Geometrical Unification of Gravitation and Electromagnetism
Sergio A. Hojman

TL;DR
The paper introduces GUGE, a geometrical unification theory of gravitation and electromagnetism that naturally derives Einstein-Maxwell equations without extra scalar fields, differing fundamentally from Kaluza-Klein theory.
Contribution
GUGE provides a new geometrical framework unifying gravity and electromagnetism, deriving the metric and field equations without additional assumptions or scalar fields, and explaining charge quantization and conservation.
Findings
GUGE metric is derived from proper time redefinition.
GUGE field equations are equivalent to Einstein-Maxwell equations.
GUGE predicts charge quantization and conservation.
Abstract
A theory which achieves a complete geometrical unification of gravitation and electromagnetism (GUGE) is presented. This new theory is based on a recent proposal of proper time redefinition that leads to the construction of a Riemann metric, which naturally unifies gravity and electromagnetism. The 5--dimensional Riemann metric which arises looks exactly the same as the one postulated in the Kaluza-Klein (KK) 5-dimensional theory. Nevertheless, there are deep differences between GUGE and KK. The GUGE metric is deduced while the KK metric is postulated. In the GUGE field theory there is no need to impose either of the so called "cylinder" or "curling of coordinates" conditions, because they emerge as direct consequences of the construction of the GUGE metric. The GUGE field equations are fully equivalent to Einstein--Maxwell equations, while KK field equations are not. The GUGE…
| KK | GUGE | |
|---|---|---|
| Assumption 1 | KK metric | Proper time redefinition Lagrangian |
| Assumption 2 | Cylinder condition | – – – – – – – |
| Assumption 3 | Compactification condition | – – – – – – – |
| Outcome 1 | – – – – – – – | GUGE metric |
| Outcome 2 | – – – – – – – | Cylinder condition |
| Outcome 3 | – – – – – – – | Compactification condition |
| Outcome 4 | Field equations similar to those of Einstein–Maxwell | Einstein–Maxwell field equations |
| Outcome 5 | Equations similar to those of relativistic charged particles | Relativistic charged particle equations |
| Outcome 6 | – – – – – – – | Electric charge conservation |
| Outcome 7 | Mass tower | Electric charge quantization |
| Outcome 8 | – – – – – – – | Electric charge contribution to particle’s energy |
| Outcome 9 | – – – – – – – | There are no massless charged particles |
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Geometrical Unification of Gravitation and Electromagnetism
Sergio A. Hojman
Departamento de Ciencias, Facultad de Artes Liberales, Universidad Adolfo Ibáñez, Santiago 7491169, Chile.
Centro de Investigación en Matemáticas, A.C., Unidad Mérida, Yuc. 97302, México
Departamento de Física, Facultad de Ciencias, Universidad de Chile, Santiago 7800003, Chile.
Centro de Recursos Educativos Avanzados, CREA, Santiago 7500018, Chile.
Abstract
A theory which unifies gravitation and electromagnetism (GUGE) is presented. This new theory is based on a recent redefinition of proper time. The 5–dimensional metric which arises is similar but not equivalent to the Kaluza–Klein (KK) one. Differences follow. The GUGE metric is deduced while the KK metric is postulated. In the GUGE field theory there is no need to impose either the “cylinder” or “curling of coordinates” conditions, because they are direct consequences of the GUGE formalism. The GUGE field equations are fully equivalent to Einstein–Maxwell equations, while KK field equations are not. The GUGE 5–dimensional (geodesic) equations are equivalent to the 4–dimensional (non–geodesic) equations for a charged particle moving in the presence of gravitational and electromagnetic fields, unlike the KK 5–dimensional (geodesic) equations which are not. No extra scalar field appears in GUGE. The physical interpretation of the fifth dimension and of the role of the extra field in KK (internal coordinate in GUGE) are totally different in both approaches. Finally, GUGE results include electric charge conservation, electric charge quantization and electric charge contribution to the energy of charged particles even in the absence of electromagnetic fields, which implies (the observed fact) that there are no massless electrically charged particles in Nature, unlike the prevailing treatments of KK theories.
I Introduction
Several successful examples of unification theories may be listed, starting from Newton’s unified explanation of gravitational phenomena both at human and astronomical scales, Maxwell’s unification of electric and magnetic phenomena, Glashow, Salam and Weinberg electro–weak unification and the Standard Model of elementary particles to name a few extremely well known ones.
