Laplacians and Dirac delta functions












18












$begingroup$


It is often quoted in physics textbooks for finding the electric potential using Green's function that



$$nabla ^2 left(frac{1}{r}right)=-4pidelta^3({bf r}),$$



or more generally



$$nabla ^2 left(frac{1}{|| vec x - vec x'||}right)=-4pidelta^3(vec x - vec x'),$$



where $delta^3$ is the 3-dimensional Dirac delta distribution.
However I don't understand how/where this comes from. Would anyone mind explaining?










share|cite|improve this question











$endgroup$

















    18












    $begingroup$


    It is often quoted in physics textbooks for finding the electric potential using Green's function that



    $$nabla ^2 left(frac{1}{r}right)=-4pidelta^3({bf r}),$$



    or more generally



    $$nabla ^2 left(frac{1}{|| vec x - vec x'||}right)=-4pidelta^3(vec x - vec x'),$$



    where $delta^3$ is the 3-dimensional Dirac delta distribution.
    However I don't understand how/where this comes from. Would anyone mind explaining?










    share|cite|improve this question











    $endgroup$















      18












      18








      18


      20



      $begingroup$


      It is often quoted in physics textbooks for finding the electric potential using Green's function that



      $$nabla ^2 left(frac{1}{r}right)=-4pidelta^3({bf r}),$$



      or more generally



      $$nabla ^2 left(frac{1}{|| vec x - vec x'||}right)=-4pidelta^3(vec x - vec x'),$$



      where $delta^3$ is the 3-dimensional Dirac delta distribution.
      However I don't understand how/where this comes from. Would anyone mind explaining?










      share|cite|improve this question











      $endgroup$




      It is often quoted in physics textbooks for finding the electric potential using Green's function that



      $$nabla ^2 left(frac{1}{r}right)=-4pidelta^3({bf r}),$$



      or more generally



      $$nabla ^2 left(frac{1}{|| vec x - vec x'||}right)=-4pidelta^3(vec x - vec x'),$$



      where $delta^3$ is the 3-dimensional Dirac delta distribution.
      However I don't understand how/where this comes from. Would anyone mind explaining?







      calculus derivatives distribution-theory






      share|cite|improve this question















      share|cite|improve this question













      share|cite|improve this question




      share|cite|improve this question








      edited May 23 '15 at 15:21









      Qmechanic

      5,07211856




      5,07211856










      asked Apr 21 '13 at 13:10









      JennaJenna

      93114




      93114






















          3 Answers
          3






          active

          oldest

          votes


















          15












          $begingroup$

          The gradient of $frac1r$ (noting that $r=sqrt{x^2+y^2+z^2}$) is



          $$
          nabla frac1r = -frac{mathbf{r}}{r^3}
          $$
          when $rneq 0$, where $mathbf{r}=xmathbf{i}+ymathbf{j}+zmathbf{k}$. Now, the divergence of this is



          $$
          nablacdot left(-frac{mathbf{r}}{r^3}right) = 0
          $$
          when $rneq 0$. Therefore, for all points for which $rneq 0$,



          $$
          nabla^2frac1r = 0
          $$
          However, if we integrate this function over a sphere, $S$, of radius $a$, then, applying Gauss's Theorem, we get



          $$
          iiint_S nabla^2frac1rdV = iint_{Delta S} -frac{mathbf{r}}{r^3}.dmathbf{S}
          $$
          where $Delta S$ is the surface of the sphere, and is outward-facing. Now, $dmathbf{S}=mathbf{hat r}dA$, where $dA=r^2sintheta dphi dtheta$. Therefore, we may write our surface integral as
          $$begin{align}
          iint_{Delta S} -frac{mathbf{r}}{r^3}.dmathbf{S}&=-int_0^piint_0^{2pi}frac{r}{r^3}r^2sintheta dphi dtheta\
          &=-int_0^pisintheta dthetaint_0^{2pi}dphi\
          &= -2cdot 2pi = -4pi
          end{align}$$
          Therefore, the value of the laplacian is zero everywhere except zero, and the integral over any volume containing the origin is equal to $-4pi$. Therefore, the laplacian is equal to $-4pi delta(mathbf{r})$.



          EDIT: The general case is then obtained by replacing $r=|mathbf{r}|$ with $s=|mathbf{r}-mathbf{r_0}|$, in which case the function shifts to $-4pi delta(mathbf{r}-mathbf{r_0})$






          share|cite|improve this answer











          $endgroup$













          • $begingroup$
            Thank you very much, Glen!
            $endgroup$
            – Jenna
            Apr 21 '13 at 14:59






          • 4




            $begingroup$
            Comment to the answer (v2): Playing the devil's advocate: The usual divergence theorem assumes that the vector field ${bf F}$ is $C^1$. But in this case, the vector field ${bf F}=-frac{bf r}{r^3}$ is singular at $r=0$. So how can the use of the divergence theorem be justified?
            $endgroup$
            – Qmechanic
            May 22 '15 at 14:36












          • $begingroup$
            @Qmechanic - for the same reason as why we use the Dirac Delta function... which isn't technically a function, but a distribution. Note that the usual definition of integration doesn't apply to the dirac delta function in one dimension, because it requires that the function be real-valued (or complex-valued, as appropriate).
            $endgroup$
            – Glen O
            May 22 '15 at 17:20






          • 1




            $begingroup$
            A distribution is usually evaluated on an arbitrary test function (within a certain class of functions). The answer (v2) makes no mentioning of test functions.
            $endgroup$
            – Qmechanic
            May 23 '15 at 14:38








          • 1




            $begingroup$
            @Cookie - there is undoubtedly some sort of generalisation, but I don't believe other cases are as simple as $n=3$. I believe the useful observation is that $nablacdot (mathbf{r}/r^n) = 0$ for $rneq 0$ and $n$ dimensions.
            $endgroup$
            – Glen O
            Jun 4 '16 at 8:28





















          17












          $begingroup$

          I'm new around here (so suggestions about posting are welcome!) and want to give my contribution to this question, even though a bit old. I feel I need to because using the divergence theorem in this context is not quite rigorous. Strictly speaking $1/r$ is not even differentiable at the origin. So here's a proof using limits of distributions.



