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Classical stability of the Galileon

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Abstract

We consider the classical equations of motion for a single Galileon field with generic parameters in the presence of non-relativistic sources. We introduce the concept of absolute stability of a theory: if one can show that a field at a single point — like infinity for instance — in spacetime is stable, then stability of the field over the rest of spacetime is guaranteed for any positive energy source configuration. The Dvali-Gabadadze-Porrati (DGP) model is stable in this manner, and previous studies of spherically symmetric solutions suggest that certain classes of the single field Galileon (of which the DGP model is a subclass) may have this property as well. We find, however, that when general solutions are considered this is not the case. In fact, when considering generic solutions there are no choices of free parameters in the Galileon theory that will lead to absolute stability except the DGP choice. Our analysis indicates that the DGP model is an exceptional choice among the large class of possible single field Galileon theories. This implies that if general solutions (non-spherically symmetric) exist they may be unstable. Given astrophysical motivation for the Galileon, further investigation into these unstable solutions may prove fruitful.

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Authors and Affiliations

  1. Department of Physics and ISCAP, Columbia University, New York, NY, 10027, USA

    Solomon Endlich & Junpu Wang

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  1. Solomon Endlich
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  2. Junpu Wang
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Correspondence to Junpu Wang.

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ArXiv ePrint: 1106.1659

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Endlich, S., Wang, J. Classical stability of the Galileon. J. High Energ. Phys. 2011, 65 (2011). https://doi.org/10.1007/JHEP11(2011)065

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  • DOI: https://doi.org/10.1007/JHEP11(2011)065

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