In the case of the unification of gravitation and electromagnetism two review articles written by Goenner goenner1 ; goenner2 give a clear perspective of both the relevance of the subject and of the efforts and attempts made for over a century to construct such a theory.
The geometrical unification of gravitation and electromagnetism (GUGE) theory presented here starts from an idea related to the description of the motion of a test particle subject to gravitational, electromagnetic and Yang–Mills interactions. The idea is inspired in a recent proposal of proper time redefinition propertime which follows the path of a unified field theory described in terms of a generalized Einsten–Hilbert Lagrangian based on the construction of a Finsler metric rund . The metric so constructed turns out to be Riemannian, which is, of course a special case of a Finsler metric. The new definition of proper time gives naturally rise to the construction of a Riemann metric, which introduces all known fundamental interactions in its definition in contradistinction to the usual one which incorporates gravitational interactions only.
Metrics are usually defined in geometrical terms using the concept of “length”, as it is done in the Riemannian case. In the case in which the particle interacts with gravitational interactions only, it turns out that the “length” is exactly proportional to the action of the Lagrangian which describes the dynamics of a massive neutral point particle moving on a gravitational background. The “length” must be a homogeneous function of degree one in the coordinate differentials, which in turn means that the Lagrangian must be a homogeneous function of degree one on the velocities, in order to be able to define a reasonable metric. It turns out that the gravitational part of the Lagrangian is a homogeneous function of degree one on the velocities. Moreover, the addition to the Lagrangian of new terms which describe both electromagnetic and general Yang–Mills interactions satisfies that condition too and, in fact, these new interaction terms are linear in the velocities propertime ; bal1 ; bal2 ; casa1 ; casa2 . Nevertheless, the usual action which describes the motion of a massive, spinless, charged test particle in the presence of an external electromagnetic field is not gauge invariant and, therefore, cannot be used to define proper time. The introduction of internal particle coordinates associated to electric and Yang–Mills charges allows for the definition of a new action which gives rise to electric charge and isotopic spin magnitude conservation, in addition to the same equations of motion for the charged particle. This new action is used to redefine proper time propertime .
In order to incorporate non–gravitational interactions, additional complex coordinates (related to electromagnetic and to Yang–Mills charges) which supplement the spacetime ones are included. The Lagrangian then, is a real and electromagnetic gauge invariant function which depends both upon real (spacetime coordinates) and complex (electromagnetic and Yang–Mills) charges variables.
For a Lagrangian which is a homogeneous function of degree one in the velocities one may define a metric as one half of the second derivatives with respect to the velocities of the square of the Lagrangian which gives rise to the equations of motion of a relativistic point particle interacting with all of the fundamental interactions propertime . This metric coincides with the Riemann metric of spacetime, if the only interactions considered are the gravitational ones.
In this work, a simplification of the full Lagrangian for gravitation and electromagnetism is achieved by using two real variables instead of the two complex ones presented in propertime . For the electromagnetic case, the resulting five–dimensional Riemmannian metric, turns out to be direction independent and looks exactly equal to the usual (5 dimensional) Kaluza–Klein (KK) metric.
The differences between the KK and GUGE approaches are summarized in a Table at the end of the article.
II Geometrical Unification of Gravitation and Electromagnetism
Proper time redefinition propertime starts from the observation that the massive spinless point particle action and proper time are proportional, as it is well known, where
[TABLE]
where is the particle’s rest mass, the Riemannian spacetime metric and the action is
[TABLE]
and is an arbitrary parameter. Set and and define, as usual, the canonical momentum
[TABLE]
which is –reparametrization invariant and homogeneous of degree zero on the velocities. Note that
[TABLE]
The usual Lagrangian for a charged massive spinless point particle interacting with an external electromagnetic field described in terms of vector potential is
[TABLE]
which yields the very well known equations of motion
[TABLE]
where denotes covariant derivative with respect to .
Nevertheless, the action associated to Lagrangian (5) is not electromagnetic gauge invariant and, consequently, cannot be thought of as proportional to proper time. This difficulty was solved in propertime by replacing Lagrangian (5),
[TABLE]
where the dot over a variable denotes (ordinary) derivative with respect to . The use of complex (internal) electric charge coordinates and (or and , in what follows) for charged particles was first introduced in four articles published by Balachandran et al and Casalbuoni bal1 ; bal2 ; casa1 ; casa2 . They are the particle description equivalent of the complex functions description of charged fields.
