Triple integral - wedge shaped solid












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Find the volume of of the wedge shaped solid that lies above the xy plane, below the $z=x$ plane and within the cylinder $x^2+y^2 = 4$.



I'm having serious trouble picturing this. I think the z bounds are [0,x], but can't figure out any of the other ones.










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    0














    Find the volume of of the wedge shaped solid that lies above the xy plane, below the $z=x$ plane and within the cylinder $x^2+y^2 = 4$.



    I'm having serious trouble picturing this. I think the z bounds are [0,x], but can't figure out any of the other ones.










    share|cite|improve this question

























      0












      0








      0


      0





      Find the volume of of the wedge shaped solid that lies above the xy plane, below the $z=x$ plane and within the cylinder $x^2+y^2 = 4$.



      I'm having serious trouble picturing this. I think the z bounds are [0,x], but can't figure out any of the other ones.










      share|cite|improve this question













      Find the volume of of the wedge shaped solid that lies above the xy plane, below the $z=x$ plane and within the cylinder $x^2+y^2 = 4$.



      I'm having serious trouble picturing this. I think the z bounds are [0,x], but can't figure out any of the other ones.







      integration multivariable-calculus volume






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      asked Mar 28 '14 at 13:01









      user127778

      118112




      118112






















          4 Answers
          4






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          0














          looks like this should be the required vol
          $$2int_{0}^{pi/2} int_{0}^{2} int_{0}^{rcostheta} rdzdrdtheta $$






          share|cite|improve this answer





















          • why is it [$0,frac{pi}{2}$] and not [$pi, 2pi]$? The $dtheta$ bound is what I'm asking about, because I got all of the other ones. Also, why do you multiply by 2?
            – user127778
            Mar 28 '14 at 13:09












          • the region in xy plane, is of 1st and 4th quadrant, so $[pi, 2pi]$ doesn't look like being there.the volume is above 1st and 4th quadrant of xy plane, so you can adjust $dtheta$ accordingly.and since i chose $[0,frac{pi}{2}]$ so multiplied by 2
            – ketan
            Mar 28 '14 at 13:14












          • $2times$ is because of symmetry. Otherwise you'd have to integrate $int_{-pi/2}^{pi/2}$.
            – orion
            Mar 28 '14 at 13:18



















          0














          I believe that you are describing a variation of the hoof of Archimedes (see figure below). If that's the case, I can give you a detailed solution and show you how to reduce the triple integral for volume to a single integration. From what you describe, the height would be $R$, rather than the $2R$ shown in the figure.



          enter image description here






          share|cite|improve this answer





























            0














            Planes $x={rm const.}$ intersect this solid $B$ in rectangles of width $2sqrt{4-x^2}$ and height $x$ (see the figure in Cye Waldman's answer). One therefore obtains
            $${rm vol}(B)=int_0^2 2sqrt{4-x^2}>x>dx=-{2over3}(4-x^2)^{3/2}biggr|_0^2={16over3} .$$






            share|cite|improve this answer





























              0














              $newcommand{bbx}[1]{,bbox[15px,border:1px groove navy]{displaystyle{#1}},}
              newcommand{braces}[1]{leftlbrace,{#1},rightrbrace}
              newcommand{bracks}[1]{leftlbrack,{#1},rightrbrack}
              newcommand{dd}{mathrm{d}}
              newcommand{ds}[1]{displaystyle{#1}}
              newcommand{expo}[1]{,mathrm{e}^{#1},}
              newcommand{ic}{mathrm{i}}
              newcommand{mc}[1]{mathcal{#1}}
              newcommand{mrm}[1]{mathrm{#1}}
              newcommand{pars}[1]{left(,{#1},right)}
              newcommand{partiald}[3]{frac{partial^{#1} #2}{partial #3^{#1}}}
              newcommand{root}[2]{,sqrt[#1]{,{#2},},}
              newcommand{totald}[3]{frac{mathrm{d}^{#1} #2}{mathrm{d} #3^{#1}}}
              newcommand{verts}[1]{leftvert,{#1},rightvert}$

