1. notice
  2. English
  3. logic_topic
  4. 1. logic
  5. 2. basic
  6. 3. map
  7. 4. order
  8. 5. combinatorics
  9. calculus
  10. 6. real_numbers
  11. 7. limit_sequence
  12. 8. division_algebra
  13. 9. Euclidean_space
  14. 10. Minkowski_space
  15. 11. polynomial
  16. 12. analytic_Euclidean
  17. 13. analytic_struct_operation
  18. 14. ordinary_differential_equation
  19. 15. convex_hull
  20. 16. volume
  21. 17. integral
  22. 18. divergence
  23. 19. limit_net
  24. 20. topology
  25. 21. compact
  26. 22. connected
  27. 23. topology_struct_operation
  28. 24. exponential
  29. 25. angle
  30. geometry
  31. 26. manifold
  32. 27. metric
  33. 28. metric_connection
  34. 29. geodesic_derivative
  35. 30. curvature_of_metric
  36. 31. Einstein_metric
  37. 32. constant_sectional_curvature
  38. 33. simple_symmetric_space
  39. 34. principal_bundle
  40. 35. group
  41. 36. stereographic_projection
  42. 37. Hopf_bundle
  43. field_theory
  44. 38. point_particle_non_relativity
  45. 39. point_particle_relativity
  46. 40. scalar_field
  47. 41. scalar_field_current
  48. 42. scalar_field_non_relativity
  49. 43. projective_lightcone
  50. 44. spacetime_momentum_spinor_representation
  51. 45. Lorentz_group
  52. 46. spinor_field
  53. 47. spinor_field_current
  54. 48. electromagnetic_field
  55. 49. Laplacian_of_tensor_field
  56. 50. Einstein_metric
  57. 51. interaction
  58. 52. harmonic_oscillator_quantization
  59. 53. spinor_field_misc
  60. 54. reference
  61. ไธญๆ–‡
  62. 55. notice
  63. ้€ป่พ‘
  64. 56. ้€ป่พ‘
  65. 57. ๅŸบ็ก€
  66. 58. ๆ˜ ๅฐ„
  67. 59. ๅบ
  68. 60. ็ป„ๅˆ
  69. ๅพฎ็งฏๅˆ†
  70. 61. ๅฎžๆ•ฐ
  71. 62. ๆ•ฐๅˆ—ๆž้™
  72. 63. ๅฏ้™คไปฃๆ•ฐ
  73. 64. Euclidean ็ฉบ้—ด
  74. 65. Minkowski ็ฉบ้—ด
  75. 66. ๅคš้กนๅผ
  76. 67. ่งฃๆž (Euclidean)
  77. 68. ่งฃๆž struct ็š„ๆ“ไฝœ
  78. 69. ๅธธๅพฎๅˆ†ๆ–น็จ‹
  79. 70. convex_hull
  80. 71. ไฝ“็งฏ
  81. 72. ็งฏๅˆ†
  82. 73. ๆ•ฃๅบฆ
  83. 74. ็ฝ‘ๆž้™
  84. 75. ๆ‹“ๆ‰‘
  85. 76. ็ดง่‡ด
  86. 77. ่ฟž้€š
  87. 78. ๆ‹“ๆ‰‘ struct ็š„ๆ“ไฝœ
  88. 79. ๆŒ‡ๆ•ฐๅ‡ฝๆ•ฐ
  89. 80. ่ง’ๅบฆ
  90. ๅ‡ ไฝ•
  91. 81. ๆตๅฝข
  92. 82. ๅบฆ่ง„
  93. 83. ๅบฆ่ง„็š„่”็ปœ
  94. 84. Levi_Civita ๅฏผๆ•ฐ
  95. 85. ๅบฆ่ง„็š„ๆ›ฒ็އ
  96. 86. Einstein ๅบฆ่ง„
  97. 87. ๅธธๆˆช้ขๆ›ฒ็އ
  98. 88. simple_symmetric_space
  99. 89. ไธปไธ›
  100. 90. ็พค
  101. 91. ็ƒๆžๆŠ•ๅฝฑ
  102. 92. Hopf ไธ›
  103. ๅœบ่ฎบ
  104. 93. ้ž็›ธๅฏน่ฎบ็‚น็ฒ’ๅญ
  105. 94. ็›ธๅฏน่ฎบ็‚น็ฒ’ๅญ
  106. 95. ็บฏ้‡ๅœบ
  107. 96. ็บฏ้‡ๅœบ็š„ๅฎˆๆ’ๆต
  108. 97. ้ž็›ธๅฏน่ฎบ็บฏ้‡ๅœบ
  109. 98. ๅ…‰้”ฅๅฐ„ๅฝฑ
  110. 99. ๆ—ถ็ฉบๅŠจ้‡็š„่‡ชๆ—‹่กจ็คบ
  111. 100. Lorentz ็พค
  112. 101. ๆ—‹้‡ๅœบ
  113. 102. ๆ—‹้‡ๅœบ็š„ๅฎˆๆ’ๆต
  114. 103. ็”ต็ฃๅœบ
  115. 104. ๅผ ้‡ๅœบ็š„ Laplacian
  116. 105. Einstein ๅบฆ่ง„
  117. 106. ็›ธไบ’ไฝœ็”จ
  118. 107. ่ฐๆŒฏๅญ้‡ๅญๅŒ–
  119. 108. ๆ—‹้‡ๅœบๆ‚้กน
  120. 109. ๅ‚่€ƒ

