Abstract
This paper presents an exterior-algebra generalization of electromagnetic fields and source currents as multivectors of grades r and \(r-1\), respectively, in a flat space-time with n space and k time dimensions. Formulas for the Maxwell equations and the Lorentz force for arbitrary values of r, n, and k are postulated in terms of interior and exterior derivatives, in a form that closely resembles their vector-calculus analogues. These formulas lead to solutions in terms of potentials of grade \(r-1\), and to conservation laws in terms of a stress–energy–momentum tensor of rank 2 for any values of r, n, and k, for which a simple explicit formula is given. As an application, an expression for the flux of the stress–energy–momentum tensor across an \((n+k-1)\)-dimensional slice of space-time is given in terms of the Fourier transform of the potentials. The abstraction of Maxwell equations with exterior calculus combines the simplicity and intuitiveness of vector calculus, as the formulas admit explicit expressions, with the power of tensors and differential forms, as the formulas can be given for any values of r, n, and k.
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Acknowledgements
This work has been funded in part by the Spanish Ministry of Science, Innovation and Universities under Grants TEC2016-78434-C3-1-R and BES-2017-081360.
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Appendix A: Proofs related to the stress–energy–momentum tensor
Appendix A: Proofs related to the stress–energy–momentum tensor
1.1 Appendix A.1: Distributive properties of the interior product
Proof of (22)
To prove this equation, we first expand the vectors and multivectors in the left-hand side of (22) in terms of their components to get
At this point, we separate the cases \(i=j\) and \(i\ne j\), namely
and it is easy to note that the first term can be written as
Regarding the second term, we first prove the equality
which we can be rewritten in the form
In fact, with the visual help of Fig. 1 it is easy to see how the sign of the permutation on the left-hand side of (A.6) is the same as that on the right-hand side. Then, the second term of the expression (A.3) can be written
\(\square \)
Proof of (24)
To prove this identity, we write separately the explicit expressions of the left and the right side of (24). On the left side, we get
while on the right side we result is
For the expressions (A.8) and (A.10) to be identical, it is sufficient that
is satisfied. With the aid of Fig. 2, we notice that both sides represent the signature of two possible permutations reordering the list \((b,I{\setminus } a{\setminus } b, a)\) into I. This proves (24). \(\square \)
Proof of (27)
We prove this relation by first writing separately the three terms of the equation. On the left-hand side, we get
The central term is
Thus, it is easy to check that \(\varDelta _{i+I,J}=\varDelta _ {ii}\varDelta _ {J\setminus i,I}\), so that the first two terms of (27) coincide. Regarding the third term on the left hand side, we obtain
which corresponds to the first two expressions since \(\varDelta _{i, J\setminus I}\varDelta _ {II} = \varDelta _{i+I,J}=\varDelta _ {ii}\varDelta _ {J\setminus i,I}\). \(\square \)
Finally, it is easy to check that \(\varDelta _{i+I,J}=\varDelta _ {ii}\varDelta _ {J{\setminus } i,I}\), so that (27) is proved. \(\square \)
1.2 Appendix A.2: Interior derivative of the tensor
For the sake of compactness, we define the bitensors \({\mathbf {T}}_\odot = \mathbf{F} \odot \mathbf{F} \) and to prove the following identities
Using equations (13), (14), (16) and (17), we write \({\mathbf {T}}_\odot \) and explicitly in terms of components. That is, we obtain
and
We start by computing the interior derivative given by
After some mathematical manipulations, Eq. (A.25) is expanded as
Since \(\varDelta _{I{\setminus } i, J{\setminus } j}\) is nonzero only if \(J{\setminus } j = I{\setminus } i\), we can use this condition in the relation \(\sigma (j,J{\setminus } j) = \sigma (j, I{\setminus } i) = \sigma (I{\setminus } i, j) (-1)^{r-1} \) such that (A.26) becomes
Exchanging the indices i and j and the labels I and J, we get the following simplified expression
A similar reasoning can be followed for the operation given by
The former equation can be expanded as
and after a few manipulations using the properties of the signatures as done to obtain (A.27), from (A.30) we have
Simplifying terms, we obtain
We next derive explicit forms for the operations and . We start by noting that can be expanded in terms of component as
As a consequence, we have that
Noting that \(A {\setminus } (B{\setminus } j)\) is a single element i such that \(A{\setminus } i = B{\setminus } j\), we finally get
Since (A.37) corresponds exactly to (A.28), we proved (A.19).