              begin{align}
              V & = iiint_{mathbb{R}^{large 3}}bracks{z > 0}
              bracks{z < x}bracks{x^{2} + y^{2} < 4}dd x,dd y,dd z
              \[5mm] & =
              int_{-infty}^{infty}int_{-infty}^{infty}
              int_{-infty}^{infty}bracks{0 < z < rhocospars{phi}}
              bracks{rho > 0}bracks{rho^{2} < 4}rho,ddrho,ddphi
              ,dd z
              \[5mm] & =
              int_{0}^{infty}int_{0}^{2pi}
              int_{0}^{2}bracks{0 < z < rhocospars{phi}}
              rho,ddrho,ddphi,dd z
              \[5mm] & =
              2int_{0}^{infty}int_{0}^{pi}
              int_{0}^{2}bracks{0 < z < -rhocospars{phi}}
              rho,ddrho,ddphi,dd z
              \[5mm] & =
              2int_{0}^{infty}int_{0}^{pi/2}
              int_{0}^{2}bracks{0 < z < rhosinpars{phi}}
              rho,ddrho,ddphi,dd z
              \[5mm] & =
              2int_{0}^{pi/2}
              int_{0}^{2}rhosinpars{phi}rho,ddrho,ddphi =
              2pars{int_{0}^{pi/2}sinpars{phi},ddphi}
              pars{int_{0}^{2}rho^{2},ddrho}
              \[5mm] & = bbx{16 over 3}
              end{align}






              share|cite|improve this answer





















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                4 Answers
                4






                active

                oldest

                votes








                4 Answers
                4






                active

                oldest

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                active

                oldest

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                active

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                0














                looks like this should be the required vol
                $$2int_{0}^{pi/2} int_{0}^{2} int_{0}^{rcostheta} rdzdrdtheta $$






                share|cite|improve this answer





















                • why is it [$0,frac{pi}{2}$] and not [$pi, 2pi]$? The $dtheta$ bound is what I'm asking about, because I got all of the other ones. Also, why do you multiply by 2?
                  – user127778
                  Mar 28 '14 at 13:09












                • the region in xy plane, is of 1st and 4th quadrant, so $[pi, 2pi]$ doesn't look like being there.the volume is above 1st and 4th quadrant of xy plane, so you can adjust $dtheta$ accordingly.and since i chose $[0,frac{pi}{2}]$ so multiplied by 2
                  – ketan
                  Mar 28 '14 at 13:14












                • $2times$ is because of symmetry. Otherwise you'd have to integrate $int_{-pi/2}^{pi/2}$.
                  – orion
                  Mar 28 '14 at 13:18
















                0














                looks like this should be the required vol
                $$2int_{0}^{pi/2} int_{0}^{2} int_{0}^{rcostheta} rdzdrdtheta $$






                share|cite|improve this answer





















                • why is it [$0,frac{pi}{2}$] and not [$pi, 2pi]$? The $dtheta$ bound is what I'm asking about, because I got all of the other ones. Also, why do you multiply by 2?
                  – user127778
                  Mar 28 '14 at 13:09












                • the region in xy plane, is of 1st and 4th quadrant, so $[pi, 2pi]$ doesn't look like being there.the volume is above 1st and 4th quadrant of xy plane, so you can adjust $dtheta$ accordingly.and since i chose $[0,frac{pi}{2}]$ so multiplied by 2
                  – ketan
                  Mar 28 '14 at 13:14












                • $2times$ is because of symmetry. Otherwise you'd have to integrate $int_{-pi/2}^{pi/2}$.
                  – orion
                  Mar 28 '14 at 13:18














                0












                0








                0






                looks like this should be the required vol
                $$2int_{0}^{pi/2} int_{0}^{2} int_{0}^{rcostheta} rdzdrdtheta $$






                share|cite|improve this answer












                looks like this should be the required vol
                $$2int_{0}^{pi/2} int_{0}^{2} int_{0}^{rcostheta} rdzdrdtheta $$







                share|cite|improve this answer












                share|cite|improve this answer



                share|cite|improve this answer










                answered Mar 28 '14 at 13:06









                ketan

                1,530822




                1,530822












                • why is it [$0,frac{pi}{2}$] and not [$pi, 2pi]$? The $dtheta$ bound is what I'm asking about, because I got all of the other ones. Also, why do you multiply by 2?
                  – user127778
                  Mar 28 '14 at 13:09












