In mathematical physics, spacetime algebra (STA) is the application of Clifford algebra Cl1,3(R), or equivalently the geometric algebra G(M4) to physics. Spacetime algebra provides a "unified, coordinate-free formulation for all of relativistic physics, including the Dirac equation, Maxwell equation and General Relativity" and "reduces the mathematical divide between classical, quantum and relativistic physics."[1]: ix 

Spacetime algebra is a vector space that allows not only vectors, but also bivectors (directed quantities describing rotations associated with rotations or particular planes, such as areas, or rotations) or blades (quantities associated with particular hyper-volumes) to be combined, as well as rotated, reflected, or Lorentz boosted.[2]: 40, 43, 97, 113  It is also the natural parent algebra of spinors in special relativity.[2]: 333  These properties allow many of the most important equations in physics to be expressed in particularly simple forms, and can be very helpful towards a more geometric understanding of their meanings.[1]: v 

In comparison to related methods, STA and Dirac algebra are both Clifford Cl1,3 algebras, but STA uses real number scalars while Dirac algebra uses complex number scalars. The STA spacetime split is similar to the algebra of physical space (APS, Pauli algebra) approach. APS represents spacetime as a paravector, a combined 3-dimensional vector space and a 1-dimensional scalar.[3]: 225–266 

Structure

edit

For any pair of STA vectors,  , there is a vector (geometric) product  , inner (dot) product   and outer (exterior, wedge) product  . The vector product is a sum of an inner and outer product:[1]: 6 

 

The inner product generates a real number (scalar), and the outer product generates a bivector. The vectors   and   are orthogonal if their inner product is zero; vectors   and   are parallel if their outer product is zero.[2]: 22–23 

The orthonormal basis vectors are a timelike vector   and 3 spacelike vectors  . The Minkowski metric tensor's nonzero terms are the diagonal terms,  . For  :

 

The Dirac matrices share these properties, and STA is equivalent to the algebra generated by the Dirac matrices over the field of real numbers;[1]: x  explicit matrix representation is unnecessary for STA.

Products of the basis vectors generate a tensor basis containing one scalar  , four vectors  , six bivectors  , four pseudovectors (trivectors)   and one pseudoscalar   with  .[1]: 11  The pseudoscalar commutes with all even-grade STA elements, but anticommutes with all odd-grade STA elements.[4]: 6 

Subalgebra

edit
 
This is an illustration of space-time algebra spinors in Cl+(1,3) under the octonionic product as a Fano plane
 
The associated octonion multiplication tables in en and STA form.

STA's even-graded elements (scalars, bivectors, pseudoscalar) form a Clifford Cl3,0(R) even subalgebra equivalent to the APS or Pauli algebra.[1]: 12  The STA bivectors are equivalent to the APS vectors and pseudovectors. The STA subalgebra becomes more explicit by renaming the STA bivectors   as   and the STA bivectors   as  .[1]: 22 [2]: 37  The Pauli matrices,  , are a matrix representation for  .[2]: 37  For any pair of  , the nonzero inner products are  , and the nonzero outer products are:[2]: 37 [1]: 16 

 

The sequence of algebra to even subalgebra continues as algebra of physical space, quaternion algebra, complex numbers and real numbers. The even STA subalgebra Cl+(1,3) of real space-time spinors in Cl(1,3) is isomorphic to the Clifford geometric algebra Cl(3,0) of Euclidean space R3 with basis elements. See the illustration of space-time algebra spinors in Cl+(1,3) under the octonionic product as a Fano plane. [5]

Division

edit

A nonzero vector   is a null vector (degree 2 nilpotent) if  .[6]: 2  An example is  . Null vectors are tangent to the light cone (null cone).[6]: 4  An element   is an idempotent if  .[7]: 103  Two idempotents   and   are orthogonal idempotents if  .[7]: 103  An example of an orthogonal idempotent pair is   and   with   . Proper zero divisors are nonzero elements whose product is zero such as null vectors or orthogonal idempotents.[8]: 191  A division algebra is an algebra that contains multiplicative inverse (reciprocal) elements for every element, but this occurs if there are no proper zero divisors and if the only idempotent is 1.[7]: 103 [9]: 211  [a] The only associative division algebras are the real numbers, complex numbers and quaternions.[10]: 366  As STA is not a division algebra, some STA elements may lack an inverse; however, division by the non-null vector   may be possible by multiplication by its inverse, defined as  .[11]: 14 

