Trace anomaly and compact stars

Abstract

A widespread assumption states that quantum effects of matter in curved spacetimes become relevant only when the inverse curvature radius approaches the Planck mass $m_{\text{P}}$. We challenge this view by showing that, relying solely on universal properties of QFTs at high energies, the trace anomaly becomes macroscopic instead at energy scales $ \left( m/m_{\text{P}} \right)^{\frac{1-\alpha}{2-\alpha}} m_{\text{P}}$, where $m\ll m_{\text{P}}$ and $\alpha<1$ are, respectively, the mass scale and exponent appearing in the matter equation of state at high energies. As an application, we consider compact stars close to their Buchdahl limit, and examine the propagation of scalar waves on the resulting backreacted geometries. At the aforementioned energy scale, the curvature becomes negative within a neighborhood of the the star's center, implying a qualitative change in the behavior of the associated spectrum of modes.