          Let $mathbf{x}inmathbb{R}^{3}$ and $r=|mathbf{x}|=sqrt{x^2+y^2+z^2}$. It is evident from direct calculation that $nabla^{2}left(frac{1}{r}right)=0$ everywhere except in $mathbf{x}=0$, where it is in fact not defined. Thus, the integral of $nabla^{2}left(frac{1}{r}right)$ over any volume non containing the origin is zero.



          So let $eta>0$ and $r_{eta}=sqrt{x^2+y^2+z^2+eta^2}$. Obviously $limlimits_{etarightarrow 0}r_{eta}=r$. Direct calculation brings
          begin{equation}
          nabla^{2}left(frac{1}{r_{eta}}right) = frac{-3eta^{2}}{r_{eta}^5}
          end{equation}
          Now let us consider the distribution represented by $nabla^{2}left(frac{1}{r_{eta}}right)$ and let $rho$ be a test function (for example in the Schwartz space). I use Dirac's bra-ket notation to express the action of a distribution over a test function. Let $S^{2}$ be the unit sphere. Thus we calculate
          begin{align}
          limlimits_{etarightarrow 0}left.leftlangle nabla^{2}left(frac{1}{r_{eta}}right)right|rhorightrangle &= limlimits_{etarightarrow 0}iiintlimits_{mathbb{R}^3}mathrm{d}^{3}x, nabla^{2}left(frac{1}{r_{eta}}right)rho(mathbf{x})\
          &=limlimits_{etarightarrow 0}left{iiintlimits_{mathbb{R}^3setminus S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})+ iiintlimits_{S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})right}\
          &=limlimits_{etarightarrow 0}iiintlimits_{S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})
          end{align}
          Where the limit of the first of the integrals in the curly braces is zero (easy to show, referring to the laplacian of $1/r$, no need for $eta$ in sets not containing the origin).
          Now Taylor expand $rho$ at $mathbf{x}=0$ and integrate using spherical polar coordinates:
          begin{equation}
          limlimits_{etarightarrow 0}int_{0}^{pi}mathrm{d}theta,sinthetaint_{0}^{2pi}mathrm{d}varphi,int_{0}^{1}mathrm{d}t,frac{-3eta^{2}t^{2}}{(t^{2}+eta^{2})^{5/2}}(rho(0)+O(t^{2}))
          end{equation}
          Integrating you will get that all the terms contained in $O(t^2)$ vanish as $etarightarrow 0$, while the term with $rho(0)$ remains. In fact you get
          begin{align}
          limlimits_{etarightarrow 0}frac{-4pirho(0)}{sqrt{1+eta^{2}}}&=-4pirho(0)\
          &=langle -4pidelta_{0}^{(3)}|rhorangle
          end{align}



          From this argument one defines the limit distribution
          begin{equation}
          nabla^{2}left(frac{1}{r}right):=limlimits_{etarightarrow 0}nabla^{2}left(frac{1}{r_{eta}}right)=-4pidelta_{0}^{(3)}
          end{equation}
          The generalization to $r=|mathbf{x}-mathbf{x}_{0}|$ is obvious.






          share|cite|improve this answer









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          • $begingroup$
            Great answer! However, could you clarify on the expansion in Taylor series? It seems to me you are supposing that $rho(mathbf{x})$ is only radial.
            $endgroup$
            – rmk236
            Aug 18 '15 at 20:17






          • 1




            $begingroup$
            @rmk236 It doesn't look that way to me. Taylor expanding inside the integral you get the $rho(0)$ term and then all the others of course. But all those other terms (which account for the possibility of $rho$ to be not radial) are included in the $O(t^{2})$. If you need the actual terms or you still have doubts I could carry out the calculation again and post more details on that part.
            $endgroup$
            – Daniele Oriani
            Aug 19 '15 at 22:25



















          0












          $begingroup$

          Here is a back-alley derivation using Fourier transform properties.
          Take the Fourier transform of $frac{1}{4 pi r}$ to get $frac{1}{k^2}$. Therefore,
          $$
          frac{1}{4pi r} = int frac{d^3k}{(2pi)^3} frac{e^{-ikcdot r}}{k^2}
          $$

          Now, apply $-nabla^2$ to get
          $$
          -nabla^2 frac{1}{4pi r} = int frac{d^3k}{(2pi)^3} e^{-ikcdot r}
          $$

          This is the delta function, but we can explicitly put in our test function:
          begin{align*}
          int d^3r left(-nabla^2 frac{1}{4 pi r}right) f(r) &=
          int frac{d^3k}{(2pi)^3} int d^3r e^{-ikcdot r} f(r) \
          &=
          int frac{d^3k}{(2pi)^3} tilde{f}(k) \
          & = f(r=0).
          end{align*}






          share|cite|improve this answer









          $endgroup$













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            3 Answers
            3






            active

            oldest

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            3 Answers
            3






            active

            oldest

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            active

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            active

            oldest

            votes









            15












            $begingroup$

            The gradient of $frac1r$ (noting that $r=sqrt{x^2+y^2+z^2}$) is



            $$
            nabla frac1r = -frac{mathbf{r}}{r^3}
            $$
            when $rneq 0$, where $mathbf{r}=xmathbf{i}+ymathbf{j}+zmathbf{k}$. Now, the divergence of this is



            $$
            nablacdot left(-frac{mathbf{r}}{r^3}right) = 0
            $$
            when $rneq 0$. Therefore, for all points for which $rneq 0$,



            $$
            nabla^2frac1r = 0
            $$
            However, if we integrate this function over a sphere, $S$, of radius $a$, then, applying Gauss's Theorem, we get



            $$
            iiint_S nabla^2frac1rdV = iint_{Delta S} -frac{mathbf{r}}{r^3}.dmathbf{S}
            $$
            where $Delta S$ is the surface of the sphere, and is outward-facing. Now, $dmathbf{S}=mathbf{hat r}dA$, where $dA=r^2sintheta dphi dtheta$. Therefore, we may write our surface integral as
            $$begin{align}
            iint_{Delta S} -frac{mathbf{r}}{r^3}.dmathbf{S}&=-int_0^piint_0^{2pi}frac{r}{r^3}r^2sintheta dphi dtheta\
            &=-int_0^pisintheta dthetaint_0^{2pi}dphi\
            &= -2cdot 2pi = -4pi
            end{align}$$
            Therefore, the value of the laplacian is zero everywhere except zero, and the integral over any volume containing the origin is equal to $-4pi$. Therefore, the laplacian is equal to $-4pi delta(mathbf{r})$.



