x-P_n^i|} \,dx \smallskip\\ &\le C^qk^{q-1}\lambda_n^{N/2} \sum_{i=1}^k \int_{{\mathbb{R}}^N\backslash \,
B_{r_n}(P^i_n)} e^{-q\gamma\sqrt{\lambda_n}|x-P_n^i|} \,dx \smallskip\\ &\le (Ck)^{q}\sum_{i=1}^k \int_{{\mathbb{R}}^N\backslash \,B_{R}(0)} e^{-q\gamma\,|y|} \,dy\le C_1 \,e^{-C_2 R}, \end{array} \] for some positive $C_1$, $C_2$. Letting $n\to +\infty$ w
e have, up to subsequences, \begin{multline*} \Bigg |\lim_{n\to +\infty}\Bigl ( \frac{\mu_n}{\lambda_n}\Bigr )^{\frac{q}{p-1}}\lambda_n^{N/2}\int_{\Omega} |u_n|^q \,dx- \sum_{i=1}^{k}\int_{B_R(0)}|V_i|^q\,dx\,\,\Bigg | \\ =\lim_{n\to +\infty}\Bigg |\Bigl (
\frac{\mu_n}{\lambda_n}\Bigr )^{\frac{q}{p-1}}\lambda_n^{N/2}\int_{\Omega} |u_n|^q \,dx- \sum_{i=1}^{k}\int_{B_R(0)}|u_{i,n}|^q\,dx\,\,\Bigg |\le C_1 \,e^{-C_2 R}. \end{multline*} Then, \eqref{convlq} follows by taking $R\to +\infty$. \end{proof} The prev
ious lemma allows us to gain some information on the asymptotic behavior of the sequences $\lambda_n$, $\mu_n$ and $\|u_n\|_{L^{p+1}(\Omega)}$. We first provide some bounds for the solutions of the limit problem \eqref{eqV} which will be useful in the sequ
el. \begin{lemma} \label{boundbelow} Let $V_i$, $i=1,\dots,k$ be as in Lemma \ref{lemlim1} (so that $m(V_i)\leq\bar k$). There exists a constant $C$, only depending on the full sequence $\{u_n\}_n$ and not on $V_i$ (and on the particular associated subsequ
ence), such that \[ \|V_i\|_{H^1}^2 = \|V_i\|_{L^{p+1}}^{p+1} \leq C. \] Furthermore, if also $m(V_i)\geq2$ (or, equivalently, if $V_i$ changes sign) the following estimates hold: \begin{equation} \label{uppstiml2} \|V_i\|^{p+1}_{L^{p+1}}> 2\,\|Z\|^{{p+1}}
_{L^{{p+1}}},\qquad \|V_i\|^2_{L^2}> 2\,\|Z\|^{2}_{L^{2}}, \end{equation} where $Z\equiv Z_{N,p}$ is the unique positive solution to \eqref{eqV}. \end{lemma} \begin{proof} To prove the bounds from above we claim that there exists $\bar R>0$, not depending
on $i$, such that $V_i$ is stable outside $\overline{B_{\bar R}}$. Then the desired estimate will follow, since \[ \|V_i\|^{p+1}_{L^{p+1}} = \int_{B_{\bar R}} |V_i|^{p+1} + \int_{{\mathbb{R}}^N\setminus B_{\bar R}} |V_i|^{p+1}, \] where the first term is u
niformly bounded by Theorem \ref{thm:unif_est_Farina}, while the second one can be estimated in an uniform way by reasoning as in the proof of \cite[Theorem 2.3]{MR2825606}. To prove the claim, recalling \eqref{defhn} and \eqref{limhr0}, let $\bar R$ be su
ch that \[ h_k(\bar R) \leq \left(\frac{1}{p}\right)^{1/(p-1)}. \] Then $|V_i(x)|^{p-1}\leq 1/p $ on ${\mathbb{R}}^N\setminus B_{\bar R}$ and thus, for any $\psi\in C^\infty_0({\mathbb{R}}^N)$, $\psi\equiv0$ in $B_{\bar R}$, it holds \[ \int_{{\mathbb{R}}^
N} |\nabla \psi|^2 + \psi^2 - p|V_i|^{p-1}\psi^2\,dx \geq \left( 1 - p \|V_i\|^{p-1}_{L^{\infty}({\mathbb{R}}^N\setminus B_{\bar R})}\right)\int_{{\mathbb{R}}^N} \psi^2 \geq 0. \] Hence $V_i$ is stable outside $B_{\bar R}$, and the first part of the lemma
