Explicit computation of euler number of tangent bundle of sphere












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This is related to Bott-Tu Sec 11, Sphere Bundles. I would like to compute the euler characteristic of sphere bundle concretely. I have figured out the following so far.



Let $S^k$ be the $k-$sphere. Consider vector field $v$ starting from south pole to north pole by flowing. Clearly this gives a section to $T(S^k)$. Now normalize this section by considering any riemannian metric $||cdot||$ by $frac{v}{||v||}$ and this gives a section on sphere bundle of $S^k$ with fiber $S^{k-1}$ away from 2 points(i.e. south and north pole).



Since Euler number can be computed by sum of local degrees at south pole and north pole, I can compute the local degree at local trivializations of sphere bundle at south pole $a$ and north pole $b$. WLOG, one can assume local trivializations look like $D(x)times S^{k-1}$ where $D(x)$ is some open disk on sphere $S^k$ centered at $x$. Then consider the following maps. $partial D(x)xrightarrow{s}D(x)times S^{k-1}xrightarrow{pi_2} S^{k-1}$ and denote total map as $f_x$. Pick volume form $omega$ on $S^{k-1}$ where $omega$ can be standard volume form.



Since the degree is computed locally, one can consider $int_{partial D(x)}f_x^star(omega)=int_{partial D(x)}s^starpsi$ where $psi$ is the global angular form defined over $E$ and $x$ can be either south or north pole. This follows from $f_x^star$ defines form restricts cohomology generator on each fiber and thus same cohomology class as global angular form. Hence they differ by a total differential and then one can apply stoke theorem to see the integral agrees.(Here I have already assumed the support of $psi$ is away from $D(x)$ and one can shrink the size of disk if necessary.)



If I denote $s(x)=(x,v(x))$ with $v(x)in S^{k-1}$, then $pi_2circ s(x)=v(x)$. Hence $int_{partial D(x)}f_x^star(omega)=int_{partial D(x)} v^star(omega)$. I can take $omega$ to be standard volume form of $k-1$ sphere.



$textbf{Q:}$ Now I do not see an obvious way to compute this integral though I can write down the formula. How do I proceed further?



Ref. Bott-Tu Differential Forms in Algebraic Topology, Sec 11, Thm 11.16, Exercise 11.21










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    1












    $begingroup$


    This is related to Bott-Tu Sec 11, Sphere Bundles. I would like to compute the euler characteristic of sphere bundle concretely. I have figured out the following so far.



    Let $S^k$ be the $k-$sphere. Consider vector field $v$ starting from south pole to north pole by flowing. Clearly this gives a section to $T(S^k)$. Now normalize this section by considering any riemannian metric $||cdot||$ by $frac{v}{||v||}$ and this gives a section on sphere bundle of $S^k$ with fiber $S^{k-1}$ away from 2 points(i.e. south and north pole).



    Since Euler number can be computed by sum of local degrees at south pole and north pole, I can compute the local degree at local trivializations of sphere bundle at south pole $a$ and north pole $b$. WLOG, one can assume local trivializations look like $D(x)times S^{k-1}$ where $D(x)$ is some open disk on sphere $S^k$ centered at $x$. Then consider the following maps. $partial D(x)xrightarrow{s}D(x)times S^{k-1}xrightarrow{pi_2} S^{k-1}$ and denote total map as $f_x$. Pick volume form $omega$ on $S^{k-1}$ where $omega$ can be standard volume form.



    Since the degree is computed locally, one can consider $int_{partial D(x)}f_x^star(omega)=int_{partial D(x)}s^starpsi$ where $psi$ is the global angular form defined over $E$ and $x$ can be either south or north pole. This follows from $f_x^star$ defines form restricts cohomology generator on each fiber and thus same cohomology class as global angular form. Hence they differ by a total differential and then one can apply stoke theorem to see the integral agrees.(Here I have already assumed the support of $psi$ is away from $D(x)$ and one can shrink the size of disk if necessary.)



    If I denote $s(x)=(x,v(x))$ with $v(x)in S^{k-1}$, then $pi_2circ s(x)=v(x)$. Hence $int_{partial D(x)}f_x^star(omega)=int_{partial D(x)} v^star(omega)$. I can take $omega$ to be standard volume form of $k-1$ sphere.



    $textbf{Q:}$ Now I do not see an obvious way to compute this integral though I can write down the formula. How do I proceed further?



    Ref. Bott-Tu Differential Forms in Algebraic Topology, Sec 11, Thm 11.16, Exercise 11.21










    share|cite|improve this question











    $endgroup$















      1












      1








      1





      $begingroup$


      This is related to Bott-Tu Sec 11, Sphere Bundles. I would like to compute the euler characteristic of sphere bundle concretely. I have figured out the following so far.



