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Titlebook: Komplementäre Methodenlehre der klinischen Forschung; Cognition-based Medi Helmut Kiene Book 2001 Springer-Verlag Berlin Heidelberg 2001 Fo

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https://doi.org/10.1007/978-3-642-59445-8Forschung; Gehör; Gesundheit; Gesundheitswesen; Grundlagen; Hoden; Medizin; Statistik; Stent; Therapie; Wissen
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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
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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
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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
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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
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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.
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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
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