1. notice
  2. ไธญๆ–‡
  3. 1. feature
  4. ้€ป่พ‘
  5. 2. ้€ป่พ‘
  6. 3. ้›†ๅˆ่ฎบ
  7. 4. ๆ˜ ๅฐ„
  8. 5. ๅบ
  9. 6. ็ป„ๅˆ
  10. ๅพฎ็งฏๅˆ†
  11. 7. ๅฎžๆ•ฐ
  12. 8. ๆ•ฐๅˆ—ๆž้™
  13. 9. โ„^n
  14. 10. Euclidean ็ฉบ้—ด
  15. 11. Minkowski ็ฉบ้—ด
  16. 12. ๅคš้กนๅผ
  17. 13. ่งฃๆž (Euclidean)
  18. 14. ่งฃๆž (Minkowski)
  19. 15. ่งฃๆž struct ็š„ๆ“ไฝœ
  20. 16. ๅธธๅพฎๅˆ†ๆ–น็จ‹
  21. 17. ไฝ“็งฏ
  22. 18. ็งฏๅˆ†
  23. 19. ๆ•ฃๅบฆ
  24. 20. ็ฝ‘ๆž้™
  25. 21. ็ดง่‡ด
  26. 22. ่ฟž้€š
  27. 23. ๆ‹“ๆ‰‘ struct ็š„ๆ“ไฝœ
  28. 24. ๆŒ‡ๆ•ฐๅ‡ฝๆ•ฐ
  29. 25. ่ง’ๅบฆ
  30. ๅ‡ ไฝ•
  31. 26. ๆตๅฝข
  32. 27. ๅบฆ่ง„
  33. 28. ๅบฆ่ง„็š„่”็ปœ
  34. 29. Levi-Civita ๅฏผๆ•ฐ
  35. 30. ๅบฆ่ง„็š„ๆ›ฒ็އ
  36. 31. Einstein ๅบฆ่ง„
  37. 32. ๅธธๆˆช้ขๆ›ฒ็އ
  38. 33. simple-symmetric-space
  39. 34. ไธปไธ›
  40. 35. ็พคไฝœ็”จ
  41. 36. ็ƒๆžๆŠ•ๅฝฑ
  42. 37. Hopf ไธ›
  43. ๅœบ่ฎบ
  44. 38. ้ž็›ธๅฏน่ฎบ็‚น็ฒ’ๅญ
  45. 39. ็›ธๅฏน่ฎบ็‚น็ฒ’ๅญ
  46. 40. ็บฏ้‡ๅœบ
  47. 41. ็บฏ้‡ๅœบ็š„ๅฎˆๆ’ๆต
  48. 42. ้ž็›ธๅฏน่ฎบ็บฏ้‡ๅœบ
  49. 43. ๅ…‰้”ฅๅฐ„ๅฝฑ
  50. 44. ๆ—ถ็ฉบๅŠจ้‡็š„่‡ชๆ—‹่กจ็คบ
  51. 45. Lorentz ็พค
  52. 46. ๆ—‹้‡ๅœบ
  53. 47. ๆ—‹้‡ๅœบ็š„ๅฎˆๆ’ๆต
  54. 48. ็”ต็ฃๅœบ
  55. 49. ๅผ ้‡ๅœบ็š„ Laplacian
  56. 50. Einstein ๅบฆ่ง„
  57. 51. ็›ธไบ’ไฝœ็”จ
  58. 52. ่ฐๆŒฏๅญ้‡ๅญๅŒ–
  59. 53. ๆ—‹้‡ๅœบๆ‚้กน
  60. 54. ๅ‚่€ƒ
  61. English
  62. 55. notice
  63. 56. feature
  64. logic-topic
  65. 57. logic
  66. 58. set-theory
  67. 59. map
  68. 60. order
  69. 61. combinatorics
  70. calculus
  71. 62. real-numbers
  72. 63. limit-sequence
  73. 64. โ„^n
  74. 65. Euclidean-space
  75. 66. Minkowski-space
  76. 67. polynomial
  77. 68. analytic-Euclidean
  78. 69. analytic-Minkowski
  79. 70. analytic-struct-operation
  80. 71. ordinary-differential-equation
  81. 72. volume
  82. 73. integral
  83. 74. divergence
  84. 75. limit-net
  85. 76. compact
  86. 77. connected
  87. 78. topology-struct-operation
  88. 79. exponential
  89. 80. angle
  90. geometry
  91. 81. manifold
  92. 82. metric
  93. 83. metric-connection
  94. 84. geodesic-derivative
  95. 85. curvature-of-metric
  96. 86. Einstein-metric
  97. 87. constant-sectional-curvature
  98. 88. simple-symmetric-space
  99. 89. principal-bundle
  100. 90. group-action
  101. 91. stereographic-projection
  102. 92. Hopf-bundle
  103. field-theory
  104. 93. point-particle-non-relativity
  105. 94. point-particle-relativity
  106. 95. scalar-field
  107. 96. scalar-field-current
  108. 97. scalar-field-non-relativity
  109. 98. projective-lightcone
  110. 99. spacetime-momentum-spinor-representation
  111. 100. Lorentz-group
  112. 101. spinor-field
  113. 102. spinor-field-current
  114. 103. electromagnetic-field
  115. 104. Laplacian-of-tensor-field
  116. 105. Einstein-metric
  117. 106. interaction
  118. 107. harmonic-oscillator-quantization
  119. 108. spinor-field-misc
  120. 109. reference

note-math

May migrate to principal-bundle-connection in the future?

cf. motivation-of-gauge-field

There are many possible connections

There are connections that cannot be local flat. For any local region, the connection field cannot be eliminated by changing the gauge.

Similar to flat-metric-iff-curvature-0

There exist local bundle coordinates or phases, where the connection is zero <==> the curvature is zero where , in coordinates

When not exist flat connection coordinate, choose minimal curvature, based on metric-volume-form

Example

case. is valued, and it is commutative . In this case , in coordinates

Transforming from local flat-connection coordinates to general coordinates gives a PDE

PDE solvable condition

From the solution of the PDE , integration gives and phase transformation

[electromagnetic-field]

In

There are many possible connections; select by minimizing curvature.

Note that means the definition of this action requires spacetime metric

eq

In coordinates

In spacetime decomposition coordinates

Of course, this decomposition method is not invariant

Question How to make obviously imply the form of the electromagnetic field equations? [Maxwell-equation]

Also

Where

Note that and exterior derivative are related to Hodge star. can also be related to Hodge star. It may be related to the behavior of Hodge star in the spatial coordinates of spacetime decomposition.

Note that Hodge star requires a metric

Using the special specification [Lorentz-gauge] , the equation becomes