            EDIT: The general case is then obtained by replacing $r=|mathbf{r}|$ with $s=|mathbf{r}-mathbf{r_0}|$, in which case the function shifts to $-4pi delta(mathbf{r}-mathbf{r_0})$






            share|cite|improve this answer











            $endgroup$













            • $begingroup$
              Thank you very much, Glen!
              $endgroup$
              – Jenna
              Apr 21 '13 at 14:59






            • 4




              $begingroup$
              Comment to the answer (v2): Playing the devil's advocate: The usual divergence theorem assumes that the vector field ${bf F}$ is $C^1$. But in this case, the vector field ${bf F}=-frac{bf r}{r^3}$ is singular at $r=0$. So how can the use of the divergence theorem be justified?
              $endgroup$
              – Qmechanic
              May 22 '15 at 14:36












            • $begingroup$
              @Qmechanic - for the same reason as why we use the Dirac Delta function... which isn't technically a function, but a distribution. Note that the usual definition of integration doesn't apply to the dirac delta function in one dimension, because it requires that the function be real-valued (or complex-valued, as appropriate).
              $endgroup$
              – Glen O
              May 22 '15 at 17:20






            • 1




              $begingroup$
              A distribution is usually evaluated on an arbitrary test function (within a certain class of functions). The answer (v2) makes no mentioning of test functions.
              $endgroup$
              – Qmechanic
              May 23 '15 at 14:38








            • 1




              $begingroup$
              @Cookie - there is undoubtedly some sort of generalisation, but I don't believe other cases are as simple as $n=3$. I believe the useful observation is that $nablacdot (mathbf{r}/r^n) = 0$ for $rneq 0$ and $n$ dimensions.
              $endgroup$
              – Glen O
              Jun 4 '16 at 8:28


















            15












            $begingroup$

            The gradient of $frac1r$ (noting that $r=sqrt{x^2+y^2+z^2}$) is



            $$
            nabla frac1r = -frac{mathbf{r}}{r^3}
            $$
            when $rneq 0$, where $mathbf{r}=xmathbf{i}+ymathbf{j}+zmathbf{k}$. Now, the divergence of this is



            $$
            nablacdot left(-frac{mathbf{r}}{r^3}right) = 0
            $$
            when $rneq 0$. Therefore, for all points for which $rneq 0$,



            $$
            nabla^2frac1r = 0
            $$
            However, if we integrate this function over a sphere, $S$, of radius $a$, then, applying Gauss's Theorem, we get



            $$
            iiint_S nabla^2frac1rdV = iint_{Delta S} -frac{mathbf{r}}{r^3}.dmathbf{S}
            $$
            where $Delta S$ is the surface of the sphere, and is outward-facing. Now, $dmathbf{S}=mathbf{hat r}dA$, where $dA=r^2sintheta dphi dtheta$. Therefore, we may write our surface integral as
            $$begin{align}
            iint_{Delta S} -frac{mathbf{r}}{r^3}.dmathbf{S}&=-int_0^piint_0^{2pi}frac{r}{r^3}r^2sintheta dphi dtheta\
            &=-int_0^pisintheta dthetaint_0^{2pi}dphi\
            &= -2cdot 2pi = -4pi
            end{align}$$
            Therefore, the value of the laplacian is zero everywhere except zero, and the integral over any volume containing the origin is equal to $-4pi$. Therefore, the laplacian is equal to $-4pi delta(mathbf{r})$.



            EDIT: The general case is then obtained by replacing $r=|mathbf{r}|$ with $s=|mathbf{r}-mathbf{r_0}|$, in which case the function shifts to $-4pi delta(mathbf{r}-mathbf{r_0})$






            share|cite|improve this answer











            $endgroup$













            • $begingroup$
              Thank you very much, Glen!
              $endgroup$
              – Jenna
              Apr 21 '13 at 14:59






            • 4




              $begingroup$
              Comment to the answer (v2): Playing the devil's advocate: The usual divergence theorem assumes that the vector field ${bf F}$ is $C^1$. But in this case, the vector field ${bf F}=-frac{bf r}{r^3}$ is singular at $r=0$. So how can the use of the divergence theorem be justified?
              $endgroup$
              – Qmechanic
              May 22 '15 at 14:36












            • $begingroup$
              @Qmechanic - for the same reason as why we use the Dirac Delta function... which isn't technically a function, but a distribution. Note that the usual definition of integration doesn't apply to the dirac delta function in one dimension, because it requires that the function be real-valued (or complex-valued, as appropriate).
              $endgroup$
              – Glen O
              May 22 '15 at 17:20






            • 1




              $begingroup$
              A distribution is usually evaluated on an arbitrary test function (within a certain class of functions). The answer (v2) makes no mentioning of test functions.
              $endgroup$
              – Qmechanic
              May 23 '15 at 14:38








            • 1




              $begingroup$
              @Cookie - there is undoubtedly some sort of generalisation, but I don't believe other cases are as simple as $n=3$. I believe the useful observation is that $nablacdot (mathbf{r}/r^n) = 0$ for $rneq 0$ and $n$ dimensions.
              $endgroup$
              – Glen O
              Jun 4 '16 at 8:28
















            15












            15








            15





            $begingroup$

            The gradient of $frac1r$ (noting that $r=sqrt{x^2+y^2+z^2}$) is



            $$
            nabla frac1r = -frac{mathbf{r}}{r^3}
            $$
            when $rneq 0$, where $mathbf{r}=xmathbf{i}+ymathbf{j}+zmathbf{k}$. Now, the divergence of this is



            $$
            nablacdot left(-frac{mathbf{r}}{r^3}right) = 0
            $$
            when $rneq 0$. Therefore, for all points for which $rneq 0$,



            $$
            nabla^2frac1r = 0
            $$
            However, if we integrate this function over a sphere, $S$, of radius $a$, then, applying Gauss's Theorem, we get



            $$
            iiint_S nabla^2frac1rdV = iint_{Delta S} -frac{mathbf{r}}{r^3}.dmathbf{S}
            $$
            where $Delta S$ is the surface of the sphere, and is outward-facing. Now, $dmathbf{S}=mathbf{hat r}dA$, where $dA=r^2sintheta dphi dtheta$. Therefore, we may write our surface integral as
            $$begin{align}
            iint_{Delta S} -frac{mathbf{r}}{r^3}.dmathbf{S}&=-int_0^piint_0^{2pi}frac{r}{r^3}r^2sintheta dphi dtheta\
            &=-int_0^pisintheta dthetaint_0^{2pi}dphi\
            &= -2cdot 2pi = -4pi
            end{align}$$
            Therefore, the value of the laplacian is zero everywhere except zero, and the integral over any volume containing the origin is equal to $-4pi$. Therefore, the laplacian is equal to $-4pi delta(mathbf{r})$.