Similarly, we next write the operation and write it out in terms of components, i.e.,
Again noting that \(j+B{\setminus } A = i\) and that \(A+i = B+j\), from (A.39) we obtain
proving the equivalence with (A.32) and therefore proving (A.20).
Combining (A.19) and (A.20) and defining the stress–energy–momentum tensor \({\mathbf {T}}\) of the Maxwell field \(\mathbf{F} \) as , we find that the interior derivative of the tensor \({\mathbf {T}}\) satisfies the following formula
Therefore, from the Maxwell equations, i.e., \(\varvec{\partial }\wedge \mathbf{F} = 0\) and , we recover the conservation law for energy–momentum relating the Lorentz force \({{\mathbf {f}}}\) (64) and the stress–energy–momentum tensor,
1.3 Appendix A.3: Explicit formulas for the tensor components for generic r
Starting with (69), we note that
for any pair of i and j, and therefore,
where we have defined the set L such that \(I{\setminus } i = J{\setminus } j = L\). The summation contains \(\smash {\left( {\begin{array}{c}k+n-2\\ r-1\end{array}}\right) }\) nonzero terms. For \(i = j\), and using that \(\sigma (L,i)\sigma (i,L) = (-1)^{r-1}\), it can be evaluated as
Moving on to (70), we note that
and we study the cases such that the lists \(i+I\) and \(j+J\) coincide. First, if \(i = j\), we have to sum over \(I = J\) such that \(i \notin I\), i.e.,
because \(\sigma (i,I)\sigma (I,i) = (-1)^r\). Second, if \(i\ne j\), we can find an \(L \in {\mathcal {I}}_{r-1}\) such that \(L = I{\setminus } j = J {\setminus } i\) and \(i,j\ne L\). Then,
The product \(\sigma (i,L+j)\sigma (L+i,j)\) is equal to \(\sigma (L,i)\sigma (j,L)\). To prove it, we write the relation \(\sigma (i,L+j)\sigma (L+i,j) = \sigma (L,i)\sigma (j,L)\) and we first multiply both sides by \(\sigma (L+i,j)\sigma (j,L)\) to obtain \(\sigma (i,L+j)\sigma (j,L) = \sigma (L+i,j)\sigma (L,i)\), namely the permutations sorting the lists (i, j, L) and (L, i, j), respectively. Secondly, we note that \(\sigma (i,j,L) = (-1)^{2(r-1)}\sigma (L,i,j) = \sigma (L,i,j)\).
Combining (A.46) and (A.53) into , we have
1.4 Appendix A.4: Stokes theorem for the interior derivative of a bitensor
Considering a bitensor field
then the Stokes theorem we wish to prove states that
The proof will follow the reasoning operating for the vector field [11, Sect. 3.5], so we start expanding the integrand on the right-hand side
The last term can be rewritten by changing the indices \(i\longleftrightarrow j\) and using the property of symmetry \(T_{ji}=T_{ij}\) as
and finally, the three terms can be compacted in
Then, taking the exterior derivative [14, Sect. 36.B], we get
On the other hand, regarding the right-hand side, we first evaluate
and the differential
Then, we get
namely (A.63) and thereby proving the stated Stokes’ Theorem.
1.5 Appendix A.5: Flux of the stress–energy–momentum tensor
The flux of the field (65) across the boundary \(\partial {\mathcal {V}}_\ell ^{k+n}\), denoted by \(\varPhi _{\partial {\mathcal {V}}_\ell ^{k+n}} ({\mathbf {T}})\), is given by the integral in (85),
The r.h.s. of (A.69) is computed w.r.t. \(x_{\ell ^c}\), being \(\ell ^c\) the set of indices excluding \(\ell \).
