Weak convergence of measures and of total variations












1












$begingroup$


I have a sequence of signed, bounded measures ${mu_n}_{nin mathbb N}$ and an open, bounded set $Omega subset mathbb R^N$.
I know that $vert mu_n vert(Omega) to vert mu vert (Omega)$ (as real numbers) for a suitable measure $mu$. In particular, the sequence $mu_n$ is uniformly norm-bounded (being the norm on the space of measures the total variation) hence by compactness there exists a measure $lambda$ such that (up to subsequences) $mu_n rightharpoonup lambda$ weakly.



Can I conclude that $lambda ll mu$? What can I say on the relationship between $lambda, mu$? I apologize for the confusion, but I am puzzled.





EDIT



This question arises essentially from reading this paper. It seems to me that, mutatis mutandis, the authors claim what I am asking at page 20. Let me present a simplified and self-contained version of the argument: let $B_1 subset mathbb R^N$ be the unit ball in $mathbb R^N$. The authors define $u^varepsilon(x) = min left{frac{d(x, mathbb R^N setminus B_1)}{varepsilon}, 1 right}$ and they assume (see eq. (17) in the paper) that
$$
vert Du^varepsilon vert(mathbb R^N) to P(B_1) = mathcal H^{N-1} llcorner_{partial B_1}(mathbb R^N) =: mu(mathbb R^N)
$$

where $mathcal H^{N-1}$ is the Hausdorff measure (the last equation is the one right under (18) in the paper). From this convergence they conclude that the vector valued measures $(Du^varepsilon mathcal L^N)$ are compact and they converge - up to subsequences - to a vector valued measure $mu^infty$ which they prove is a.c. w.r.t. $mathcal H^{N-1}llcorner_{partial B_1}$... What have I misunderstood? Am I missing something?










share|cite|improve this question











$endgroup$

















    1












    $begingroup$


    I have a sequence of signed, bounded measures ${mu_n}_{nin mathbb N}$ and an open, bounded set $Omega subset mathbb R^N$.
    I know that $vert mu_n vert(Omega) to vert mu vert (Omega)$ (as real numbers) for a suitable measure $mu$. In particular, the sequence $mu_n$ is uniformly norm-bounded (being the norm on the space of measures the total variation) hence by compactness there exists a measure $lambda$ such that (up to subsequences) $mu_n rightharpoonup lambda$ weakly.



    Can I conclude that $lambda ll mu$? What can I say on the relationship between $lambda, mu$? I apologize for the confusion, but I am puzzled.





    EDIT



    This question arises essentially from reading this paper. It seems to me that, mutatis mutandis, the authors claim what I am asking at page 20. Let me present a simplified and self-contained version of the argument: let $B_1 subset mathbb R^N$ be the unit ball in $mathbb R^N$. The authors define $u^varepsilon(x) = min left{frac{d(x, mathbb R^N setminus B_1)}{varepsilon}, 1 right}$ and they assume (see eq. (17) in the paper) that
    $$
    vert Du^varepsilon vert(mathbb R^N) to P(B_1) = mathcal H^{N-1} llcorner_{partial B_1}(mathbb R^N) =: mu(mathbb R^N)
    $$

    where $mathcal H^{N-1}$ is the Hausdorff measure (the last equation is the one right under (18) in the paper). From this convergence they conclude that the vector valued measures $(Du^varepsilon mathcal L^N)$ are compact and they converge - up to subsequences - to a vector valued measure $mu^infty$ which they prove is a.c. w.r.t. $mathcal H^{N-1}llcorner_{partial B_1}$... What have I misunderstood? Am I missing something?










    share|cite|improve this question











    $endgroup$















      1












      1








      1





      $begingroup$


      I have a sequence of signed, bounded measures ${mu_n}_{nin mathbb N}$ and an open, bounded set $Omega subset mathbb R^N$.
      I know that $vert mu_n vert(Omega) to vert mu vert (Omega)$ (as real numbers) for a suitable measure $mu$. In particular, the sequence $mu_n$ is uniformly norm-bounded (being the norm on the space of measures the total variation) hence by compactness there exists a measure $lambda$ such that (up to subsequences) $mu_n rightharpoonup lambda$ weakly.



      Can I conclude that $lambda ll mu$? What can I say on the relationship between $lambda, mu$? I apologize for the confusion, but I am puzzled.





      EDIT



      This question arises essentially from reading this paper. It seems to me that, mutatis mutandis, the authors claim what I am asking at page 20. Let me present a simplified and self-contained version of the argument: let $B_1 subset mathbb R^N$ be the unit ball in $mathbb R^N$. The authors define $u^varepsilon(x) = min left{frac{d(x, mathbb R^N setminus B_1)}{varepsilon}, 1 right}$ and they assume (see eq. (17) in the paper) that
      $$
      vert Du^varepsilon vert(mathbb R^N) to P(B_1) = mathcal H^{N-1} llcorner_{partial B_1}(mathbb R^N) =: mu(mathbb R^N)
      $$

      where $mathcal H^{N-1}$ is the Hausdorff measure (the last equation is the one right under (18) in the paper). From this convergence they conclude that the vector valued measures $(Du^varepsilon mathcal L^N)$ are compact and they converge - up to subsequences - to a vector valued measure $mu^infty$ which they prove is a.c. w.r.t. $mathcal H^{N-1}llcorner_{partial B_1}$... What have I misunderstood? Am I missing something?










      share|cite|improve this question











      $endgroup$




      I have a sequence of signed, bounded measures ${mu_n}_{nin mathbb N}$ and an open, bounded set $Omega subset mathbb R^N$.
      I know that $vert mu_n vert(Omega) to vert mu vert (Omega)$ (as real numbers) for a suitable measure $mu$. In particular, the sequence $mu_n$ is uniformly norm-bounded (being the norm on the space of measures the total variation) hence by compactness there exists a measure $lambda$ such that (up to subsequences) $mu_n rightharpoonup lambda$ weakly.



