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Knowledge Base Question Answering by Case-based Reasoning over Subgraphs

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arxiv 2202.10610 v2 pith:PMKDAYN3 submitted 2022-02-22 cs.CL cs.AIcs.LG

Knowledge Base Question Answering by Case-based Reasoning over Subgraphs

classification cs.CL cs.AIcs.LG
keywords subgraphsubgraphsreasoningpatternsanswercbr-subgqueriesquery
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Question answering (QA) over knowledge bases (KBs) is challenging because of the diverse, essentially unbounded, types of reasoning patterns needed. However, we hypothesize in a large KB, reasoning patterns required to answer a query type reoccur for various entities in their respective subgraph neighborhoods. Leveraging this structural similarity between local neighborhoods of different subgraphs, we introduce a semiparametric model (CBR-SUBG) with (i) a nonparametric component that for each query, dynamically retrieves other similar $k$-nearest neighbor (KNN) training queries along with query-specific subgraphs and (ii) a parametric component that is trained to identify the (latent) reasoning patterns from the subgraphs of KNN queries and then apply them to the subgraph of the target query. We also propose an adaptive subgraph collection strategy to select a query-specific compact subgraph, allowing us to scale to full Freebase KB containing billions of facts. We show that CBR-SUBG can answer queries requiring subgraph reasoning patterns and performs competitively with the best models on several KBQA benchmarks. Our subgraph collection strategy also produces more compact subgraphs (e.g. 55\% reduction in size for WebQSP while increasing answer recall by 4.85\%)\footnote{Code, model, and subgraphs are available at \url{https://github.com/rajarshd/CBR-SUBG}}.

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Cited by 2 Pith papers

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    astro-ph.HE 2026-06 conditional novelty 6.0

    Using a re-fitted BNS-sGRB population model and AfterglowPy simulations, the paper forecasts ~5 on-axis and ~11 orphan afterglows per year for LSST, and <1.4 joint optical-GW afterglows per year in LIGO O5.

  2. Short-Duration Gamma-ray Burst and Afterglow Rates in the Rubin and Roman Era

    astro-ph.HE 2026-06 unverdicted novelty 5.0

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