            EDIT: The general case is then obtained by replacing $r=|mathbf{r}|$ with $s=|mathbf{r}-mathbf{r_0}|$, in which case the function shifts to $-4pi delta(mathbf{r}-mathbf{r_0})$






            share|cite|improve this answer











            $endgroup$



            The gradient of $frac1r$ (noting that $r=sqrt{x^2+y^2+z^2}$) is



            $$
            nabla frac1r = -frac{mathbf{r}}{r^3}
            $$
            when $rneq 0$, where $mathbf{r}=xmathbf{i}+ymathbf{j}+zmathbf{k}$. Now, the divergence of this is



            $$
            nablacdot left(-frac{mathbf{r}}{r^3}right) = 0
            $$
            when $rneq 0$. Therefore, for all points for which $rneq 0$,



            $$
            nabla^2frac1r = 0
            $$
            However, if we integrate this function over a sphere, $S$, of radius $a$, then, applying Gauss's Theorem, we get



            $$
            iiint_S nabla^2frac1rdV = iint_{Delta S} -frac{mathbf{r}}{r^3}.dmathbf{S}
            $$
            where $Delta S$ is the surface of the sphere, and is outward-facing. Now, $dmathbf{S}=mathbf{hat r}dA$, where $dA=r^2sintheta dphi dtheta$. Therefore, we may write our surface integral as
            $$begin{align}
            iint_{Delta S} -frac{mathbf{r}}{r^3}.dmathbf{S}&=-int_0^piint_0^{2pi}frac{r}{r^3}r^2sintheta dphi dtheta\
            &=-int_0^pisintheta dthetaint_0^{2pi}dphi\
            &= -2cdot 2pi = -4pi
            end{align}$$
            Therefore, the value of the laplacian is zero everywhere except zero, and the integral over any volume containing the origin is equal to $-4pi$. Therefore, the laplacian is equal to $-4pi delta(mathbf{r})$.



            EDIT: The general case is then obtained by replacing $r=|mathbf{r}|$ with $s=|mathbf{r}-mathbf{r_0}|$, in which case the function shifts to $-4pi delta(mathbf{r}-mathbf{r_0})$







            share|cite|improve this answer














            share|cite|improve this answer



            share|cite|improve this answer








            edited Apr 21 '13 at 13:52

























            answered Apr 21 '13 at 13:43









            Glen OGlen O

            8,9931528




            8,9931528












            • $begingroup$
              Thank you very much, Glen!
              $endgroup$
              – Jenna
              Apr 21 '13 at 14:59






            • 4




              $begingroup$
              Comment to the answer (v2): Playing the devil's advocate: The usual divergence theorem assumes that the vector field ${bf F}$ is $C^1$. But in this case, the vector field ${bf F}=-frac{bf r}{r^3}$ is singular at $r=0$. So how can the use of the divergence theorem be justified?
              $endgroup$
              – Qmechanic
              May 22 '15 at 14:36












            • $begingroup$
              @Qmechanic - for the same reason as why we use the Dirac Delta function... which isn't technically a function, but a distribution. Note that the usual definition of integration doesn't apply to the dirac delta function in one dimension, because it requires that the function be real-valued (or complex-valued, as appropriate).
              $endgroup$
              – Glen O
              May 22 '15 at 17:20






            • 1




              $begingroup$
              A distribution is usually evaluated on an arbitrary test function (within a certain class of functions). The answer (v2) makes no mentioning of test functions.
              $endgroup$
              – Qmechanic
              May 23 '15 at 14:38








            • 1




              $begingroup$
              @Cookie - there is undoubtedly some sort of generalisation, but I don't believe other cases are as simple as $n=3$. I believe the useful observation is that $nablacdot (mathbf{r}/r^n) = 0$ for $rneq 0$ and $n$ dimensions.
              $endgroup$
              – Glen O
              Jun 4 '16 at 8:28




















            • $begingroup$
              Thank you very much, Glen!
              $endgroup$
              – Jenna
              Apr 21 '13 at 14:59






            • 4




              $begingroup$
              Comment to the answer (v2): Playing the devil's advocate: The usual divergence theorem assumes that the vector field ${bf F}$ is $C^1$. But in this case, the vector field ${bf F}=-frac{bf r}{r^3}$ is singular at $r=0$. So how can the use of the divergence theorem be justified?
              $endgroup$
              – Qmechanic
              May 22 '15 at 14:36












            • $begingroup$
              @Qmechanic - for the same reason as why we use the Dirac Delta function... which isn't technically a function, but a distribution. Note that the usual definition of integration doesn't apply to the dirac delta function in one dimension, because it requires that the function be real-valued (or complex-valued, as appropriate).
              $endgroup$
              – Glen O
              May 22 '15 at 17:20






            • 1




              $begingroup$
              A distribution is usually evaluated on an arbitrary test function (within a certain class of functions). The answer (v2) makes no mentioning of test functions.
              $endgroup$
              – Qmechanic
              May 23 '15 at 14:38








            • 1




              $begingroup$
              @Cookie - there is undoubtedly some sort of generalisation, but I don't believe other cases are as simple as $n=3$. I believe the useful observation is that $nablacdot (mathbf{r}/r^n) = 0$ for $rneq 0$ and $n$ dimensions.
              $endgroup$
              – Glen O
              Jun 4 '16 at 8:28


















