Solution for Cauchy Problem $u_t-u_{xx} = 0$ belongs to the Gevrey class of order $1/2$












2















Let $u(x,t)$be the solution for the Cauchy Problem



$$u_t-u_{xx} = 0 mbox{ in $mathbb{R}times ]0, infty[$}$$ $$u(x,0)
= u_0(x) mbox{ in $mathbb{R}$} $$



where $u_0in S(mathbb{R})$(schwartz space in $mathbb{R})$. Conclude that, for each fixed $t_0>0$,
the function $xto u(x,t_0)$ belongs to the Gevrey class of order
$1/2$ in $mathbb{R}$




I already defined the Gevrey class here: $sup_K |partial^{alpha}u|le C^{|alpha|+1}alpha!^s$ then $u$ is analytic for $sle 1$ but here is the definition again:




A function $uin C^{infty}$ belongs to the Gevrey Class of order $s$
if for every compact $K$ of $Omega$ there is a constant $C$ such that



$$sup_K |partial^{alpha}u|le C^{|alpha|+1}alpha!^s, alphainmathbb{Z}_+^N$$




this exercise comes after this one:




define, for $xinmathbb{R}$,



$$v(x) = int_{mathbb{R}}e^{ixlambda-alambda^2}dlambda$$



Show that $v$ belongs to the Gevrey cass of order $1/2$ in
$mathbb{R}$




So maybe they have something in common. The last exercise above looks like a fourier transform.



UPDATE



$$||partial_x^n phi||_{L^2} = (frac{1}{sqrt{4pi t}}int|partial_{x}^n| e^{-(xsqrt{4t})^2}dx)^{1/2} = (frac{1}{sqrt{pi}}int|partial_x^n e^{-x^2}|dx)^{1/2} = ||partial_x^n phi_{1/4}||L^2$$










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    2















    Let $u(x,t)$be the solution for the Cauchy Problem



    $$u_t-u_{xx} = 0 mbox{ in $mathbb{R}times ]0, infty[$}$$ $$u(x,0)
    = u_0(x) mbox{ in $mathbb{R}$} $$



    where $u_0in S(mathbb{R})$(schwartz space in $mathbb{R})$. Conclude that, for each fixed $t_0>0$,
    the function $xto u(x,t_0)$ belongs to the Gevrey class of order
    $1/2$ in $mathbb{R}$




    I already defined the Gevrey class here: $sup_K |partial^{alpha}u|le C^{|alpha|+1}alpha!^s$ then $u$ is analytic for $sle 1$ but here is the definition again:




    A function $uin C^{infty}$ belongs to the Gevrey Class of order $s$
    if for every compact $K$ of $Omega$ there is a constant $C$ such that



    $$sup_K |partial^{alpha}u|le C^{|alpha|+1}alpha!^s, alphainmathbb{Z}_+^N$$




    this exercise comes after this one:




    define, for $xinmathbb{R}$,



    $$v(x) = int_{mathbb{R}}e^{ixlambda-alambda^2}dlambda$$



    Show that $v$ belongs to the Gevrey cass of order $1/2$ in
    $mathbb{R}$




    So maybe they have something in common. The last exercise above looks like a fourier transform.



    UPDATE



    $$||partial_x^n phi||_{L^2} = (frac{1}{sqrt{4pi t}}int|partial_{x}^n| e^{-(xsqrt{4t})^2}dx)^{1/2} = (frac{1}{sqrt{pi}}int|partial_x^n e^{-x^2}|dx)^{1/2} = ||partial_x^n phi_{1/4}||L^2$$










    share|cite|improve this question



























      2












      2








      2


      0






      Let $u(x,t)$be the solution for the Cauchy Problem



      $$u_t-u_{xx} = 0 mbox{ in $mathbb{R}times ]0, infty[$}$$ $$u(x,0)
      = u_0(x) mbox{ in $mathbb{R}$} $$



      where $u_0in S(mathbb{R})$(schwartz space in $mathbb{R})$. Conclude that, for each fixed $t_0>0$,
      the function $xto u(x,t_0)$ belongs to the Gevrey class of order
      $1/2$ in $mathbb{R}$




      I already defined the Gevrey class here: $sup_K |partial^{alpha}u|le C^{|alpha|+1}alpha!^s$ then $u$ is analytic for $sle 1$ but here is the definition again:




      A function $uin C^{infty}$ belongs to the Gevrey Class of order $s$
      if for every compact $K$ of $Omega$ there is a constant $C$ such that



      $$sup_K |partial^{alpha}u|le C^{|alpha|+1}alpha!^s, alphainmathbb{Z}_+^N$$




      this exercise comes after this one:




      define, for $xinmathbb{R}$,



      $$v(x) = int_{mathbb{R}}e^{ixlambda-alambda^2}dlambda$$



      Show that $v$ belongs to the Gevrey cass of order $1/2$ in
      $mathbb{R}$




      So maybe they have something in common. The last exercise above looks like a fourier transform.



