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  2. Euler's three-body problem - Wikipedia

    en.wikipedia.org/wiki/Euler's_three-body_problem

    The problem of two fixed centers conserves energy; in other words, the total energy is a constant of motion.The potential energy is given by =where represents the particle's position, and and are the distances between the particle and the centers of force; and are constants that measure the strength of the first and second forces, respectively.

  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. List of equations in quantum mechanics - Wikipedia

    en.wikipedia.org/wiki/List_of_equations_in...

    One particle: N particles: One dimension ^ = ^ + = + ^ = = ^ + (,,) = = + (,,) where the position of particle n is x n. = + = = +. (,) = /.There is a further restriction — the solution must not grow at infinity, so that it has either a finite L 2-norm (if it is a bound state) or a slowly diverging norm (if it is part of a continuum): [1] ‖ ‖ = | |.

  5. Mathematical formulation of the Standard Model - Wikipedia

    en.wikipedia.org/wiki/Mathematical_formulation...

    Standard Model of Particle Physics. The diagram shows the elementary particles of the Standard Model (the Higgs boson, the three generations of quarks and leptons, and the gauge bosons), including their names, masses, spins, charges, chiralities, and interactions with the strong, weak and electromagnetic forces.

  6. Position operator - Wikipedia

    en.wikipedia.org/wiki/Position_operator

    We write the eigenvalue equation in position coordinates, ^ = = recalling that ^ simply multiplies the wave-functions by the function , in the position representation. Since the function x {\displaystyle \mathrm {x} } is variable while x 0 {\displaystyle x_{0}} is a constant, ψ {\displaystyle \psi } must be zero everywhere except at the point ...

  7. Matrix mechanics - Wikipedia

    en.wikipedia.org/wiki/Matrix_mechanics

    Before matrix mechanics, the old quantum theory described the motion of a particle by a classical orbit, with well defined position and momentum X(t), P(t), with the restriction that the time integral over one period T of the momentum times the velocity must be a positive integer multiple of the Planck constant = =.

  8. Uncertainty principle - Wikipedia

    en.wikipedia.org/wiki/Uncertainty_principle

    Position x and momentum p wavefunctions corresponding to quantum particles. The colour opacity of the particles corresponds to the probability density of finding the particle with position x or momentum component p. Top: If wavelength λ is unknown, so are momentum p, wave-vector k and energy E (de Broglie relations).

  9. Dirac equation - Wikipedia

    en.wikipedia.org/wiki/Dirac_equation

    The Dirac equation in the form originally proposed by Dirac is: [7]: 291 [8] (+ =) (,) = (,) where ψ(x, t) is the wave function for an electron of rest mass m with spacetime coordinates x, t. p 1, p 2, p 3 are the components of the momentum, understood to be the momentum operator in the Schrödinger equation.