Causal Modifications of Gravity and Their Observational Bounds
arXiv:2209.07525 · doi:10.1103/PhysRevD.107.024037
Abstract
Since general relativity is the unique theory of massless spin 2 particles at large distances, the most reasonable way to have significant modifications is to introduce one or more light scalars that mediate a new long-range force. Most existing studies of such scalars invoke models that exhibit some kind of "screening" at short distances to hide the force from solar system tests. However, as is well known, such modifications also exhibit superluminality, which can be interpreted as a form of acausality. In this work we explore explicitly subluminal and causal scalar field models. In particular, we study a conformally coupled scalar , with a small coupling to matter to obey solar system bounds, and a non-canonical kinetic term () that obeys all subluminality constraints and is hyperbolic. We consider that is canonical for small , but beyond some nonlinear scale enters a new scaling regime of power , with (the DBI kinetic term is the limit and a canonical scalar is ). As opposed to screening (and superluminality), this new force becomes more and more important in the regime of high densities (and subluminality). We then turn to the densest environments to put bounds on this new interaction. We compute constraints from precession in binary systems such as Hulse-Taylor, we compute corrections to neutron star hydrostatic equilibrium, and we compute power in radiation, both tensor mode corrections and the new scalar mode, which can be important during mergers.
arXiv comment44 pages, 6 figures. V3: Updated toward version published in PRD
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