            $begingroup$
            Thank you very much, Glen!
            $endgroup$
            – Jenna
            Apr 21 '13 at 14:59




            $begingroup$
            Thank you very much, Glen!
            $endgroup$
            – Jenna
            Apr 21 '13 at 14:59




            4




            4




            $begingroup$
            Comment to the answer (v2): Playing the devil's advocate: The usual divergence theorem assumes that the vector field ${bf F}$ is $C^1$. But in this case, the vector field ${bf F}=-frac{bf r}{r^3}$ is singular at $r=0$. So how can the use of the divergence theorem be justified?
            $endgroup$
            – Qmechanic
            May 22 '15 at 14:36






            $begingroup$
            Comment to the answer (v2): Playing the devil's advocate: The usual divergence theorem assumes that the vector field ${bf F}$ is $C^1$. But in this case, the vector field ${bf F}=-frac{bf r}{r^3}$ is singular at $r=0$. So how can the use of the divergence theorem be justified?
            $endgroup$
            – Qmechanic
            May 22 '15 at 14:36














            $begingroup$
            @Qmechanic - for the same reason as why we use the Dirac Delta function... which isn't technically a function, but a distribution. Note that the usual definition of integration doesn't apply to the dirac delta function in one dimension, because it requires that the function be real-valued (or complex-valued, as appropriate).
            $endgroup$
            – Glen O
            May 22 '15 at 17:20




            $begingroup$
            @Qmechanic - for the same reason as why we use the Dirac Delta function... which isn't technically a function, but a distribution. Note that the usual definition of integration doesn't apply to the dirac delta function in one dimension, because it requires that the function be real-valued (or complex-valued, as appropriate).
            $endgroup$
            – Glen O
            May 22 '15 at 17:20




            1




            1




            $begingroup$
            A distribution is usually evaluated on an arbitrary test function (within a certain class of functions). The answer (v2) makes no mentioning of test functions.
            $endgroup$
            – Qmechanic
            May 23 '15 at 14:38






            $begingroup$
            A distribution is usually evaluated on an arbitrary test function (within a certain class of functions). The answer (v2) makes no mentioning of test functions.
            $endgroup$
            – Qmechanic
            May 23 '15 at 14:38






            1




            1




            $begingroup$
            @Cookie - there is undoubtedly some sort of generalisation, but I don't believe other cases are as simple as $n=3$. I believe the useful observation is that $nablacdot (mathbf{r}/r^n) = 0$ for $rneq 0$ and $n$ dimensions.
            $endgroup$
            – Glen O
            Jun 4 '16 at 8:28






            $begingroup$
            @Cookie - there is undoubtedly some sort of generalisation, but I don't believe other cases are as simple as $n=3$. I believe the useful observation is that $nablacdot (mathbf{r}/r^n) = 0$ for $rneq 0$ and $n$ dimensions.
            $endgroup$
            – Glen O
            Jun 4 '16 at 8:28













            17












            $begingroup$

            I'm new around here (so suggestions about posting are welcome!) and want to give my contribution to this question, even though a bit old. I feel I need to because using the divergence theorem in this context is not quite rigorous. Strictly speaking $1/r$ is not even differentiable at the origin. So here's a proof using limits of distributions.



            Let $mathbf{x}inmathbb{R}^{3}$ and $r=|mathbf{x}|=sqrt{x^2+y^2+z^2}$. It is evident from direct calculation that $nabla^{2}left(frac{1}{r}right)=0$ everywhere except in $mathbf{x}=0$, where it is in fact not defined. Thus, the integral of $nabla^{2}left(frac{1}{r}right)$ over any volume non containing the origin is zero.



            So let $eta>0$ and $r_{eta}=sqrt{x^2+y^2+z^2+eta^2}$. Obviously $limlimits_{etarightarrow 0}r_{eta}=r$. Direct calculation brings
            begin{equation}
            nabla^{2}left(frac{1}{r_{eta}}right) = frac{-3eta^{2}}{r_{eta}^5}
            end{equation}
            Now let us consider the distribution represented by $nabla^{2}left(frac{1}{r_{eta}}right)$ and let $rho$ be a test function (for example in the Schwartz space). I use Dirac's bra-ket notation to express the action of a distribution over a test function. Let $S^{2}$ be the unit sphere. Thus we calculate
            begin{align}
            limlimits_{etarightarrow 0}left.leftlangle nabla^{2}left(frac{1}{r_{eta}}right)right|rhorightrangle &= limlimits_{etarightarrow 0}iiintlimits_{mathbb{R}^3}mathrm{d}^{3}x, nabla^{2}left(frac{1}{r_{eta}}right)rho(mathbf{x})\
            &=limlimits_{etarightarrow 0}left{iiintlimits_{mathbb{R}^3setminus S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})+ iiintlimits_{S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})right}\
            &=limlimits_{etarightarrow 0}iiintlimits_{S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})
            end{align}
            Where the limit of the first of the integrals in the curly braces is zero (easy to show, referring to the laplacian of $1/r$, no need for $eta$ in sets not containing the origin).
            Now Taylor expand $rho$ at $mathbf{x}=0$ and integrate using spherical polar coordinates:
            begin{equation}
            limlimits_{etarightarrow 0}int_{0}^{pi}mathrm{d}theta,sinthetaint_{0}^{2pi}mathrm{d}varphi,int_{0}^{1}mathrm{d}t,frac{-3eta^{2}t^{2}}{(t^{2}+eta^{2})^{5/2}}(rho(0)+O(t^{2}))
            end{equation}
            Integrating you will get that all the terms contained in $O(t^2)$ vanish as $etarightarrow 0$, while the term with $rho(0)$ remains. In fact you get
            begin{align}
            limlimits_{etarightarrow 0}frac{-4pirho(0)}{sqrt{1+eta^{2}}}&=-4pirho(0)\
            &=langle -4pidelta_{0}^{(3)}|rhorangle
            end{align}



            From this argument one defines the limit distribution
            begin{equation}
            nabla^{2}left(frac{1}{r}right):=limlimits_{etarightarrow 0}nabla^{2}left(frac{1}{r_{eta}}right)=-4pidelta_{0}^{(3)}
            end{equation}
            The generalization to $r=|mathbf{x}-mathbf{x}_{0}|$ is obvious.