note-math

[co_vector_of_Hermitian_tensor]

induces the co-vector of Hermitian_tensor

Since is a Hermitian matrix, then , so

Because is Hermitian or self-adjoint with respect to the inner product of , can be considered to act symmetrically on the two slots

The base of the vector space gives the coefficients of the co-vector

The action of on the co-vector is

It also corresponds to the transformation of the dual base, i.e., the base of the co-vector space , which is

parity dual and induced action

Similarly, co-vectors can also be defined for anti-Hermitian tensors

For complex conjugate two-tensors

[spinor_field_motivation]

  • formally corresponds momentum to gradient momentum , and to spacetime_momentum_spinor_representation

  • formally used for co-vector generated by to obtain field

  • action + product rule + divergence + zero boundary + integral quadratic form ==> self-adjoint operator

[massless_spinor_Lagrangian] alias [Weyl_Lagrangian]

or or

where is integrated using + quadratic form of as

The only one that works is , because is a divergence quantity, using Stokesโ€™ theorem + zero boundary

variation gives linear part

[massless_spinor_equation] alias [Weyl_equation]

or or

Similar to via , varying with respect to -valued is equivalent to varying with respect to -valued

can be interpreted as the gradient momentum of the field (after metric-dual) , compounded to, the multiplication of momentum and spinor

[Weyl_parity]

parity dual action uses spinor

parity dual eq

or or

[Weyl_eq_plane_wave]

Plane wave solution with and

A linear equation with indicates non-zero solutions. The solution space is one-dimensional, and the solution can be written as with

[massive_spinor_Lagrangian] action for mass-coupled spinors, alias [Dirac_Lagrangian]

couple Weyl spinors and their parity to

,

invariant non couple term

non-couple term variation with respect to gives

according to cancelation by parity

invariant couple term

couple term variation with respect to gives

  • overall variation with respect to gives
  • overall variation with respect to gives
  • when , decouples into two parity-dual massless-spinors

These two PDEs imply

and as โ€œsquare root of โ€œ [square_root_of_spacetime_Laplacian]

Overall , square root of KG. If a field satisfies the Dirac eq, then it satisfies the KG eq. Therefore, Dirac eq can approximate to KG eq, or further approximate to Schrodinger eq. But note that compared to the case of value, the difference from is that the angular momentum operator represented by or will have a spin part that affects the range space, similar to spinor_angular_momentum

All partial derivatives of the action is zero , giving [massive_spinor_equation] , alias [Dirac_equation]

Similar to via , variation with respect to valued is equivalent to variation with respect to valued

If the couple term is replaced by , the action is still invariant. However, the eq can no longer be decomposed into that simpler form

Question For any , the invariant matrix is probably only

[Dirac_eq_plane_wave]

Plane wave solution with and

The latter is a linear equation, so the solution is not difficult. The solution space is two-dimensional, and the solution can be written as (ref-17, p.100)

The conjugate phase plane wave satisfies the condition , and the solution can be written as

Similar to the scalar field case, superposition can be performed on the hyperboloid where the momentum lies. [linear_superposition_of_Dirac_eq]

[squrae_root_of_spacetime_momentum_spinor_representation]

Although it might be possible to use the eigenvalues of the Hermite matrix (), we will calculate it directly here. let or

==>

==> Use

==> Quadratic equation for : , solution

==>

or

Still Hermite. Calculation yields

Example

then

If , then

1,3 metric square root or square root . But you can also use to get the true square

Since , the transformation does not come from coordinate change

[motivation_of_gauge_field]

Ignored some issues

Tangent projective light cone bundle is well-defined

But is a field or a field needed? There are too many choices to lift a field to a field (or to a field); all lifting choices form a field

And there are only two ways to lift to

On a curved manifold, there may not even be a global single-valued lift.

The change in the lifting method from a field to a field corresponds to โ€œchanging the gaugeโ€, by multiplying the spinor by to change the gauge.

If the conserved current of the action is to be simpler, then use gauge transformation instead of . does not change the Lagrangian action, which simplifies the calculation of conserved currents (cf. the case of scalar field calculating 4-current for symmetry).

Changing the gauge is not compatible with taking derivatives of tangent spaces in bundle coordinates, so an additional structure โ€” connection โ€” must be introduced.

