论文标题

流体性质限制了Horndeski重力

Fluid nature constrains Horndeski gravity

论文作者

Miranda, Marcello, Vernieri, Daniele, Capozziello, Salvatore, Faraoni, Valerio

论文摘要

在一种新方法中阐明了Horndeski重力的难以捉摸的物理性质,该方法将这类理论描述为耗散性的有效液体。要求后者的本构方程是牛顿流体的方程,这将理论限制为“可行” Horndeski重力的两个断开子类。因此,Horndeski有效流体的应力能量张量,在流体4速度的第一个衍生物中线性,是一个足够的条件,足以使引力波以轻速的速度传播。所有其他Horndeski理论对应于异国情调的非牛顿有效液体。

The elusive physical nature of Horndeski gravity is elucidated in a new approach depicting this class of theories as a dissipative effective fluid. Requiring the constitutive equations of the latter to be those of a Newtonian fluid restricts the theory to only two disconnected subclasses of "viable" Horndeski gravity. Therefore, a stress-energy tensor of Horndeski effective fluid, linear in the first derivatives of the fluid's 4-velocity, is a sufficient condition for gravitational waves to propagate at light speed. All other Horndeski theories correspond to exotic non-Newtonian effective fluids.

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