                • the region in xy plane, is of 1st and 4th quadrant, so $[pi, 2pi]$ doesn't look like being there.the volume is above 1st and 4th quadrant of xy plane, so you can adjust $dtheta$ accordingly.and since i chose $[0,frac{pi}{2}]$ so multiplied by 2
                  – ketan
                  Mar 28 '14 at 13:14












                • $2times$ is because of symmetry. Otherwise you'd have to integrate $int_{-pi/2}^{pi/2}$.
                  – orion
                  Mar 28 '14 at 13:18


















                • why is it [$0,frac{pi}{2}$] and not [$pi, 2pi]$? The $dtheta$ bound is what I'm asking about, because I got all of the other ones. Also, why do you multiply by 2?
                  – user127778
                  Mar 28 '14 at 13:09












                • the region in xy plane, is of 1st and 4th quadrant, so $[pi, 2pi]$ doesn't look like being there.the volume is above 1st and 4th quadrant of xy plane, so you can adjust $dtheta$ accordingly.and since i chose $[0,frac{pi}{2}]$ so multiplied by 2
                  – ketan
                  Mar 28 '14 at 13:14












                • $2times$ is because of symmetry. Otherwise you'd have to integrate $int_{-pi/2}^{pi/2}$.
                  – orion
                  Mar 28 '14 at 13:18
















                why is it [$0,frac{pi}{2}$] and not [$pi, 2pi]$? The $dtheta$ bound is what I'm asking about, because I got all of the other ones. Also, why do you multiply by 2?
                – user127778
                Mar 28 '14 at 13:09






                why is it [$0,frac{pi}{2}$] and not [$pi, 2pi]$? The $dtheta$ bound is what I'm asking about, because I got all of the other ones. Also, why do you multiply by 2?
                – user127778
                Mar 28 '14 at 13:09














                the region in xy plane, is of 1st and 4th quadrant, so $[pi, 2pi]$ doesn't look like being there.the volume is above 1st and 4th quadrant of xy plane, so you can adjust $dtheta$ accordingly.and since i chose $[0,frac{pi}{2}]$ so multiplied by 2
                – ketan
                Mar 28 '14 at 13:14






                the region in xy plane, is of 1st and 4th quadrant, so $[pi, 2pi]$ doesn't look like being there.the volume is above 1st and 4th quadrant of xy plane, so you can adjust $dtheta$ accordingly.and since i chose $[0,frac{pi}{2}]$ so multiplied by 2
                – ketan
                Mar 28 '14 at 13:14














                $2times$ is because of symmetry. Otherwise you'd have to integrate $int_{-pi/2}^{pi/2}$.
                – orion
                Mar 28 '14 at 13:18




                $2times$ is because of symmetry. Otherwise you'd have to integrate $int_{-pi/2}^{pi/2}$.
                – orion
                Mar 28 '14 at 13:18











                0














                I believe that you are describing a variation of the hoof of Archimedes (see figure below). If that's the case, I can give you a detailed solution and show you how to reduce the triple integral for volume to a single integration. From what you describe, the height would be $R$, rather than the $2R$ shown in the figure.



                enter image description here






                share|cite|improve this answer


























                  0














                  I believe that you are describing a variation of the hoof of Archimedes (see figure below). If that's the case, I can give you a detailed solution and show you how to reduce the triple integral for volume to a single integration. From what you describe, the height would be $R$, rather than the $2R$ shown in the figure.



                  enter image description here






                  share|cite|improve this answer
























                    0












                    0








                    0






                    I believe that you are describing a variation of the hoof of Archimedes (see figure below). If that's the case, I can give you a detailed solution and show you how to reduce the triple integral for volume to a single integration. From what you describe, the height would be $R$, rather than the $2R$ shown in the figure.



                    enter image description here






                    share|cite|improve this answer












                    I believe that you are describing a variation of the hoof of Archimedes (see figure below). If that's the case, I can give you a detailed solution and show you how to reduce the triple integral for volume to a single integration. From what you describe, the height would be $R$, rather than the $2R$ shown in the figure.