      UPDATE



      $$||partial_x^n phi||_{L^2} = (frac{1}{sqrt{4pi t}}int|partial_{x}^n| e^{-(xsqrt{4t})^2}dx)^{1/2} = (frac{1}{sqrt{pi}}int|partial_x^n e^{-x^2}|dx)^{1/2} = ||partial_x^n phi_{1/4}||L^2$$










      share|cite|improve this question
















      Let $u(x,t)$be the solution for the Cauchy Problem



      $$u_t-u_{xx} = 0 mbox{ in $mathbb{R}times ]0, infty[$}$$ $$u(x,0)
      = u_0(x) mbox{ in $mathbb{R}$} $$



      where $u_0in S(mathbb{R})$(schwartz space in $mathbb{R})$. Conclude that, for each fixed $t_0>0$,
      the function $xto u(x,t_0)$ belongs to the Gevrey class of order
      $1/2$ in $mathbb{R}$




      I already defined the Gevrey class here: $sup_K |partial^{alpha}u|le C^{|alpha|+1}alpha!^s$ then $u$ is analytic for $sle 1$ but here is the definition again:




      A function $uin C^{infty}$ belongs to the Gevrey Class of order $s$
      if for every compact $K$ of $Omega$ there is a constant $C$ such that



      $$sup_K |partial^{alpha}u|le C^{|alpha|+1}alpha!^s, alphainmathbb{Z}_+^N$$




      this exercise comes after this one:




      define, for $xinmathbb{R}$,



      $$v(x) = int_{mathbb{R}}e^{ixlambda-alambda^2}dlambda$$



      Show that $v$ belongs to the Gevrey cass of order $1/2$ in
      $mathbb{R}$




      So maybe they have something in common. The last exercise above looks like a fourier transform.



      UPDATE



      $$||partial_x^n phi||_{L^2} = (frac{1}{sqrt{4pi t}}int|partial_{x}^n| e^{-(xsqrt{4t})^2}dx)^{1/2} = (frac{1}{sqrt{pi}}int|partial_x^n e^{-x^2}|dx)^{1/2} = ||partial_x^n phi_{1/4}||L^2$$







      real-analysis integration pde supremum-and-infimum wave-equation






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      share|cite|improve this question













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      edited Dec 5 '18 at 14:49







      Lucas Zanella

















      asked Nov 29 '18 at 15:13









      Lucas ZanellaLucas Zanella

      93411330




      93411330






















          2 Answers
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          1














          By your second box, we have the result that




          If $v_a$ is defined by
          $$v_a(x) = int_{mathbb{R}} e^{ixlambda -alambda^2};dlambda$$
          the $v_a$ is in the Gervy class of order $frac{1}{2}$.




          In fact, if you look at the result from Finding $sup_{lambda ge 0}{lambda^k e^{−alambda^2/2}}$, you see that we actually have something better:



          $$sup_{x in mathbb{R}} partial^alpha v(x) le C^{|alpha| + 1} alpha!^frac{1}{2}$$



          Moreover, $v_t$ is actually (up to a scaling factor) the fundamental solution of the heat equation. We can obtain it by taking the Fourier transform in $x$ with frequency variable $lambda$, solving the resulting ODE, and inverting the transform.



          Thus, it would suffice to prove the following result:




          $$sup_{x} partial^alpha v_t * g (x) le C^{alpha + 1}alpha!^frac{1}{2}$$ for any Schwartz class $g$.