      Can I conclude that $lambda ll mu$? What can I say on the relationship between $lambda, mu$? I apologize for the confusion, but I am puzzled.





      EDIT



      This question arises essentially from reading this paper. It seems to me that, mutatis mutandis, the authors claim what I am asking at page 20. Let me present a simplified and self-contained version of the argument: let $B_1 subset mathbb R^N$ be the unit ball in $mathbb R^N$. The authors define $u^varepsilon(x) = min left{frac{d(x, mathbb R^N setminus B_1)}{varepsilon}, 1 right}$ and they assume (see eq. (17) in the paper) that
      $$
      vert Du^varepsilon vert(mathbb R^N) to P(B_1) = mathcal H^{N-1} llcorner_{partial B_1}(mathbb R^N) =: mu(mathbb R^N)
      $$

      where $mathcal H^{N-1}$ is the Hausdorff measure (the last equation is the one right under (18) in the paper). From this convergence they conclude that the vector valued measures $(Du^varepsilon mathcal L^N)$ are compact and they converge - up to subsequences - to a vector valued measure $mu^infty$ which they prove is a.c. w.r.t. $mathcal H^{N-1}llcorner_{partial B_1}$... What have I misunderstood? Am I missing something?







      real-analysis measure-theory weak-convergence






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      share|cite|improve this question













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      edited Jan 20 at 10:10







      Romeo

















      asked Jan 20 at 0:11









      RomeoRomeo

      3,05721148




      3,05721148






















          1 Answer
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          $begingroup$

          I suspect that when you wrote $|mu_n|(Omega)to|mu|(Omega)$ maybe that's not exactly what you meant. Replying to the question as stated:



          You assume so little about $mu$ that it really has nothing to do with the rest of what's going on; there's no relationship between $lambda$ and $mu$. One doesn't need to "construct" a counterexample, any almost random choice of $mu_n$ and $mu$ works.



          Say $mu_n=delta_{1/n}$, a point mass at $1/n$. So $mu_ntodelta_0$. Let $Omega=(-1,1)$ and let $mu$ be any positive measure with $mu(Omega)=1$.



          Or maybe to better illustrate how $mu$ really has nothing to do with $lambda$, let $Omega=(2,3)$ and let $mu$ be any measure with $mu(Omega)=0$. Or $Omega=emptyset$ and $mu=0$.



          Heh, let $mu_n$ be any norm-bounded sequence, $Omega=emptyset$, $mu=0$.



          Edit: Regarding the edit made to the question, and the comment asking whether there's any significant difference: Well of course there's a huge difference, since in the new version we have a specific "sequence" of measures! In particular, for example, if I'm reading things correctly $mu_epsilon$ is supported in the annulus $A_epsilon={1-epsilonle|x|le1}$.



          If I have the picture right it seems clear that the gradient of $u_epsilon$ is $nabla u_epsilon(x)=-frac1epsilonfrac x{|x|}$ or something like that in $A_epsilon$, $0$ elsewhere. So it seems clear that $mu_epsilontolambda$, where $dlambda=-n(x),dH$ (where $n$ is the outward unit normal on the sphere and $H$ is surface area on the sphere), which certainly appears to be ac wrt $H$.



          Of course that could be all wrong, it's just my first impression. But note that the various things I say "seem clear" seem clear to me based on my picture of what $mu_epsilon$ actually is, not because of any general principle analogous to what you ask about in the original version of the question!



          As a general rule, if they assert P and you don't see why P holds you might be better off actually stating what they actually assert and asking why it holds, instead of sort of guessing that they seem to be saying that P follows from Q and asking whether Q implies P.



          Second edit: Two things.



          (i) A conjecture regarding the sort of "soft" or "abstract" argument the authors might have had in mind: It's easy tp see that $||mu_epsilon||$ is bounded. And $mu_epsilon$ has a certain sort of rotational symmetry (which I'm not going to try to define precisely; this isn't my argument after all); hence any weak limit $lambda$ must have the same symmetry. It's clear that $lambda$ must be supported on $S={|x|=1}$, since the support of $mu_epsilon$ shrinks to $S$, and the only vector-valued measure on $S$ with that symmetry is $cn,dH$.



          That's pretty vague; I'm not going to try to make it more precise, since it's just my guess regarding sort of what the authors may have had in mind. But:



          (ii) Why it seems clear to me that $mu_epsilon$ simply does converge to what I say it does:



          First, in general if $u$ is a radial function, $$u(x)=phi(|x|),$$then $$nabla u(x)=phi'(|x|)frac x{|x|}.$$("Advanced calculus": $nabla u$ is the directional derivative in the direction of greatest increase, which is to say in a direction orthogonal to the level sets of $u$...) Hence $nabla u_epsilon$ is what I say it is above.