                    enter image description here







                    share|cite|improve this answer












                    share|cite|improve this answer



                    share|cite|improve this answer










                    answered Jun 7 '17 at 17:04









                    Cye Waldman

                    4,0952523




                    4,0952523























                        0














                        Planes $x={rm const.}$ intersect this solid $B$ in rectangles of width $2sqrt{4-x^2}$ and height $x$ (see the figure in Cye Waldman's answer). One therefore obtains
                        $${rm vol}(B)=int_0^2 2sqrt{4-x^2}>x>dx=-{2over3}(4-x^2)^{3/2}biggr|_0^2={16over3} .$$






                        share|cite|improve this answer


























                          0














                          Planes $x={rm const.}$ intersect this solid $B$ in rectangles of width $2sqrt{4-x^2}$ and height $x$ (see the figure in Cye Waldman's answer). One therefore obtains
                          $${rm vol}(B)=int_0^2 2sqrt{4-x^2}>x>dx=-{2over3}(4-x^2)^{3/2}biggr|_0^2={16over3} .$$






                          share|cite|improve this answer
























                            0












                            0








                            0






                            Planes $x={rm const.}$ intersect this solid $B$ in rectangles of width $2sqrt{4-x^2}$ and height $x$ (see the figure in Cye Waldman's answer). One therefore obtains
                            $${rm vol}(B)=int_0^2 2sqrt{4-x^2}>x>dx=-{2over3}(4-x^2)^{3/2}biggr|_0^2={16over3} .$$






                            share|cite|improve this answer












                            Planes $x={rm const.}$ intersect this solid $B$ in rectangles of width $2sqrt{4-x^2}$ and height $x$ (see the figure in Cye Waldman's answer). One therefore obtains
                            $${rm vol}(B)=int_0^2 2sqrt{4-x^2}>x>dx=-{2over3}(4-x^2)^{3/2}biggr|_0^2={16over3} .$$







                            share|cite|improve this answer












                            share|cite|improve this answer



                            share|cite|improve this answer










                            answered Jul 9 '17 at 9:08









                            Christian Blatter

                            172k7112325




                            172k7112325























                                0














                                $newcommand{bbx}[1]{,bbox[15px,border:1px groove navy]{displaystyle{#1}},}
                                newcommand{braces}[1]{leftlbrace,{#1},rightrbrace}
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                                newcommand{dd}{mathrm{d}}
                                newcommand{ds}[1]{displaystyle{#1}}
                                newcommand{expo}[1]{,mathrm{e}^{#1},}
                                newcommand{ic}{mathrm{i}}
                                newcommand{mc}[1]{mathcal{#1}}
                                newcommand{mrm}[1]{mathrm{#1}}
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                                newcommand{partiald}[3]{frac{partial^{#1} #2}{partial #3^{#1}}}
                                newcommand{root}[2]{,sqrt[#1]{,{#2},},}
                                newcommand{totald}[3]{frac{mathrm{d}^{#1} #2}{mathrm{d} #3^{#1}}}
                                newcommand{verts}[1]{leftvert,{#1},rightvert}$

                                begin{align}
                                V & = iiint_{mathbb{R}^{large 3}}bracks{z > 0}
                                bracks{z < x}bracks{x^{2} + y^{2} < 4}dd x,dd y,dd z
                                \[5mm] & =
                                int_{-infty}^{infty}int_{-infty}^{infty}
                                int_{-infty}^{infty}bracks{0 < z < rhocospars{phi}}
                                bracks{rho > 0}bracks{rho^{2} < 4}rho,ddrho,ddphi
                                ,dd z
                                \[5mm] & =
                                int_{0}^{infty}int_{0}^{2pi}
                                int_{0}^{2}bracks{0 < z < rhocospars{phi}}
                                rho,ddrho,ddphi,dd z
                                \[5mm] & =
                                2int_{0}^{infty}int_{0}^{pi}
                                int_{0}^{2}bracks{0 < z < -rhocospars{phi}}
                                rho,ddrho,ddphi,dd z
                                \[5mm] & =
                                2int_{0}^{infty}int_{0}^{pi/2}
                                int_{0}^{2}bracks{0 < z < rhosinpars{phi}}
                                rho,ddrho,ddphi,dd z
                                \[5mm] & =
                                2int_{0}^{pi/2}
                                int_{0}^{2}rhosinpars{phi}rho,ddrho,ddphi =
                                2pars{int_{0}^{pi/2}sinpars{phi},ddphi}
                                pars{int_{0}^{2}rho^{2},ddrho}
                                \[5mm] & = bbx{16 over 3}
                                end{align}