We next write the flux (A.69) in terms of the Fourier transform of \({\mathbf {F}}\), denoted as \({\hat{\mathbf{F }}} (\varvec{\xi })\) as in (51). Assuming that the Fourier transform of \({\mathbf {F}}\) is supported only in the set \(\varvec{\xi }\cdot \varvec{\xi }=0\), as postulated in (57), we express \({\mathbf {F}}\) as
Inserting (A.70) in (68) and using the linearity properties of \(\odot \) and , we obtain that the stress–energy–momentum tensor \({\mathbf {T}}\) can be written as
Using (A.71) back in (A.69), we obtain that
Since the integration w.r.t. \(x_{\ell ^c}\) only acts on the exponential term in (A.72), interchanging the integration order and using the definition of the delta function, we can find the inverse Fourier transform of the exponential as
Plugging the r.h.s. of (A.73) in (A.72) and defining \(\varphi (\varvec{\xi },\varvec{\xi }')\) as
we write the flux as
In order to solve the integration w.r.t. \(\xi _\ell \), we rewrite the condition \(\varvec{\xi }\cdot \varvec{\xi }=0\) as
where \(\varvec{\xi }_{{\bar{\ell }}} = \varvec{\xi }-\xi _\ell {\mathbf {e}}_\ell \). We can solve this equation for \(\xi _\ell \) as long as \(-\varDelta _{\ell \ell } \varvec{\xi }_{{\bar{\ell }}}\cdot \varvec{\xi }_{{\bar{\ell }}} \ge 0\), in which case we define \(\chi _\ell \) as the positive root of the equation
and we thus take for \(\xi _\ell \) the two possible values \(\xi _\ell = \pm \chi _\ell \). We similarly have the analogous versions of (A.76) and (A.77) for \(\xi _\ell '\).
Using [16, p. 184] w.r.t. the integration variables \(\xi _\ell \) and \(\xi _\ell '\) and the limitation in the integration range, Eq. (A.75) is expressed as
Since the remaining Dirac delta function conditions imply that \(\xi '_m=-\xi _m\) for every \(m\ne \ell \), we also have that \(\xi '_\ell =\pm \chi _\ell \). To further deal with the four terms in the summation in (A.78), we define the vectors
and the counterparts \(\varvec{\xi }'_+=-\varvec{\xi }_-\) and \(\varvec{\xi }'_-=-\varvec{\xi }_+\). Using these definitions to solve the integration w.r.t. \(\xi '_{\ell ^c}\), we obtain that
It remains to study the four summands in (A.81) by exploiting the properties of exterior algebra. We start by writing \(\varphi (\varvec{\xi }_+,\varvec{\xi }_+')\) from its definition in (A.74) and use the fact that \({\hat{\mathbf{F }}}(\varvec{\xi }'_+)={\hat{\mathbf{F }}}(-\varvec{\xi }_-)={\hat{\mathbf{F }}}^*(\varvec{\xi }_-)\) to obtain
where for the sake of clarity we defined the tensor \({\mathbf {T}}_1\) as
Using the definitions of \(\odot \) and in (69) and (70), respectively, and the identity (22), we may write the ijth component of \({\mathbf {T}}_1\) as
It will prove convenient to study Eq. (A.85) in terms of the \((r-1)\)-vector potential \({\mathbf {A}}\), which is related to \({\mathbf {F}}\) as in (48), or in the Fourier domain,
where \({\hat{{\mathbf {A}}}} (\varvec{\xi })\) denotes the Fourier transform of \({\mathbf {A}}\). Substituting (A.86) in the definitions of \(\alpha _{1,ij}\) and \(\beta _{1,ij}\) in (A.85) and using the identity (21), we obtain that
We start by expanding \(\alpha _{1,ij}\). Using the identity (26), we get
Computing the products, rearranging terms, and using the relations (22), (24)–(25) and (27) in various places, we obtain
We next simplify the terms of the form and . To do so, we note that \(\varvec{\xi }_+\) and \(\varvec{\xi }_-\), respectively, given in (A.79) and (A.80) are related as
Recalling that the gauge condition in the Fourier domain is given by
equations (A.91) and (A.92) imply that
Similar relations are obtained for the right interior product. Applying (A.93) and (A.94) into (A.90), we obtain for \(\alpha _{1,ij}\) that