          Note that
          $$begin{align*}
          sup_{x} |partial^alpha (v_t * g)(x)| &=leftlVert(partial^alpha v_t) * g (x)rightrVert_{L^infty}\
          &le lVert partial^alpha v_trVert_{L^infty} lVert g rVert_{L^1}\
          &le C^{|alpha|+1}lVert g rVert_{L^1} alpha!^frac{1}{2}
          end{align*}$$

          by Holder's inequality. It follows that $u(x,t) = v_t * g$ is in the Gervy class of order $frac{1}{2}$ for any fixed $t > 0$.






          share|cite|improve this answer































            2





            +100









            In this answer, all norms are spatial norms (i.e. there is no integration/supremum wrt the parameter $t_0$ that was already fixed in the question, and I have dropped the subscript $0$).



            The unique solution to the heat equation with nice initial data is well known as the convolution with the Gaussian kernel,
            $$ u(x,t) = phi_t * u_0(x) = frac1 {sqrt{4pi t}}int_{mathbb R} e^{-|x-y|^2/4t} u_0(y) dy.$$



            Then by Cauchy-Schwarz ($|int fg|le |f|_{L^2}|g|_{L^2}$ ),
            begin{align}
            &|partial_x^n u(x,t)|_{L^infty} \
            & = |(partial_x^n phi_t) * u_0|_{L^infty} \
            & = left |int_{mathbb R}partial^n_xphi_t(x-y) u_0(y) dyright |_{L_x^infty} \
            & le left | |partial^n_xphi_t(x-y)|_{L^2_y} |u_0|_{L^2}right |_{L_x^infty} \
            & = left | |partial^n_xphi_t|_{L^2} |u_0|_{L^2}right |_{L_x^infty} \
            & = |partial^n_xphi_t|_{L^2} |u_0|_{L^2} \
            &le C^{n+1} |partial_x^n phi_{1/4}|_{L^2} |u_0|_{L^2} \
            &le C_1^{n+1} |partial_x^n phi_{1/4}|_{L^2} end{align}

            Above, we used Chain rule,
            $$partial^n_xphi_t(x) = C(t) partial^n_x exp(-x^2/(4t)) = frac{1}{(sqrt{4t})^{n}} (partial_x^nphi_{1/4})(x/sqrt{4t}) $$
            and also $ int_{mathbb R} f(lambda x)^2 dx = frac1lambda int_{mathbb R} f^2(y) dy $, so that
            $$ |partial^n_xphi_t|_{L^2} le C^{n+1}|partial_x^n phi_{1/4}|_{L^2} $$
            Note that $$partial_x^n phi_{1/4}(x) = (-1)^nH_n(x) phi_{1/4}(x),$$ where $H_n$ is the $n$th (physicist) Hermite polynomial.
            The Hermite polynomials have the well known $L^2$ norm when weighted with $phi_{1/4}$ (which I quote from that same wikipedia page),
            $$int H_n^2 phi_{1/4}^2 le |phi_{1/4}|_{L^infty} int H_n^2 phi_{1/4} le C sqrt{2pi} n! $$
            Thus
            $$ |partial_x^n u(x,t)|_{L^infty} le C_2^{n+1} sqrt{n!}.$$





            Response to update in OP: note that you seem to have avoided chain rule by using
            $$ int |partial_x^n [phi_{1/4} (lambda x) ]|^2 dx overset{?}{=} int |[partial_x^n phi_{1/4}] (lambda x)|^2 dx $$
            Note the very intentional bracketing. This isn't true, try writing it out explicitly for $n=1$.






            share|cite|improve this answer























            • Comments are not for extended discussion; this conversation has been moved to chat.
              – Aloizio Macedo
              Dec 6 '18 at 14:35










            • @AloizioMacedo sorry, I do understand that. Do you know if chat will implement LaTeX or if a workaround exists?
              – Calvin Khor
              Dec 6 '18 at 14:38






            • 1




              There are browser tools for that. Search for "latex chrome extension" if you use google chrome, for example, and you will find extensions which do that.
              – Aloizio Macedo
              Dec 6 '18 at 14:41











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            2 Answers
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            active

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            1














            By your second box, we have the result that




            If $v_a$ is defined by
            $$v_a(x) = int_{mathbb{R}} e^{ixlambda -alambda^2};dlambda$$
            the $v_a$ is in the Gervy class of order $frac{1}{2}$.




            In fact, if you look at the result from Finding $sup_{lambda ge 0}{lambda^k e^{−alambda^2/2}}$, you see that we actually have something better:



            $$sup_{x in mathbb{R}} partial^alpha v(x) le C^{|alpha| + 1} alpha!^frac{1}{2}$$



            Moreover, $v_t$ is actually (up to a scaling factor) the fundamental solution of the heat equation. We can obtain it by taking the Fourier transform in $x$ with frequency variable $lambda$, solving the resulting ODE, and inverting the transform.