The electric charge is conserved for the dynamics defined by Lagrangian (7) as it can be easily seen by varying it with respect to , , , and . Note that the electric charge is, in principle, a function of time , which is conserved by virtue of the dynamical equations of motion propertime .
In propertime two complex charge variables and (and their complex conjugates) were included in the Lagrangian to make sure that the conserved electric charge might assume either positive or negative (or zero) values. It is a direct matter to show that the equations of motion derived from (7) imply the correct equations (6) in addition to the conservation of electric charge , (instead of using an externally prescribed parameter ).
If one proceeds to compute and then define the metric by using , where , with for , and one gets a singular 6–dimensional Finsler metric of rank 4. This seems to be a dead end as far as the goal is constructing a unified field theory à la Einstein goenner1 ; goenner2 .
In this article I take an alternative road. Define a Lagrangian based on a unique complex charge variable (and its complex conjugate)
[TABLE]
It is a straightforward matter to realize that the (positive) electric charge is conserved by virtue of the equations of motion for and derived from (8). Note that the complex coordinates and may be rewritten as
[TABLE]
and the Lagrangian written in terms of the new internal electric charge coordinates and is
[TABLE]
The conserved charge is positive and the equations of motion need to incorporate the fact that charged particles may have either positive or negative electric charge. One way to recover the contents of equations (6) is to write two separate equations of motion for positive and negative charges, i.e.,
[TABLE]
and
[TABLE]
The electric charge conservation equation , and the particles equations of motion (11) and (12) may be derived by using the (matrix) Lagrangian
[TABLE]
which are written in terms of the Pauli matrices, by varying with respect to and .
The Pauli matrices are
\sigma_{1}=\left(\begin{array}[]{cc}0&1\\ 1&0\\ \end{array}\right),
\sigma_{2}=\left(\begin{array}[]{cc}0&-i\\ i&0\\ \end{array}\right),
and
\sigma_{3}=\left(\begin{array}[]{cc}1&0\\ 0&-1\\ \end{array}\right).
The identity matrix is
\sigma_{0}=\left(\begin{array}[]{cc}1&0\\ 0&1\\ \end{array}\right).
The dynamical variables in Lagrangians (13) are and , while plays the role of a Lagrange multiplier.
Note that the electric charge is, in principle a function of time , which is conserved by virtue of the equation of motion obtained by varying . The equations are the same as (6) (or equations (11) and (12)) except that the external parameter is replaced by the dynamically conserved electric charge .
The constraint associated to the variation of defines as a path–dependent phase much in the same sense as the ones introduced by both Mandelstam and Białynicki–Birula mandelstam ; bb ,
[TABLE]
or
[TABLE]
which shows how the coordinate is related to “Wilson lines” and “Wilson loops” wilson . Here is an integration constant. Note that no fields depend on in this approach. The particle’s Lagrangian depends only on ’s velocity, .
The usual gauge transformations for the electromagnetic potentials and the phase
[TABLE]
and
[TABLE]
for an arbitrary function , leave Lagrangians (13) invariant. Thus, these new (electromagnetic gauge invariant) Lagrangians (and associated actions) reproduce the usual dynamical equations for the coordinates and, additionally, yield electric charge conservation.
Define the Lagrangian , by
[TABLE]
and get
[TABLE]
Written in detail reads
[TABLE]
Lagrangians (13) are homogeneous functions of degree one in the velocities and and, therefore a five–dimensional metric may be defined by rund
[TABLE]
where , because no appears in the Lagrangians (13) so that . The first four velocities are the spacetime ones and . It is immediate to note that the metric , i.e., the Riemann metric does not depend on . Therefore, the (regular minor of the) Riemann metric happens to be five–dimensional and plays no dynamical role from now on.
The 5–dimensional regular Riemann metric, denoted by , is such that happens to look exactly like the Riemannian, isotropic, i.e., velocity or direction independent, Kaluza–Klein metric with
[TABLE]
where
[TABLE]
[TABLE]
[TABLE]
Note, nevertheless, that the fifth–dimension is associated to the internal electric charge phase while is not a new independent field as it is usually assumed in the prevailing treatments of Kaluza–Klein theory goenner1 ; goenner2 . As it has been seen, is the sixth (non–dynamical) internal electric charge coordinate, which is, of course, independent of all other five coordinates and . Note that is independent, i.e., the cylindrical condition is identically met in this formalism.