For \(\beta _{1,ij}\), we first use (22) directly into (A.88) so that it is written as
In view of (A.91) and \(\varvec{\xi }_+ \cdot \varvec{\xi }_+ = 0\), the \(\varvec{\xi }_+\cdot \varvec{\xi }_-\) term in the previous equation equals
Therefore, using (A.93), (A.94) and (A.98) we finally obtain
Although we derived expressions of \(\alpha _{1,ij}\), \(\alpha _{1,ji}\) and \(\beta _{1,ij}\) in (A.95) and (A.99), needed to obtain \(T_{1,ij}\) in (A.85) for arbitrary ij, we are only interested in such terms containing the \(\ell \)th component, since \(\varphi (\varvec{\xi }_+,\varvec{\xi }_+')\) in (A.82) involves computing the quantity
We start with the first case in which \(i=\ell \ne j\). Using that , from (A.95) we get
Similarly, we also have
Furthermore, the fact that \(\varDelta _{ij}=0\) for \(i\ne j\) implies from (A.99) that
Combining (A.101), (A.102) and (A.103) in the initial expression of \(T_{1,\ell j}\) in (A.85), using that \(\xi _{\pm ,\ell } = \pm \chi _\ell \), and writing the right interior products as left interior products, we get
We note that the last two summands in the former equation trivially cancel out, whereas the remaining two also do so because \(\xi _{-,j}=\xi _{+,j}\) for \(j\ne \ell \). Hence,
We continue with the second case \(j=\ell \ne i\) and we have, as in the first case
and
We rearrange (A.106), (A.107) and (A.108) in the initial expression (A.85), using \(\xi _{\pm ,\ell = \pm \chi _\ell }\) and that \(\xi _{-,i}=\xi _{+,i}\) for \(i \ne \ell \), we obtain It results to be zero since for \(i \ne \ell \) we have \(\xi _{-,i}=\xi _{+,i}\), namely
Regarding the last case \(i=j=\ell \), we evaluate \(\alpha _{1,\ell \ell } \) from (A.95) writing all the right interior products as left interior products
and from (A.99)
We substitute \(\alpha _{1,\ell \ell }=\beta _{1,\ell \ell }\) from (A.110) and \(\gamma _{1,\ell \ell }\) from (A.110) into \(T_{1,\ell \ell }\) (A.85) and considering that \(\xi _{\pm _\ell } = \pm \chi _\ell \), we directly get
In conclusion, from (A.100) we realize that
We continue studying the second summand in (A.81). We consider \(\varphi (\varvec{\xi }_+,\varvec{\xi }_-')\) using its definition in (A.74) joint with the fact that \({\hat{\mathbf{F }}}(\varvec{\xi }'_-) = {\hat{\mathbf{F }}}(-\varvec{\xi }_+) ={\hat{\mathbf{F }}}^*(\varvec{\xi }_+)\) and we get
where the tensor \({\mathbf {T}}_2\) is defined as
As for \({\mathbf {T}}_1\), we use the definitions of \(\odot \) and in (69) and (70) and the identity (22) and we spread out the ijth component of \({\mathbf {T}}_2\), which is written
and we substitute the Maxwell field in terms of the potential in the Fourier domain thanks to (A.86), so that we find
We start from (A.117) and we use the relation (26) after writing . Thus, we get
Again, carrying out all the products, and applying (22) and (26), we obtain
We note that (24) implies
and we can simplify \(\alpha _{2,ij}\) thanks to the facts that \(\varvec{\xi }_+ \cdot \varvec{\xi }_+ = 0\) and to the gauge condition from (A.92), obtaining
Hence, as a consequence,
Regarding \(\beta _{2,ij}\), we write \(\varvec{\xi }_+ \wedge {\hat{{\mathbf {A}}}}^*(\varvec{\xi }_+) = (-1)^{r-1}{\hat{{\mathbf {A}}}}^*(\varvec{\xi }_+) \wedge \varvec{\xi }_+\) and we apply again (22) in (A.118) so that we immediately verify that it vanishes
As a consequence, the result for \(T_{2,ij} \) in (A.116) is
and we finally evaluate the tensor \({\mathbf {T}}_2\) as
We move on to the third term of (A.81). The equality \({\hat{\mathbf{F }}}(\varvec{\xi }'_+)={\hat{\mathbf{F }}}^*(\varvec{\xi }_-)\) allows us to write \(\varphi (\varvec{\xi }_-,\varvec{\xi }_+')\) as