Reciprocal frame

edit

Associated with the orthogonal basis   is the reciprocal basis set   satisfying these equations: [1]: 63 

 

These reciprocal frame vectors differ only by a sign, with  , but  .

A vector   may be represented using either the basis vectors or the reciprocal basis vectors   with summation over  , according to the Einstein notation. The inner product of vector and basis vectors or reciprocal basis vectors generates the vector components.

 

The metric and index gymnastics raise or lower indices:

 

Spacetime gradient

edit

The spacetime gradient, like the gradient in a Euclidean space, is defined such that the directional derivative relationship is satisfied:[12]: 45 

 

This requires the definition of the gradient to be

 

Written out explicitly with  , these partials are

 

Spacetime split

edit
Spacetime split – examples:
 
 [13]: 257 
 [13]: 257 
where   is the Lorentz factor
 [13]: 259 

In STA, a spacetime split is a projection from four-dimensional space into (3+1)-dimensional space in a chosen reference frame by means of the following two operations:

  • a collapse of the chosen time axis, yielding a 3-dimensional space spanned by bivectors, equivalent to the standard 3-dimensional basis vectors in the algebra of physical space and
  • a projection of the 4D space onto the chosen time axis, yielding a 1-dimensional space of scalars, representing the scalar time.[14]: 180 

This is achieved by pre-multiplication or post-multiplication by a timelike basis vector  , which serves to split a four vector into a scalar timelike and a bivector spacelike component, in the reference frame co-moving with  . With   we have

 

Spacetime split is a method for representing an even-graded vector of spacetime as a vector in the Pauli algebra, an algebra where time is a scalar separated from vectors that occur in 3 dimensional space. The method replaces these spacetime vectors  [1]: 22–24 

As these bivectors   square to unity, they serve as a spatial basis. Utilizing the Pauli matrix notation, these are written  . Spatial vectors in STA are denoted in boldface; then with   and  , the  -spacetime split  , and its reverse   are:

 

However, the above formulas only work in the Minkowski metric with signature (+ - - -). For forms of the spacetime split that work in either signature, alternate definitions in which   and   must be used.

Transformations

edit

To rotate a vector   in geometric algebra, the following formula is used:[15]: 50–51 

 ,

where   is the angle to rotate by, and   is the normalized bivector representing the plane of rotation so that  .

For a given spacelike bivector,  , so Euler's formula applies,[2]: 401  giving the rotation

 .

For a given timelike bivector,  , so a "rotation through time" uses the analogous equation for the split-complex numbers:

 .

Interpreting this equation, these rotations along the time direction are simply hyperbolic rotations. These are equivalent to Lorentz boosts in special relativity.

Both of these transformations are known as Lorentz transformations, and the combined set of all of them is the Lorentz group. To transform an object in STA from any basis (corresponding to a reference frame) to another, one or more of these transformations must be used.[1]: 47–62 

Any spacetime element   is transformed by multiplication with the pseudoscalar to form its dual element  .[12]: 114  Duality rotation transforms spacetime element   to element   through angle   with pseudoscalar   is:[1]: 13 

 

Duality rotation occurs only for non-singular Clifford algebra, non-singular meaning a Clifford algebra containing pseudoscalars with a non-zero square.[1]: 13 

Grade involution (main involution, inversion) transforms every r-vector   to  :[1]: 13 [16]

 

Reversion transformation occurs by decomposing any spacetime element as a sum of products of vectors and then reversing the order of each product.[1]: 13 [17] For multivector   arising from a product of vectors,   the reversion is  :

 