III 5–dimensional GUGE action
Consider now, the action for the 5–dimensional GUGE theory. It is important to realize that the dynamical variables for the action are and , which are the variables whose time derivatives and appear in Lagrangians given in (13). The 5–dimensional metric which is computed by taking derivatives of with respect to those very velocities, does not depend on , therefore it is not necessary to invoke the so called “cylinder condition”. Moreover, is a phase so its integral over spacetime is just equal to . The 5–dimensional metric turns out to be Riemannian.
The 6 coordinates , and are independent and the action constructed from gets varied with respect to the first five of them only, so no derivatives of appear in the variation of the action (because is the sixth coordinate and it is, therefore, independent of the other five coordinates and ). The 5–dimensional GUGE action (which is formally identical to the Kaluza–Klein one presented in ce and in williams ) is, using the notation of this work,
[TABLE]
[TABLE]
because there is no dependence. The action is
[TABLE]
and may be rewritten as
[TABLE]
which is exactly proportional to the Einstein–Maxwell action, after a four dimensional conformal transformation is performed (and the ′ is dropped). Note that does not depend on either or as mentioned earlier. This approach, based on previous work propertime allows one to deduce exactly the Einstein–Maxwell theory, unlike the Kaluza–Klein theory which produces equations which are not equivalent to the Einstein–Maxwell ones.
Note that no extra assumptions such as “cylinder condition” or “curling of coordinates” (“compactification”) are needed as the action does not depend on and is naturally curled, being a phase.
IV 5–dimensional GUGE geodesics
Consider the GUGE Lagrangian which defines the dynamics of a particle as the geodesics of the 5–dimensional GUGE metric given in (23), (24), and (25), after performing a four dimensional conformal transformation , dropping the ′ and dismissing the non–dynamical factor ,
[TABLE]
which also defines the new length differential which, in turn, is proportional to a newly defined (5–dimensional) proper time differential propertime .
The Lagrangian does not depend on , therefore its canonically conjugated momentum is equal to a constant of motion ,
[TABLE]
Note that the derivatives in (31) are taken with respect to the new proper time .
Compute the momentum which appears when varying with respect to ,
[TABLE]
or
[TABLE]
Finally, use Eq.(31) to get
[TABLE]
which is exactly the 4–dimensional expression for the momentum as computed by using given by (10) except that the derivative is taken with respect the new proper time and the conserved charge is now (instead of or ). Note that may be either positive or negative.
Similarly, one gets
[TABLE]
after using Eq.(31), so gives rise to the usual equations of motion (6) for a charged particle of (dynamically conserved) charge (which may be either positive or negative), instead of the external parameter . Note that the derivatives are taken with respect to .
The 5–dimensional GUGE Lagrangian produces (geodesic, in 5–dimensions) equations of motion which are completely equivalent to the usual (non–geodesic) ones for a charged particle in 4–dimensional spacetime (6).
V Further Results
Consider the simplest flat spacetime and no electromagnetic field case. The (5–)momentum constraint equation (reintroducing , for the sake of clarity) reads
[TABLE]
or
[TABLE]
which clearly shows that, even in the absence of electromagnetic fields, the electric charge contributes to the energy of a charged particle. Therefore, the rest energy of the particle (for ) does not vanish if even if vanishes, which means that there are no massless electrically charged particles, as observed.
This result may be interpreted as a redefinition of the rest mass for charged particles.
The Klein–Gordon equation associated to (36), the fact that plus the usual requirement that the wave function be single valued leads to (its canonically conjugated momentum ) charge quantization, namely, ), which is, of course, observed. This quantization happens much in the same way as the –direction angular momentum quantization for rotationally symmetric potentials in quantum mechanics. This same argument has led in the prevailing treatment of Kaluza–Klein theory to the so called “mass towers”, using ad hoc cylinder and compactification conditions for an artificially defined cyclical length–like dimensional coordinate grard .
