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

In flat spaces, linear and affine are often mixed. Similarly, in flat spaces, polynomials are also like this. Zero-order polynomials correspond to the base point in affine.

First, handle the one-dimensional real case.

exponential power function

[polynomial-function-1d] Polynomial functions are finite linear combinations of power functions. (Affine) base point , (vector) offset

The representation of a polynomial function is not affine invariant, i.e., switching the base point yields a representation of the same degree but with different coefficients. Scaling is also like this.

[change-base-point-polynomial] Switching base point

Then

Proof Expand and compute, compare the coefficients of to get the expression for . Use the commutativity of summation to collect power function terms.

If using as the base point in coordinates and changing the symbol , then the polynomial function is expressed as

Generalizing from polynomials as finite linear combinations to countably infinite linear combinations, called exponential power series of functions.

Some functions are not defined directly from exponential power series. Example can be defined directly through division, without needing to use power series for definition.

Besides as countable infinite data, can also be used.

Changing the exponential power function to the exponential power function introduces new aspects that require attention.

  • requires a multiplicative inverse.

  • requires solving the equation and addressing the issue of whether the solution is unique.

  • is unbounded at .

  • When , repeated differentiation does not terminate .

For now, we only deal with power series, abbreviated as power series.

Now handle the higher-dimensional case i.e. .

If the codomain is , we can additionally define function multiplication and multiplicative inverse .

First, attempt to base the definitions of polynomial functions and power series on tensors i.e. multilinearity.

If not necessary, there is no need to take the linear direct sum for tensors of all orders (known as the tensor algebra) for now.

[polynomial-function] Using codomain and multilinear functions . Base point , offset , define polynomial function

Affine transformations, i.e., changing the base point i.e. translation, or linear transformations i.e. (including scaling), do not change the degree of the polynomial.

may not be collinear.

Generalization to is straightforward. For the cases of , due to non-commutativity and non-associativity, it becomes very troublesome.

There may be different tensors that give the same polynomial, but a polynomial corresponds to a unique symmetric tensor .

Change notation.

  • [power-tensor]

Using difference techniques, one can recover the -th order symmetric tensor from the -th order monomial or power tensor .

In the -th order monomial of , there is a term , but there are many other interfering terms.

The entire problem is symmetric in , so a symmetric construction should be used.

In second order

[difference-symmetric-tensor] Symmetric tensor th order difference

Question Is there an intuitive understanding of th order difference?

[successive-difference] th order difference can be written as successive first-order differences

where , ,

Due to the commutativity of summation, the order of successive differences does not affect the final result

Proof of difference-symmetric-tensor

Fully expand

A function can be viewed as a function . Thus

Define weight

Prop For any non-empty finite set ,

Proof

All can be classified according to , each corresponds to choices (combination). Thus

for

define

define

There is a bijection

Weight

Final condition

  • When , it always holds for all
  • When , it fails only when is a bijection i.e. is all th order permutations, then

    • and

Symmetric tensors make

Remaining

There are permutations of order

So the result is

The symmetry of a symmetric multilinear function allows the property of difference to be inherited

[difference-polynomial] The -th order difference of is

The -th order difference of is

From this we obtain

Prop A polynomial function determines its symmetric multilinear function representation

Proof Suppose polynomial has two symmetric multilinear function representations

First, the -th order difference gives the same . Simultaneously removing the -th order term yields a polynomial of degree and its two symmetric multilinear representations . Induction on yields the conclusion

For power series, finite-order differences can never yield zero

Formally, division and limits can be used to eliminate higher-order terms