• Title/Summary/Keyword: DAVIS

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Analyzing the Performance of a Davis-Putnam based Optimization Algorithm for the Index Selection Problem of Database Systems (데이터베이스 색인선택 문제에 대한 Davis-Putnam 기반 최적화 알고리즘의 성능 분석)

  • 서상구
    • The Journal of Information Technology and Database
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    • v.7 no.2
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    • pp.47-59
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    • 2000
  • In this paper, we analyze the applicability of a general optimization algorithm to a database optimization problem. The index selection problem Is the problem to choose a set of indexes for a database in a way that the cost to process queries in the given workload is minimized subject to a given storage space restriction for storing indexes. The problem is well known in database research fields, and many optimization and/or heuristic algorithms have been proposed. Our work differs from previous research in that we formalize the problem in the form of non-linear Integer Programming model, and investigate the feasibility and applicability of a general purpose optimization algorithm, called OPBDP, through experiments. We implemented algorithms to generate workload data sets and problem instances for the experiment. The OPBDP algorithm, which is a non-linear 0-1 Integer Programming problem solver based on Davis-Putnam method, worked generally well for our problem formulation. The experiment result showed various performance characteristics depending on the types of decision variables, variable navigation methods and ocher algorithm parameters, and indicates the need of further study on the exploitation of the general purpose optimization techniques for the optimization problems in database area.

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Where is the Dark Matter in the Double Radio Relic Galaxy Cluster PLCKG287.0+32.9?

  • Finner, Kyle;Jee, Myungkook J.;Dawson, William;Golovich, Nathan;Gruen, Daniel;Lemaux, Brian;Wittman, David
    • The Bulletin of The Korean Astronomical Society
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    • v.42 no.1
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    • pp.51.2-51.2
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    • 2017
  • Diffuse radio relics are often detected in merging galaxy clusters and are emitted by synchrotron process. Radio relics are believed to trace the shock waves in the intracluster medium induced by ram pressure during a major cluster merger. Radio halos and relics are found in approximately 50 galaxy clusters to date that are all in a state of merging. The rarest of these galaxy clusters contain pairs of relics of similar brightness as well as a radio halo. The massive galaxy cluster PLCKG287.0+32.9 belongs to this rare population and is the second most significant detection from the Planck SZ All-sky Survey. Perhaps even more intriguing is that the radio relics are observed at vastly different distances from the X-ray peak requiring a complex merging scenario. In this study, we use weak-lensing to peer deeper into the merging scenario by reconstructing the dark matter distribution. We relate the mass distribution to the radio, X-ray, and optical emissions to provide constraints for future simulations of the merger. Fitting an NFW profile to the tangential shear we infer the mass of the cluster and discuss its implications for the merging scenario.

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