follows. On the other hand, if $V_i$ is a sign-changing solution to \eqref{eqV}, the associated energy functional \begin{equation} \nonumber E(V_i)= \frac{1}{2}\|\nabla V_i\|^2_{L^2}+\frac{1}{2}\|V_i\|^2_{L^2}-\frac{1}{p+1}\|V_i\|^{p+1}_{L^{p+1}} \end{e
quation} satisfies the following \emph{energy doubling property} (see \cite{MR2263672}): $$E(V_i)>2\,E(Z)$$ On the other hand, by using the equation $E'(V_i)V_i=0$ and the Pohozaev identity one gets \begin{equation} \label{eulp} \|V_i\|^{p+1}_{L^{p+1}
}= 2\,\frac{p+1}{p-1}\,E(V_i),\qquad \|V_i\|^2_{L^2}= \frac{N+2-p\,(N-2)}{p-1}\,E(V_i) \end{equation} Since the ground state solution $Z$ satisfies the same identities, the bounds \eqref{uppstiml2} are readily verified. \end{proof} \begin{proposition} Let
\eqref{eq:mainass_secMorse} hold and the functions $V_i$ be defined as in Lemma \ref{lemlim1}. We have, as $n\to +\infty$, \begin{eqnarray} \label{convl2} {\mu_n}^{\frac{2}{p-1}}\,\lambda_n^{N/2-2/(p-1)}&\longrightarrow \sum_{i=1}^{k}\int_{{\mathbb{R}}^n}|
V_i|^2\,dx \\ \label{convlp} {\mu_n}^{\frac{p+1}{p-1}}\,\lambda_n^{N/2-(p+1)/(p-1)}\int_{\Omega} |u_n|^{p+1} \,dx&\longrightarrow \sum_{i=1}^{k}\int_{{\mathbb{R}}^n}|V_i|^{p+1}\,dx \\ \label{convl2grad} \alpha_n\,{\mu_n}^{\frac{2}{p-1}}\,\lambda_n^{N/2-(p+
1)/(p-1)}&\longrightarrow \sum_{i=1}^{k}\int_{{\mathbb{R}}^n}|\nabla V_i|^2\,dx. \end{eqnarray} \end{proposition} \begin{proof} The limits \eqref{convl2} and \eqref{convlp} follow respectively by choosing $q=2$ and $q=p+1$ in \eqref{convlq} (recall that $\
|u_n\|_{L^{2}}=1$). Furthermore, from the equations for $u_n$ and $V_k$, we have \[ \alpha_n+\lambda_n=\mu_n\|u_n\|_{L^{p+1}}^{p+1},\qquad \int_{{\mathbb{R}}^n}|\nabla V_i|^2\,dx + \int_{{\mathbb{R}}^n}|V_i|^2\,dx = \int_{{\mathbb{R}}^n}|V_i|^{p+1}\,dx, \]
and also \eqref{convl2grad} follows. \end{proof} \begin{corollary} \label{limmass} With the same assumptions as above, we have that \begin{enumerate} \item if $1<p<1+\frac{4}{N}$, then $\mu_n\to +\infty$ \item if $p=1+\frac{4}{N}$, then $\mu_n\to \big
(\sum_{i=1}^{k}\|V_i\|_{L^2}^2\big )^{2/N}\ge k^{2/N} \|Z\|_{L^2}^{4/N}$ \item if $1+\frac{4}{N}<p<2^*-1$, then $\mu_n\to 0$. \end{enumerate} Furthermore \begin{equation} \label{limalphalam} \frac{\alpha_n}{\lambda_n}\longrightarrow \frac{N(p-1)}{N+2-
p(N-2)}. \end{equation} \end{corollary} \begin{proof} The limits of $\mu_n$ follow by the previous proposition. To prove the lower bound in $2$, recall that either $V_i=Z$ or $V_i$ satisfies \eqref{uppstiml2}. Finally, taking the quotient between \eqref{co
nvl2grad} and \eqref{convl2}, we have $$ \frac{\alpha_n}{\lambda_n}\longrightarrow \frac{\sum_{i=1}^{k}\int_{{\mathbb{R}}^n}|\nabla V_i|^2\,dx}{\sum_{i=1}^{k}\int_{{\mathbb{R}}^n}| V_i|^2\,dx} $$ On the other hand, for every $i=1,2,...,k$ it holds $$ \|\na