            share|cite|improve this answer









            $endgroup$













            • $begingroup$
              Great answer! However, could you clarify on the expansion in Taylor series? It seems to me you are supposing that $rho(mathbf{x})$ is only radial.
              $endgroup$
              – rmk236
              Aug 18 '15 at 20:17






            • 1




              $begingroup$
              @rmk236 It doesn't look that way to me. Taylor expanding inside the integral you get the $rho(0)$ term and then all the others of course. But all those other terms (which account for the possibility of $rho$ to be not radial) are included in the $O(t^{2})$. If you need the actual terms or you still have doubts I could carry out the calculation again and post more details on that part.
              $endgroup$
              – Daniele Oriani
              Aug 19 '15 at 22:25
















            17












            $begingroup$

            I'm new around here (so suggestions about posting are welcome!) and want to give my contribution to this question, even though a bit old. I feel I need to because using the divergence theorem in this context is not quite rigorous. Strictly speaking $1/r$ is not even differentiable at the origin. So here's a proof using limits of distributions.



            Let $mathbf{x}inmathbb{R}^{3}$ and $r=|mathbf{x}|=sqrt{x^2+y^2+z^2}$. It is evident from direct calculation that $nabla^{2}left(frac{1}{r}right)=0$ everywhere except in $mathbf{x}=0$, where it is in fact not defined. Thus, the integral of $nabla^{2}left(frac{1}{r}right)$ over any volume non containing the origin is zero.



            So let $eta>0$ and $r_{eta}=sqrt{x^2+y^2+z^2+eta^2}$. Obviously $limlimits_{etarightarrow 0}r_{eta}=r$. Direct calculation brings
            begin{equation}
            nabla^{2}left(frac{1}{r_{eta}}right) = frac{-3eta^{2}}{r_{eta}^5}
            end{equation}
            Now let us consider the distribution represented by $nabla^{2}left(frac{1}{r_{eta}}right)$ and let $rho$ be a test function (for example in the Schwartz space). I use Dirac's bra-ket notation to express the action of a distribution over a test function. Let $S^{2}$ be the unit sphere. Thus we calculate
            begin{align}
            limlimits_{etarightarrow 0}left.leftlangle nabla^{2}left(frac{1}{r_{eta}}right)right|rhorightrangle &= limlimits_{etarightarrow 0}iiintlimits_{mathbb{R}^3}mathrm{d}^{3}x, nabla^{2}left(frac{1}{r_{eta}}right)rho(mathbf{x})\
            &=limlimits_{etarightarrow 0}left{iiintlimits_{mathbb{R}^3setminus S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})+ iiintlimits_{S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})right}\
            &=limlimits_{etarightarrow 0}iiintlimits_{S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})
            end{align}
            Where the limit of the first of the integrals in the curly braces is zero (easy to show, referring to the laplacian of $1/r$, no need for $eta$ in sets not containing the origin).
            Now Taylor expand $rho$ at $mathbf{x}=0$ and integrate using spherical polar coordinates:
            begin{equation}
            limlimits_{etarightarrow 0}int_{0}^{pi}mathrm{d}theta,sinthetaint_{0}^{2pi}mathrm{d}varphi,int_{0}^{1}mathrm{d}t,frac{-3eta^{2}t^{2}}{(t^{2}+eta^{2})^{5/2}}(rho(0)+O(t^{2}))
            end{equation}
            Integrating you will get that all the terms contained in $O(t^2)$ vanish as $etarightarrow 0$, while the term with $rho(0)$ remains. In fact you get
            begin{align}
            limlimits_{etarightarrow 0}frac{-4pirho(0)}{sqrt{1+eta^{2}}}&=-4pirho(0)\
            &=langle -4pidelta_{0}^{(3)}|rhorangle
            end{align}



            From this argument one defines the limit distribution
            begin{equation}
            nabla^{2}left(frac{1}{r}right):=limlimits_{etarightarrow 0}nabla^{2}left(frac{1}{r_{eta}}right)=-4pidelta_{0}^{(3)}
            end{equation}
            The generalization to $r=|mathbf{x}-mathbf{x}_{0}|$ is obvious.






            share|cite|improve this answer









            $endgroup$













            • $begingroup$
              Great answer! However, could you clarify on the expansion in Taylor series? It seems to me you are supposing that $rho(mathbf{x})$ is only radial.
              $endgroup$
              – rmk236
              Aug 18 '15 at 20:17






            • 1




              $begingroup$
              @rmk236 It doesn't look that way to me. Taylor expanding inside the integral you get the $rho(0)$ term and then all the others of course. But all those other terms (which account for the possibility of $rho$ to be not radial) are included in the $O(t^{2})$. If you need the actual terms or you still have doubts I could carry out the calculation again and post more details on that part.
              $endgroup$
              – Daniele Oriani
              Aug 19 '15 at 22:25














            17












            17








            17





            $begingroup$

            I'm new around here (so suggestions about posting are welcome!) and want to give my contribution to this question, even though a bit old. I feel I need to because using the divergence theorem in this context is not quite rigorous. Strictly speaking $1/r$ is not even differentiable at the origin. So here's a proof using limits of distributions.



            Let $mathbf{x}inmathbb{R}^{3}$ and $r=|mathbf{x}|=sqrt{x^2+y^2+z^2}$. It is evident from direct calculation that $nabla^{2}left(frac{1}{r}right)=0$ everywhere except in $mathbf{x}=0$, where it is in fact not defined. Thus, the integral of $nabla^{2}left(frac{1}{r}right)$ over any volume non containing the origin is zero.



