Galileon scalar electrodynamics
Ashu Kushwaha, S. Shankaranarayanan (IIT Bombay)

TL;DR
This paper develops a Galileon scalar electrodynamics model that maintains Galilean symmetry, gauge invariance, and second-order equations of motion, with potential applications to early Universe accelerated expansion and inflation.
Contribution
It introduces a novel Galileon scalar electrodynamics model with non-minimal couplings that preserve key symmetries and stability, extending previous scalar Galileon theories.
Findings
Model satisfies Galilean symmetry and gauge invariance.
Equations of motion contain only second-order derivatives.
Potential to explain early Universe accelerated expansion.
Abstract
We construct a consistent model of Galileon scalar electrodynamics. The model satisfies three essential requirements: (1) The action contains higher-order derivative terms, and obey the Galilean symmetry, (2) Equations of motion also satisfy Galilean symmetry and contain only up to second-order derivative terms in the matter fields and, hence do not suffer from instability, and (3) local U(1) gauge invariance is preserved. We show that the non-minimal coupling terms in our model are different from that of the real scalar Galileon models; however, they match with the Galileon real scalar field action. We show that the model can lead to an accelerated expansion in the early Universe. We discuss the implications of the model for cosmological inflation.
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