bla V_i\|_{L^2}^2=\Bigg (\frac{\| V_i\|_{L^{p+1}}^{p+1}}{\|V_i\|_{L^2}^2} -1 \Bigg )\|V_i\|_{L^2}^2= \frac{N(p-1)}{N+2-p(N-2)}\, \|V_i\|_{L^2}^2 $$ where the last equality follows by \eqref{eulp}. By inserting this into the above limit, we get \eqref{limal
phalam}. \end{proof} \begin{proof}[Proof of Theorem \ref{thm:bbd_index}] Let $(U_n,\lambda_n)$ solve \eqref{eq:main_prob_U}, with $\rho=\rho_n\to +\infty$ and $m(U_n)\leq k$. Changing variables as in \eqref{eq:main_prob_u}, we have that $u_n=\rho_n^{-1/2}
U_n$ satisfies \eqref{eq:auxiliary_n} with $\mu_n = \rho_n^{(p-1)/2} \to +\infty$. As a consequence, Lemma \ref{lemma:case_alpha_n_bounded} guarantees that $\alpha_n\to+\infty$, and Corollary \ref{limmass} yields $p<1+4/N$. On the other hand, by direct mi
nimization of the energy one can show that, if $p<1+4/N$, for every $\rho>0$ there exists a solution of \eqref{eq:main_prob_U} having Morse index one (see also Section \ref{sec:1const}). \end{proof} \begin{remark} \label{limGN} Reasoning as above we can al
so show that \begin{equation} \label{newcnp1} \frac{\int_{\Omega} |u_n|^{p+1} \,dx}{\alpha_n^{N(p-1)/4}}\longrightarrow C_{N,p}\,\frac{\|Z\|_{L^2}^{p-1}}{\big (\sum_{i=1}^{k}\| V_i\|_{L^2}^2\big )^{(p-1)/2}}. \end{equation} \end{remark} \section{Max-min
principles with two constraints}\label{sec:2const} In this section we deal with the maximization problem with two constraints introduced in \cite{MR3318740}, aiming at considering more general max-min classes of critical points. Let ${\mathcal{M}}$ be def
ined in \eqref{Emu} and, for any fixed $\alpha>\lambda_1(\Omega)$, let $\mathcal{B}_\alpha$, $\mathcal{U}_\alpha$ be defined as in \eqref{eq:defBU}. We will look for critical points of the $\mathcal{C}^2$ functional \[ f(u)=\int_{\Omega}|u|^{p+1},\quad\qua
d\quad u\in {\mathcal{M}}, \] constrained to $\mathcal{U}_\alpha$. To start with, we notice that the topological properties of such set depend on $\alpha$. \begin{lemma}\label{lemma:tilde_U_manifold} Let $\alpha>\lambda_1(\Omega)$. Then the set \[ {\mathca
l{U}}_{\alpha}\setminus\left\{ \varphi\in {\mathcal{U}}_\alpha : -\Delta\varphi = \alpha\varphi\right\} \] is a smooth submanifold of $H^1_0(\Omega)$ of codimension 2. In particular, this property holds true for ${\mathcal{U}}_\alpha$ itself, provided $\al
pha\neq\lambda_k(\Omega)$, for every $k$. \end{lemma} \begin{proof} Let us set $F(u)=(\int_\Omega u^2\,dx-1, \ \int_\Omega|\nabla u|^2\,dx)$. For every $u\in{\mathcal{U}}_\alpha$, if the range of $F'(u)$ is ${\mathbb{R}}^2$ then ${\mathcal{U}}_\alpha$ is a
smooth manifold at $u$. Since \[ F'(u)[v]=2\left(\int_\Omega uv\,dx, \ \int_\Omega\nabla u\cdot\nabla v\,dx\right), \qquad\text{for every }v\in H^1_0(\Omega), \] and $F'(u)[u]=2(1,\alpha)$, we have that $F'(u)$ is not surjective if and only if \[ \int_\Om