            Thus, it would suffice to prove the following result:




            $$sup_{x} partial^alpha v_t * g (x) le C^{alpha + 1}alpha!^frac{1}{2}$$ for any Schwartz class $g$.




            Note that
            $$begin{align*}
            sup_{x} |partial^alpha (v_t * g)(x)| &=leftlVert(partial^alpha v_t) * g (x)rightrVert_{L^infty}\
            &le lVert partial^alpha v_trVert_{L^infty} lVert g rVert_{L^1}\
            &le C^{|alpha|+1}lVert g rVert_{L^1} alpha!^frac{1}{2}
            end{align*}$$

            by Holder's inequality. It follows that $u(x,t) = v_t * g$ is in the Gervy class of order $frac{1}{2}$ for any fixed $t > 0$.






            share|cite|improve this answer




























              1














              By your second box, we have the result that




              If $v_a$ is defined by
              $$v_a(x) = int_{mathbb{R}} e^{ixlambda -alambda^2};dlambda$$
              the $v_a$ is in the Gervy class of order $frac{1}{2}$.




              In fact, if you look at the result from Finding $sup_{lambda ge 0}{lambda^k e^{−alambda^2/2}}$, you see that we actually have something better:



              $$sup_{x in mathbb{R}} partial^alpha v(x) le C^{|alpha| + 1} alpha!^frac{1}{2}$$



              Moreover, $v_t$ is actually (up to a scaling factor) the fundamental solution of the heat equation. We can obtain it by taking the Fourier transform in $x$ with frequency variable $lambda$, solving the resulting ODE, and inverting the transform.



              Thus, it would suffice to prove the following result:




              $$sup_{x} partial^alpha v_t * g (x) le C^{alpha + 1}alpha!^frac{1}{2}$$ for any Schwartz class $g$.




              Note that
              $$begin{align*}
              sup_{x} |partial^alpha (v_t * g)(x)| &=leftlVert(partial^alpha v_t) * g (x)rightrVert_{L^infty}\
              &le lVert partial^alpha v_trVert_{L^infty} lVert g rVert_{L^1}\
              &le C^{|alpha|+1}lVert g rVert_{L^1} alpha!^frac{1}{2}
              end{align*}$$

              by Holder's inequality. It follows that $u(x,t) = v_t * g$ is in the Gervy class of order $frac{1}{2}$ for any fixed $t > 0$.






              share|cite|improve this answer


























                1












                1








                1






                By your second box, we have the result that




                If $v_a$ is defined by
                $$v_a(x) = int_{mathbb{R}} e^{ixlambda -alambda^2};dlambda$$
                the $v_a$ is in the Gervy class of order $frac{1}{2}$.




                In fact, if you look at the result from Finding $sup_{lambda ge 0}{lambda^k e^{−alambda^2/2}}$, you see that we actually have something better:



                $$sup_{x in mathbb{R}} partial^alpha v(x) le C^{|alpha| + 1} alpha!^frac{1}{2}$$



                Moreover, $v_t$ is actually (up to a scaling factor) the fundamental solution of the heat equation. We can obtain it by taking the Fourier transform in $x$ with frequency variable $lambda$, solving the resulting ODE, and inverting the transform.



                Thus, it would suffice to prove the following result:




                $$sup_{x} partial^alpha v_t * g (x) le C^{alpha + 1}alpha!^frac{1}{2}$$ for any Schwartz class $g$.




                Note that
                $$begin{align*}
                sup_{x} |partial^alpha (v_t * g)(x)| &=leftlVert(partial^alpha v_t) * g (x)rightrVert_{L^infty}\
                &le lVert partial^alpha v_trVert_{L^infty} lVert g rVert_{L^1}\
                &le C^{|alpha|+1}lVert g rVert_{L^1} alpha!^frac{1}{2}
                end{align*}$$

                by Holder's inequality. It follows that $u(x,t) = v_t * g$ is in the Gervy class of order $frac{1}{2}$ for any fixed $t > 0$.






                share|cite|improve this answer














                By your second box, we have the result that




                If $v_a$ is defined by
                $$v_a(x) = int_{mathbb{R}} e^{ixlambda -alambda^2};dlambda$$
                the $v_a$ is in the Gervy class of order $frac{1}{2}$.




