Ricci Tensor in an Einstein Manifold












3












$begingroup$


I must prove that an hypersurface $M$ on $mathbb{R}^{n+1}$ that is Einstein and compact can be only the $n-$dimensional sphere when $n>2$



The Einstein condition we permits to say that scalar curvature of $M$ is costant because $n>2$.
The fact that it is an hypersfurface of $mathbb{R}^{n+1}$ can be use to consider the gauss equation and the Codazzi-Mainardi equation. The fist equation we say that



$H^2-|h|^2=cost=R^M$



Where $H$ is the mean curvature and $h$ is the second fundamental form of $M$.



In the case in which $n=3$ we have that



$cost=H^2-|h|^2=2lambdamu=2det(h)$



So the Gaussian curvature of $M$ is costant but $M$ is compact so it is the 2-sphere on $mathbb{R}^3$.



How can conclude in the case in which $n>3$?










share|cite|improve this question









$endgroup$

















    3












    $begingroup$


    I must prove that an hypersurface $M$ on $mathbb{R}^{n+1}$ that is Einstein and compact can be only the $n-$dimensional sphere when $n>2$



    The Einstein condition we permits to say that scalar curvature of $M$ is costant because $n>2$.
    The fact that it is an hypersfurface of $mathbb{R}^{n+1}$ can be use to consider the gauss equation and the Codazzi-Mainardi equation. The fist equation we say that



    $H^2-|h|^2=cost=R^M$



    Where $H$ is the mean curvature and $h$ is the second fundamental form of $M$.



    In the case in which $n=3$ we have that



    $cost=H^2-|h|^2=2lambdamu=2det(h)$



    So the Gaussian curvature of $M$ is costant but $M$ is compact so it is the 2-sphere on $mathbb{R}^3$.



    How can conclude in the case in which $n>3$?










    share|cite|improve this question









    $endgroup$















      3












      3








      3


      2



      $begingroup$


      I must prove that an hypersurface $M$ on $mathbb{R}^{n+1}$ that is Einstein and compact can be only the $n-$dimensional sphere when $n>2$



      The Einstein condition we permits to say that scalar curvature of $M$ is costant because $n>2$.
      The fact that it is an hypersfurface of $mathbb{R}^{n+1}$ can be use to consider the gauss equation and the Codazzi-Mainardi equation. The fist equation we say that



      $H^2-|h|^2=cost=R^M$



      Where $H$ is the mean curvature and $h$ is the second fundamental form of $M$.



      In the case in which $n=3$ we have that



      $cost=H^2-|h|^2=2lambdamu=2det(h)$



      So the Gaussian curvature of $M$ is costant but $M$ is compact so it is the 2-sphere on $mathbb{R}^3$.



      How can conclude in the case in which $n>3$?










      share|cite|improve this question









      $endgroup$




      I must prove that an hypersurface $M$ on $mathbb{R}^{n+1}$ that is Einstein and compact can be only the $n-$dimensional sphere when $n>2$



      The Einstein condition we permits to say that scalar curvature of $M$ is costant because $n>2$.
      The fact that it is an hypersfurface of $mathbb{R}^{n+1}$ can be use to consider the gauss equation and the Codazzi-Mainardi equation. The fist equation we say that



      $H^2-|h|^2=cost=R^M$



      Where $H$ is the mean curvature and $h$ is the second fundamental form of $M$.



      In the case in which $n=3$ we have that



      $cost=H^2-|h|^2=2lambdamu=2det(h)$



      So the Gaussian curvature of $M$ is costant but $M$ is compact so it is the 2-sphere on $mathbb{R}^3$.



      How can conclude in the case in which $n>3$?







      geometry riemannian-geometry riemann-surfaces






      share|cite|improve this question













      share|cite|improve this question











      share|cite|improve this question




      share|cite|improve this question










      asked Jan 14 at 20:20









      Federico FalluccaFederico Fallucca

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