Parabola
发表于 2025-3-23 13:33:54
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类型
发表于 2025-3-23 15:23:53
https://doi.org/10.1007/978-3-642-59445-8Forschung; Gehör; Gesundheit; Gesundheitswesen; Grundlagen; Hoden; Medizin; Statistik; Stent; Therapie; Wissen
insidious
发表于 2025-3-23 19:26:25
n. Thus, if the average distribution of matter in the universe is put into Einstein’s field equations, the average space-time structure of the whole universe may be deduced. This is a very interesting exercise, and it is part of the subject of cosmology. Cosmology is the study of the dynamical struc
EXALT
发表于 2025-3-24 01:52:14
Helmut Kienen. Thus, if the average distribution of matter in the universe is put into Einstein’s field equations, the average space-time structure of the whole universe may be deduced. This is a very interesting exercise, and it is part of the subject of cosmology. Cosmology is the study of the dynamical struc
Perceive
发表于 2025-3-24 04:47:22
Helmut Kienen. Thus, if the average distribution of matter in the universe is put into Einstein’s field equations, the average space-time structure of the whole universe may be deduced. This is a very interesting exercise, and it is part of the subject of cosmology. Cosmology is the study of the dynamical struc
DEAWL
发表于 2025-3-24 09:43:07
Helmut Kienetext of a beyond-Newtonian approximation [.]. We shall begin by discussing the construction of the beyond-Newtonian potential in the so-called Fodor–Hoenselaers–Perjés procedure where we keep first order non-Newtonian contributions in both the mass and spin. Using this potential, we shall then discu
Habituate
发表于 2025-3-24 10:44:10
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theta-waves
发表于 2025-3-24 15:02:30
Helmut Kienefeasible and opened a major experimental channel for probing the gravitational interaction in the strong field regime. Although considered historically as a property of the black hole spacetimes, the shadow is not exclusively a black hole effect and does not require the presence of an event horizon.
暴发户
发表于 2025-3-24 21:26:14
Helmut Kienetext of a beyond-Newtonian approximation [.]. We shall begin by discussing the construction of the beyond-Newtonian potential in the so-called Fodor–Hoenselaers–Perjés procedure where we keep first order non-Newtonian contributions in both the mass and spin. Using this potential, we shall then discu
Spina-Bifida
发表于 2025-3-25 02:53:35
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