                In fact, if you look at the result from Finding $sup_{lambda ge 0}{lambda^k e^{−alambda^2/2}}$, you see that we actually have something better:



                $$sup_{x in mathbb{R}} partial^alpha v(x) le C^{|alpha| + 1} alpha!^frac{1}{2}$$



                Moreover, $v_t$ is actually (up to a scaling factor) the fundamental solution of the heat equation. We can obtain it by taking the Fourier transform in $x$ with frequency variable $lambda$, solving the resulting ODE, and inverting the transform.



                Thus, it would suffice to prove the following result:




                $$sup_{x} partial^alpha v_t * g (x) le C^{alpha + 1}alpha!^frac{1}{2}$$ for any Schwartz class $g$.




                Note that
                $$begin{align*}
                sup_{x} |partial^alpha (v_t * g)(x)| &=leftlVert(partial^alpha v_t) * g (x)rightrVert_{L^infty}\
                &le lVert partial^alpha v_trVert_{L^infty} lVert g rVert_{L^1}\
                &le C^{|alpha|+1}lVert g rVert_{L^1} alpha!^frac{1}{2}
                end{align*}$$

                by Holder's inequality. It follows that $u(x,t) = v_t * g$ is in the Gervy class of order $frac{1}{2}$ for any fixed $t > 0$.







                share|cite|improve this answer














                share|cite|improve this answer



                share|cite|improve this answer








                edited Dec 10 '18 at 14:39

























                answered Dec 7 '18 at 16:11









                StrantsStrants

                5,49221736




                5,49221736























                    2





                    +100









                    In this answer, all norms are spatial norms (i.e. there is no integration/supremum wrt the parameter $t_0$ that was already fixed in the question, and I have dropped the subscript $0$).



                    The unique solution to the heat equation with nice initial data is well known as the convolution with the Gaussian kernel,
                    $$ u(x,t) = phi_t * u_0(x) = frac1 {sqrt{4pi t}}int_{mathbb R} e^{-|x-y|^2/4t} u_0(y) dy.$$



                    Then by Cauchy-Schwarz ($|int fg|le |f|_{L^2}|g|_{L^2}$ ),
                    begin{align}
                    &|partial_x^n u(x,t)|_{L^infty} \
                    & = |(partial_x^n phi_t) * u_0|_{L^infty} \
                    & = left |int_{mathbb R}partial^n_xphi_t(x-y) u_0(y) dyright |_{L_x^infty} \
                    & le left | |partial^n_xphi_t(x-y)|_{L^2_y} |u_0|_{L^2}right |_{L_x^infty} \
                    & = left | |partial^n_xphi_t|_{L^2} |u_0|_{L^2}right |_{L_x^infty} \
                    & = |partial^n_xphi_t|_{L^2} |u_0|_{L^2} \
                    &le C^{n+1} |partial_x^n phi_{1/4}|_{L^2} |u_0|_{L^2} \
                    &le C_1^{n+1} |partial_x^n phi_{1/4}|_{L^2} end{align}

                    Above, we used Chain rule,
                    $$partial^n_xphi_t(x) = C(t) partial^n_x exp(-x^2/(4t)) = frac{1}{(sqrt{4t})^{n}} (partial_x^nphi_{1/4})(x/sqrt{4t}) $$
                    and also $ int_{mathbb R} f(lambda x)^2 dx = frac1lambda int_{mathbb R} f^2(y) dy $, so that
                    $$ |partial^n_xphi_t|_{L^2} le C^{n+1}|partial_x^n phi_{1/4}|_{L^2} $$
                    Note that $$partial_x^n phi_{1/4}(x) = (-1)^nH_n(x) phi_{1/4}(x),$$ where $H_n$ is the $n$th (physicist) Hermite polynomial.
                    The Hermite polynomials have the well known $L^2$ norm when weighted with $phi_{1/4}$ (which I quote from that same wikipedia page),
                    $$int H_n^2 phi_{1/4}^2 le |phi_{1/4}|_{L^infty} int H_n^2 phi_{1/4} le C sqrt{2pi} n! $$
                    Thus
                    $$ |partial_x^n u(x,t)|_{L^infty} le C_2^{n+1} sqrt{n!}.$$