ega\nabla u\cdot\nabla v\,dx = \alpha \int_\Omega uv\,dx \qquad\text{for every }v\in H^1_0(\Omega). \qedhere \] \end{proof} \begin{remark} If $\varphi$ belongs to the eigenspace corresponding to $\lambda_k(\Omega)$, then $\varphi \in {\mathcal{U}}_{\lambda
_k(\Omega)}$. As a consequence ${\mathcal{U}}_{\lambda_k(\Omega)}$ may not be smooth near $\varphi$. For instance, ${\mathcal{U}}_{\lambda_1(\Omega)}$ consists of two isolated points, $\pm\varphi_1$. \end{remark} Of course ${\mathcal{U}}_\alpha$ is closed
and odd, for any $\alpha$. Recalling Definition \ref{def:genus} we deduce that its genus $\gamma({\mathcal{U}}_\alpha)$ is well defined. \begin{lemma} If $\alpha<\lambda_{k+1}(\Omega)$, for some $k$, then $\gamma({\mathcal{U}}_\alpha)\leq k$. \end{lemma} \
begin{proof} Let $V_k:=\spann\{\varphi_1,\dots,\varphi_k\}$. Since \[ \min\left\{\int_\Omega |\nabla u|^2\,dx : u\in V_k^\perp,\, \int_\Omega u^2\,dx=1\right\}=\lambda_{k+1}(\Omega), \] we have that ${\mathcal{U}} \cap V_k^\perp = \emptyset$, thus the proj
ection \[ g := \proj_{V_k} \colon {\mathcal{U}}_\alpha \to V_k\setminus\{0\} \] is a continuous odd map of ${\mathcal{U}}_\alpha$ into $V_k\setminus\{0\}$. Now, let $h\colon{\mathbb{S}}^{m}\to {\mathcal{U}}$ be continuous and odd. Then $g\circ h$ is contin
uous and odd from ${\mathbb{S}}^{m}$ to $V_k\setminus\{0\}$, and Borsuk-Ulam's Theorem forces $m\leq k-1$. \end{proof} \begin{lemma}\label{lemma:genusbigger} If $\alpha>\lambda_{k}(\Omega)$, for some $k$, then $\gamma({\mathcal{U}}_\alpha)\geq k$. \end{lem
ma} \begin{proof} To prove the lemma we will construct a continuous map $h\colon {\mathbb{S}}^{k-1} \to {\mathcal{U}}$. Let $\ell\in{\mathbb{N}}$ be such that $\lambda_{\ell+1}(\Omega)>\alpha$. For every $i=1,\dots,k$ we define the functions \[ u_i:=\left(
\frac{\lambda_{\ell+i}(\Omega)-\alpha}{\lambda_{\ell+i}(\Omega)-\lambda_i(\Omega)}\right)^{1/2}\varphi_i +\left(\frac{\alpha-\lambda_{i}(\Omega)}{\lambda_{\ell+i}(\Omega)-\lambda_i(\Omega)}\right)^{1/2}\varphi_{\ell+i}. \] We obtain the following straightf
orward consequences: \begin{enumerate} \item as $\lambda_i(\Omega)<\alpha<\lambda_{\ell+i}(\Omega)$, for every $i$, $u_i$ is well defined; \item $\int_\Omega u_i^2\,dx=1$, $\int_\Omega |\nabla u_i|^2\,dx=\alpha$; \item for every $j\neq i$ it holds $\int
_\Omega u_iu_j\,dx=\int_\Omega \nabla u_i\cdot\nabla u_j \,dx=0$. \end{enumerate} Therefore the map $h\colon {\mathbb{S}}^{k-1} \to {\mathcal{U}}$ defined as \[ h\colon x=(x_1,\dots,x_k) \mapsto \sum_{i=1}^k x_iu_i \] has the required properties. \end{pro
of} Now we turn to the properties of the functional $f$. To start with, it satisfies the Palais-Smale (P.S. for short) condition on $\overline{\mathcal{B}}_{\alpha}$; more precisely, the following holds. \begin{lemma} \label{psball} Every P.S. sequence $u