There are many possible connections. A good connection is one with the smallest curvature cf. electromagnetic_field

The bundle in curved spacetime can be directly defined in the bundle coordinates of the principal bundle (orthonormal frame bundle). Using the correspondence, changing bundle coordinates automatically corresponds to changing bundle coordinates.

In curved spacetime, one needs to deal with the covariant derivative of the spinor field with respect to the metric, which is derived from the metric_connection of the tangent vector field.

For spinors, one might need to use an orthonormal frame instead of a coordinate frame, i.e., use principal bundle. Does this introduce new difficulties for calculating covariant derivatives?

Even if the topology of the spacetime base manifold is non-trivial, there might exist different bundle types for gauge fields.

One problem is that, unlike spinor fields, gauge bundles do not seem to be directly related to tangent bundles.

It seems that all types of bundle types based on the base manifold must be considered simultaneously.

In the homotopy sense, has only one type of bundle type.

[spinor_field_gauge_imaginary_automorphism]

Although the cost is using dimensional spacetime, tangent space , but if we consider octonions , and if we choose a unit imaginary element to construct the spinor Lagrangian, then the octonionโ€™s imaginary automorphism group โ€˜s isotropy on leads to the decomposition , the isotropy group is isomorphic to , and it derives the action of on . cf. (ref-19, th.4)

Note that the octonion imaginary automorphism group is not . So this is not a group of gauge connection in the traditional sense.

It is said that is the gauge group of strong interaction. The advantage of the octonion method here is that there is no longer a need to additionally assume the separate existence of and and perform tensor operations on and Dirac spinor out of thin air. The tensor from comes from the connection of acting on the spinor or .

The isotropy in isomorphic to will change the phase or the gauge field of the gauge transformation, leading to the action on the part. Should it be said that there is a gauge field of the gauge transformation for the or gauge field of a gauge transformation, and then introduce the Yangโ€“Mills eq of minimal curvature again like the electromagnetic field?

Question What about the case of quaternions ? In the case of , the symmetry group of imaginary unit is . When fixing one imaginary unit, it become

In octonion spinor theory, there is still as the space where the spinor field resides, the projective light cone is , gives a double cover of , and spacetime corresponds to a second-order Hermitian octonion matrix , where corresponds to the spacetime metric. Moreover, spacetime, spinor , and a real number can be embedded into a third-order Hermitian octonion matrix (and the projectivization of is a generalization of the projective light cone ), the group that preserves the of is , which can be well embedded into and spinor gauge theory and cf. (ref-20, th.6)

The quark lepton fermion model of the Standard Model can be written as acting on , so some people embed into (probably through , ), and then embed it into , and then correspond with . These embeddings are called โ€œGUTโ€. breaks to

Mathematically, I think we can consider whether has something similar to the GUT quark lepton model, note that it is similar not identical

The motivation for considering this model is that , and the spinor and , are very close, so that no additional assumption of is needed, and the breaking may be completed by fixing a unit imaginary element, or equivalently fixing .

[spin_connection]

The frame bundle of derived from the tangent bundle metric and the connection of the frame bundle derived from metric_connection behave as is locally type , acting on tangent vector fields by

The way to derive the spin-connection is to map the part of the induced metric-connection to in the orthonormal-frame, yielding the connection of the bundle, locally type , acting on the spinor field by with

Although the definition of the Pauli matrix for spin representation requires , both and Lie algebra can be expressed by the โ€œsquareโ€ of thereafter.

spin-connection also denoted by

[motivation_of_scalar_field] can scalar field be related to tautological bundle of projective-lightcone ?

According to the concept of spinor fields in spacetime manifold, โ€œrotation by 720 degreesโ€ and โ€œparityโ€ should occur in the tangent space construction, not in the spacetime manifold.

Since the tangent spaces of the spacetime manifold are all , can spinor fields be generalized to general spacetime manifolds?

[spinor_on_Lorentz_manifold] Question

massless-spinor-action

massless-spinor-equation

I havenโ€™t verified if this definition is conceptually reasonable. Compare with flat spacetime, try to prove or disprove it.

  • is self-adjoint
  • Only contributes to the variation of the action.
  • i.e. square-root-of spacetime Laplacian (closer to the Laplacian of tangent vector fields rather than scalar fields)

massive-spinor-Lagrangian

massive-spinor-equation

Question As long as it locally quotients back from to , it can avoid the problem of continuous global single-valued lift to .

We know that the KG eq has a non-relativity approximation limit . Does the massive-spinor construction have a non-relativity approximation limit ?

Static doesnโ€™t need a non-relativity approximation limit , despite the presence of , just like static electromagnetic field equations donโ€™t need a non-relativity approximation limit . This is also true for the KG equation.

let static

static massless spinor eq

static massive spinor eq

They can couple to static electromagnetic gauge potential or just static electric or just static magnetic

In the presence of electromagnetic potential, the parity dual of massless particles might be different, for example, just static electric

When electromagnetic potential = 0, the parity dual eq is the same.