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Fault Tolerant Routing in Star Graphs Using Fault Vector

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Book cover Distributed Computing – IWDC 2005 (IWDC 2005)

Part of the book series: Lecture Notes in Computer Science ((LNTCS,volume 3741))

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Abstract

In this paper a fault tolerant routing algorithm for unicasting on star graph is proposed. The routing algorithm does not involve back tracking and uses fault-vectors. Each node in an n-star has a fault-vector of \(\lfloor\frac{3(n-1)}{2}\rfloor\) bits. The kth bit of a node’s fault-vector is a measure of its routing ability to nodes which are at distance k from itself. The fault-vector of each node can easily be calculated through \(\lfloor\frac{3(n-1)}{2}\rfloor\) rounds of information exchanges among neighbor nodes. For a given source destination pair (u,v), the routing algorithm finds a path of length d + h where d is the length of the shortest path between u and v in a fault-free star graph and h = 0, 2 or 4. The space requirement for storing the fault vector is O(n) in each node. Simulation results show that the proposed algorithm far outperforms the routing algorithm based on safety vectors [13].

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© 2005 Springer-Verlag Berlin Heidelberg

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Das, R.K. (2005). Fault Tolerant Routing in Star Graphs Using Fault Vector. In: Pal, A., Kshemkalyani, A.D., Kumar, R., Gupta, A. (eds) Distributed Computing – IWDC 2005. IWDC 2005. Lecture Notes in Computer Science, vol 3741. Springer, Berlin, Heidelberg. https://doi.org/10.1007/11603771_52

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  • DOI: https://doi.org/10.1007/11603771_52

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-30959-8

  • Online ISBN: 978-3-540-32428-7

  • eBook Packages: Computer ScienceComputer Science (R0)

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