            So let $eta>0$ and $r_{eta}=sqrt{x^2+y^2+z^2+eta^2}$. Obviously $limlimits_{etarightarrow 0}r_{eta}=r$. Direct calculation brings
            begin{equation}
            nabla^{2}left(frac{1}{r_{eta}}right) = frac{-3eta^{2}}{r_{eta}^5}
            end{equation}
            Now let us consider the distribution represented by $nabla^{2}left(frac{1}{r_{eta}}right)$ and let $rho$ be a test function (for example in the Schwartz space). I use Dirac's bra-ket notation to express the action of a distribution over a test function. Let $S^{2}$ be the unit sphere. Thus we calculate
            begin{align}
            limlimits_{etarightarrow 0}left.leftlangle nabla^{2}left(frac{1}{r_{eta}}right)right|rhorightrangle &= limlimits_{etarightarrow 0}iiintlimits_{mathbb{R}^3}mathrm{d}^{3}x, nabla^{2}left(frac{1}{r_{eta}}right)rho(mathbf{x})\
            &=limlimits_{etarightarrow 0}left{iiintlimits_{mathbb{R}^3setminus S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})+ iiintlimits_{S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})right}\
            &=limlimits_{etarightarrow 0}iiintlimits_{S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})
            end{align}
            Where the limit of the first of the integrals in the curly braces is zero (easy to show, referring to the laplacian of $1/r$, no need for $eta$ in sets not containing the origin).
            Now Taylor expand $rho$ at $mathbf{x}=0$ and integrate using spherical polar coordinates:
            begin{equation}
            limlimits_{etarightarrow 0}int_{0}^{pi}mathrm{d}theta,sinthetaint_{0}^{2pi}mathrm{d}varphi,int_{0}^{1}mathrm{d}t,frac{-3eta^{2}t^{2}}{(t^{2}+eta^{2})^{5/2}}(rho(0)+O(t^{2}))
            end{equation}
            Integrating you will get that all the terms contained in $O(t^2)$ vanish as $etarightarrow 0$, while the term with $rho(0)$ remains. In fact you get
            begin{align}
            limlimits_{etarightarrow 0}frac{-4pirho(0)}{sqrt{1+eta^{2}}}&=-4pirho(0)\
            &=langle -4pidelta_{0}^{(3)}|rhorangle
            end{align}



            From this argument one defines the limit distribution
            begin{equation}
            nabla^{2}left(frac{1}{r}right):=limlimits_{etarightarrow 0}nabla^{2}left(frac{1}{r_{eta}}right)=-4pidelta_{0}^{(3)}
            end{equation}
            The generalization to $r=|mathbf{x}-mathbf{x}_{0}|$ is obvious.






            share|cite|improve this answer









            $endgroup$



            I'm new around here (so suggestions about posting are welcome!) and want to give my contribution to this question, even though a bit old. I feel I need to because using the divergence theorem in this context is not quite rigorous. Strictly speaking $1/r$ is not even differentiable at the origin. So here's a proof using limits of distributions.



            Let $mathbf{x}inmathbb{R}^{3}$ and $r=|mathbf{x}|=sqrt{x^2+y^2+z^2}$. It is evident from direct calculation that $nabla^{2}left(frac{1}{r}right)=0$ everywhere except in $mathbf{x}=0$, where it is in fact not defined. Thus, the integral of $nabla^{2}left(frac{1}{r}right)$ over any volume non containing the origin is zero.



            So let $eta>0$ and $r_{eta}=sqrt{x^2+y^2+z^2+eta^2}$. Obviously $limlimits_{etarightarrow 0}r_{eta}=r$. Direct calculation brings
            begin{equation}
            nabla^{2}left(frac{1}{r_{eta}}right) = frac{-3eta^{2}}{r_{eta}^5}
            end{equation}
            Now let us consider the distribution represented by $nabla^{2}left(frac{1}{r_{eta}}right)$ and let $rho$ be a test function (for example in the Schwartz space). I use Dirac's bra-ket notation to express the action of a distribution over a test function. Let $S^{2}$ be the unit sphere. Thus we calculate
            begin{align}
            limlimits_{etarightarrow 0}left.leftlangle nabla^{2}left(frac{1}{r_{eta}}right)right|rhorightrangle &= limlimits_{etarightarrow 0}iiintlimits_{mathbb{R}^3}mathrm{d}^{3}x, nabla^{2}left(frac{1}{r_{eta}}right)rho(mathbf{x})\
            &=limlimits_{etarightarrow 0}left{iiintlimits_{mathbb{R}^3setminus S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})+ iiintlimits_{S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})right}\
            &=limlimits_{etarightarrow 0}iiintlimits_{S^{2}}mathrm{d}^{3}x, frac{-3eta^{2}}{r_{eta}^5}rho(mathbf{x})
            end{align}
            Where the limit of the first of the integrals in the curly braces is zero (easy to show, referring to the laplacian of $1/r$, no need for $eta$ in sets not containing the origin).
            Now Taylor expand $rho$ at $mathbf{x}=0$ and integrate using spherical polar coordinates:
            begin{equation}
            limlimits_{etarightarrow 0}int_{0}^{pi}mathrm{d}theta,sinthetaint_{0}^{2pi}mathrm{d}varphi,int_{0}^{1}mathrm{d}t,frac{-3eta^{2}t^{2}}{(t^{2}+eta^{2})^{5/2}}(rho(0)+O(t^{2}))
            end{equation}
            Integrating you will get that all the terms contained in $O(t^2)$ vanish as $etarightarrow 0$, while the term with $rho(0)$ remains. In fact you get
            begin{align}
            limlimits_{etarightarrow 0}frac{-4pirho(0)}{sqrt{1+eta^{2}}}&=-4pirho(0)\
            &=langle -4pidelta_{0}^{(3)}|rhorangle
            end{align}



            From this argument one defines the limit distribution
            begin{equation}
            nabla^{2}left(frac{1}{r}right):=limlimits_{etarightarrow 0}nabla^{2}left(frac{1}{r_{eta}}right)=-4pidelta_{0}^{(3)}
            end{equation}
            The generalization to $r=|mathbf{x}-mathbf{x}_{0}|$ is obvious.







            share|cite|improve this answer












            share|cite|improve this answer



            share|cite|improve this answer










            answered Jun 28 '15 at 21:59









            Daniele OrianiDaniele Oriani

            17112




            17112












            • $begingroup$
              Great answer! However, could you clarify on the expansion in Taylor series? It seems to me you are supposing that $rho(mathbf{x})$ is only radial.
              $endgroup$
              – rmk236
              Aug 18 '15 at 20:17






            • 1




              $begingroup$
              @rmk236 It doesn't look that way to me. Taylor expanding inside the integral you get the $rho(0)$ term and then all the others of course. But all those other terms (which account for the possibility of $rho$ to be not radial) are included in the $O(t^{2})$. If you need the actual terms or you still have doubts I could carry out the calculation again and post more details on that part.
              $endgroup$
              – Daniele Oriani
              Aug 19 '15 at 22:25


















