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Self-simulation for the Passive Optical Star model

  • Session 6. Chair: Alan Gibbons
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Book cover Algorithms — ESA '95 (ESA 1995)

Part of the book series: Lecture Notes in Computer Science ((LNCS,volume 979))

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Abstract

In the context of parallel computing, optical technology offers simple interconnection schemes with straightforward layouts that support complex logical interconnection patterns. The Passive Optical Star (Pos) is often suggested as a platform for implementing the optical network: logically it offers an all-to-all broadcast capability.

We investigate the self-simulation or scalability properties of the Pos. A family of parallel machines is said to be self-simulating or scalable if reducing the number of processors by a factor of k (by going to a smaller member of the family) increases the computation time by a factor of (the optimal) O(k).

We present a randomized algorithm for an n-processor Pos that simulates a kn-processor Pos with a slowdown of O(k+log* n) using local control only, thus coming close to the self-simulation ideal of O(k). We also analyze direct algorithms that send messages directly from their origin to their destination; for this case we prove that Θ(k 2) is the exact complexity.

This work was supported in part by ANM, C3, the French-Israeli grant for cooperation in Computer Science, by a grant from the Israeli Ministry of Science, and by the ESPRIT Basic Research Actions Program of the EU under contract No. 7141 (project ALCOM II).

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Paul Spirakis

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© 1995 Springer-Verlag Berlin Heidelberg

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Berthomé, P., Duboux, T., Hagerup, T., Newman, I., Schuster, A. (1995). Self-simulation for the Passive Optical Star model. In: Spirakis, P. (eds) Algorithms — ESA '95. ESA 1995. Lecture Notes in Computer Science, vol 979. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-60313-1_156

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  • DOI: https://doi.org/10.1007/3-540-60313-1_156

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-60313-9

  • Online ISBN: 978-3-540-44913-3

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