Clifford conjugation of a spacetime element   combines reversion and grade involution transformations, indicated as  :[18]

 

The grade involution, reversion and Clifford conjugation transformations are involutions.[19]

Classical electromagnetism

edit

The Faraday bivector

edit

In STA, the electric field and magnetic field can be unified into a single bivector field, known as the Faraday bivector, equivalent to the Faraday tensor.[2]: 230  It is defined as:

 

where   and   are the usual electric and magnetic fields, and   is the STA pseudoscalar.[2]: 230  Alternatively, expanding   in terms of components,   is defined that

 

The separate   and   fields are recovered from   using

 

The   term represents a given reference frame, and as such, using different reference frames will result in apparently different relative fields, exactly as in standard special relativity.[2]: 233 

Since the Faraday bivector is a relativistic invariant, further information can be found in its square, giving two new Lorentz-invariant quantities, one scalar, and one pseudoscalar:

 

The scalar part corresponds to the Lagrangian density for the electromagnetic field, and the pseudoscalar part is a less-often seen Lorentz invariant.[2]: 234 

Maxwell's equation

edit

STA formulates Maxwell's equations in a simpler form as one equation,[20]: 230  rather than the 4 equations of vector calculus.[21]: 2–3  Similarly to the above field bivector, the electric charge density and current density can be unified into a single spacetime vector, equivalent to a four-vector. As such, the spacetime current   is given by[22]: 26 

 

where the components   are the components of the classical 3-dimensional current density. When combining these quantities in this way, it makes it particularly clear that the classical charge density is nothing more than a current travelling in the timelike direction given by  .

Combining the electromagnetic field and current density together with the spacetime gradient as defined earlier, we can combine all four of Maxwell's equations into a single equation in STA. [20]: 230 

Maxwell's equation:

 

The fact that these quantities are all covariant objects in the STA automatically guarantees Lorentz covariance of the equation, which is much easier to show than when separated into four separate equations.

In this form, it is also much simpler to prove certain properties of Maxwell's equations, such as the conservation of charge. Using the fact that for any bivector field, the divergence of its spacetime gradient is  , one can perform the following manipulation:[23]: 231 

 

This equation has the clear meaning that the divergence of the current density is zero, i.e. the total charge and current density over time is conserved.

Using the electromagnetic field, the form of the Lorentz force on a charged particle can also be considerably simplified using STA.[24]: 156 

Lorentz force on a charged particle:

 

Potential formulation

edit

In the standard vector calculus formulation, two potential functions are used: the electric scalar potential, and the magnetic vector potential. Using the tools of STA, these two objects are combined into a single vector field  , analogous to the electromagnetic four-potential in tensor calculus. In STA, it is defined as

 

where   is the scalar potential, and   are the components of the magnetic potential. As defined, this field has SI units of webers per meter (V⋅s⋅m−1).

The electromagnetic field can also be expressed in terms of this potential field, using

 

However, this definition is not unique. For any twice-differentiable scalar function  , the potential given by

 

will also give the same   as the original, due to the fact that

 

This phenomenon is called gauge freedom. The process of choosing a suitable function   to make a given problem simplest is known as gauge fixing. However, in relativistic electrodynamics, the Lorenz condition is often imposed, where  .[2]: 231 

To reformulate the STA Maxwell equation in terms of the potential  ,   is first replaced with the above definition.

 

Substituting in this result, one arrives at the potential formulation of electromagnetism in STA:[2]: 232 

Potential equation:

 

Lagrangian formulation

edit

Analogously to the tensor calculus formalism, the potential formulation in STA naturally leads to an appropriate Lagrangian density.[2]: 453 

Electromagnetic Lagrangian density:

 

The multivector-valued Euler-Lagrange equations for the field can be derived, and being loose with the mathematical rigor of taking the partial derivative with respect to something that is not a scalar, the relevant equations become:[25]: 440 

 

To begin to re-derive the potential equation from this form, it is simplest to work in the Lorenz gauge, setting[2]: 232 

 

This process can be done regardless of the chosen gauge, but this makes the resulting process considerably clearer. Due to the structure of the geometric product, using this condition results in  .