                    Response to update in OP: note that you seem to have avoided chain rule by using
                    $$ int |partial_x^n [phi_{1/4} (lambda x) ]|^2 dx overset{?}{=} int |[partial_x^n phi_{1/4}] (lambda x)|^2 dx $$
                    Note the very intentional bracketing. This isn't true, try writing it out explicitly for $n=1$.






                    share|cite|improve this answer























                    • Comments are not for extended discussion; this conversation has been moved to chat.
                      – Aloizio Macedo
                      Dec 6 '18 at 14:35










                    • @AloizioMacedo sorry, I do understand that. Do you know if chat will implement LaTeX or if a workaround exists?
                      – Calvin Khor
                      Dec 6 '18 at 14:38






                    • 1




                      There are browser tools for that. Search for "latex chrome extension" if you use google chrome, for example, and you will find extensions which do that.
                      – Aloizio Macedo
                      Dec 6 '18 at 14:41
















                    2





                    +100









                    In this answer, all norms are spatial norms (i.e. there is no integration/supremum wrt the parameter $t_0$ that was already fixed in the question, and I have dropped the subscript $0$).



                    The unique solution to the heat equation with nice initial data is well known as the convolution with the Gaussian kernel,
                    $$ u(x,t) = phi_t * u_0(x) = frac1 {sqrt{4pi t}}int_{mathbb R} e^{-|x-y|^2/4t} u_0(y) dy.$$



                    Then by Cauchy-Schwarz ($|int fg|le |f|_{L^2}|g|_{L^2}$ ),
                    begin{align}
                    &|partial_x^n u(x,t)|_{L^infty} \
                    & = |(partial_x^n phi_t) * u_0|_{L^infty} \
                    & = left |int_{mathbb R}partial^n_xphi_t(x-y) u_0(y) dyright |_{L_x^infty} \
                    & le left | |partial^n_xphi_t(x-y)|_{L^2_y} |u_0|_{L^2}right |_{L_x^infty} \
                    & = left | |partial^n_xphi_t|_{L^2} |u_0|_{L^2}right |_{L_x^infty} \
                    & = |partial^n_xphi_t|_{L^2} |u_0|_{L^2} \
                    &le C^{n+1} |partial_x^n phi_{1/4}|_{L^2} |u_0|_{L^2} \
                    &le C_1^{n+1} |partial_x^n phi_{1/4}|_{L^2} end{align}

                    Above, we used Chain rule,
                    $$partial^n_xphi_t(x) = C(t) partial^n_x exp(-x^2/(4t)) = frac{1}{(sqrt{4t})^{n}} (partial_x^nphi_{1/4})(x/sqrt{4t}) $$
                    and also $ int_{mathbb R} f(lambda x)^2 dx = frac1lambda int_{mathbb R} f^2(y) dy $, so that
                    $$ |partial^n_xphi_t|_{L^2} le C^{n+1}|partial_x^n phi_{1/4}|_{L^2} $$
                    Note that $$partial_x^n phi_{1/4}(x) = (-1)^nH_n(x) phi_{1/4}(x),$$ where $H_n$ is the $n$th (physicist) Hermite polynomial.
                    The Hermite polynomials have the well known $L^2$ norm when weighted with $phi_{1/4}$ (which I quote from that same wikipedia page),
                    $$int H_n^2 phi_{1/4}^2 le |phi_{1/4}|_{L^infty} int H_n^2 phi_{1/4} le C sqrt{2pi} n! $$
                    Thus
                    $$ |partial_x^n u(x,t)|_{L^infty} le C_2^{n+1} sqrt{n!}.$$





                    Response to update in OP: note that you seem to have avoided chain rule by using
                    $$ int |partial_x^n [phi_{1/4} (lambda x) ]|^2 dx overset{?}{=} int |[partial_x^n phi_{1/4}] (lambda x)|^2 dx $$
                    Note the very intentional bracketing. This isn't true, try writing it out explicitly for $n=1$.






                    share|cite|improve this answer























                    • Comments are not for extended discussion; this conversation has been moved to chat.
                      – Aloizio Macedo
                      Dec 6 '18 at 14:35










                    • @AloizioMacedo sorry, I do understand that. Do you know if chat will implement LaTeX or if a workaround exists?
                      – Calvin Khor
                      Dec 6 '18 at 14:38






                    • 1




                      There are browser tools for that. Search for "latex chrome extension" if you use google chrome, for example, and you will find extensions which do that.
                      – Aloizio Macedo
                      Dec 6 '18 at 14:41














                    2





                    +100







                    2





                    +100



                    2




                    +100




                    In this answer, all norms are spatial norms (i.e. there is no integration/supremum wrt the parameter $t_0$ that was already fixed in the question, and I have dropped the subscript $0$).



