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Algebra of physical space

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Algebra of 4D spacetime
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Inphysics, thealgebra of physical space (APS) is the use of theClifford orgeometric algebra Cl3,0(R) of the three-dimensionalEuclidean space as a model for (3+1)-dimensionalspacetime, representing a point in spacetime via aparavector (3-dimensional vector plus a 1-dimensional scalar).

The Clifford algebra Cl3,0(R) has afaithful representation, generated byPauli matrices, on thespin representationC2; further, Cl3,0(R) is isomorphic to the even subalgebra Cl[0]
3,1
(R) of the Clifford algebra Cl3,1(R).

APS can be used to construct a compact, unified and geometrical formalism for both classical and quantum mechanics.

APS should not be confused withspacetime algebra (STA), which concerns theClifford algebra Cl1,3(R) of the four-dimensionalMinkowski spacetime.

Special relativity

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Spacetime position paravector

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In APS, thespacetime position is represented as the paravectorx=x0+x1e1+x2e2+x3e3,{\displaystyle x=x^{0}+x^{1}\mathbf {e} _{1}+x^{2}\mathbf {e} _{2}+x^{3}\mathbf {e} _{3},}where the time is given by the scalar partx0 =t, ande1,e2,e3 is abasis for position space. Throughout, units such thatc = 1 are used, callednatural units. In thePauli matrix representation, the unit basis vectors are replaced by the Pauli matrices and the scalar part by the identity matrix. This means that the Pauli matrix representation of the space-time position isx(x0+x3x1ix2x1+ix2x0x3){\displaystyle x\rightarrow {\begin{pmatrix}x^{0}+x^{3}&&x^{1}-ix^{2}\\x^{1}+ix^{2}&&x^{0}-x^{3}\end{pmatrix}}}

Lorentz transformations and rotors

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Main articles:Lorentz transformation andRotor (mathematics)

The restricted Lorentz transformations that preserve the direction of time and include rotations and boosts can be performed by an exponentiation of the spacetime rotationbiparavectorWL=eW/2.{\displaystyle L=e^{W/2}.}

In the matrix representation, the Lorentz rotor is seen to form an instance of theSL(2,C) group (special linear group of degree 2 over thecomplex numbers), which is the double cover of theLorentz group. The unimodularity of the Lorentz rotor is translated in the following condition in terms of the product of the Lorentz rotor with its Clifford conjugationLL¯=L¯L=1.{\displaystyle L{\bar {L}}={\bar {L}}L=1.}

This Lorentz rotor can be always decomposed in two factors, oneHermitianB =B, and the otherunitaryR =R−1, such thatL=BR.{\displaystyle L=BR.}

The unitary elementR is called arotor because this encodes rotations, and the Hermitian elementB encodes boosts.

Four-velocity paravector

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Thefour-velocity, also calledproper velocity, is defined as thederivative of the spacetime position paravector with respect toproper timeτ:u=dxdτ=dx0dτ+ddτ(x1e1+x2e2+x3e3)=dx0dτ[1+ddx0(x1e1+x2e2+x3e3)].{\displaystyle u={\frac {dx}{d\tau }}={\frac {dx^{0}}{d\tau }}+{\frac {d}{d\tau }}(x^{1}\mathbf {e} _{1}+x^{2}\mathbf {e} _{2}+x^{3}\mathbf {e} _{3})={\frac {dx^{0}}{d\tau }}\left[1+{\frac {d}{dx^{0}}}(x^{1}\mathbf {e} _{1}+x^{2}\mathbf {e} _{2}+x^{3}\mathbf {e} _{3})\right].}

This expression can be brought to a more compact form by defining the ordinary velocity asv=ddx0(x1e1+x2e2+x3e3),{\displaystyle \mathbf {v} ={\frac {d}{dx^{0}}}(x^{1}\mathbf {e} _{1}+x^{2}\mathbf {e} _{2}+x^{3}\mathbf {e} _{3}),}and recalling the definition of thegamma factor:γ(v)=11|v|2c2,{\displaystyle \gamma (\mathbf {v} )={\frac {1}{\sqrt {1-{\frac {|\mathbf {v} |^{2}}{c^{2}}}}}},}so that the proper velocity is more compactly:u=γ(v)(1+v).{\displaystyle u=\gamma (\mathbf {v} )(1+\mathbf {v} ).}

The proper velocity is a positiveunimodular paravector, which implies the following condition in terms of theClifford conjugationuu¯=1.{\displaystyle u{\bar {u}}=1.}