          Now assume $fin C_c(Bbb R^n)$ and integrate in polar coordinates:



          $$int_{Bbb R^n}f(x)nabla u_epsilon(x),dx=int_Sfrac{-1}{epsilon}int_{1-epsilon}^1f(rxi)xi r^{n-1},drdH(xi).$$And since $f$ is continuous it's clear that $$lim_{epsilonto0}frac{-1}{epsilon}int_{1-epsilon}^1f(rxi)xi r^{n-1},dr=-f(xi)xi,$$uniformly over $xiin S$.



          ("Polar coordinates": In general $$int_{Bbb R^n}g(x),dx=c_nint_Sint_0^infty g(rxi)r^{n-1},drdH(xi).$$Note that if $H$ is actual "surface area" on $S$, in particular not normalized to be a probability measure as is sometimes done in that formula, then $c_n=1$. See Folland Real Analysis or various other places.)






          share|cite|improve this answer











          $endgroup$













          • $begingroup$
            Thank you very much for your kind reply. I see your point and I totally agree with you, the question is essentially ill-posed. However, I am still in troubles, see the edit to my question. It seems to me that the authors kind of claim what I asked. Is there any significative difference in their "particular" case? Have I misunderstood anything? Thanks for your help.
            $endgroup$
            – Romeo
            Jan 20 at 10:13










          • $begingroup$
            Understood, you gave me a "lesson of method" and I thank you for it. Yet, I believe that in the aforementioned paper the peculiar form of the sequence seems to be not so relevant (at least this was my impression). In some sense, reading your edit, one might see the picture simply as: well, we have $(mu_epsilon)_epsilon$ which has a specific form and this sequence converges to the surface measure. But this is not the way the authors propose the arguments. Last question, I promise: Could you please justify why it seems clear to you that $mu_epsilon to lambda$ (in your notation)? Thanks.
            $endgroup$
            – Romeo
            Jan 20 at 15:10










          • $begingroup$
            Cux you just write down what $int f,dmu_epsilon$ is and let $epsilonto0$. See edit....
            $endgroup$
            – David C. Ullrich
            Jan 20 at 15:43










          • $begingroup$
            "Cux" $to$ "Cuz"
            $endgroup$
            – David C. Ullrich
            Jan 20 at 15:50










          • $begingroup$
            @Romeo Hmm. A way one could deduce that $lambda<<H$ without saying anything about what $lambda$ is: If $Esubset S$ say $V(E)={rxi:r>0,xiin E}$. Suppose there exists a function $phi$ with $lim_{tto0}phi(t)=0$ such that $mu_n(V(E)lephi(H(E))$ for all $n$.. If $mu_ntolambda$ weakly and $lambda$ is supported on $S$ then $lambda<<H$.
            $endgroup$
            – David C. Ullrich
            Jan 20 at 17:04











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          $begingroup$

          I suspect that when you wrote $|mu_n|(Omega)to|mu|(Omega)$ maybe that's not exactly what you meant. Replying to the question as stated:



          You assume so little about $mu$ that it really has nothing to do with the rest of what's going on; there's no relationship between $lambda$ and $mu$. One doesn't need to "construct" a counterexample, any almost random choice of $mu_n$ and $mu$ works.



          Say $mu_n=delta_{1/n}$, a point mass at $1/n$. So $mu_ntodelta_0$. Let $Omega=(-1,1)$ and let $mu$ be any positive measure with $mu(Omega)=1$.



          Or maybe to better illustrate how $mu$ really has nothing to do with $lambda$, let $Omega=(2,3)$ and let $mu$ be any measure with $mu(Omega)=0$. Or $Omega=emptyset$ and $mu=0$.



          Heh, let $mu_n$ be any norm-bounded sequence, $Omega=emptyset$, $mu=0$.



          Edit: Regarding the edit made to the question, and the comment asking whether there's any significant difference: Well of course there's a huge difference, since in the new version we have a specific "sequence" of measures! In particular, for example, if I'm reading things correctly $mu_epsilon$ is supported in the annulus $A_epsilon={1-epsilonle|x|le1}$.



          If I have the picture right it seems clear that the gradient of $u_epsilon$ is $nabla u_epsilon(x)=-frac1epsilonfrac x{|x|}$ or something like that in $A_epsilon$, $0$ elsewhere. So it seems clear that $mu_epsilontolambda$, where $dlambda=-n(x),dH$ (where $n$ is the outward unit normal on the sphere and $H$ is surface area on the sphere), which certainly appears to be ac wrt $H$.



          Of course that could be all wrong, it's just my first impression. But note that the various things I say "seem clear" seem clear to me based on my picture of what $mu_epsilon$ actually is, not because of any general principle analogous to what you ask about in the original version of the question!



          As a general rule, if they assert P and you don't see why P holds you might be better off actually stating what they actually assert and asking why it holds, instead of sort of guessing that they seem to be saying that P follows from Q and asking whether Q implies P.



