对物理学的基本检验：银河系超大质量暗天体
A fundamental test for physics: the galactic supermassive obscure bodies
摘要：
天文学家在几个星系核中观测到的巨大的引力效应问题似乎令人费解。这些天体太大，不可能是由原始恒星的超新星产生的中子星，又太小，不可能被认为是一种新的模糊星系。这个矛盾是一个基本的检验，它可能会摧毁已建立的引力理论。我们提出了一个新的物理范式，它取代了三个多世纪前牛顿所猜测的旧的“引力质量“。
英文摘要：
The problem of the enormous gravitational effects observed by the astronomers in several galactic nuclei with obscure bodies appears puzzling. These bodies are too large to be neutron stars generated by supernovae of primeval stars and are too small to be considered a new kind of obscure galaxies. This contradiction represents a fundamental test which might destroy the established gravitational theories. We present a new physical paradigm which substitutes the old "gravitational mass" guessed by Newton more than tree centuries ago.
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