The proper velocity transforms under the action of theLorentz rotorL asuu=LuL.{\displaystyle u\rightarrow u^{\prime }=LuL^{\dagger }.}

Four-momentum paravector

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Thefour-momentum in APS can be obtained by multiplying the proper velocity with the mass asp=mu,{\displaystyle p=mu,}with themass shell condition translated intop¯p=m2.{\displaystyle {\bar {p}}p=m^{2}.}

Classical electrodynamics

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Main article:Classical electrodynamics

Electromagnetic field, potential, and current

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Theelectromagnetic field is represented as a bi-paravectorF:F=E+iB,{\displaystyle F=\mathbf {E} +i\mathbf {B} ,}with the Hermitian part representing theelectric fieldE and the anti-Hermitian part representing themagnetic fieldB. In the standard Pauli matrix representation, the electromagnetic field is:F(E3E1iE2E1+iE2E3)+i(B3B1iB2B1+iB2B3).{\displaystyle F\rightarrow {\begin{pmatrix}E_{3}&E_{1}-iE_{2}\\E_{1}+iE_{2}&-E_{3}\end{pmatrix}}+i{\begin{pmatrix}B_{3}&B_{1}-iB_{2}\\B_{1}+iB_{2}&-B_{3}\end{pmatrix}}\,.}

The source of the fieldF is the electromagneticfour-current:j=ρ+j,{\displaystyle j=\rho +\mathbf {j} \,,}where the scalar part equals theelectric charge densityρ, and the vector part theelectric current densityj. Introducing theelectromagnetic potential paravector defined as:A=ϕ+A,{\displaystyle A=\phi +\mathbf {A} \,,}in which the scalar part equals theelectric potentialϕ, and the vector part themagnetic potentialA. The electromagnetic field is then also:F=A¯.{\displaystyle F=\partial {\bar {A}}.}The field can be split into electricE=A¯V{\displaystyle E=\langle \partial {\bar {A}}\rangle _{V}}and magneticB=iA¯BV{\displaystyle B=i\langle \partial {\bar {A}}\rangle _{BV}}components. Here,=t+e1x+e2y+e3z{\displaystyle \partial =\partial _{t}+\mathbf {e} _{1}\,\partial _{x}+\mathbf {e} _{2}\,\partial _{y}+\mathbf {e} _{3}\,\partial _{z}}andF is invariant under agauge transformation of the formAA+χ,{\displaystyle A\rightarrow A+\partial \chi \,,}whereχ{\displaystyle \chi } is ascalar field.

The electromagnetic field iscovariant under Lorentz transformations according to the lawFF=LFL¯.{\displaystyle F\rightarrow F^{\prime }=LF{\bar {L}}\,.}

Maxwell's equations and the Lorentz force

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TheMaxwell equations can be expressed in a single equation:¯F=1ϵj¯,{\displaystyle {\bar {\partial }}F={\frac {1}{\epsilon }}{\bar {j}}\,,}where the overbar represents theClifford conjugation.

TheLorentz force equation takes the formdpdτ=eFuR.{\displaystyle {\frac {dp}{d\tau }}=e\langle Fu\rangle _{R}\,.}

Electromagnetic Lagrangian

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The electromagneticLagrangian isL=12FFSAj¯S,{\displaystyle L={\frac {1}{2}}\langle FF\rangle _{S}-\langle A{\bar {j}}\rangle _{S}\,,}which is a real scalar invariant.

Relativistic quantum mechanics

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Main article:Relativistic quantum mechanics

TheDirac equation, for an electricallycharged particle of massm and chargee, takes the form:i¯Ψe3+eA¯Ψ=mΨ¯,{\displaystyle i{\bar {\partial }}\Psi \mathbf {e} _{3}+e{\bar {A}}\Psi =m{\bar {\Psi }}^{\dagger },}wheree3 is an arbitrary unitary vector, andA is the electromagnetic paravector potential as above. Theelectromagnetic interaction has been included viaminimal coupling in terms of the potentialA.

Classical spinor

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Main article:Spinor

Thedifferential equation of the Lorentz rotor that is consistent with the Lorentz force isdΛdτ=e2mcFΛ,{\displaystyle {\frac {d\Lambda }{d\tau }}={\frac {e}{2mc}}F\Lambda ,}such that the proper velocity is calculated as the Lorentz transformation of the proper velocity at restu=ΛΛ,{\displaystyle u=\Lambda \Lambda ^{\dagger },}which can be integrated to find the space-time trajectoryx(τ){\displaystyle x(\tau )} with the additional use ofdxdτ=u.{\displaystyle {\frac {dx}{d\tau }}=u.}

See also

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References

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