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| {{Algebra of Physical Space}}
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| The [[Dirac equation]], as the [[Theory of relativity|relativistic]] equation that describes
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| spin 1/2 particles in [[quantum mechanics]] can be written in terms of the [[Algebra of physical space]] (APS), which is a case of a [[Clifford algebra]] or [[geometric algebra]]
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| that is based in the use of [[paravectors]].
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| The Dirac equation in APS, including the electromagnetic interaction, reads | |
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| :<math> i \bar{\partial} \Psi\mathbf{e}_3 + e \bar{A} \Psi = m \bar{\Psi}^\dagger </math>
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| Another form of the Dirac equation in terms of the Space time algebra was given earlier by [[David Hestenes]].
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| In general, the Dirac equation in the formalism of geometric algebra has the advantage of
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| providing a direct geometric interpretation.
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| ==Relation with the standard form==
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| The [[spinor]] can be written in a null basis as
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| :<math>
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| \Psi = \psi_{11} P_3 - \psi_{12} P_3 \mathbf{e}_1 + \psi_{21} \mathbf{e}_1 P_3 +
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| \psi_{22} \bar{P}_3, | |
| </math>
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| such that the representation of the spinor in terms of the [[Pauli matrices]] is
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| :<math> | |
| \Psi \rightarrow
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| \begin{pmatrix}
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| \psi_{11} & \psi_{12} \\ \psi_{21} & \psi_{22}
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| \end{pmatrix}
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| </math>
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| :<math>
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| \bar{\Psi}^\dagger \rightarrow
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| \begin{pmatrix}
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| \psi_{22}^* & -\psi_{21}^* \\ -\psi_{12}^* & \psi_{11}^*
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| \end{pmatrix}
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| </math>
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| The standard form of the Dirac equation can be recovered by decomposing the spinor in its right and left-handed spinor components, which are extracted with the help of the projector
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| :<math> P_3 = \frac{1}{2}( 1 + \mathbf{e}_3), </math>
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| such that
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| :<math>
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| \Psi_L = \bar{\Psi}^\dagger P_3
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| </math>
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| :<math>
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| \Psi_R = \Psi P_3^{ }
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| </math>
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| with the following matrix representation
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| :<math>
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| \Psi_L \rightarrow
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| \begin{pmatrix}
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| \psi_{22}^* & 0 \\ -\psi_{12}^* & 0
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| \end{pmatrix}
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| </math>
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| :<math>
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| \Psi_R \rightarrow
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| \begin{pmatrix}
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| \psi_{11} & 0 \\ \psi_{21} & 0
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| \end{pmatrix}
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| </math>
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| The Dirac equation can be also written as
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| :<math> i \partial \bar{\Psi}^\dagger \mathbf{e}_3 + e A \bar{\Psi}^\dagger = m \Psi </math>
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| Without electromagnetic interaction, the following equation is obtained from
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| the two equivalent forms of the Dirac equation
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| :<math>
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| \begin{pmatrix}
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| 0 & i \bar{\partial}\\
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| i \partial & 0
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| \end{pmatrix}
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| \begin{pmatrix}
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| \bar{\Psi}^\dagger P_3 \\ \Psi P_3
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| \end{pmatrix}
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| = m
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| \begin{pmatrix}
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| \bar{\Psi}^\dagger P_3 \\ \Psi P_3
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| \end{pmatrix}
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| </math>
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| so that
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| :<math>
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| \begin{pmatrix}
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| 0 & i \partial_0 + i\nabla \\
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| i \partial_0 - i \nabla & 0
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| \end{pmatrix}
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| \begin{pmatrix}
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| \Psi_L \\ \Psi_R
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| \end{pmatrix}
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| = m
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| \begin{pmatrix}
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| \Psi_L \\ \Psi_R
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| \end{pmatrix}
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| </math>
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| or in matrix representation
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| :<math>
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| i \left(
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| \begin{pmatrix}
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| 0 & 1 \\
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| 1 & 0
