Results 71 to 80 of about 26,245 (203)
Cohomology with compact supports for Stein spaces.
Journal für die reine und angewandte Mathematik (Crelles Journal), 1987 It is known that if X is a Stein manifold of dimension n then \(H_ i(X;{\mathbb{Z}})=0\) for ...
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Lyn Hejinian’s Writing. Poetic Language as Language of Inquiry [PDF]
Литература двух АмерикThe article is devoted to the poetics of contemporary American writer Lyn Hejinian (1941–2024), considered one of the most consistent successors of Gertrude Stein's experimentalism in Anglophone literary writing.
Vladimir V. Feshchenko
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On Space-Time and Ontology: Extract from a Letter to Adolf Grünbaum
, 1977 1 online resource (PDF, page 374-402)Stein, Howard. (1977). On Space-Time and Ontology: Extract from a Letter to Adolf Grünbaum.
Stein, Howard
core
, 2020 In this bachelor thesis, we describe the construction of rotation invariant differential operators of first order on the Euklidean space Rn given by E. Stein and G. Weiss. For this construction we show how to find an irreducible decomposition of a tensor
Malý, Marek
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HOLOMORPHIC EMBEDDINGS OF STEIN SPACES IN INFINITE-DIMENSIONAL PROJECTIVE SPACES [PDF]
Journal of the Korean Mathematical Society, 2005 The author shows that if \(X\) is a reduced Stein space and \(L\) is a holomorphic line bundle on \(X\), if one considers any locally convex vector topology on \( H^{0}(X, L) ^{\ast}\) which is stronger than the weak topology, then the image of the canonical holomorphic embedding \( h_{L} : X \rightarrow H^{0}(X, L) ^{\ast}\) is sequentially closed and
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Discover SpacePc5 geomagnetic pulsations (PGPs) are ultra-low frequency (ULF) waves within the 1–7 mHz frequency band observed both in space and on the ground. PGPs offer versatile methods for studying the interaction between the magnetosphere and ionosphere in space.
Sebwato Nasurudiin +4 more
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Global Stein theorem on Hardy spaces
Analysis MathematicaLet f be an integrable function which has integral 0 on R n. What is the largest condition on |f | that guarantees that f is in the Hardy space H 1 (R n)? When f is compactly supported, it is well-known that it is necessary and sufficient that |f | belongs to L log L(R n). We are interested here in conditions at $\infty$.
Bonami, A., Grellier, S., Sehba, B. F.
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Optimal Task Migration in Service-Oriented Systems: Algorithms and Mechanisms
, 2010 In service-oriented systems, such as grids and clouds, users are able to outsource complex computational tasks by procuring resources on demand from remote service providers.
Jennings, Nick +2 more
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Effective gravitational wave stress-energy tensor in alternative theories of gravity
, 2010 The inspiral of binary systems in vacuum is controlled by the stress-energy of gravitational radiation and any other propagating degrees of freedom. For gravitational waves, the dominant contribution is characterized by an effective stress-energy tensor ...
Leo C. Stein +3 more
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Post-Newtonian, quasicircular binary inspirals in quadratic modified gravity [PDF]
, 2011 We consider a general class of quantum gravity-inspired, modified gravity theories, where the Einstein-Hilbert action is extended through the addition of all terms quadratic in the curvature tensor coupled to scalar fields with standard kinetic energy ...
Stein, Leo Chaim +4 more
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