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  2. Schwinger model - Wikipedia

    en.wikipedia.org/wiki/Schwinger_model

    This model exhibits confinement of the fermions and as such, is a toy model for QCD. A handwaving argument why this is so is because in two dimensions, classically, the potential between two charged particles goes linearly as r {\displaystyle r} , instead of 1 / r {\displaystyle 1/r} in 4 dimensions, 3 spatial, 1 time.

  3. Dyon - Wikipedia

    en.wikipedia.org/wiki/Dyon

    Dyons were first proposed by Julian Schwinger in 1969 as a phenomenological alternative to quarks. [1] He extended the Dirac quantization condition to the dyon and used the model to predict the existence of a particle with the properties of the J/ψ meson prior to its discovery in 1974.

  4. Keldysh formalism - Wikipedia

    en.wikipedia.org/wiki/Keldysh_formalism

    In non-equilibrium physics, the Keldysh formalism or Keldysh–Schwinger formalism is a general framework for describing the quantum mechanical evolution of a system in a non-equilibrium state or systems subject to time varying external fields (electrical field, magnetic field etc.).

  5. Interaction picture - Wikipedia

    en.wikipedia.org/wiki/Interaction_picture

    By utilizing the interaction picture, one can use time-dependent perturbation theory to find the effect of H 1,I, [15]: 355ff e.g., in the derivation of Fermi's golden rule, [15]: 359–363 or the Dyson series [15]: 355–357 in quantum field theory: in 1947, Shin'ichirō Tomonaga and Julian Schwinger appreciated that covariant perturbation ...

  6. Color confinement - Wikipedia

    en.wikipedia.org/wiki/Color_confinement

    In addition to QCD in four spacetime dimensions, the two-dimensional Schwinger model also exhibits confinement. [9] Compact Abelian gauge theories also exhibit confinement in 2 and 3 spacetime dimensions. [10] Confinement has been found in elementary excitations of magnetic systems called spinons. [11]

  7. Quantum cosmology - Wikipedia

    en.wikipedia.org/wiki/Quantum_cosmology

    Quantum cosmology [1] [2] is the attempt in theoretical physics to develop a quantum theory of the universe.This approach attempts to answer open questions of classical physical cosmology, particularly those related to the first phases of the universe.

  8. Relativistic wave equations - Wikipedia

    en.wikipedia.org/wiki/Relativistic_wave_equations

    In 1941, Rarita and Schwinger focussed on spin-3 ⁄ 2 particles and derived the Rarita–Schwinger equation, including a Lagrangian to generate it, and later generalized the equations analogous to spin n + 1 ⁄ 2 for integer n. In 1945, Pauli suggested Majorana's 1932 paper to Bhabha, who returned to the general ideas introduced by Majorana ...

  9. Schwinger's quantum action principle - Wikipedia

    en.wikipedia.org/wiki/Schwinger's_quantum_action...

    In Schwinger's approach, the action principle is targeted towards quantum mechanics. The action becomes a quantum action , i.e. an operator, S {\displaystyle S} . Although it is superficially different from the path integral formulation where the action is a classical function, the modern formulation of the two formalisms are identical.