          Second edit: Two things.



          (i) A conjecture regarding the sort of "soft" or "abstract" argument the authors might have had in mind: It's easy tp see that $||mu_epsilon||$ is bounded. And $mu_epsilon$ has a certain sort of rotational symmetry (which I'm not going to try to define precisely; this isn't my argument after all); hence any weak limit $lambda$ must have the same symmetry. It's clear that $lambda$ must be supported on $S={|x|=1}$, since the support of $mu_epsilon$ shrinks to $S$, and the only vector-valued measure on $S$ with that symmetry is $cn,dH$.



          That's pretty vague; I'm not going to try to make it more precise, since it's just my guess regarding sort of what the authors may have had in mind. But:



          (ii) Why it seems clear to me that $mu_epsilon$ simply does converge to what I say it does:



          First, in general if $u$ is a radial function, $$u(x)=phi(|x|),$$then $$nabla u(x)=phi'(|x|)frac x{|x|}.$$("Advanced calculus": $nabla u$ is the directional derivative in the direction of greatest increase, which is to say in a direction orthogonal to the level sets of $u$...) Hence $nabla u_epsilon$ is what I say it is above.



          Now assume $fin C_c(Bbb R^n)$ and integrate in polar coordinates:



          $$int_{Bbb R^n}f(x)nabla u_epsilon(x),dx=int_Sfrac{-1}{epsilon}int_{1-epsilon}^1f(rxi)xi r^{n-1},drdH(xi).$$And since $f$ is continuous it's clear that $$lim_{epsilonto0}frac{-1}{epsilon}int_{1-epsilon}^1f(rxi)xi r^{n-1},dr=-f(xi)xi,$$uniformly over $xiin S$.



          ("Polar coordinates": In general $$int_{Bbb R^n}g(x),dx=c_nint_Sint_0^infty g(rxi)r^{n-1},drdH(xi).$$Note that if $H$ is actual "surface area" on $S$, in particular not normalized to be a probability measure as is sometimes done in that formula, then $c_n=1$. See Folland Real Analysis or various other places.)






          share|cite|improve this answer











          $endgroup$













          • $begingroup$
            Thank you very much for your kind reply. I see your point and I totally agree with you, the question is essentially ill-posed. However, I am still in troubles, see the edit to my question. It seems to me that the authors kind of claim what I asked. Is there any significative difference in their "particular" case? Have I misunderstood anything? Thanks for your help.
            $endgroup$
            – Romeo
            Jan 20 at 10:13










          • $begingroup$
            Understood, you gave me a "lesson of method" and I thank you for it. Yet, I believe that in the aforementioned paper the peculiar form of the sequence seems to be not so relevant (at least this was my impression). In some sense, reading your edit, one might see the picture simply as: well, we have $(mu_epsilon)_epsilon$ which has a specific form and this sequence converges to the surface measure. But this is not the way the authors propose the arguments. Last question, I promise: Could you please justify why it seems clear to you that $mu_epsilon to lambda$ (in your notation)? Thanks.
            $endgroup$
            – Romeo
            Jan 20 at 15:10










          • $begingroup$
            Cux you just write down what $int f,dmu_epsilon$ is and let $epsilonto0$. See edit....
            $endgroup$
            – David C. Ullrich
            Jan 20 at 15:43










          • $begingroup$
            "Cux" $to$ "Cuz"
            $endgroup$
            – David C. Ullrich
            Jan 20 at 15:50










          • $begingroup$
            @Romeo Hmm. A way one could deduce that $lambda<<H$ without saying anything about what $lambda$ is: If $Esubset S$ say $V(E)={rxi:r>0,xiin E}$. Suppose there exists a function $phi$ with $lim_{tto0}phi(t)=0$ such that $mu_n(V(E)lephi(H(E))$ for all $n$.. If $mu_ntolambda$ weakly and $lambda$ is supported on $S$ then $lambda<<H$.
            $endgroup$
            – David C. Ullrich
            Jan 20 at 17:04
















          1












          $begingroup$

          I suspect that when you wrote $|mu_n|(Omega)to|mu|(Omega)$ maybe that's not exactly what you meant. Replying to the question as stated:



          You assume so little about $mu$ that it really has nothing to do with the rest of what's going on; there's no relationship between $lambda$ and $mu$. One doesn't need to "construct" a counterexample, any almost random choice of $mu_n$ and $mu$ works.



          Say $mu_n=delta_{1/n}$, a point mass at $1/n$. So $mu_ntodelta_0$. Let $Omega=(-1,1)$ and let $mu$ be any positive measure with $mu(Omega)=1$.



          Or maybe to better illustrate how $mu$ really has nothing to do with $lambda$, let $Omega=(2,3)$ and let $mu$ be any measure with $mu(Omega)=0$. Or $Omega=emptyset$ and $mu=0$.



          Heh, let $mu_n$ be any norm-bounded sequence, $Omega=emptyset$, $mu=0$.



          Edit: Regarding the edit made to the question, and the comment asking whether there's any significant difference: Well of course there's a huge difference, since in the new version we have a specific "sequence" of measures! In particular, for example, if I'm reading things correctly $mu_epsilon$ is supported in the annulus $A_epsilon={1-epsilonle|x|le1}$.



