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Titlebook: At the Frontier of Spacetime; Scalar-Tensor Theory Torsten Asselmeyer-Maluga Book 2016 Springer International Publishing Switzerland 2016 B

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樓主: metamorphose
11#
發(fā)表于 2025-3-23 09:46:55 | 只看該作者
12#
發(fā)表于 2025-3-23 16:07:13 | 只看該作者
13#
發(fā)表于 2025-3-23 19:12:52 | 只看該作者
14#
發(fā)表于 2025-3-24 02:15:58 | 只看該作者
https://doi.org/10.1007/978-3-319-70464-7tic smooth structures are especially abundant in dimension four—the dimension of the physical spacetime. These facts spurred research into possible the physical role of exotic smoothness, an interesting but not an easy task, as we will show.
15#
發(fā)表于 2025-3-24 05:28:55 | 只看該作者
The Politics of Alliance Policy,Hill et al. [.] on the non-existence of Kervaire invariant one elements in all dimensions . with . We obtain the main theorem: The n-dimensional sphere, . admits exotic smoothness structures of 2-primary order for all dimensions . such that . is not congruent to 4 modulo 8 and also . not equal to 12
16#
發(fā)表于 2025-3-24 09:07:16 | 只看該作者
https://doi.org/10.1057/9780230277908bra can be understood as a deformation quantization of the classical Poisson algebra of observables given by holonomies. The structure of this operator algebra induces an action by using the quantized calculus of Connes. The scaling behavior of this action is analyzed to obtain the classical theory
17#
發(fā)表于 2025-3-24 12:26:18 | 只看該作者
0168-1222 his Festschrift, one finds an outstanding and unique collection of articles about exotic smoothness. Also featured are Bell‘s inequality and Mach‘s principle..Personal memories and historical aspects round off the collection..978-3-319-81008-9978-3-319-31299-6Series ISSN 0168-1222 Series E-ISSN 2365-6425
18#
發(fā)表于 2025-3-24 18:45:08 | 只看該作者
Nonminimal Couplings in the Early Universe: Multifield Models of Inflation and the Latest Observatioields. Inflationary models make specific, quantitative predictions for several observable quantities, including particular patterns of temperature anistropies in the cosmic microwave background radiation. Realistic models of high-energy physics include many scalar fields at high energies. Moreover,
19#
發(fā)表于 2025-3-24 21:44:39 | 只看該作者
20#
發(fā)表于 2025-3-25 01:20:28 | 只看該作者
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