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Titlebook: Relativistic Cosmology; An Introduction Jean Heidmann Book 1980 Springer-Verlag Berlin Heidelberg 1980 Cosmology.Kosmos.Universe.general re

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21#
發(fā)表于 2025-3-25 04:12:39 | 只看該作者
Jean Heidmanneted within 19 months after contract go-ahead, 2) array dc power output exceeded 375-kW in February 1982 at an array field efficiency of 10.4%, 3) concentrator array module progressed from development stage to a commercial high production type within a year, and 4) it has the first operational array
22#
發(fā)表于 2025-3-25 08:06:42 | 只看該作者
23#
發(fā)表于 2025-3-25 15:38:48 | 只看該作者
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發(fā)表于 2025-3-25 16:17:02 | 只看該作者
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發(fā)表于 2025-3-25 23:53:11 | 只看該作者
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發(fā)表于 2025-3-26 01:22:20 | 只看該作者
Jean Heidmann examination, the parameter space of the problem is mapped, with particular attention given to problematic areas such as the highly quantum mechanical weak-coupling regime and the highly nonlinear intermediate-coupling regime, and to the self-trapping transition that may be said to mark the onset of
27#
發(fā)表于 2025-3-26 04:21:52 | 只看該作者
Jean Heidmannnals). In fact they show some efficiency in performing “associative, adaptive memory” (as manifested in retrieval of memories and recognition of simple patterns). The methods used for their study stem from statistical mechanics and the theory of stochastic processes. This is particularly evident in
28#
發(fā)表于 2025-3-26 12:26:24 | 只看該作者
29#
發(fā)表于 2025-3-26 13:48:00 | 只看該作者
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發(fā)表于 2025-3-26 20:14:38 | 只看該作者
iant of the problem is also known as .. This problem has been investigated assuming powerful inter-agent communication mechanisms: . at all nodes. Indeed, in this model, the black hole search problem can be solved with a minimal team size and performing a polynomial number of moves..In this paper, w
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