          If I have the picture right it seems clear that the gradient of $u_epsilon$ is $nabla u_epsilon(x)=-frac1epsilonfrac x{|x|}$ or something like that in $A_epsilon$, $0$ elsewhere. So it seems clear that $mu_epsilontolambda$, where $dlambda=-n(x),dH$ (where $n$ is the outward unit normal on the sphere and $H$ is surface area on the sphere), which certainly appears to be ac wrt $H$.



          Of course that could be all wrong, it's just my first impression. But note that the various things I say "seem clear" seem clear to me based on my picture of what $mu_epsilon$ actually is, not because of any general principle analogous to what you ask about in the original version of the question!



          As a general rule, if they assert P and you don't see why P holds you might be better off actually stating what they actually assert and asking why it holds, instead of sort of guessing that they seem to be saying that P follows from Q and asking whether Q implies P.



          Second edit: Two things.



          (i) A conjecture regarding the sort of "soft" or "abstract" argument the authors might have had in mind: It's easy tp see that $||mu_epsilon||$ is bounded. And $mu_epsilon$ has a certain sort of rotational symmetry (which I'm not going to try to define precisely; this isn't my argument after all); hence any weak limit $lambda$ must have the same symmetry. It's clear that $lambda$ must be supported on $S={|x|=1}$, since the support of $mu_epsilon$ shrinks to $S$, and the only vector-valued measure on $S$ with that symmetry is $cn,dH$.



          That's pretty vague; I'm not going to try to make it more precise, since it's just my guess regarding sort of what the authors may have had in mind. But:



          (ii) Why it seems clear to me that $mu_epsilon$ simply does converge to what I say it does:



          First, in general if $u$ is a radial function, $$u(x)=phi(|x|),$$then $$nabla u(x)=phi'(|x|)frac x{|x|}.$$("Advanced calculus": $nabla u$ is the directional derivative in the direction of greatest increase, which is to say in a direction orthogonal to the level sets of $u$...) Hence $nabla u_epsilon$ is what I say it is above.



          Now assume $fin C_c(Bbb R^n)$ and integrate in polar coordinates:



          $$int_{Bbb R^n}f(x)nabla u_epsilon(x),dx=int_Sfrac{-1}{epsilon}int_{1-epsilon}^1f(rxi)xi r^{n-1},drdH(xi).$$And since $f$ is continuous it's clear that $$lim_{epsilonto0}frac{-1}{epsilon}int_{1-epsilon}^1f(rxi)xi r^{n-1},dr=-f(xi)xi,$$uniformly over $xiin S$.



          ("Polar coordinates": In general $$int_{Bbb R^n}g(x),dx=c_nint_Sint_0^infty g(rxi)r^{n-1},drdH(xi).$$Note that if $H$ is actual "surface area" on $S$, in particular not normalized to be a probability measure as is sometimes done in that formula, then $c_n=1$. See Folland Real Analysis or various other places.)






          share|cite|improve this answer











          $endgroup$













          • $begingroup$
            Thank you very much for your kind reply. I see your point and I totally agree with you, the question is essentially ill-posed. However, I am still in troubles, see the edit to my question. It seems to me that the authors kind of claim what I asked. Is there any significative difference in their "particular" case? Have I misunderstood anything? Thanks for your help.
            $endgroup$
            – Romeo
            Jan 20 at 10:13










          • $begingroup$
            Understood, you gave me a "lesson of method" and I thank you for it. Yet, I believe that in the aforementioned paper the peculiar form of the sequence seems to be not so relevant (at least this was my impression). In some sense, reading your edit, one might see the picture simply as: well, we have $(mu_epsilon)_epsilon$ which has a specific form and this sequence converges to the surface measure. But this is not the way the authors propose the arguments. Last question, I promise: Could you please justify why it seems clear to you that $mu_epsilon to lambda$ (in your notation)? Thanks.
            $endgroup$
            – Romeo
            Jan 20 at 15:10










          • $begingroup$
            Cux you just write down what $int f,dmu_epsilon$ is and let $epsilonto0$. See edit....
            $endgroup$
            – David C. Ullrich
            Jan 20 at 15:43










          • $begingroup$
            "Cux" $to$ "Cuz"
            $endgroup$
            – David C. Ullrich
            Jan 20 at 15:50










          • $begingroup$
            @Romeo Hmm. A way one could deduce that $lambda<<H$ without saying anything about what $lambda$ is: If $Esubset S$ say $V(E)={rxi:r>0,xiin E}$. Suppose there exists a function $phi$ with $lim_{tto0}phi(t)=0$ such that $mu_n(V(E)lephi(H(E))$ for all $n$.. If $mu_ntolambda$ weakly and $lambda$ is supported on $S$ then $lambda<<H$.
            $endgroup$
            – David C. Ullrich
            Jan 20 at 17:04














          1












          1








          1





          $begingroup$

          I suspect that when you wrote $|mu_n|(Omega)to|mu|(Omega)$ maybe that's not exactly what you meant. Replying to the question as stated:



          You assume so little about $mu$ that it really has nothing to do with the rest of what's going on; there's no relationship between $lambda$ and $mu$. One doesn't need to "construct" a counterexample, any almost random choice of $mu_n$ and $mu$ works.