After substituting in  , the same equation of motion as above for the potential field   is easily obtained.

The Pauli equation

edit

STA allows the description of the Pauli particle in terms of a real theory in place of a matrix theory. The matrix theory description of the Pauli particle is:[26]

 

where   is a spinor,   is the imaginary unit with no geometric interpretation,   are the Pauli matrices (with the 'hat' notation indicating that   is a matrix operator and not an element in the geometric algebra), and   is the Schrödinger Hamiltonian.

The STA approach transforms the matrix spinor representation   to the STA representation   using elements,  , of the even-graded spacetime subalgebra and the pseudoscalar  :[2]: 37 [27]: 270, 271 

 

The Pauli particle is described by the real Pauli–Schrödinger equation:[26]

 

where now   is an even multi-vector of the geometric algebra, and the Schrödinger Hamiltonian is  . Hestenes refers to this as the real Pauli–Schrödinger theory to emphasize that this theory reduces to the Schrödinger theory if the term that includes the magnetic field is dropped.[26]: 30  The vector   is an arbitrarily selected fixed vector; a fixed rotation can generate any alternative selected fixed vector  .[28]: 30 

The Dirac equation

edit

STA enables a description of the Dirac particle in terms of a real theory in place of a matrix theory. The matrix theory description of the Dirac particle is:[29]

 

where   are the Dirac matrices and   is the imaginary unit with no geometric interpretation.

Using the same approach as for Pauli equation, the STA approach transforms the matrix upper spinor   and matrix lower spinor   of the matrix Dirac bispinor   to the corresponding geometric algebra spinor representations   and  . These are then combined to represent the full geometric algebra Dirac bispinor  .[30]: 279 

 

Following Hestenes' derivation, the Dirac particle is described by the equation:[29][31]: 283 

Dirac equation in STA:

 

Here,   is the spinor field,   and   are elements of the geometric algebra,   is the electromagnetic four-potential, and   is the spacetime vector derivative.

Dirac spinors

edit

A relativistic Dirac spinor   can be expressed as:[32][33][34]: 280 

 

where, according to its derivation by David Hestenes,   is an even multivector-valued function on spacetime,   is a unimodular spinor or "rotor",[35] and   and   are scalar-valued functions.[32] In this construction, the components of   directly correspond with the components of a Dirac spinor, both having 8 scalar degrees of freedom.

This equation is interpreted as connecting spin with the imaginary pseudoscalar.[36]: 104–121 

The rotor,  , Lorentz transforms the frame of vectors   into another frame of vectors   by the operation  ;[37]: 15  note that   indicates the reverse transformation.

This has been extended to provide a framework for locally varying vector- and scalar-valued observables and support for the Zitterbewegung interpretation of quantum mechanics originally proposed by Schrödinger.[38][1]: vi 

Hestenes has compared his expression for   with Feynman's expression for it in the path integral formulation:

 

where   is the classical action along the  -path.[32]

Using the spinors, the current density from the field can be expressed by[39]: 8 

 

Symmetries

edit

Global phase symmetry is a constant global phase shift of the wave function that leaves the Dirac equation unchanged.[40]: 41–48  Local phase symmetry is a spatially varying phase shift that leaves the Dirac equation unchanged if accompanied by a gauge transformation of the electromagnetic four-potential as expressed by these combined substitutions.[41]: 269, 283 

 

In these equations, the local phase transformation is a phase shift   at spacetime location   with pseudovector   and   of even-graded spacetime subalgebra applied to wave function  ; the gauge transformation is a subtraction of the gradient of the phase shift   from the electromagnetic four-potential   with particle electric charge  .[41]: 269, 283 

Researchers have applied STA and related Clifford algebra approaches to gauge theories, electroweak interaction, Yang–Mills theory, and the standard model.[42]: 1345–1347 

The discrete symmetries are parity  , charge conjugation   and time reversal   applied to wave function  . These effects are:[43]: 283 

 

General relativity

edit

General relativity

edit

Researchers have applied STA and related Clifford algebra approaches to relativity, gravity and cosmology.[42]: 1343  The gauge theory gravity (GTG) uses STA to describe an induced curvature on Minkowski space while admitting a gauge symmetry under "arbitrary smooth remapping of events onto spacetime" leading to this geodesic equation.[44][45][4][13]

 

and the covariant derivative

 

where   is the connection associated with the gravitational potential, and   is an external interaction such as an electromagnetic field.