                                share|cite|improve this answer


























                                  0














                                  $newcommand{bbx}[1]{,bbox[15px,border:1px groove navy]{displaystyle{#1}},}
                                  newcommand{braces}[1]{leftlbrace,{#1},rightrbrace}
                                  newcommand{bracks}[1]{leftlbrack,{#1},rightrbrack}
                                  newcommand{dd}{mathrm{d}}
                                  newcommand{ds}[1]{displaystyle{#1}}
                                  newcommand{expo}[1]{,mathrm{e}^{#1},}
                                  newcommand{ic}{mathrm{i}}
                                  newcommand{mc}[1]{mathcal{#1}}
                                  newcommand{mrm}[1]{mathrm{#1}}
                                  newcommand{pars}[1]{left(,{#1},right)}
                                  newcommand{partiald}[3]{frac{partial^{#1} #2}{partial #3^{#1}}}
                                  newcommand{root}[2]{,sqrt[#1]{,{#2},},}
                                  newcommand{totald}[3]{frac{mathrm{d}^{#1} #2}{mathrm{d} #3^{#1}}}
                                  newcommand{verts}[1]{leftvert,{#1},rightvert}$

                                  begin{align}
                                  V & = iiint_{mathbb{R}^{large 3}}bracks{z > 0}
                                  bracks{z < x}bracks{x^{2} + y^{2} < 4}dd x,dd y,dd z
                                  \[5mm] & =
                                  int_{-infty}^{infty}int_{-infty}^{infty}
                                  int_{-infty}^{infty}bracks{0 < z < rhocospars{phi}}
                                  bracks{rho > 0}bracks{rho^{2} < 4}rho,ddrho,ddphi
                                  ,dd z
                                  \[5mm] & =
                                  int_{0}^{infty}int_{0}^{2pi}
                                  int_{0}^{2}bracks{0 < z < rhocospars{phi}}
                                  rho,ddrho,ddphi,dd z
                                  \[5mm] & =
                                  2int_{0}^{infty}int_{0}^{pi}
                                  int_{0}^{2}bracks{0 < z < -rhocospars{phi}}
                                  rho,ddrho,ddphi,dd z
                                  \[5mm] & =
                                  2int_{0}^{infty}int_{0}^{pi/2}
                                  int_{0}^{2}bracks{0 < z < rhosinpars{phi}}
                                  rho,ddrho,ddphi,dd z
                                  \[5mm] & =
                                  2int_{0}^{pi/2}
                                  int_{0}^{2}rhosinpars{phi}rho,ddrho,ddphi =
                                  2pars{int_{0}^{pi/2}sinpars{phi},ddphi}
                                  pars{int_{0}^{2}rho^{2},ddrho}
                                  \[5mm] & = bbx{16 over 3}
                                  end{align}






                                  share|cite|improve this answer
























                                    0












                                    0








                                    0






                                    $newcommand{bbx}[1]{,bbox[15px,border:1px groove navy]{displaystyle{#1}},}
                                    newcommand{braces}[1]{leftlbrace,{#1},rightrbrace}
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                                    newcommand{expo}[1]{,mathrm{e}^{#1},}
                                    newcommand{ic}{mathrm{i}}
                                    newcommand{mc}[1]{mathcal{#1}}
                                    newcommand{mrm}[1]{mathrm{#1}}
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                                    newcommand{partiald}[3]{frac{partial^{#1} #2}{partial #3^{#1}}}
                                    newcommand{root}[2]{,sqrt[#1]{,{#2},},}
                                    newcommand{totald}[3]{frac{mathrm{d}^{#1} #2}{mathrm{d} #3^{#1}}}
                                    newcommand{verts}[1]{leftvert,{#1},rightvert}$