          Say $mu_n=delta_{1/n}$, a point mass at $1/n$. So $mu_ntodelta_0$. Let $Omega=(-1,1)$ and let $mu$ be any positive measure with $mu(Omega)=1$.



          Or maybe to better illustrate how $mu$ really has nothing to do with $lambda$, let $Omega=(2,3)$ and let $mu$ be any measure with $mu(Omega)=0$. Or $Omega=emptyset$ and $mu=0$.



          Heh, let $mu_n$ be any norm-bounded sequence, $Omega=emptyset$, $mu=0$.



          Edit: Regarding the edit made to the question, and the comment asking whether there's any significant difference: Well of course there's a huge difference, since in the new version we have a specific "sequence" of measures! In particular, for example, if I'm reading things correctly $mu_epsilon$ is supported in the annulus $A_epsilon={1-epsilonle|x|le1}$.



          If I have the picture right it seems clear that the gradient of $u_epsilon$ is $nabla u_epsilon(x)=-frac1epsilonfrac x{|x|}$ or something like that in $A_epsilon$, $0$ elsewhere. So it seems clear that $mu_epsilontolambda$, where $dlambda=-n(x),dH$ (where $n$ is the outward unit normal on the sphere and $H$ is surface area on the sphere), which certainly appears to be ac wrt $H$.



          Of course that could be all wrong, it's just my first impression. But note that the various things I say "seem clear" seem clear to me based on my picture of what $mu_epsilon$ actually is, not because of any general principle analogous to what you ask about in the original version of the question!



          As a general rule, if they assert P and you don't see why P holds you might be better off actually stating what they actually assert and asking why it holds, instead of sort of guessing that they seem to be saying that P follows from Q and asking whether Q implies P.



          Second edit: Two things.



          (i) A conjecture regarding the sort of "soft" or "abstract" argument the authors might have had in mind: It's easy tp see that $||mu_epsilon||$ is bounded. And $mu_epsilon$ has a certain sort of rotational symmetry (which I'm not going to try to define precisely; this isn't my argument after all); hence any weak limit $lambda$ must have the same symmetry. It's clear that $lambda$ must be supported on $S={|x|=1}$, since the support of $mu_epsilon$ shrinks to $S$, and the only vector-valued measure on $S$ with that symmetry is $cn,dH$.



          That's pretty vague; I'm not going to try to make it more precise, since it's just my guess regarding sort of what the authors may have had in mind. But:



          (ii) Why it seems clear to me that $mu_epsilon$ simply does converge to what I say it does:



          First, in general if $u$ is a radial function, $$u(x)=phi(|x|),$$then $$nabla u(x)=phi'(|x|)frac x{|x|}.$$("Advanced calculus": $nabla u$ is the directional derivative in the direction of greatest increase, which is to say in a direction orthogonal to the level sets of $u$...) Hence $nabla u_epsilon$ is what I say it is above.



          Now assume $fin C_c(Bbb R^n)$ and integrate in polar coordinates:



          $$int_{Bbb R^n}f(x)nabla u_epsilon(x),dx=int_Sfrac{-1}{epsilon}int_{1-epsilon}^1f(rxi)xi r^{n-1},drdH(xi).$$And since $f$ is continuous it's clear that $$lim_{epsilonto0}frac{-1}{epsilon}int_{1-epsilon}^1f(rxi)xi r^{n-1},dr=-f(xi)xi,$$uniformly over $xiin S$.



          ("Polar coordinates": In general $$int_{Bbb R^n}g(x),dx=c_nint_Sint_0^infty g(rxi)r^{n-1},drdH(xi).$$Note that if $H$ is actual "surface area" on $S$, in particular not normalized to be a probability measure as is sometimes done in that formula, then $c_n=1$. See Folland Real Analysis or various other places.)






          share|cite|improve this answer











          $endgroup$



          I suspect that when you wrote $|mu_n|(Omega)to|mu|(Omega)$ maybe that's not exactly what you meant. Replying to the question as stated:



          You assume so little about $mu$ that it really has nothing to do with the rest of what's going on; there's no relationship between $lambda$ and $mu$. One doesn't need to "construct" a counterexample, any almost random choice of $mu_n$ and $mu$ works.



          Say $mu_n=delta_{1/n}$, a point mass at $1/n$. So $mu_ntodelta_0$. Let $Omega=(-1,1)$ and let $mu$ be any positive measure with $mu(Omega)=1$.



          Or maybe to better illustrate how $mu$ really has nothing to do with $lambda$, let $Omega=(2,3)$ and let $mu$ be any measure with $mu(Omega)=0$. Or $Omega=emptyset$ and $mu=0$.



          Heh, let $mu_n$ be any norm-bounded sequence, $Omega=emptyset$, $mu=0$.



          Edit: Regarding the edit made to the question, and the comment asking whether there's any significant difference: Well of course there's a huge difference, since in the new version we have a specific "sequence" of measures! In particular, for example, if I'm reading things correctly $mu_epsilon$ is supported in the annulus $A_epsilon={1-epsilonle|x|le1}$.