_n$ for $f\big |_{\overline{\mathcal{B}}_{\alpha}}$ is a P.S. sequence for $f\big |_{\mathcal{U}_{\alpha}}$ and has a strongly convergent subsequence in $\mathcal{U}_{\alpha}$. \end{lemma} \begin{proof} We first show that there are no P.S. sequences in ${
\mathcal{B}_{\alpha}}$. In fact, if $u_n$ is such a sequence, there is a sequence of real numbers $k_n$ such that \begin{equation} \label{ps} \int_{\Omega}|u_n|^{p-1}u_n\,v-k_n\int_{\Omega}u_n\,v=o(1)\,\|v\|_{H^1_0} \end{equation} for every $v\in H^1_0(\Om
ega)$. Since $u_n$ is bounded in $H^1_0(\Omega)$, there is a subsequence (still denoted by $u_n$) weakly convergent to $u\in H^1_0(\Omega)$; moreover, $u_n$ converges strongly in $L^{p+1}(\Omega)$ and in $L^2(\Omega)$ to the same limit. By choosing $v=u_n$
, we see that $k_n$ is bounded, so that we can also assume that $k_n\rightarrow k$. By taking the limit of \eqref{ps} for $n\to\infty$ we get \begin{equation} \nonumber \int_{\Omega}|u|^{p-1}u\,v=k\int_{\Omega}u\,v \end{equation} for every $v\in H^1_0(\Ome
ga)$. Hence $u$ is constant, but this contradicts $u\in {\mathcal{M}}$. Now, if $u_n$ is a P.S. sequence for $f$ on ${\mathcal{U}}_{\alpha}$, there are sequences of real numbers $k_n$, $l_n$ such that \begin{equation} \label{ps1} \int_{\Omega}|u_n|^{p-1}u
_n\,v-k_n\int_{\Omega}u_n\,v-l_n\int_{\Omega}\nabla u_n\,\nabla v=o(1)\,\|v\|_{H^1_0}. \end{equation} It is readily seen that $l_n$ is bounded away from zero, otherwise \eqref{ps1} is equivalent to \eqref{ps} (for some subsequence) and we still reach a con
tradiction. Then, we can divide both sides by $l_n$ and find that there are sequences $\{\lambda_n\}_n$, $\{\mu_n\}_n$, with $\mu_n$ bounded, such that \begin{equation} \nonumber \int_{\Omega}\nabla u_n\,\nabla v+\lambda_n\int_{\Omega}u_n\,v-\mu_n\int_{\Om
ega}|u_n|^{p-1}u_n\,v=o(1)\,\|v\|_{H^1_0}. \end{equation} Now, by reasoning as before one finds that also the sequence $\{\lambda_n\}_n$ is bounded, so that by the relation $$-\Delta u_n+\lambda_n u_n-\mu_n |u_n|^{p-1}u_n=o(1)\quad \mathrm{in}\,\, H^{-1}(\
Omega)$$ and by the compactness of the embedding $H^1_0(\Omega)\hookrightarrow L^{p+1}(\Omega)$, the P.S. condition holds for the functional $f\big |_{{\mathcal{U}}_{\alpha}}$. \end{proof} We can combine the previous lemmas to prove one of the main result
s stated in the introduction. \begin{proof}[Proof of Theorem \ref{thm:genus_2constr}] Lemma \ref{psball} allows to apply standard variational methods (see e.g. \cite[Thm. II.5.7]{St_2008}). We deduce that $M_{\alpha,\,k}$ is achieved at some critical point
$u$ of $f\big |_{\mathcal{U}_{\alpha}}$. This amounts to say that $u$ satisfies \eqref{lagreq} for some real $\lambda$ and $\mu\neq 0$. We claim that there exists at least one $u\in f^{-1}(M_{\alpha,\,k})\cap \mathcal{U}_{\alpha}$ such that \eqref{lagreq}
