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Frames and coordinate systems in the formalization of Einsteins special principle of relativity Judit X. Madarsz and Mike Stannett and Gergely Szkely LC18 conference July 27, 2018 Rindlers book: SPR Isotropy &


  1. Frames and coordinate systems in the formalization of Einstein’s special principle of relativity Judit X. Madarász and Mike Stannett and Gergely Székely LC18 conference July 27, 2018

  2. � Rindler’s book: SPR ⇐ ⇒ Isotropy & (spacetime) Homogeneity Our CQG paper (joint with Andréka & Németi): ⇒ Isotropy SPR = SPR := Principle of Relativity

  3. � Rindler’s book: ⇒ Isotropy SPR = Our CQG paper (joint with Andréka & Németi): ⇒ Isotropy SPR = SPR := Principle of Relativity

  4. Who is right?

  5. Who is right? Both of us!

  6. Who is right? Both of us! You are also right!

  7. So let’s see how can all of us be right.

  8. SPR according to Einstein in 1905: From Einstein’s paper „Zur Elektrodynamik Bewegter Körper.”

  9. SPR is an (Hence it can be formulated several different ways.)

  10. SPR is an (Hence it can be formulated several different ways.) So the right question to ask is: How are these formalizations related?

  11. W ( k , b , x , y , z , t ) � „observer k coordinatizes body b at spacetime location � x , y , z , t � .” k t b � x , y , z , t � x y Worldline of body b according to observer k = {� x , y , z , t � ∈ Q 4 : W ( k , b , x , y , z , t ) } def wline k ( b )

  12. Language: { B , IOb , Q , + , · , ≤ , W Ph , Etc . } � Q , + , · , ≤� B W IOb Ph B � Bodies (things that move) IOb � Inertial Observers Q � Quantities + , · and ≤ � field operations and ordering W � Worldview (a 6-ary relation of sort BBQQQQ ) Ph � Photons (light signals)

  13. AxOField: The structure of quantities � Q , + , · , ≤� is an ordered field, Rational numbers: Q , √ √ Q ( 2 ) , Q ( 3 ) , Q ( π ) , . . . Computable numbers, Constructable numbers, Real algebraic numbers: A ∩ R , Real numbers : R , Hyperrational numbers: Q ∗ , Hyperreal numbers: R ∗ , Etc.

  14. A principle of relativity S – the set of experimental scenarios .

  15. A principle of relativity S – the set of experimental scenarios . CoordSPR: Every experimental scenario ϕ ∈ S is either realizable by every inertial observer or by none of them. For all ϕ ∈ S : IOb ( k ) , IOb ( k ′ ) = ⇒ ϕ ( k ′ , ¯ � � ⇒ ϕ ( k , ¯ x ) ⇐ x ) .

  16. Example CoordSPR: For all ϕ ∈ S : IOb ( k ) , IOb ( k ′ ) = ⇒ ϕ ( k ′ , ¯ ⇒ � x ) ⇐ � ϕ ( k , ¯ x ) . k ′ k b ′ b � � ϕ ( k , c ) ≡ ( ∃ b ∈ B ) speed k ( b ) > c

  17. Example CoordSPR: For all ϕ ∈ S : IOb ( k ) , IOb ( k ′ ) = ⇒ ϕ ( k ′ , ¯ ⇒ � x ) ⇐ � ϕ ( k , ¯ x ) . k ′ b ′ k b � � ϕ ( k , c ) ≡ ( ∃ b ∈ B ) speed k ( b ) > c

  18. CoordSPR: For all ϕ ∈ S : IOb ( k ) , IOb ( k ′ ) = ⇒ ϕ ( k ′ , ¯ � � ⇒ ϕ ( k , ¯ x ) ⇐ x ) . Experimental scenarios ( S ) = ???

  19. CoordSPR: For all ϕ ∈ S : IOb ( k ) , IOb ( k ′ ) = ⇒ ϕ ( k ′ , ¯ � � ⇒ ϕ ( k , ¯ x ) ⇐ x ) . Experimental scenarios ( S ) = ??? S ⊆ „Formulas expressible in the language of the theory.”

  20. CoordSPR: For all ϕ ∈ S : IOb ( k ) , IOb ( k ′ ) = ⇒ ϕ ( k ′ , ¯ � � ⇒ ϕ ( k , ¯ x ) ⇐ x ) . Experimental scenarios ( S ) = ??? S ⊆ „Formulas expressible in the language of the theory.” We need a free variable for the observer on which we will evaluate the formula.

  21. CoordSPR: For all ϕ ∈ S : IOb ( k ) , IOb ( k ′ ) = ⇒ ϕ ( k ′ , ¯ � � ⇒ ϕ ( k , ¯ x ) ⇐ x ) . Experimental scenarios ( S ) = ??? S ⊆ „Formulas expressible in the language of the theory.” We need a free variable for the observer on which we will evaluate the formula. We would like to use numbers as parameters.