                    The unique solution to the heat equation with nice initial data is well known as the convolution with the Gaussian kernel,
                    $$ u(x,t) = phi_t * u_0(x) = frac1 {sqrt{4pi t}}int_{mathbb R} e^{-|x-y|^2/4t} u_0(y) dy.$$



                    Then by Cauchy-Schwarz ($|int fg|le |f|_{L^2}|g|_{L^2}$ ),
                    begin{align}
                    &|partial_x^n u(x,t)|_{L^infty} \
                    & = |(partial_x^n phi_t) * u_0|_{L^infty} \
                    & = left |int_{mathbb R}partial^n_xphi_t(x-y) u_0(y) dyright |_{L_x^infty} \
                    & le left | |partial^n_xphi_t(x-y)|_{L^2_y} |u_0|_{L^2}right |_{L_x^infty} \
                    & = left | |partial^n_xphi_t|_{L^2} |u_0|_{L^2}right |_{L_x^infty} \
                    & = |partial^n_xphi_t|_{L^2} |u_0|_{L^2} \
                    &le C^{n+1} |partial_x^n phi_{1/4}|_{L^2} |u_0|_{L^2} \
                    &le C_1^{n+1} |partial_x^n phi_{1/4}|_{L^2} end{align}

                    Above, we used Chain rule,
                    $$partial^n_xphi_t(x) = C(t) partial^n_x exp(-x^2/(4t)) = frac{1}{(sqrt{4t})^{n}} (partial_x^nphi_{1/4})(x/sqrt{4t}) $$
                    and also $ int_{mathbb R} f(lambda x)^2 dx = frac1lambda int_{mathbb R} f^2(y) dy $, so that
                    $$ |partial^n_xphi_t|_{L^2} le C^{n+1}|partial_x^n phi_{1/4}|_{L^2} $$
                    Note that $$partial_x^n phi_{1/4}(x) = (-1)^nH_n(x) phi_{1/4}(x),$$ where $H_n$ is the $n$th (physicist) Hermite polynomial.
                    The Hermite polynomials have the well known $L^2$ norm when weighted with $phi_{1/4}$ (which I quote from that same wikipedia page),
                    $$int H_n^2 phi_{1/4}^2 le |phi_{1/4}|_{L^infty} int H_n^2 phi_{1/4} le C sqrt{2pi} n! $$
                    Thus
                    $$ |partial_x^n u(x,t)|_{L^infty} le C_2^{n+1} sqrt{n!}.$$





                    Response to update in OP: note that you seem to have avoided chain rule by using
                    $$ int |partial_x^n [phi_{1/4} (lambda x) ]|^2 dx overset{?}{=} int |[partial_x^n phi_{1/4}] (lambda x)|^2 dx $$
                    Note the very intentional bracketing. This isn't true, try writing it out explicitly for $n=1$.






                    share|cite|improve this answer














                    In this answer, all norms are spatial norms (i.e. there is no integration/supremum wrt the parameter $t_0$ that was already fixed in the question, and I have dropped the subscript $0$).



                    The unique solution to the heat equation with nice initial data is well known as the convolution with the Gaussian kernel,
                    $$ u(x,t) = phi_t * u_0(x) = frac1 {sqrt{4pi t}}int_{mathbb R} e^{-|x-y|^2/4t} u_0(y) dy.$$



                    Then by Cauchy-Schwarz ($|int fg|le |f|_{L^2}|g|_{L^2}$ ),
                    begin{align}
                    &|partial_x^n u(x,t)|_{L^infty} \
                    & = |(partial_x^n phi_t) * u_0|_{L^infty} \
                    & = left |int_{mathbb R}partial^n_xphi_t(x-y) u_0(y) dyright |_{L_x^infty} \
                    & le left | |partial^n_xphi_t(x-y)|_{L^2_y} |u_0|_{L^2}right |_{L_x^infty} \
                    & = left | |partial^n_xphi_t|_{L^2} |u_0|_{L^2}right |_{L_x^infty} \
                    & = |partial^n_xphi_t|_{L^2} |u_0|_{L^2} \
                    &le C^{n+1} |partial_x^n phi_{1/4}|_{L^2} |u_0|_{L^2} \
                    &le C_1^{n+1} |partial_x^n phi_{1/4}|_{L^2} end{align}

