论文标题
新的张量矢量量表理论中穿着的黑洞
Dressed black holes in the new tensor-vector-scalar theory
论文作者
论文摘要
随着重力在其素数中的化身，黑洞可以说是我们脱神经重力的最佳目标。牢记黑洞在引力波天文学中的重要作用，理论必须拥有黑洞解决方案，而只有可衡量的一般相对论也可以拥有黑洞解决方案。在本文中，我们在相对论修改后的牛顿动力学的张量 - 矢量量表中介绍了黑洞。我们发现该理论允许Schwarzschild和几乎是Schwarzschild黑洞作为解决方案，而非平凡的标量和矢量场通常在事件地平线上有所不同。无论这是物理病理，是否对这些解决方案和扩展为模型构成挑战。但是，即使是，当黑洞头发消失时，这种病理也可以克服。
As incarnations of gravity in its prime, black holes are arguably the best target for us to demystify gravity. Keeping in mind the prominent role black holes play in gravitational wave astronomy, it becomes a must for a theory to possess black hole solutions with only measurable departures from their general relativity counterparts. In this paper, we present black holes in a tensor-vector-scalar representation of relativistic modified Newtonian dynamics. We find that the theory allows Schwarzschild and nearly-Schwarzschild black holes as solutions, while the nontrivial scalar and vector fields generally diverge at the event horizon. Whether this is a physical pathology or not poses a challenge for these solutions, and by extension, the model. However, even if it is, this pathology could be overcome when the black hole hair vanishes.