      Let $S^k$ be the $k-$sphere. Consider vector field $v$ starting from south pole to north pole by flowing. Clearly this gives a section to $T(S^k)$. Now normalize this section by considering any riemannian metric $||cdot||$ by $frac{v}{||v||}$ and this gives a section on sphere bundle of $S^k$ with fiber $S^{k-1}$ away from 2 points(i.e. south and north pole).



      Since Euler number can be computed by sum of local degrees at south pole and north pole, I can compute the local degree at local trivializations of sphere bundle at south pole $a$ and north pole $b$. WLOG, one can assume local trivializations look like $D(x)times S^{k-1}$ where $D(x)$ is some open disk on sphere $S^k$ centered at $x$. Then consider the following maps. $partial D(x)xrightarrow{s}D(x)times S^{k-1}xrightarrow{pi_2} S^{k-1}$ and denote total map as $f_x$. Pick volume form $omega$ on $S^{k-1}$ where $omega$ can be standard volume form.



      Since the degree is computed locally, one can consider $int_{partial D(x)}f_x^star(omega)=int_{partial D(x)}s^starpsi$ where $psi$ is the global angular form defined over $E$ and $x$ can be either south or north pole. This follows from $f_x^star$ defines form restricts cohomology generator on each fiber and thus same cohomology class as global angular form. Hence they differ by a total differential and then one can apply stoke theorem to see the integral agrees.(Here I have already assumed the support of $psi$ is away from $D(x)$ and one can shrink the size of disk if necessary.)



      If I denote $s(x)=(x,v(x))$ with $v(x)in S^{k-1}$, then $pi_2circ s(x)=v(x)$. Hence $int_{partial D(x)}f_x^star(omega)=int_{partial D(x)} v^star(omega)$. I can take $omega$ to be standard volume form of $k-1$ sphere.



      $textbf{Q:}$ Now I do not see an obvious way to compute this integral though I can write down the formula. How do I proceed further?



      Ref. Bott-Tu Differential Forms in Algebraic Topology, Sec 11, Thm 11.16, Exercise 11.21










      share|cite|improve this question











      $endgroup$




      This is related to Bott-Tu Sec 11, Sphere Bundles. I would like to compute the euler characteristic of sphere bundle concretely. I have figured out the following so far.



      Let $S^k$ be the $k-$sphere. Consider vector field $v$ starting from south pole to north pole by flowing. Clearly this gives a section to $T(S^k)$. Now normalize this section by considering any riemannian metric $||cdot||$ by $frac{v}{||v||}$ and this gives a section on sphere bundle of $S^k$ with fiber $S^{k-1}$ away from 2 points(i.e. south and north pole).



      Since Euler number can be computed by sum of local degrees at south pole and north pole, I can compute the local degree at local trivializations of sphere bundle at south pole $a$ and north pole $b$. WLOG, one can assume local trivializations look like $D(x)times S^{k-1}$ where $D(x)$ is some open disk on sphere $S^k$ centered at $x$. Then consider the following maps. $partial D(x)xrightarrow{s}D(x)times S^{k-1}xrightarrow{pi_2} S^{k-1}$ and denote total map as $f_x$. Pick volume form $omega$ on $S^{k-1}$ where $omega$ can be standard volume form.



      Since the degree is computed locally, one can consider $int_{partial D(x)}f_x^star(omega)=int_{partial D(x)}s^starpsi$ where $psi$ is the global angular form defined over $E$ and $x$ can be either south or north pole. This follows from $f_x^star$ defines form restricts cohomology generator on each fiber and thus same cohomology class as global angular form. Hence they differ by a total differential and then one can apply stoke theorem to see the integral agrees.(Here I have already assumed the support of $psi$ is away from $D(x)$ and one can shrink the size of disk if necessary.)



      If I denote $s(x)=(x,v(x))$ with $v(x)in S^{k-1}$, then $pi_2circ s(x)=v(x)$. Hence $int_{partial D(x)}f_x^star(omega)=int_{partial D(x)} v^star(omega)$. I can take $omega$ to be standard volume form of $k-1$ sphere.



      $textbf{Q:}$ Now I do not see an obvious way to compute this integral though I can write down the formula. How do I proceed further?



      Ref. Bott-Tu Differential Forms in Algebraic Topology, Sec 11, Thm 11.16, Exercise 11.21







      general-topology geometry differential-geometry algebraic-topology






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      edited Feb 1 at 3:43







      user45765

















      asked Feb 1 at 3:30









      user45765user45765

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