  22. CoordSPR: For all ϕ ∈ S : IOb ( k ) , IOb ( k ′ ) = ⇒ ϕ ( k ′ , ¯ � � ⇒ ϕ ( k , ¯ x ) ⇐ x ) . Experimental scenarios ( S ) = ??? S ⊆ „Formulas expressible in the language of the theory.” We need a free variable for the observer on which we will evaluate the formula. We would like to use numbers as parameters. CoordSPR + : when S contains all the formulas having only 1 free variable of sort bodies.

  23. What does SPR imply?

  24. AxLight: There is at least one inertial observer according to who, every light signal moves with the same velocity in every direction. k t ¯ y y ) 2 time (¯ x , ¯ p x space 2 (¯ x , ¯ y ) x ¯ y  � �  ( ∃ p ∈ Ph ) x , ¯ ¯ y ∈ wline k ( p ) y ∈ Q 4 ) ( ∃ k ∈ IOb )( ∃ c ∈ Q )( ∀ ¯ x ¯ �   y ) = c 2 · time (¯ space 2 (¯ y ) 2 x , ¯ x , ¯

  25. AxPh: According to every inertial observer, every light signal moves with the same velocity in every direction. k ′ t k t y ¯ y ¯ y ) 2 y ) 2 time (¯ x , ¯ time (¯ x , ¯ p p ′ x x space 2 (¯ space 2 (¯ x , ¯ y ) x , ¯ y ) ¯ x x ¯ y y  � �  ( ∃ p ∈ Ph ) x , ¯ ¯ y ∈ wline k ( p ) y ∈ Q 4 ) ( ∀ k ∈ IOb )( ∃ c ∈ Q )( ∀ ¯ x ¯ �   y ) = c 2 · time (¯ space 2 (¯ y ) 2 x , ¯ x , ¯

  26. Proposition: (Assuming AxOField) CoordSPR + , AxLight = ⇒ AxPh � � ϕ ( k , ¯ x , ¯ y ) ≡ ( ∃ p ∈ Ph ) ¯ x , ¯ y ∈ wline k ( p ) ∈ S .

  27. Isotropy: Rotations do not effect the outcomes of experiments (and the experiments can be rotated). For all ϕ ∈ S : w kk ′ „is a rotation restricted to space,” IOb ( k ) , IOb ( k ′ ) = ⇒ ϕ ( k ′ , ¯ � � ⇒ ϕ ( k , ¯ x ) ⇐ x ) . and ( ∀ k ∈ IOb )( ∀ R „spatial rotation” )( ∃ k ′ ∈ IOb ) � � w kk ′ = R where w kk ′ is the worldview transformation between k and k ′ : def w kk ′ ( x , y , z , t : x ′ , y ′ , z ′ , t ′ ) ⇒ W ( k ′ , b , x ′ , y ′ , z ′ , t ′ ) . ⇐ ⇒ ∀ b W ( k , b , x , y , z , t ) ⇐

  28. Proposition: (assuming AxOField) AxTriv , CoordSPR = ⇒ Isotropy AxTriv: The rotated (around the time-axis) and translated versions of an inertial coordinate systems are also inertial coordinate system.

  29. Coordinates vs frames

  30. Frames vs. coordinate systems From Rindler’s book „Relativity: Special, General, and Cosmological.”

  31. How can we introduce reference frames?

  32. A reference frame is an equivalence class of observers: def k ∼ h ⇐ ⇒ w kh = T ◦ R for some rotation R around the time-axis and (spacetime) translation T .

  33. FrameSPR: Every ϕ ∈ S experimental scenario is either realizable in every inertial frame of reference or in none of them. For all ϕ ∈ S : IOb ( k ) , IOb ( k ′ ) = ⇒ � k ∼ h � k ′ ∼ h ′ � � �� ⇒ ( ∃ h ′ ∈ IOb ) ( ∃ h ∈ IOb ) ⇐ ϕ ( h ′ , ¯ ϕ ( h , ¯ x ) x )

  34. Proposition: (Assuming AxOField) FrameSPR + , AxLight , AxRest = ⇒ AxPh AxRest: Restricted to time or space the worldview transformation between any two inertial observers stationary with respect to each other is a similarity (i.e., isometry up to scaling).

  35. � Proposition: (Assuming AxOField) FrameSPR + , AxLight , AxRest = ⇒ AxPh AxRest: Restricted to time or space the worldview transformation between any two inertial observers stationary with respect to each other is a similarity (i.e., isometry up to scaling). Proposition: FrameSPR + , AxTriv , AxRest , Etc . = ⇒ Isotropy

  36. � ⇒ = FrameSPR CoordSPR ⇐ =

  37. � ⇒ = FrameSPR CoordSPR ⇐ = Thank you for your attention!

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