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| \end{pmatrix} \partial_0 +
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| \begin{pmatrix}
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| 0 & \sigma \\
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| -\sigma & 0 | |
| \end{pmatrix} \cdot \nabla
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| \right)
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| \begin{pmatrix}
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| \psi_L \\ \psi_R
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| \end{pmatrix}
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| = m
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| \begin{pmatrix}
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| \psi_L \\ \psi_R
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| \end{pmatrix},
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| </math>
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| where the second column of the right and left spinors can be dropped by defining the
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| single column chiral spinors as
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| :<math>
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| \psi_L \rightarrow
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| \begin{pmatrix}
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| \psi_{22}^* \\ -\psi_{12}^*
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| \end{pmatrix}
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| </math>
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| :<math>
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| \psi_R \rightarrow
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| \begin{pmatrix}
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| \psi_{11} \\ \psi_{21}
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| \end{pmatrix}
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| </math>
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| The standard relativistic covariant form of the Dirac equation in the Weyl
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| representation can be easily identified
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| <math>
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| i \gamma^{\mu} \partial_{\mu} \psi = m \psi,
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| </math>
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| such that
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| :<math>
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| \psi_=
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| \begin{pmatrix}
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| \psi_{22}^* \\ -\psi_{12}^* \\
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| \psi_{11} \\ \psi_{21}
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| \end{pmatrix}
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| </math>
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| Given two spinors <math>\Psi</math> and <math>\Phi</math> in APS and
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| their respective spinors in the standard form as <math>\psi</math> and
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| <math>\phi</math>, one can verify the following identity
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| :<math>
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| \phi^\dagger \gamma^0 \psi = \langle \bar{\Phi}\Psi +
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| (\bar{\Psi}\Phi)^\dagger \rangle_S
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| </math>,
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| such that
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| :<math>
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| \psi^\dagger \gamma^0 \psi = 2 \langle \bar{\Psi}\Psi \rangle_{S R}
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| </math>
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| ==Electromagnetic gauge==
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| The Dirac equation is invariant under a global right rotation applied
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| on the spinor of the type
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| :<math>
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| \Psi \rightarrow \Psi^\prime = \Psi R_0
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| </math>
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| so that the kinetic term of the Dirac equation transforms as
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| :<math>
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| i\bar{\partial} \Psi \mathbf{e}_3 \rightarrow
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| i\bar{\partial} \Psi R_0 \mathbf{e}_3 R_0^\dagger R_0 =
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| ( i\bar{\partial} \Psi \mathbf{e}_3^\prime ) R_0,
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| </math>
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| where we identify the following rotation
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| :<math>
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| \mathbf{e}_3 \rightarrow \mathbf{e}_3^\prime = R_0 \mathbf{e}_3 R_0^\dagger
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| </math>
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| The mass term transforms as
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| :<math>
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| m \overline{\Psi^\dagger} \rightarrow
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| m \overline{(\Psi R_0)^\dagger} = m \overline{ \Psi^\dagger }R_0,
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| </math>
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| so that we can verify the invariance of the form of the Dirac equation.
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| A more demanding requirement is that the Dirac equation should be
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| [[local gauge invariance|invariant under a local gauge transformation]] of the type <math>R=\exp(-i e \chi \mathbf{e}_3) </math>
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| In this case, the kinetic term transforms as
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| :<math>
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| i\bar{\partial} \Psi \mathbf{e}_3 \rightarrow
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| (i \bar{\partial} \Psi) R \mathbf{e}_3 + (e\bar{\partial}\chi) \Psi R
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| </math>,
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| so that the left side of the Dirac equation transforms covariantly as
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| :<math>
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| i\bar{\partial} \Psi \mathbf{e}_3 -e \bar{A}\Psi \rightarrow
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| (i\bar{\partial} \Psi R \mathbf{e}_3 R^\dagger -e \overline{(A + \partial \chi)}\Psi)R,
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| </math>
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| where we identify the need to perform an electromagnetic gauge transformation.
