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

note-math

Consider the subspace

The following are equivalent

  • not co-linear

if , according to the intuition of (draw a picture), bases of the following types are all possible

  • 2 time(-like)
  • 2 space
  • 1 time, 1 space
  • 1 time, 1 light
  • 1 space, 1 light
  • 2 light

Example

  • 2 time(-like)

    , where

    can linearly generate , thus spanning
  • 2 space
    , where
  • 1 time, 1 space
  • 1 time, 1 light
  • 1 space, 1 light similarly
  • 2 light
    Example . Note .
    generate

Consider a general in

[signature-of-2d-subspace-of-spacetime] Prop The possible signatures of a in Minkowski are

We will prove later that signatures are impossible

Intuitively, the plane spanned by two lines (imagine the case of )

  • intersects both the interior and exterior of the light cone. Although all types of bases are possible, all bases of the following types are of signature

    • 2 time
    • 1 time, 1 light
    • 2 light
  • only intersects the exterior of the light cone

    • 2 space
  • is tangent to the light cone, does not intersect the interior of the light cone, and intersects the light cone only along a single light-like line

    • 1 light, 1 space

Prop can have signature subspaces. Proof โ€˜s

Prop time-like is orthogonal only to space-like

let be time-like. Using orthogonal decomposition , let then ==> is space-like

Prop light-like is not orthogonal to

  • time-like. because time-like is orthogonal only to space-like
  • light-like vectors other than those colinear with itself [metric-cannot-distinguish-colinear-light-like]

Proof

Take an orthogonal decomposition , let be light-like and orthogonal

are space-like. According to the Euclidean inner product inequality

but , so the Euclidean inner product inequality takes equality, thus are colinear .

This implies , thus

Prop The signature of a two-dimensional subspace of cannot be or

Proof Use the previous theorem

Question Is there a proof that does not rely on orthogonal decomposition of time and space? But note, this proposition does not hold for general . In , the following are orthogonal and non-collinear

  • 1 time, 1 light
  • 2 light

A further concept is โ€œTotally Isotropic Subspaceโ€

Prop When , all signatures are possible for the subspace of

Proof In this case contains the subspace , where it is easy to construct subspaces of all possible signatures

Prop For two non-collinear time-like vectors in , the signature of their span is

Proof Use one of the time-like vectors as the initial basis to generate an orthogonal basis for , but the signature cannot be , so it must be

Prop In let be light-like, be time-like or light-like, and be non-collinear. Then

Proof

are not orthogonal,

Fix a , consider

By adjusting , positive or negative results can be obtained, thus having time-like and space-like, so the signatures are both , it can only be

Another method. The quadratic form corresponds to matrix in basis . Transforming to signature standard form corresponds to matrix transformation

Thus are one positive and one negative, corresponding to signature

[simultaneity-relativity] Relativity of Simultaneity

According to orthogonal basis extension, it can be proved

in , the orthogonal complement of a space-like subspace is a time-like subspace

  • ( space-like) <==> (there exists a time-like orthogonal to both )
    Proof Note, time-like is only orthogonal to space-like

    • (==>) Start extension from . The time-like basis vector is orthogonal to the space-like basis vectors
    • (<==) Start extension from . All space-like basis vectors form the orthogonal complement space of . are orthogonal to , so belong to , and all subspaces of Euclidean space are Euclidean

Thus the contrapositive also holds

  • ( not space-like) <==> (there does not exist a time-like orthogonal to both space-like )

Intuition: Different space-like subspaces may not have compatible time measurement methods or the time-like orthogonal complements of may be different

Take a spacetime orthogonal decomposition of

Prop ==> The sign of the product of time components determines the sign of the inner product

Proof Case analysis for

  • . let . . Similarly for . Then by the Euclidean inner product inequality

    Thus , i.e., same sign as

  • . let . Set and apply the conclusion from

in Euclidean, we have

Inner product inequality ==> Triangle inequality

in signature quadratic form, this generally does not hold

As mentioned earlier, the quadratic form under the basis corresponds to the matrix . Transforming to the standard quadratic form, the corresponding matrix transformation is

[quadratic-form-inequality-Minkowski] Inner product inequality


  • one positive and one negative, corresponding to signature

  • with the same sign, corresponding to or signature

  • Other signatures or are collinear

[triangel-inequality-Minkowski] signature triangle inequality

  • 2 time

,

  • ==>
  • ==>
  • 1 time, 1 light

==>

  • ==>
  • ==>

Proof of 2 time-like

use quadratic-form-inequality-Minkowski

==>

==>

==>

==>

==>

Note is uncertain

Example let . let be past time-like

The limit or continuity in Euclidean space is directly defined using open balls (to simplify the discussion, only consider the origin as the center)

