3,870 research outputs found

    A ternary variety generated by lattices

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    Amalgamating commutative regular rings

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    Quasicomplemented lattices

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    THE ROLE OF VITAMIN B 6 IN THE TOXICITY OF HYDRAZINES *

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    Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/73785/1/j.1749-6632.1969.tb54264.x.pd

    On the Chinese remainder theorem of H. Draškovičová

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    Co-accelerated particles in the C-metric

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    With appropriately chosen parameters, the C-metric represents two uniformly accelerated black holes moving in the opposite directions on the axis of the axial symmetry (the z-axis). The acceleration is caused by nodal singularities located on the z-axis. In the~present paper, geodesics in the~C-metric are examined. In general there exist three types of timelike or null geodesics in the C-metric: geodesics describing particles 1) falling under the black hole horizon; 2)crossing the acceleration horizon; and 3) orbiting around the z-axis and co-accelerating with the black holes. Using an effective potential, it can be shown that there exist stable timelike geodesics of the third type if the product of the parameters of the C-metric, mA, is smaller than a certain critical value. Null geodesics of the third type are always unstable. Special timelike and null geodesics of the third type are also found in an analytical form.Comment: 10 pages, 12 EPS figures, changes mainly in abstract & introductio

    Platinum-Based Alloys and Coatings: Materials for the Future?

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    Reconstructing the global topology of the universe from the cosmic microwave background

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    If the universe is multiply-connected and sufficiently small, then the last scattering surface wraps around the universe and intersects itself. Each circle of intersection appears as two distinct circles on the microwave sky. The present article shows how to use the matched circles to explicitly reconstruct the global topology of space.Comment: 6 pages, 2 figures, IOP format. To be published in the proceedings of the Cleveland Cosmology and Topology Workshop 17-19 Oct 1997. Submitted to Class. Quant. Gra
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