Abstract
We take a quick look at the different possible universally coupled scalar fields in nature. Then, we discuss how the gauging of the group of scale transformations (dilations), together with the Poincaré group, leads to a Weyl-Cartan spacetime structure. There the dilaton field finds a natural surrounding. Moreover, we describe shortly the phenomenology of the hypothetical axion field. In the second part of our essay, we consider a spacetime, the structure of which is exclusively specified by the premetric Maxwell equations and a fourth rank electromagnetic response tensor density \(\chi ^{ijkl}= -\chi ^{jikl}= -\chi ^{ijlk}\) with 36 independent components. This tensor density incorporates the permittivities, permeabilities, and the magneto-electric moduli of spacetime. No metric, no connection, no further property is prescribed. If we forbid birefringence (double-refraction) in this model of spacetime, we eventually end up with the fields of an axion, a dilaton, and the 10 components of a metric tensor with Lorentz signature. If the dilaton becomes a constant (the vacuum admittance) and the axion field vanishes, we recover the Riemannian spacetime of general relativity theory. Thus, the metric is encapsulated in \(\chi ^{ijkl}\), it can be derived from it.
Universally coupled, thus gravitational, scalar fields are still active players in contemporary theoretical physics. So, what is the relationship between the scalar of scalar-tensor theories, the dilaton and the inflaton? Clearly this is an unanswered and important question. The scalar field is still alive and active, if not always well, in current gravity research.
Carl H. Brans (1997)
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Notes
- 1.
Carl Brans is one of the pioneers of the scalar-tensor theory of gravitation. This essay is dedicated to Carl on the occasion of his 80th birthday with all best wishes to him and his family. During the year of 1998, we had the privilege to host Carl, as an Alexander von Humboldt awardee, for several months at the University of Cologne. I remember with pleasure the many lively discussions we had on scalars, on structures of spacetime, on physics in general, and on various other topics.
- 2.
We skip here the plethora of scalar mesons,
$$\begin{aligned}&{\pi ^\pm ,\pi ^0,\eta ,f_0(500), \eta ' (958),f_0(980),a_0(980),...,} \\&K^\pm ,K^0,K^0_{S}, K^0_{L},K^*_0(1430), {D^\pm ,D^0,D^*_0 (2400)^0,D^\pm _s,...\,;} \end{aligned}$$they are all composed of two quarks. Thus, the scalar mesons do not belong to the fundamental particles.
- 3.
Schuller et al. [90] took the \(\chi ^{ijkl}\)-tensor density, which arises so naturally in electrodynamics, called the tensor proportional to it “area metric”, and generalized it to n dimensions and to string theory. For reconstructing a volume element, they have, depending on the circumstances, two different recipes, like, for example, taking the sixth root of a determinant. From the point of view of 4-dimensional electrodynamics, the procedure of Schuller et al. looks contrived to us.
- 4.
See [28, Sect. 28-8].
- 5.
See [35, Sect. E.2.2].
- 6.
See [35, Sect. E.2.3].
- 7.
See [35, Sect. E.2.4].
- 8.
See [35, Sect. E.2.5].
- 9.
Here, in this context, \(\alpha \) is not the axion field!.
- 10.
In the early 1980s, Ni [69] has shown the following: Suppressing the birefringence is a necessary and sufficient condition for a Lagrangian based constitutive tensor to be decomposable into metric+dilaton+axion in a weak gravitational field (weak violation of the Einstein equivalence principle), a remarkable result. Note that Ni assumed the existence of a metric. We, in (4.23), derived the metric from the electromagnetic response tensor density \(\chi ^{ijkl}\).
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Acknowledgments
This project was partly supported by the German-Israeli Research Foundation (GIF) by the grant GIF/No. 1078-107.14/2009. I am grateful to Claus Kiefer (Cologne) for helpful remarks re Higgs cosmology, to Yuri Obukhov (Moscow) re questions of torsion and of the Hadamard method, to Helmut Rumpf (Vienna) re the Mukhanov bound of \(10^{-29}\,\mathrm{{m}}\), and to Volker Perlick (Bremen) re gravity versus electromagnetism and what is more fundamental. I would like to thank Ari Sihvola and Ismo Lindell (both Espoo/Helsinki) and Alberto Favaro (London) for the permission to use the image in Fig.2. Many useful comments on a draft of this paper were supplied by Hubert Goenner (Göttingen), Yakov Itin (Jerusalem), Claus Lämmerzahl (Bremen), Ecardo Mielke (Mexico City), Wei-Tou Ni (Hsinchu), Erhard Scholz (Wuppertal), Frederic Schuller (Erlangen), and Dirk Puetzfeld (Bremen). I am grateful to Alan Kostelecký (Bloomington) for a last-minute exchange of emails.
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Hehl, F.W. (2016). Axion and Dilaton + Metric Emerge Jointly from an Electromagnetic Model Universe with Local and Linear Response Behavior. In: Asselmeyer-Maluga, T. (eds) At the Frontier of Spacetime. Fundamental Theories of Physics, vol 183. Springer, Cham. https://doi.org/10.1007/978-3-319-31299-6_4
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