                                    begin{align}
                                    V & = iiint_{mathbb{R}^{large 3}}bracks{z > 0}
                                    bracks{z < x}bracks{x^{2} + y^{2} < 4}dd x,dd y,dd z
                                    \[5mm] & =
                                    int_{-infty}^{infty}int_{-infty}^{infty}
                                    int_{-infty}^{infty}bracks{0 < z < rhocospars{phi}}
                                    bracks{rho > 0}bracks{rho^{2} < 4}rho,ddrho,ddphi
                                    ,dd z
                                    \[5mm] & =
                                    int_{0}^{infty}int_{0}^{2pi}
                                    int_{0}^{2}bracks{0 < z < rhocospars{phi}}
                                    rho,ddrho,ddphi,dd z
                                    \[5mm] & =
                                    2int_{0}^{infty}int_{0}^{pi}
                                    int_{0}^{2}bracks{0 < z < -rhocospars{phi}}
                                    rho,ddrho,ddphi,dd z
                                    \[5mm] & =
                                    2int_{0}^{infty}int_{0}^{pi/2}
                                    int_{0}^{2}bracks{0 < z < rhosinpars{phi}}
                                    rho,ddrho,ddphi,dd z
                                    \[5mm] & =
                                    2int_{0}^{pi/2}
                                    int_{0}^{2}rhosinpars{phi}rho,ddrho,ddphi =
                                    2pars{int_{0}^{pi/2}sinpars{phi},ddphi}
                                    pars{int_{0}^{2}rho^{2},ddrho}
                                    \[5mm] & = bbx{16 over 3}
                                    end{align}






                                    share|cite|improve this answer












                                    $newcommand{bbx}[1]{,bbox[15px,border:1px groove navy]{displaystyle{#1}},}
                                    newcommand{braces}[1]{leftlbrace,{#1},rightrbrace}
                                    newcommand{bracks}[1]{leftlbrack,{#1},rightrbrack}
                                    newcommand{dd}{mathrm{d}}
                                    newcommand{ds}[1]{displaystyle{#1}}
                                    newcommand{expo}[1]{,mathrm{e}^{#1},}
                                    newcommand{ic}{mathrm{i}}
                                    newcommand{mc}[1]{mathcal{#1}}
                                    newcommand{mrm}[1]{mathrm{#1}}
                                    newcommand{pars}[1]{left(,{#1},right)}
                                    newcommand{partiald}[3]{frac{partial^{#1} #2}{partial #3^{#1}}}
                                    newcommand{root}[2]{,sqrt[#1]{,{#2},},}
                                    newcommand{totald}[3]{frac{mathrm{d}^{#1} #2}{mathrm{d} #3^{#1}}}
                                    newcommand{verts}[1]{leftvert,{#1},rightvert}$

                                    begin{align}
                                    V & = iiint_{mathbb{R}^{large 3}}bracks{z > 0}
                                    bracks{z < x}bracks{x^{2} + y^{2} < 4}dd x,dd y,dd z
                                    \[5mm] & =
                                    int_{-infty}^{infty}int_{-infty}^{infty}
                                    int_{-infty}^{infty}bracks{0 < z < rhocospars{phi}}
                                    bracks{rho > 0}bracks{rho^{2} < 4}rho,ddrho,ddphi
                                    ,dd z
                                    \[5mm] & =
                                    int_{0}^{infty}int_{0}^{2pi}
                                    int_{0}^{2}bracks{0 < z < rhocospars{phi}}
                                    rho,ddrho,ddphi,dd z
                                    \[5mm] & =
                                    2int_{0}^{infty}int_{0}^{pi}
                                    int_{0}^{2}bracks{0 < z < -rhocospars{phi}}
                                    rho,ddrho,ddphi,dd z
                                    \[5mm] & =
                                    2int_{0}^{infty}int_{0}^{pi/2}
                                    int_{0}^{2}bracks{0 < z < rhosinpars{phi}}
                                    rho,ddrho,ddphi,dd z
                                    \[5mm] & =
                                    2int_{0}^{pi/2}
                                    int_{0}^{2}rhosinpars{phi}rho,ddrho,ddphi =
                                    2pars{int_{0}^{pi/2}sinpars{phi},ddphi}
                                    pars{int_{0}^{2}rho^{2},ddrho}
                                    \[5mm] & = bbx{16 over 3}
                                    end{align}







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                                    answered Dec 6 at 20:23









                                    Felix Marin

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