In Minkowski space or p,q quadratic form space, a direct imitation of the Euclidean case is

  • timelike , spacelike , or
  • When merging classes, the class is empty

But note that at this time

  1. The limit meaning represented by is different from the Euclidean case. For example, although two distinct points on the light cone are โ€œseparated,โ€ their quadratic distance is zero. For a point on the light cone, although it is separated from , it can be transformed via so that the coordinates of approach arbitrarily. Taking as an example, let . After transformation, , then . under the orbit of the action is the ray
  2. Taking as an example, should be the analogue of the sphere in . Based on graphical intuition in , some points on appear far from the origin , but in fact the distance of any point on is the same; any two points on can be transformed into each other via an transformation, just like the situation with . On , when the quadratic form distance , it can be considered as the timelike geodesic distance or the proper time of an inertial particle. Timelike points on can be transformed via to have zero spatial coordinates, meaning transforming from uniform motion to rest, where proper time = time. Similar conclusions likely hold for as well.

โ€œFortunatelyโ€, the โ€œcontinuity of coordinate distanceโ€ in , i.e., the product distance of , implies the โ€œcontinuity of quadratic form distanceโ€ in , because , and further implies differentiability/analyticity.

Conversely, in the case of non-Euclidean geometry, continuity of the quadratic form distance does not imply continuity of the coordinate distance.

When dealing with objects in Minkowski space , many useful functions are also โ€œcontinuous or analytic with respect to spacetime coordinate distanceโ€, i.e., continuous or analytic under the product distance in one coordinate.

When dealing with differentiability/analyticity, since dividing by may be encountered in the direction of the light cone in the domain or codomain, those points are generally considered to be differentiable/analytic.

However, there may exist useful functions that are continuous/analytic under the quadratic form distance but not continuous/not analytic under the spacetime coordinate distance.

Possible clue for the rationality of the quadratic form distance: , via the tensor as a linear map space, inherits a tensor quadratic form. When restricted to , it becomes proportional to the Killing form quadratic form of Killing-form-of-orthogonal-group. Signature , where is the number of boosts, are time-like rotations, and are space-like rotations. Under the Killing form, boosts have positive distance, while time/space rotations both have negative distance.

โ€˜s timelike region . It can be decomposed into the radial space part and the directional space part

Similar to polar coordinates in , we can use hyperbolic polar coordinates , where is the quadratic form distance, and is the geodesic length on , also called the hyperbolic angle [hyperbolic-angle] or rapidity [rapidity]

[polor-coordinate-hyperbolic] Hyperbolic polar coordinates

[hyperbolic-cosine-formula] Hyperbolic Cosine Formula

let

let

let future time-like.

Hyperbolic Cosine Formula

[isom-top-hyperbolic-Euclidean]

Limit structure of under the distance geodesic distance Euclidean

Proof

let ,

let

use

use continuity

Generalize to , Euclidean

Proof

use geodesic coordinates

similar to , try to prove

where

  • are the geodesic coordinates of
  • is the Euclidean distance in geodesic coordinates

Geodesics on quadratic manifolds can be defined using purely quadratic form techniques

The tangent space at point of the quadratic manifold can be defined as the (affine) subspace orthogonal to the radial vector

The initial direction of the geodesic starting from point is in the tangent space of at point ,

The geodesic is defined as

type (p. 19 of ref-9)

type

is a Riemann manifold with constant negative curvature

is a Lorentz manifold with constant positive curvature

alias de Sitter space

The base points (โ€œnorth and south polesโ€) of the stereographic projection of the sphere lie on . More than two coordinate charts are needed to cover the entire

[stereographic-projective-hyperbolic] For the time-like hyperboloid , consider stereographic projection. The two base points lie on the two sheets of the hyperboloid respectively, and the projection forms separated singularities in the light cone direction (the cross shape in the figure below)

In the projection coordinates of the future base point, the coordinates of the past base point are zero, but the coordinates of the future base point are either absent or are

is special, so the future coordinates in the figure above are disconnected. However, when the spatial dimension is , the future coordinates should be connected

For the space-like hyperboloid, use space-like base points to define the hyperbolic projection. The projection coordinate chart is a Minkowski space of one lower dimension

Perform a 3D plot for the case of , drawing the light cone of the base point (note that the light cone is โ€œverticalโ€)

Even if the visual intuition for plotting might be difficult, the analytical calculation should not be hard