Solar constraints on new couplings between electromagnetism and gravity
S.K. Solanki (1), O.Preuss (1), M.P. Haugan (2), A. Gandorfer (1,3),, H. P. Povel (3), P. Steiner (3), K. Stucki (3), P. N. Bernasconi (4), D., Soltau (5), ((1) Max-Planck-Institut fuer Aeronomie, Katlenburg-Lindau,, Germany; (2) Purdue University

TL;DR
This paper investigates how nonminimal couplings between electromagnetism and gravity, specifically torsion in a metric-affine gauge theory, can be constrained using solar spectropolarimetric observations, setting new limits on the coupling constant.
Contribution
It introduces constraints on nonminimal electromagnetic-gravity couplings in a metric-affine gravity theory using solar polarization data.
Findings
Strong constraints on the coupling constant k: k^2 < (2.5 km)^2
Polarization phase differences can be used to test gravity theories
Solar observations provide competitive bounds on new couplings
Abstract
The unification of quantum field theory and general relativity is a fundamental goal of modern physics. In many cases, theoretical efforts to achieve this goal introduce auxiliary gravitational fields, ones in addition to the familiar symmetric second-rank tensor potential of general relativity, and lead to nonmetric theories because of direct couplings between these auxiliary fields and matter. Here, we consider an example of a metric-affine gauge theory of gravity in which torsion couples nonminimally to the electromagnetic field. This coupling causes a phase difference to accumulate between different polarization states of light as they propagate through the metric-affine gravitational field. Solar spectropolarimetric observations are reported and used to set strong constraints on the relevant coupling constant k: k^2 < (2.5 km)^2.
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