VI Summary and Outlook
A GUGE based on a Riemann metric is presented. The Riemann metric is constructed from a newly defined Lagrangian propertime which describes the dynamics of a point massive test particle interacting with gravitation, electromagnetism and Yang–Mills fields. The new Lagrangian, which is similar to the usual one, is created by requiring that it be gauge invariant under the usual electromagnetic and Yang–Mills gauge transformations (unlike the usual one). This gauge invariance is achieved by introducing new internal complex coordinates which are associated to electromagnetic and Yang–Mills charges. This requirement is based on the condition that its action be proportional to proper time even when the non–gravitational fundamental interactions are present propertime . Its equations of motion include the usual ones and, in addition, predict electric charge conservation. The 5–dimensional GUGE metric for the case of unification of gravitational and electromagnetic interactions may be written as where looks identical to the usual 5–dimensional Kaluza–Klein metric but its different in several respects. To get the GUGE theory, one may construct the Einstein–Hilbert Lagrangian based on .
One may consider this approach as a way of getting GUGE theory metric instead of postulating it as it is done in the Kaluza–Klein approach. The GUGE theory is completely equivalent to Maxwell–Einstein theory both for the (geodesic) motion of point particles in the GUGE background metric and as a theory to describe interacting gravitational and electromagnetic fields.
In addition, there is no need to invoke either the cylinder or the curling of coordinates conditions, as they are consequences of the GUGE theory. Furthermore, no extra scalar field appears. Note that the coordinate disappears completely in the unified description of gravitation and electromagnetism. It is important to emphasize that the fifth dimension has a clear physical interpretation in this approach.
The Riemann metric in which is based, yields a redefinition of proper time whose possible implications and experimental verification are presented in propertime . Lorentz transformations in addition to translations may also be incorporated to the unification of fundamental interactions using this scheme (see, propertime ).
A comparison between GUGE and KK seems in order. one important point is that the GUGE metric is deduced from results obtained in propertime while the KK metric is postulated. In the GUGE field theory presented here, the “cylinder” and the “curling of coordinates” emerge as direct consequences of the construction of the GUGE metric instead of being postulated as it is done in the KK theory. The GUGE field equations are completely equivalent to the Einstein–Maxwell field equations, while KK field equations are not. The GUGE 5–dimensional (Riemannian geodesic) equations are fully equivalent to the 4–dimensional (non–geodesic) equations for a charged particle moving in the presence of gravitational and electromagnetic fields, unlike the KK 5–dimensional (geodesic) equations which are not and, in addition, yield non–gauge covariant geodesic equations. The Kaluza–Klein theory has an extra scalar field with no clear physical meaning while no extra scalar field appears in GUGE. Finally, the physical interpretation of the fifth dimension and of the role of the extra field in KK (internal coordinate in GUGE) are totally different in both approaches.
In addition to electric charge conservation, the GUGE approach yields electric charge quantization and electric charge contribution to the particle’s energy which means the there are no massless electrically charged particles in Nature, as it has been observed, so far.
Future research includes the study of quantum aspects of the GUGE proposal, computing the magnitude (and the feasibility of observation) of the predictions associated to the new definition of proper time, to the electric charge dependence of the particle’s energy and to the unification scheme presented here. The inclusion of Yang–Mills interactions is also the subject of ongoing work.
Acknowledgements.
It is a pleasure to thank Felipe A. Asenjo and Benjamin Koch for very many enlightening discussions. The author also wishes to express his gratitude to Matthew Dawson, Andrés Gomberoff, Francisco Rojas, Oscar Adolfo Sánchez–Valenzuela and Gianni Tallarita.
The reference list from the paper itself. Each links out to its DOI / PubMed record.
- 1(1) Hubert F.M. Goenner, Living Rev. Relativity, 7 , (2004), 2 http://www.livingreviews.org/lrr-2004-2.
- 2(2) Hubert F.M. Goenner, Living Rev. Relativity, 17 , (2014), 5, http://www.livingreviews.org/lrr-2014-5.
- 3(3) H. Rund, The Differential Geometry of Finsler Spaces (Springer Verlag, Berlin-Götingen-Heidelberg, 1959).
- 4(4) Sergio A. Hojman, Phys. Rev, D 98 , 084037 (2018).
- 5(5) A. P. Balachandran, Per Salomonson, Bo–Sture Skagerstam, and Jan–Olov Winnberg, Phys. Rev. D 15 , 2308 (1977).
- 6(6) A. P. Balachandran, S. Borchardt, and A. Stern, Phys. Rev. D 17 , 3247 (1978).
- 7(7) R. Casalbuoni, Phys. Lett. 62B , 44 (1976).
- 8(8) R. Casalbuoni, Nuovo Cimento 33A , 389 (1976).