holds with $\mu>0$. Assume by contradiction that for \emph{every} critical point of $f\big |_{\mathcal{U}_{\alpha}}$ at level $M_{\alpha,k}$ it holds $\mu< 0$ in equation \eqref{lagreq}. Let us define the functional $T:\,H^1_0(\Omega)\to {\mathbb{R}}$ as
$$T(u)=\frac{1}{2}\int_{\Omega}|\nabla u|^2.$$ By denoting with $D$ the Fr\'{e}chet derivative and by $<\,,\,>$ the pairing between $H_0^1$ and its dual $H^{-1}$, our assumption can be restated as follows: \noindent if there are $u\in f^{-1}(M_{\alpha,\,
k})\cap\mathcal{U}_{\alpha}$ and $\mu\neq 0$ such that \begin{equation} \label{lagreq1} \langle DT(u),\phi\rangle=\mu\langle Df(u),\phi\rangle \end{equation} for every $\phi\in H^1_0(\Omega)$ satisfying $\int_{\Omega}\phi u=0$ (that is for every $\phi$ ta
ngent to ${\mathcal{M}}$ at $u$) then $\mu<0$. We stress that both $DT(u)$ and $Df(u)$ in the above equation are bounded away from zero, since there are no Dirichlet eigenfunctions in $\mathcal{U}_{\alpha}$ nor critical points of $f$ on ${\mathcal{M}}$. H
ence, by denoting with $\nabla_{T{\mathcal{M}}}$ the gradient of a functional (in $H^1_0$) in the direction tangent to ${\mathcal{M}}$, if $u\in f^{-1}(M_{\alpha,\,k})\cap \mathcal{U}_{\alpha}$ then $\nabla_{T{\mathcal{M}}}T(u)$ and $\nabla_{T{\mathcal{M}}
}f(u)$ \emph{are either opposite or not parallel}. Moreover, the angle between these (non vanishing) vectors is \emph{bounded away from zero}; otherwise, we would find sequences $u_n\in \mathcal{U}_{\alpha}$, $\mu_n>0$ such that \begin{equation} \label{no
paral} (\nabla_{T{\mathcal{M}}}T(u_n),v)_{H^1_0}-\mu_n(\nabla_{T{\mathcal{M}}}f(u_n),v)_{H^1_0}=o(1)\|v\|_{H^1_0} \end{equation} for every $v\in H^1_0(\Omega)$; but since $$(\nabla_{T{\mathcal{M}}}T(u_n),v)_{H^1_0}=\int_{\Omega}\nabla u_n\,\nabla v-\lambda
_n^T\int_{\Omega}u_n\, v\,,$$ $$(\nabla_{T{\mathcal{M}}}f(u_n),v)_{H^1_0}=\int_{\Omega}|u_n|^{p-1}u_n\,v-\lambda_n^f\int_{\Omega}u_n\, v\,,$$ for suitable bounded sequences $\lambda_n^T$, $\lambda_n^f$, this is equivalent to saying that $u_n$ is a P.S. seq
uence for $f\big |_{\mathcal{U}_{\alpha}}$, so that, by Lemma \ref{psball}, we would get a constrained critical point with $\mu>0$. Then, by choosing suitable linear combinations of the above tangential components one can define a bounded $\mathcal{C}^1$
map $u\mapsto v(u)\in H_0^1(\Omega)$, with $v(u)$ tangent to ${\mathcal{M}}$ and satisfying the following property: there is $\delta>0$ such that \begin{equation} \label{diseqv} \int_{\Omega}\nabla u\,\nabla v(u)< -\delta\, ,\quad\quad \int_{\Omega}|u|^{p-
1}u\,v(u)>\delta\,, \end{equation} for every $u\in f^{-1}(M_{\alpha,\,k})\cap \mathcal{U}_{\alpha}$. By continuity and possibly by decreasing $\delta$, inequalities \eqref{diseqv} extend to \begin{equation} \label{diseqv1} f^{-1}(M_{\alpha,\,k}-\bar\vareps
