435,147 research outputs found

    Epimorphisms of C*-algebras are surjective

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    We answer a question raised by V.G.Pestov in the affirmative.Comment: 2 page

    F-adjunction

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    In this paper we study singularities defined by the action of Frobenius in characteristic p>0p > 0. We prove results analogous to inversion of adjunction along a center of log canonicity. For example, we show that if XX is a Gorenstein normal variety then to every normal center of sharp FF-purity WXW \subseteq X such that XX is FF-pure at the generic point of WW, there exists a canonically defined \bQ-divisor ΔW\Delta_{W} on WW satisfying (K_X)|_W \sim_{\bQ} K_{W} + \Delta_{W}. Furthermore, the singularities of XX near WW are "the same" as the singularities of (W,ΔW)(W, \Delta_{W}). As an application, we show that there are finitely many subschemes of a quasi-projective variety that are compatibly split by a given Frobenius splitting. We also reinterpret Fedder's criterion in this context, which has some surprising implications.Comment: 31 pages; to appear in Algebra and Number Theory. Typos corrected, presentation improved throughout. Section 7 subdivided into two sections (7 and 8). The proofs of 4.8, 5.8 and 9.5 improve

    Detection of Gravitational Waves from Eccentric Compact Binaries

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    Coalescing compact binaries have been pointed out as the most promising source of gravitational waves for kilometer-size interferometers such as LIGO. Gravitational wave signals are extracted from the noise in the detectors by matched filtering. This technique performs really well if an a priori theoretical knowledge of the signal is available. The information known about the possible sources is used to construct a model of the expected waveforms (templates). A common assumption made when constructing templates for coalescing compact binaries is that the companions move in a quasi-circular orbit. Some scenarios, however, predict the existence of eccentric binaries. We investigate the loss in signal-to-noise ratio induced by non-optimal filtering of eccentric signals.Comment: 5 pages, 2 figures, to appear in the proceedings of the 8th Canadian Conference on General Relativity and Relativistic Astrophysic
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