The theory shows some promise for the treatment of black holes, as its form of the Schwarzschild solution does not break down at singularities; most of the results of general relativity have been mathematically reproduced, and the relativistic formulation of classical electrodynamics has been extended to quantum mechanics and the Dirac equation.

See also

edit

Notes

edit
  1. ^ An example: given idempotent  , define  , then  ,  , and  . Find the inverse   satisfying  . Thus,  . However, there is no   satisfying  , so this idempotent has no inverse.

Citations

edit
  1. ^ a b c d e f g h i j k l m n o p Hestenes 2015.
  2. ^ a b c d e f g h i j k l m n o p Doran & Lasenby 2003.
  3. ^ Baylis 2012.
  4. ^ a b Lasenby, Doran & Gull 1995.
  5. ^ Lasenby 2022.
  6. ^ a b O'Donnell 2003.
  7. ^ a b c Vaz & da Rocha 2016.
  8. ^ Warner 1990, Theorems 21.2, 21.3.
  9. ^ Warner 1990.
  10. ^ Palais 1968.
  11. ^ Hestenes & Sobczyk 1984.
  12. ^ a b Hestenes & Sobczyk 2012c.
  13. ^ a b c d Lasenby & Doran 2002.
  14. ^ Arthur 2011.
  15. ^ Hestenes 2015, Eqs. (16.22),(16.23).
  16. ^ Floerchinger 2021, Eq. (18).
  17. ^ Floerchinger 2021, Eq. (25).
  18. ^ Floerchinger 2021, Eq. (27).
  19. ^ Floerchinger 2021.
  20. ^ a b Doran & Lasenby 2003, Eq. (7.14).
  21. ^ Jackson 1998.
  22. ^ Hestenes 2015, Eq. (8.4).
  23. ^ Doran & Lasenby 2003, Eq. (7.16).
  24. ^ Doran & Lasenby 2003, Eq. (5.170).
  25. ^ Doran & Lasenby 2003, Eq. (12.3).
  26. ^ a b c Hestenes 2003a, Eqs. (75),(81).
  27. ^ Doran & Lasenby 2003, Eqs. (8.16),(8.20),(8.23).
  28. ^ Hestenes 2003a, Eqs. (82),(83),(84).
  29. ^ a b Doran et al. 1996, Eqs. (3.43),(3.44).
  30. ^ Doran & Lasenby 2003, Eq. (8.69).
  31. ^ Doran & Lasenby 2003, Eq. (8.89).
  32. ^ a b c Hestenes 2012b, Eqs. (3.1),(4.1),pp 169-182.
  33. ^ Gull, Lasenby & Doran 1993, Eq. (5.13).
  34. ^ Doran & Lasenby 2003, Eq. (8.80).
  35. ^ Hestenes 2003b, Eq. (205).
  36. ^ Hestenes 2003a.
  37. ^ Hestenes 2003b, Eq. (79).
  38. ^ Hestenes 2010.
  39. ^ Hestenes 1967, Eq. (4.5).
  40. ^ Quigg 2021.
  41. ^ a b Doran & Lasenby 2003, Eqs. (8.8),(8.9),(8.10),(8.92),(8.93).
  42. ^ a b Hitzer, Lavor & Hildenbrand 2024.
  43. ^ Doran & Lasenby 2003, Eq. (8.90).
  44. ^ Doran, Lasenby & Gull 1993.
  45. ^ Lasenby, Doran & Gull 1998.

References

edit
edit