where we defined the tensor \({\mathbf {T}}_3\) as follow
Comparing (A.128) and (A.115), we note that the difference is only in the presence of \(\varvec{\xi }_-\) instead of \(\varvec{\xi }_+\). Thus, the mathematical steps are identical, including that the relation \(\varvec{\xi }_+ \cdot \varvec{\xi }_+ = 0\) has its counterpart \(\varvec{\xi }_- \cdot \varvec{\xi }_- = 0\). The gauge conditions in (A.92) can also be written as
So, in analogy with the result obtained in (A.126), the final expression for \({\mathbf {T}}_3\) is
We conclude the evaluation of the initial integral in (A.81) computing \(\varphi (\varvec{\xi }_-, \varvec{\xi }_-')\). From its definition in (A.74) and using \({\hat{\mathbf{F }}}(\varvec{\xi }'_-)={\hat{\mathbf{F }}}^*(\varvec{\xi }_+)\), we get
defined, as in the previous cases,
We can further expand (A.132) in components which would appear
As in the analysis of \(T_{1,ij}\), we express \(\alpha _{4,ij}\) and \(\beta _{4,ij}\) in terms of the potential
We can now note that the differences between (A.132) and (A.83) are in \(\varvec{\xi }_+\) exchanged with \(\varvec{\xi }_-\), \({\hat{\mathbf{F }}}(\varvec{\xi }_+)\) with \({\hat{\mathbf{F }}}(\varvec{\xi }_-)\) and \({\hat{\mathbf{F }}}^*(\varvec{\xi }_-)\) with \({\hat{\mathbf{F }}}^*(\varvec{\xi }_+)\). So, the differences among (A.134) and (A.135) with respect to (A.87) and (A.88) are, in addition to the aforementioned, \({\hat{{\mathbf {A}}}}(\varvec{\xi }_+)\) interchanged with \({\hat{{\mathbf {A}}}}(\varvec{\xi }_-)\) and \({\hat{{\mathbf {A}}}}^*(\varvec{\xi }_-)\) with \({\hat{{\mathbf {A}}}}^*(\varvec{\xi }_+)\). We consider (A.91) and the gauge condition (A.129), and we replace the conditions (A.93) and (A.94) with
If we follow the same procedure applied to obtain \({\mathbf {T}}_1\) with the conditions (A.129), (A.136) and (A.137), we can rapidly state
Then, we write the integral for the flux in (A.81) substituting the definition (A.74). Removing the first and the last summands thanks to (A.113) and (A.138), it results
Using (A.126) and (A.130), we get
We consider that \(\chi _\ell ^2 = \xi _{+,\ell }^2 = \xi _{-,\ell }^2 \) and we expand the product thanks to (85) and then use that \(\sum _i \xi _{\pm ,i}{\mathbf {e}}_i = \varvec{\xi }_\pm \), so that (A.140) is
As an aside, we may use [16, p. 184] and that \(\chi _\ell = \xi _{+,\ell } = -\xi _{-,\ell }\) to undo the step leading to (A.78) to recover the Dirac delta function
Returning to (A.141), we split the integral into \(I_{\ell ,+}+I_{\ell ,-}\), where
Taking into account that \(\mathbf{A }({\mathbf {x}})\) is real, we may express the squared modulus of \({\hat{{\mathbf {A}}}}(\varvec{\xi }_-)\) as \(\bigl |{\hat{{\mathbf {A}}}}(\varvec{\xi }_-)\bigr |^2={\hat{{\mathbf {A}}}}(-\varvec{\xi }_-){\hat{{\mathbf {A}}}}^*(-\varvec{\xi }_-)\). Therefore, the integral \(I_{\ell ,-}\) becomes
Changing the integration variables according to \(\varvec{\xi }_{{\bar{\ell }}} \rightarrow \varvec{\zeta }_{{\bar{\ell }}} =-\varvec{\xi }_{{\bar{\ell }}}\), together with the definition \(\varvec{\zeta }_\pm = (\zeta _0, \ldots c,\zeta _{\ell -1},\pm \chi _\ell ,\zeta _{\ell +1}, \ldots c,\zeta _{n+k-1})\), yields
Since (A.145) is formally equivalent to \(I_{\ell ,+}\), the flux can be rewritten as
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Colombaro, I., Font-Segura, J. & Martinez, A. Generalized Maxwell equations for exterior-algebra multivectors in (k, n) space-time dimensions. Eur. Phys. J. Plus 135, 305 (2020). https://doi.org/10.1140/epjp/s13360-020-00305-y
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DOI: https://doi.org/10.1140/epjp/s13360-020-00305-y