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  2. Standard Model - Wikipedia

    en.wikipedia.org/wiki/Standard_Model

    The Standard Model of particle physics is the theory describing three of the four known fundamental forces (electromagnetic, weak and strong interactions – excluding gravity) in the universe and classifying all known elementary particles.

  3. Three-body problem - Wikipedia

    en.wikipedia.org/wiki/Three-body_problem

    While a system of 3 bodies interacting gravitationally is chaotic, a system of 3 bodies interacting elastically is not. [clarification needed] There is no general closed-form solution to the three-body problem. [1] In other words, it does not have a general solution that can be expressed in terms of a finite number of standard mathematical ...

  4. Kuramoto model - Wikipedia

    en.wikipedia.org/wiki/Kuramoto_model

    Similarly, the state space of the N=3 case is a 2-dimensional torus, and so the system evolves as a flow on the 2-torus, which cannot be chaotic. Chaos first occurs when N=4. For some settings of ω 1 , ω 2 , ω 3 , K {\displaystyle \omega _{1},\omega _{2},\omega _{3},K} , the system has a strange attractor .

  5. Absolute space and time - Wikipedia

    en.wikipedia.org/wiki/Absolute_space_and_time

    The space R 3 is endowed with a scalar product , . Time is a scalar which is the same in all space E 3 and is denoted as t. The ordered set { t} is called a time axis. Motion (also path or trajectory) is a function r : Δ → R 3 that maps a point in the interval Δ from the time axis to a position (radius vector) in R 3.

  6. Skylab 3 - Wikipedia

    en.wikipedia.org/wiki/Skylab_3

    Skylab 3 (also SL-3 and SLM-2 [2]) was the second crewed mission to the first American space station, Skylab. The mission began on July 28, 1973, with the launch of NASA astronauts Alan Bean , Owen Garriott , and Jack Lousma in the Apollo command and service module on the Saturn IB rocket, and lasted 59 days, 11 hours and 9 minutes. [ 3 ]

  7. Reaction (physics) - Wikipedia

    en.wikipedia.org/wiki/Reaction_(physics)

    F 3. force by support on object (upward) F 4. force by object on support (downward) Forces F 1 and F 2 are equal, due to Newton's third law; the same is true for forces F 3 and F 4. Forces F 1 and F 3 are equal if and only if the object is in equilibrium, and no other forces are applied. (This has nothing to do with Newton's third law.)

  8. Potts model - Wikipedia

    en.wikipedia.org/wiki/Potts_model

    The four-state Potts model is sometimes known as the Ashkin–Teller model, [3] after Julius Ashkin and Edward Teller, who considered an equivalent model in 1943. The Potts model is related to, and generalized by, several other models, including the XY model, the Heisenberg model and the N-vector model.

  9. Stellar kinematics - Wikipedia

    en.wikipedia.org/wiki/Stellar_kinematics

    Barnard's Star, showing position every 5 years in the period 1985–2005.Barnard's Star is the star with the highest proper motion. [1]In astronomy, stellar kinematics is the observational study or measurement of the kinematics or motions of stars through space.