Results 1 - 4 of 4

WYSTERIA: A Programming Language for Generic, Mixed-Mode Multiparty Computations

by Aseem Rastogi, Matthew A. Hammer, Michael Hicks
"... distrusting parties use cryptographic techniques to cooperatively compute over their private data; in the process each party learns only explicitly revealed outputs. In this paper, we present WYSTERIA, a high-level programming language for writing SMCs. As with past languages, like Fairplay, WYSTERI ..."
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, WYSTERIA compiles secure computations to circuits that are executed by an underlying engine. Unlike past work, WYSTERIA provides support for mixed-mode programs, which combine local, private computations with synchronous SMCs. WYSTERIA complements a standard feature set with built-in support for secret

Endothelial coordination of cerebral vasomotion via myoendothelial gap junctions containing connexins 37 and 40

by Rebecca E. Haddock, T. Hilton Grayson, Therese D. Brackenbury, Kate R. Meaney, Craig B. Neylon, Shaun L. S, Caryl E. Hill, Rebecca E, T. Hilton Grayson, Therese D. Brack, Kate R. Meaney, Craig B. Neylon, Shaun L. S , 2006
"... bral vasculature differs from that of systemic vessels outside the blood-brain barrier. The hypothesis that the endothelium modulates vasomotion via direct myoendothelial coupling was investigated in a small vessel of the cerebral circulation. In the primary branch of the rat basilar artery, membran ..."
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-resolution ultrastruc-tural and confocal immunohistochemistry and quantitative PCR. Membrane potential oscillations were present in both endothelial cells and smooth muscle cells (SMCs), and these preceded rhythmical contractions during which adjacent SMC intracellular calcium con-centration ([Ca2]i) waves were

Dynamical Influences of the Last Magellanic Interaction On the Magellanic Clouds

by Kenji Bekki A, Masashi Chiba B , 2007
"... Abstract: We investigate the present distributions of gas and young stars in the Large and Small Magellanic Clouds (LMC and SMC) based on fully self-consistent numerical simulations of the Clouds for the last ∼ 0.8 Gyr. Our principal results, which can be tested against observations, are as follows. ..."
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to the interaction. A small but non-negligible fraction of stellar and gaseous components can be transferred from the SMC into the LMC during the interaction to form diffuse halo components around the LMC. The burst of star formation in the SMC can be synchronized with that of the LMC about 0.2 Gyr ago in some

Dynamical Influences of the Last Magellanic Interaction on the Magellanic Clouds

by Kenji Bekkia, Masashi Chibab , 2006
"... Abstract: We investigate the present distributions of gas and young stars in the Large and Small Magellanic Clouds (LMC and SMC) based on fully self-consistent numerical simulations of the Clouds for the last ∼0.8 Gyr. Our principal results, which can be tested against observations, are as follows. ..."
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to the interaction. A small but non-negligible fraction of stellar and gaseous components can be transferred from the SMC into the LMC during the interaction to form diffuse halo components around the LMC. The burst of star formation in the SMC can be synchronized with that of the LMC about 0.2 Gyr ago in some
Results 1 - 4 of 4