ilon, M_{\alpha,\,k}+\bar\varepsilon)\cap \big (\overline{\mathcal{B}}_{\alpha} \backslash \overline{\mathcal{B}}_{\alpha-\tau}\big ) \end{equation} for small enough, positive $\bar\varepsilon$ and $\tau$. Finally, since there are no critical points of $f$
in ${\mathcal{B}}_{\alpha}$ we can take that the \emph{second of \eqref{diseqv} holds on} \begin{equation} \label{diseqv2} f^{-1}(M_{\alpha,\,k}- \bar\varepsilon, M_{\alpha,\,k}+\bar\varepsilon)\cap \overline{\mathcal{B}}_{\alpha}. \end{equation} Let $\v
arphi$ be a $\mathcal{C}^1$ function on ${\mathbb{R}}$ such that: $$0\le\varphi\le 1, \quad\varphi\equiv 1\,\, \mathrm{in}\,\,(M_{\alpha,\,k}-\bar\varepsilon/2, M_{\alpha,\,k}+\bar\varepsilon/2),\quad \varphi\equiv 0\,\, \mathrm{in}\,\,{\mathbb{R}}\backsla
sh (M_{\alpha,\,k}-\bar\varepsilon, M_{\alpha,\,k}+\bar\varepsilon),$$ and define \begin{equation} \label{vectfield} e(u)=\varphi(f(u))\,v(u). \end{equation} Clearly, $e$ is a $\mathcal{C}^1$ vector field on ${\mathcal{M}}$ and is uniformly bounded, so th
at there exists a global solution $\Phi(u,t)$ of the initial value problem $$\partial_t\Phi(u,t)=e\big (\Phi(u,t)),\quad\quad \Phi(u,0)=0.$$ By definition \eqref{vectfield} and by the first of \eqref{diseqv} (on \eqref{diseqv1}) we get $\Phi(u,t_0) \in \o
verline{\mathcal{B}}_{\alpha}$ for $t_0> 0$ and for any $u\in \overline{\mathcal{B}}_{\alpha}$; moreover, by the second inequality of \eqref{diseqv} (on \eqref{diseqv2}) there exists $\varepsilon\in (0,\bar\varepsilon)$ such that $$f(\Phi(u,t_0))>M_{\alpha
,\,k}+\varepsilon$$ for every $u\in f^{-1}(M_{\alpha,\,k}-\varepsilon, +\infty)\cap \overline{\mathcal{B}}_{\alpha}$. Now, by \eqref{maxmin}, there is $A_{\varepsilon}\subset \overline{\mathcal{B}}_{\alpha}$ such that $\gamma(A_{\varepsilon})\ge k$ and $$
\inf_{u\in A_{\varepsilon}} f(u)\ge M_{\alpha,\,k}-\varepsilon.$$ Hence, $\gamma\big (\Phi(A_{\varepsilon},t_0) \big )\ge k$ and $$\inf_{u\in \Phi(A_{\varepsilon},t_0)} f(u)\ge M_{\alpha,\,k}+\varepsilon$$ contradicting the definition of $M_{\alpha,\,k}$.
\end{proof} \begin{remark} \label{rem1} If $\mu>0$, by testing \eqref{lagreq} with $u$ and by integration by parts we readily get $\lambda>-\alpha$. An alternative lower bound, independent of $\alpha$, could be obtained by adapting arguments from \cite{MR9
68487,MR954951,MR991264} in order to prove that the Morse index of $u$ (as a solution of \eqref{lagreq}) is less or equal than $k$. Then Lemma \ref{lem:lambda_bdd_below} would provide $\lambda\geq-\lambda_{k}$. \end{remark} \begin{remark}\label{rem:MvsCNp}
By the Gagliardo-Nirenberg inequality \eqref{sobest} we readily obtain that, for every $k\geq1$, \[ M_{\alpha,k}\leq C_{N,p} \alpha^{N(p-1)/4}. \] Taking into account the previous remark, this agrees with Remark \ref{limGN}. \end{remark} We conclude this