          If I have the picture right it seems clear that the gradient of $u_epsilon$ is $nabla u_epsilon(x)=-frac1epsilonfrac x{|x|}$ or something like that in $A_epsilon$, $0$ elsewhere. So it seems clear that $mu_epsilontolambda$, where $dlambda=-n(x),dH$ (where $n$ is the outward unit normal on the sphere and $H$ is surface area on the sphere), which certainly appears to be ac wrt $H$.



          Of course that could be all wrong, it's just my first impression. But note that the various things I say "seem clear" seem clear to me based on my picture of what $mu_epsilon$ actually is, not because of any general principle analogous to what you ask about in the original version of the question!



          As a general rule, if they assert P and you don't see why P holds you might be better off actually stating what they actually assert and asking why it holds, instead of sort of guessing that they seem to be saying that P follows from Q and asking whether Q implies P.



          Second edit: Two things.



          (i) A conjecture regarding the sort of "soft" or "abstract" argument the authors might have had in mind: It's easy tp see that $||mu_epsilon||$ is bounded. And $mu_epsilon$ has a certain sort of rotational symmetry (which I'm not going to try to define precisely; this isn't my argument after all); hence any weak limit $lambda$ must have the same symmetry. It's clear that $lambda$ must be supported on $S={|x|=1}$, since the support of $mu_epsilon$ shrinks to $S$, and the only vector-valued measure on $S$ with that symmetry is $cn,dH$.



          That's pretty vague; I'm not going to try to make it more precise, since it's just my guess regarding sort of what the authors may have had in mind. But:



          (ii) Why it seems clear to me that $mu_epsilon$ simply does converge to what I say it does:



          First, in general if $u$ is a radial function, $$u(x)=phi(|x|),$$then $$nabla u(x)=phi'(|x|)frac x{|x|}.$$("Advanced calculus": $nabla u$ is the directional derivative in the direction of greatest increase, which is to say in a direction orthogonal to the level sets of $u$...) Hence $nabla u_epsilon$ is what I say it is above.



          Now assume $fin C_c(Bbb R^n)$ and integrate in polar coordinates:



          $$int_{Bbb R^n}f(x)nabla u_epsilon(x),dx=int_Sfrac{-1}{epsilon}int_{1-epsilon}^1f(rxi)xi r^{n-1},drdH(xi).$$And since $f$ is continuous it's clear that $$lim_{epsilonto0}frac{-1}{epsilon}int_{1-epsilon}^1f(rxi)xi r^{n-1},dr=-f(xi)xi,$$uniformly over $xiin S$.



          ("Polar coordinates": In general $$int_{Bbb R^n}g(x),dx=c_nint_Sint_0^infty g(rxi)r^{n-1},drdH(xi).$$Note that if $H$ is actual "surface area" on $S$, in particular not normalized to be a probability measure as is sometimes done in that formula, then $c_n=1$. See Folland Real Analysis or various other places.)







          share|cite|improve this answer














          share|cite|improve this answer



          share|cite|improve this answer








          edited Jan 20 at 16:11

























          answered Jan 20 at 2:28









          David C. UllrichDavid C. Ullrich

          61.1k43994




          61.1k43994












          • $begingroup$
            Thank you very much for your kind reply. I see your point and I totally agree with you, the question is essentially ill-posed. However, I am still in troubles, see the edit to my question. It seems to me that the authors kind of claim what I asked. Is there any significative difference in their "particular" case? Have I misunderstood anything? Thanks for your help.
            $endgroup$
            – Romeo
            Jan 20 at 10:13










          • $begingroup$
            Understood, you gave me a "lesson of method" and I thank you for it. Yet, I believe that in the aforementioned paper the peculiar form of the sequence seems to be not so relevant (at least this was my impression). In some sense, reading your edit, one might see the picture simply as: well, we have $(mu_epsilon)_epsilon$ which has a specific form and this sequence converges to the surface measure. But this is not the way the authors propose the arguments. Last question, I promise: Could you please justify why it seems clear to you that $mu_epsilon to lambda$ (in your notation)? Thanks.
            $endgroup$
            – Romeo
            Jan 20 at 15:10










          • $begingroup$
            Cux you just write down what $int f,dmu_epsilon$ is and let $epsilonto0$. See edit....
            $endgroup$
            – David C. Ullrich
            Jan 20 at 15:43










          • $begingroup$
            "Cux" $to$ "Cuz"
            $endgroup$
            – David C. Ullrich
            Jan 20 at 15:50










          • $begingroup$
            @Romeo Hmm. A way one could deduce that $lambda<<H$ without saying anything about what $lambda$ is: If $Esubset S$ say $V(E)={rxi:r>0,xiin E}$. Suppose there exists a function $phi$ with $lim_{tto0}phi(t)=0$ such that $mu_n(V(E)lephi(H(E))$ for all $n$.. If $mu_ntolambda$ weakly and $lambda$ is supported on $S$ then $lambda<<H$.
            $endgroup$
            – David C. Ullrich
            Jan 20 at 17:04


















          • $begingroup$
            Thank you very much for your kind reply. I see your point and I totally agree with you, the question is essentially ill-posed. However, I am still in troubles, see the edit to my question. It seems to me that the authors kind of claim what I asked. Is there any significative difference in their "particular" case? Have I misunderstood anything? Thanks for your help.
            $endgroup$
            – Romeo
            Jan 20 at 10:13










