On the Disformal Transformation of the Einstein-Hilbert Action
arXiv:2010.00956 · doi:10.47011/16.5
Abstract
Disformal transformation is a generalisation of the well-known conformal transformation commonly elaborated in mainstream graduate texts in gravity (relativity) and modern cosmology. This transformation is one of the most important mathematical operations in scalar tensor theories attempting to address pressing problems involving dark energy and dark matter. With this topic yet to penetrate these texts, we present a pedagogically oriented derivation of the disformal transformation of the Einstein-Hilbert action. Along the way of calculation, we encounter apparently problematic terms that could be construed as leading to equations of motion that go beyond second order in derivatives, signalling instability. We demonstrate that these terms can be eliminated and absorbed through the definition of the Riemann curvature tensor. The transformed Einstein-Hilbert action turns out to be a special case of the Horndeski action and the equations of motion for the scalar field that it describes are all up to second order only in derivatives, implying stability.
arXiv commentaccepted for publication in Jordan Journal of Physics, 10 pages, one figure, revisions: fixed typographical errors in some equations, updated one reference
References in corpus (9)
- The Relation between Physical and Gravitational Geometry
- Degenerate higher order scalar-tensor theories beyond Horndeski and disformal transformations
- Disformal invariance of second order tensor-scalar theories: framing the Horndeski action
- A stratified framework for scalar-tensor theories of Modified Dynamics
- Disformal transformation of cosmological perturbations
- The Conformal Transformation in General Single Field Inflation with Non-Minimal Coupling
- Disformal invariance of Maxwell's field equations
- Transformation of Primordial Cosmological Perturbations Under the General Extended Disformal Transformation
- Adiabatic regularization of power spectrum in nonminimally coupled general single-field inflation