A Black-Box Workload Barrier for Exact Girth via Multi-Scale Nearest-Source Estimation in CONGEST
Indraveni Chebolu, Bhavani Singh Rajpurohit, Arnab Mallick
Abstract
Recent multi-scale nearest-source methods give polynomially sublinear girth approximations in CONGEST. We isolate the direct black-box route for making this framework exact: sequential calls to the same estimator on fresh exchangeable source sets, with source cardinalities and nearest-source capacities chosen adaptively from previous scalar outputs and with an adaptive stopping rule. On a bounded-degree, logarithmic-diameter family Ht with nt vertices and a unique girth-gt=Θ( nt) cycle, exactness requires a sampled cycle source to survive at an antipodal edge despite a linear number of strictly closer competitors. For any such exactification A, a permutation-rank argument yields the implementation-independent workload bound [ A(Ht)=gt]≤(3gt/nt)\, E[Σj=1T\Qj,kj\], where T is the number of executed calls, Qj is the source-set cardinality, and kj is the nearest-source capacity of call j. Thus constant exactness probability requires Ω(nt/gt)=Ω(nt/ nt) expected retained-source workload. We formally show that retuning the recent multi-scale template solely through its scale count/order, Bernoulli or fixed-cardinality sampling, capacities, and scalar-output stopping rules lies in this class. For the standard sequential packetized estimator realization, the workload theorem gives an Ω(nt/ nt) expected-round corollary. This is a barrier to a defined black-box exactification strategy, not a lower bound for unrestricted exact girth in CONGEST.
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