12,870 research outputs found

    On a symplectic generalization of Petrie's conjecture

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    Motivated by the Petrie conjecture, we consider the following questions: Let a circle act in a Hamiltonian fashion on a compact symplectic manifold (M,ω)(M,\omega) which satisfies H^{2i}(M;\R) = H^{2i}(\CP^n,\R) for all ii. Is H^j(M;\Z) = H^j(\CP^n;\Z) for all jj? Is the total Chern class of MM determined by the cohomology ring H(M;Z)H^*(M;\Z)? We answer these questions in the six dimensional case by showing that Hj(M;Z)H^j(M;\Z) is equal to H^j(\CP^3;\Z) for all jj, by proving that only four cohomology rings can arise, and by computing the total Chern class in each case. We also prove that there are no exotic actions. More precisely, if H(M;Z)H^*(M;\Z) is isomorphic to H^*(\CP^3;\Z) or H^*(\Tilde{G}_2(\R^5);\Z), then the representations at the fixed components are compatible with one of the standard actions; in the remaining two case, the representation is strictly determined by the cohomology ring. Finally, our results suggest a natural question: do the remaining two cohomology rings actually arise? This question is closely related to some interesting problems in symplectic topology, such as embeddings of ellipsoids.Comment: 34 pages; accepted to Transactions of the AM

    More complete discussion of the time-dependence of the non-static line element for the universe

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    In a previous article,(1) I have shown that a continuous transformation of matter into radiation, occurring throughout the universe, as postulated by the astrophysicists, would necessitate a nonstatic line element for the universe, and have shown that the non-static character thus introduced might provide an explanation of the red shift in the light from the extra-galactic nebulae. In the present article, I wish to discuss the form of dependence of the line element on the time more completely than was possible on the previous occasion. This is a matter of considerable importance, since changes in the approximations which must be introduced to obtain a usable result affect to quite a different extent the expressions for the relation between red shift and distance and for the rate of annihilation of matter. Indeed, the possibility arises of slight changes from the treatment previously given which would leave the theoretical relation between red shift and distance still approximately linear, as observationally found, and yet produce a very considerable change in the calculated rate for the annihilation of matter

    Hamiltonian circle actions on eight dimensional manifolds with minimal fixed sets

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    Consider a Hamiltonian circle action on a closed 88-dimensional symplectic manifold MM with exactly five fixed points, which is the smallest possible fixed set. In their paper, L. Godinho and S. Sabatini show that if MM satisfies an extra "positivity condition" then the isotropy weights at the fixed points of MM agree with those of some linear action on CP4\mathbb{CP}^4. Therefore, the (equivariant) cohomology rings and the (equivariant) Chern classes of MM and CP4\mathbb{CP}^4 agree; in particular, H(M;Z)Z[y]/y5H^*(M;\mathbb{Z}) \simeq \mathbb{Z}[y]/y^5 and c(TM)=(1+y)5c(TM) = (1+y)^5. In this paper, we prove that this positivity condition always holds for these manifolds. This completes the proof of the "symplectic Petrie conjecture" for Hamiltonian circle actions on on 8-dimensional closed symplectic manifolds with minimal fixed sets.Comment: To appear in Transformation Group
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