Most of the large galaxies host a supermassive black hole, but their origin is still not well understood. In this paper, we look at a possible connection between the gravitational binding energies of large galaxies, etc., and the masses of their central black holes. Using this relation (between the gravitational binding energy of the host structure and the black hole energy), we argue why globular clusters are unlikely to harbour large black holes and why dwarf galaxies, if they have to host black holes, should have observed mass-to-light ratios of ~100.

中文翻译：

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星系的结合能是否与其核心黑洞质量有关？

大多数大型星系都拥有一个超大质量的黑洞，但是它们的起源仍不为人所知。在本文中，我们研究了大星系等的引力结合能与其中心黑洞质量之间的可能联系。利用这种关系（主体结构的引力结合能和黑洞能之间的关系），我们认为为什么球状星团不太可能藏有大黑洞，为什么矮星系（如果必须拥有黑洞）应该观察到质量-照明比约为100。