Refine
Has Fulltext
- yes (245) (remove)
Year of publication
Document Type
- Conference Proceeding (245) (remove)
Language
- English (185)
- German (49)
- Multiple languages (10)
- French (1)
Keywords
- Archiv (4)
- Information Structure (4)
- Nachlass (4)
- Cloud Computing (3)
- E-Learning (3)
- middleware (3)
- Constraint Solving (2)
- Deduction (2)
- EMOTIKON (2)
- Forschungsprojekte (2)
Institute
- Extern (137)
- Interdisziplinäres Zentrum für Musterdynamik und Angewandte Fernerkundung (23)
- Institut für Künste und Medien (20)
- Institut für Informatik und Computational Science (15)
- Institut für Slavistik (14)
- Institut für Physik und Astronomie (11)
- Institut für Geowissenschaften (10)
- Hasso-Plattner-Institut für Digital Engineering gGmbH (9)
- Sonderforschungsbereich 632 - Informationsstruktur (7)
- Bürgerliches Recht (6)
A deterministic cycle scheduling of partitions at the operating system level is supposed for a multiprocessor system. In this paper, we propose a tool for generating such schedules. We use constraint based programming and develop methods and concepts for a combined interactive and automatic partition scheduling system. This paper is also devoted to basic methods and techniques for modeling and solving this partition scheduling problem. Initial application of our partition scheduling tool has proved successful and demonstrated the suitability of the methods used.
We propose a paraconsistent declarative semantics of possibly inconsistent generalized logic programs which allows for arbitrary formulas in the body and in the head of a rule (i.e. does not depend on the presence of any specific connective, such as negation(-as-failure), nor on any specific syntax of rules). For consistent generalized logic programs this semantics coincides with the stable generated models introduced in [HW97], and for normal logic programs it yields the stable models in the sense of [GL88].
Massive stars usually form groups such as OB associations. Their fast stellar winds sweep up collectively the surrounding insterstellar medium (ISM) to generate superbubbles. Observations suggest that superbubble evolution on the surrounding ISM can be very irregular. Numerical simulations considering these conditions could help to understand the evolution of these superbubbles and to clarify the dynamics of these objects as well as the difference between observed X-ray luminosities and the predicted ones by the standard model (Weaver et al. 1977).