          • $begingroup$
            Understood, you gave me a "lesson of method" and I thank you for it. Yet, I believe that in the aforementioned paper the peculiar form of the sequence seems to be not so relevant (at least this was my impression). In some sense, reading your edit, one might see the picture simply as: well, we have $(mu_epsilon)_epsilon$ which has a specific form and this sequence converges to the surface measure. But this is not the way the authors propose the arguments. Last question, I promise: Could you please justify why it seems clear to you that $mu_epsilon to lambda$ (in your notation)? Thanks.
            $endgroup$
            – Romeo
            Jan 20 at 15:10










          • $begingroup$
            Cux you just write down what $int f,dmu_epsilon$ is and let $epsilonto0$. See edit....
            $endgroup$
            – David C. Ullrich
            Jan 20 at 15:43










          • $begingroup$
            "Cux" $to$ "Cuz"
            $endgroup$
            – David C. Ullrich
            Jan 20 at 15:50










          • $begingroup$
            @Romeo Hmm. A way one could deduce that $lambda<<H$ without saying anything about what $lambda$ is: If $Esubset S$ say $V(E)={rxi:r>0,xiin E}$. Suppose there exists a function $phi$ with $lim_{tto0}phi(t)=0$ such that $mu_n(V(E)lephi(H(E))$ for all $n$.. If $mu_ntolambda$ weakly and $lambda$ is supported on $S$ then $lambda<<H$.
            $endgroup$
            – David C. Ullrich
            Jan 20 at 17:04
















          $begingroup$
          Thank you very much for your kind reply. I see your point and I totally agree with you, the question is essentially ill-posed. However, I am still in troubles, see the edit to my question. It seems to me that the authors kind of claim what I asked. Is there any significative difference in their "particular" case? Have I misunderstood anything? Thanks for your help.
          $endgroup$
          – Romeo
          Jan 20 at 10:13




          $begingroup$
          Thank you very much for your kind reply. I see your point and I totally agree with you, the question is essentially ill-posed. However, I am still in troubles, see the edit to my question. It seems to me that the authors kind of claim what I asked. Is there any significative difference in their "particular" case? Have I misunderstood anything? Thanks for your help.
          $endgroup$
          – Romeo
          Jan 20 at 10:13












          $begingroup$
          Understood, you gave me a "lesson of method" and I thank you for it. Yet, I believe that in the aforementioned paper the peculiar form of the sequence seems to be not so relevant (at least this was my impression). In some sense, reading your edit, one might see the picture simply as: well, we have $(mu_epsilon)_epsilon$ which has a specific form and this sequence converges to the surface measure. But this is not the way the authors propose the arguments. Last question, I promise: Could you please justify why it seems clear to you that $mu_epsilon to lambda$ (in your notation)? Thanks.
          $endgroup$
          – Romeo
          Jan 20 at 15:10




          $begingroup$
          Understood, you gave me a "lesson of method" and I thank you for it. Yet, I believe that in the aforementioned paper the peculiar form of the sequence seems to be not so relevant (at least this was my impression). In some sense, reading your edit, one might see the picture simply as: well, we have $(mu_epsilon)_epsilon$ which has a specific form and this sequence converges to the surface measure. But this is not the way the authors propose the arguments. Last question, I promise: Could you please justify why it seems clear to you that $mu_epsilon to lambda$ (in your notation)? Thanks.
          $endgroup$
          – Romeo
          Jan 20 at 15:10












          $begingroup$
          Cux you just write down what $int f,dmu_epsilon$ is and let $epsilonto0$. See edit....
          $endgroup$
          – David C. Ullrich
          Jan 20 at 15:43




          $begingroup$
          Cux you just write down what $int f,dmu_epsilon$ is and let $epsilonto0$. See edit....
          $endgroup$
          – David C. Ullrich
          Jan 20 at 15:43












          $begingroup$
          "Cux" $to$ "Cuz"
          $endgroup$
          – David C. Ullrich
          Jan 20 at 15:50




          $begingroup$
          "Cux" $to$ "Cuz"
          $endgroup$
          – David C. Ullrich
          Jan 20 at 15:50












          $begingroup$
          @Romeo Hmm. A way one could deduce that $lambda<<H$ without saying anything about what $lambda$ is: If $Esubset S$ say $V(E)={rxi:r>0,xiin E}$. Suppose there exists a function $phi$ with $lim_{tto0}phi(t)=0$ such that $mu_n(V(E)lephi(H(E))$ for all $n$.. If $mu_ntolambda$ weakly and $lambda$ is supported on $S$ then $lambda<<H$.
          $endgroup$
          – David C. Ullrich
          Jan 20 at 17:04




          $begingroup$
          @Romeo Hmm. A way one could deduce that $lambda<<H$ without saying anything about what $lambda$ is: If $Esubset S$ say $V(E)={rxi:r>0,xiin E}$. Suppose there exists a function $phi$ with $lim_{tto0}phi(t)=0$ such that $mu_n(V(E)lephi(H(E))$ for all $n$.. If $mu_ntolambda$ weakly and $lambda$ is supported on $S$ then $lambda<<H$.
          $endgroup$
          – David C. Ullrich
          Jan 20 at 17:04


















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