            • $begingroup$
              Great answer! However, could you clarify on the expansion in Taylor series? It seems to me you are supposing that $rho(mathbf{x})$ is only radial.
              $endgroup$
              – rmk236
              Aug 18 '15 at 20:17






            • 1




              $begingroup$
              @rmk236 It doesn't look that way to me. Taylor expanding inside the integral you get the $rho(0)$ term and then all the others of course. But all those other terms (which account for the possibility of $rho$ to be not radial) are included in the $O(t^{2})$. If you need the actual terms or you still have doubts I could carry out the calculation again and post more details on that part.
              $endgroup$
              – Daniele Oriani
              Aug 19 '15 at 22:25
















            $begingroup$
            Great answer! However, could you clarify on the expansion in Taylor series? It seems to me you are supposing that $rho(mathbf{x})$ is only radial.
            $endgroup$
            – rmk236
            Aug 18 '15 at 20:17




            $begingroup$
            Great answer! However, could you clarify on the expansion in Taylor series? It seems to me you are supposing that $rho(mathbf{x})$ is only radial.
            $endgroup$
            – rmk236
            Aug 18 '15 at 20:17




            1




            1




            $begingroup$
            @rmk236 It doesn't look that way to me. Taylor expanding inside the integral you get the $rho(0)$ term and then all the others of course. But all those other terms (which account for the possibility of $rho$ to be not radial) are included in the $O(t^{2})$. If you need the actual terms or you still have doubts I could carry out the calculation again and post more details on that part.
            $endgroup$
            – Daniele Oriani
            Aug 19 '15 at 22:25




            $begingroup$
            @rmk236 It doesn't look that way to me. Taylor expanding inside the integral you get the $rho(0)$ term and then all the others of course. But all those other terms (which account for the possibility of $rho$ to be not radial) are included in the $O(t^{2})$. If you need the actual terms or you still have doubts I could carry out the calculation again and post more details on that part.
            $endgroup$
            – Daniele Oriani
            Aug 19 '15 at 22:25











            0












            $begingroup$

            Here is a back-alley derivation using Fourier transform properties.
            Take the Fourier transform of $frac{1}{4 pi r}$ to get $frac{1}{k^2}$. Therefore,
            $$
            frac{1}{4pi r} = int frac{d^3k}{(2pi)^3} frac{e^{-ikcdot r}}{k^2}
            $$

            Now, apply $-nabla^2$ to get
            $$
            -nabla^2 frac{1}{4pi r} = int frac{d^3k}{(2pi)^3} e^{-ikcdot r}
            $$

            This is the delta function, but we can explicitly put in our test function:
            begin{align*}
            int d^3r left(-nabla^2 frac{1}{4 pi r}right) f(r) &=
            int frac{d^3k}{(2pi)^3} int d^3r e^{-ikcdot r} f(r) \
            &=
            int frac{d^3k}{(2pi)^3} tilde{f}(k) \
            & = f(r=0).
            end{align*}






            share|cite|improve this answer









            $endgroup$


















              0












              $begingroup$

              Here is a back-alley derivation using Fourier transform properties.
              Take the Fourier transform of $frac{1}{4 pi r}$ to get $frac{1}{k^2}$. Therefore,
              $$
              frac{1}{4pi r} = int frac{d^3k}{(2pi)^3} frac{e^{-ikcdot r}}{k^2}
              $$

              Now, apply $-nabla^2$ to get
              $$
              -nabla^2 frac{1}{4pi r} = int frac{d^3k}{(2pi)^3} e^{-ikcdot r}
              $$

              This is the delta function, but we can explicitly put in our test function:
              begin{align*}
              int d^3r left(-nabla^2 frac{1}{4 pi r}right) f(r) &=
              int frac{d^3k}{(2pi)^3} int d^3r e^{-ikcdot r} f(r) \
              &=
              int frac{d^3k}{(2pi)^3} tilde{f}(k) \
              & = f(r=0).
              end{align*}






              share|cite|improve this answer









              $endgroup$
















                0












                0








                0





                $begingroup$

                Here is a back-alley derivation using Fourier transform properties.
                Take the Fourier transform of $frac{1}{4 pi r}$ to get $frac{1}{k^2}$. Therefore,
                $$
                frac{1}{4pi r} = int frac{d^3k}{(2pi)^3} frac{e^{-ikcdot r}}{k^2}
                $$

                Now, apply $-nabla^2$ to get
                $$
                -nabla^2 frac{1}{4pi r} = int frac{d^3k}{(2pi)^3} e^{-ikcdot r}
                $$

                This is the delta function, but we can explicitly put in our test function:
                begin{align*}
                int d^3r left(-nabla^2 frac{1}{4 pi r}right) f(r) &=
                int frac{d^3k}{(2pi)^3} int d^3r e^{-ikcdot r} f(r) \
                &=
                int frac{d^3k}{(2pi)^3} tilde{f}(k) \
                & = f(r=0).
                end{align*}






                share|cite|improve this answer









                $endgroup$



                Here is a back-alley derivation using Fourier transform properties.
                Take the Fourier transform of $frac{1}{4 pi r}$ to get $frac{1}{k^2}$. Therefore,
                $$
                frac{1}{4pi r} = int frac{d^3k}{(2pi)^3} frac{e^{-ikcdot r}}{k^2}
                $$

                Now, apply $-nabla^2$ to get
                $$
                -nabla^2 frac{1}{4pi r} = int frac{d^3k}{(2pi)^3} e^{-ikcdot r}
                $$

                This is the delta function, but we can explicitly put in our test function:
                begin{align*}
                int d^3r left(-nabla^2 frac{1}{4 pi r}right) f(r) &=
                int frac{d^3k}{(2pi)^3} int d^3r e^{-ikcdot r} f(r) \
                &=
                int frac{d^3k}{(2pi)^3} tilde{f}(k) \
                & = f(r=0).
                end{align*}







                share|cite|improve this answer












                share|cite|improve this answer



                share|cite|improve this answer










                answered Dec 21 '18 at 6:52









                l8erg8erl8erg8er

                11




                11






























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