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| The mass term transforms as in the case with global rotation, so, the form
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| of the Dirac equation remains invariant.
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| ==Current==
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| The current is defined as
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| :<math>
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| J = \Psi\Psi^\dagger,
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| </math> | |
| which satisfies the continuity equation
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| :<math>
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| \left\langle \bar{\partial} J \right\rangle_{S}=0
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| </math>
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| ==Second order Dirac equation==
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| An application of the Dirac equation on itself leads to the second order Dirac equation
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| :<math>
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| (-\partial \bar{\partial} +
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| A \bar{A}) \Psi - i( 2e\left\langle A \bar{\partial} \right\rangle_S + eF) \Psi \mathbf{e}_3 = m^2 \Psi
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| </math>
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| ==Free particle solutions==
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| ===Positive energy solutions===
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| A solution for the free particle with momentum <math> p = p^0 + \mathbf{p} </math> and positive energy <math>p^0>0</math> is
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| :<math>
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| \Psi = \sqrt{\frac{p}{m}} R(0) \exp(-i\left\langle p \bar{x}\right\rangle_S \mathbf{e}_3).
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| </math>
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| This solution is unimodular
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| :<math>
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| \Psi \bar{\Psi} = 1
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| </math>
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| and the current resembles the classical proper velocity
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| :<math>u = \frac{p}{m} </math>
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| :<math> | |
| J = \Psi {\Psi}^\dagger = \frac{p}{m}
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| </math>
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| ===Negative energy solutions===
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| A solution for the free particle with negative energy and momentum
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| <math> p = -|p^0| - \mathbf{p} = - p^\prime</math> is
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| :<math>
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| \Psi = i\sqrt{\frac{p^\prime}{m}} R(0) \exp(i\left\langle p^\prime \bar{x}\right\rangle_S \mathbf{e}_3) ,
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| </math>
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| This solution is anti-unimodular
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| :<math>
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| \Psi \bar{\Psi} = -1
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| </math>
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| and the current resembles the classical proper velocity <math>u = \frac{p}{m} </math>
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| :<math>
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| J = \Psi {\Psi}^\dagger = -\frac{p}{m},
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| </math>
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| but with a remarkable feature: "the time runs backwards"
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| :<math>
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| \frac{d t}{d \tau} = \left\langle \frac{p}{m} \right\rangle_S < 0
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| </math>
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| ==Dirac Lagrangian==
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| The Dirac Lagrangian is
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| :<math> L =
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| \langle i \partial \bar{\Psi}^\dagger \mathbf{e}_3 \bar{\Psi}
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| - e A \bar{\Psi}^\dagger \bar{\Psi} -m \Psi \bar{\Psi}
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| \rangle_0 </math>
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| ==See also==
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| *[[Paravector]]
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| *[[Algebra of physical space]]
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| *[[Geometric algebra]]
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| *[[Two-body Dirac equations]]
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| ==References==
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| ===Textbooks===
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| * Baylis, William (2002). ''Electrodynamics: A Modern Geometric Approach'' (2nd ed.). Birkhäuser. ISBN 0-8176-4025-8
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| * W. E. Baylis, editor, ''Clifford (Geometric) Algebra with Applications to Physics, Mathematics, and Engineering'', Birkhäuser, Boston 1996.
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| ===Articles===
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| * Baylis, William, ''Classical eigenspinors and the Dirac equation'', [http://prola.aps.org/abstract/PRA/v45/i7/p4293_1 Phys. Rev. A 45, 4293–4302] (1992)
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| * [[David Hestenes|Hestenes]] D., ''Observables, operators, and complex numbers in the Dirac theory'', [[Journal of Mathematical Physics|J. Math. Phys.]] 16, 556 (1975)
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| [[Category:Quantum mechanics]]
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| [[Category:Quantum field theory]]
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| [[Category:Spinors]]
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| [[Category:Equations of physics]]
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| [[Category:Paul Dirac|Equation in the algebra of physical space]]
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| [[Category:Dirac equation|Algebra of physical space]]
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