Dynamical trapping and relaxation of scalar gravitational fields
C. H.-T. Wang, A. O. Hodson, A. St J. Murphy, T. B. Davies, J. T., Mendonca, R. Bingham

TL;DR
This paper introduces a new scalar-tensor gravity model that dynamically traps and relaxes scalar fields during high-energy events, offering an alternative inflation mechanism and potential observable effects in supernovae.
Contribution
It proposes a novel dynamical trapping and relaxation framework for scalar gravity, addressing inflation and supernova phenomena in a unified way.
Findings
Provides a viable inflation alternative free from previous issues
Suggests observable gravitational energy release in supernovae
Links the model to potential experimental tests at CERN
Abstract
We present a framework for nonlinearly coupled scalar-tensor theory of gravity to address both inflation and core-collapse supernova problems. The unified approach is based on a novel dynamical trapping and relaxation of scalar gravity in highly energetic regimes. The new model provides a viable alternative mechanism of inflation free from various issues known to affect previous proposals. Furthermore, it could be related to observable violent astronomical events, specifically by releasing a significant amount of additional gravitational energy during core-collapse supernovae. A recent experiment at CERN relevant for testing this new model is briefly outlined.
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