                    Above, we used Chain rule,
                    $$partial^n_xphi_t(x) = C(t) partial^n_x exp(-x^2/(4t)) = frac{1}{(sqrt{4t})^{n}} (partial_x^nphi_{1/4})(x/sqrt{4t}) $$
                    and also $ int_{mathbb R} f(lambda x)^2 dx = frac1lambda int_{mathbb R} f^2(y) dy $, so that
                    $$ |partial^n_xphi_t|_{L^2} le C^{n+1}|partial_x^n phi_{1/4}|_{L^2} $$
                    Note that $$partial_x^n phi_{1/4}(x) = (-1)^nH_n(x) phi_{1/4}(x),$$ where $H_n$ is the $n$th (physicist) Hermite polynomial.
                    The Hermite polynomials have the well known $L^2$ norm when weighted with $phi_{1/4}$ (which I quote from that same wikipedia page),
                    $$int H_n^2 phi_{1/4}^2 le |phi_{1/4}|_{L^infty} int H_n^2 phi_{1/4} le C sqrt{2pi} n! $$
                    Thus
                    $$ |partial_x^n u(x,t)|_{L^infty} le C_2^{n+1} sqrt{n!}.$$





                    Response to update in OP: note that you seem to have avoided chain rule by using
                    $$ int |partial_x^n [phi_{1/4} (lambda x) ]|^2 dx overset{?}{=} int |[partial_x^n phi_{1/4}] (lambda x)|^2 dx $$
                    Note the very intentional bracketing. This isn't true, try writing it out explicitly for $n=1$.







                    share|cite|improve this answer














                    share|cite|improve this answer



                    share|cite|improve this answer








                    edited Dec 5 '18 at 17:05

























                    answered Dec 1 '18 at 17:49









                    Calvin KhorCalvin Khor

                    11.2k21438




                    11.2k21438












                    • Comments are not for extended discussion; this conversation has been moved to chat.
                      – Aloizio Macedo
                      Dec 6 '18 at 14:35










                    • @AloizioMacedo sorry, I do understand that. Do you know if chat will implement LaTeX or if a workaround exists?
                      – Calvin Khor
                      Dec 6 '18 at 14:38






                    • 1




                      There are browser tools for that. Search for "latex chrome extension" if you use google chrome, for example, and you will find extensions which do that.
                      – Aloizio Macedo
                      Dec 6 '18 at 14:41


















                    • Comments are not for extended discussion; this conversation has been moved to chat.
                      – Aloizio Macedo
                      Dec 6 '18 at 14:35










                    • @AloizioMacedo sorry, I do understand that. Do you know if chat will implement LaTeX or if a workaround exists?
                      – Calvin Khor
                      Dec 6 '18 at 14:38






                    • 1




                      There are browser tools for that. Search for "latex chrome extension" if you use google chrome, for example, and you will find extensions which do that.
                      – Aloizio Macedo
                      Dec 6 '18 at 14:41
















                    Comments are not for extended discussion; this conversation has been moved to chat.
                    – Aloizio Macedo
                    Dec 6 '18 at 14:35




                    Comments are not for extended discussion; this conversation has been moved to chat.
                    – Aloizio Macedo
                    Dec 6 '18 at 14:35












                    @AloizioMacedo sorry, I do understand that. Do you know if chat will implement LaTeX or if a workaround exists?
                    – Calvin Khor
                    Dec 6 '18 at 14:38




                    @AloizioMacedo sorry, I do understand that. Do you know if chat will implement LaTeX or if a workaround exists?
                    – Calvin Khor
                    Dec 6 '18 at 14:38




                    1




                    1




                    There are browser tools for that. Search for "latex chrome extension" if you use google chrome, for example, and you will find extensions which do that.
                    – Aloizio Macedo
                    Dec 6 '18 at 14:41




                    There are browser tools for that. Search for "latex chrome extension" if you use google chrome, for example, and you will find extensions which do that.
                    – Aloizio Macedo
                    Dec 6 '18 at 14:41


















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