议程
发表于 2025-3-26 21:35:07
http://reply.papertrans.cn/32/3114/311375/311375_31.png
预知
发表于 2025-3-27 02:43:58
http://reply.papertrans.cn/32/3114/311375/311375_32.png
悠然
发表于 2025-3-27 07:29:27
http://reply.papertrans.cn/32/3114/311375/311375_33.png
花束
发表于 2025-3-27 12:44:02
https://doi.org/10.1007/978-3-031-37034-2sed on the maximum entropy principle, and is equivalent to the standard statistical mechanics formulation in each of the quantum and classical cases. The latter case is of particular interest, as it provides a novel Hamilton–Jacobi picture of classical thermodynamics.
Injunction
发表于 2025-3-27 14:00:32
https://doi.org/10.1007/978-94-007-7987-7ricted to particles but can also be used to derive bosonic field equations. It is remarkable that the basic underlying concept, the addition of nonclassical momentum fluctuations to a classical ensemble, carries through from quantum particles to quantum fields, without creating conceptual difficulti
CLAMP
发表于 2025-3-27 18:12:42
The Scientific Study of Personal Wisdompace of probabilities only, to a metric over the full phase space. This requires satisfying certain conditions which ensure the compatibility of the metric and symplectic structures. These conditions are equivalent to requiring that the space have a Kähler structure. In this way, we are led to a Käh
丰满中国
发表于 2025-3-28 01:55:53
https://doi.org/10.1007/978-1-4757-6791-9into account, and now the observables must provide a representation of .. We show in this case that, in addition to a model equivalent to the quantum theory of a pair of qubits, it may also be possible to have non-quantum local models.
细胞
发表于 2025-3-28 02:20:02
http://reply.papertrans.cn/32/3114/311375/311375_38.png
松软
发表于 2025-3-28 06:52:28
http://reply.papertrans.cn/32/3114/311375/311375_39.png
即席
发表于 2025-3-28 13:48:27
https://doi.org/10.1007/b138529 gravity. Having derived the equations for the general case, we move on to the simpler case of spherical symmetric spacetimes and derive the corresponding equations for midisuperspace models of spherically symmetric gravity. We consider the example of classical ensembles of black holes in this midis