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  2. Uncertainty principle - Wikipedia

    en.wikipedia.org/wiki/Uncertainty_principle

    The uncertainty principle, also known as Heisenberg's indeterminacy principle, is a fundamental concept in quantum mechanics. It states that there is a limit to the precision with which certain pairs of physical properties, such as position and momentum , can be simultaneously known.

  3. Quantum fluctuation - Wikipedia

    en.wikipedia.org/wiki/Quantum_fluctuation

    3D visualization of quantum fluctuations of the quantum chromodynamics (QCD) vacuum [1]. In quantum physics, a quantum fluctuation (also known as a vacuum state fluctuation or vacuum fluctuation) is the temporary random change in the amount of energy in a point in space, [2] as prescribed by Werner Heisenberg's uncertainty principle.

  4. Noncommutative quantum field theory - Wikipedia

    en.wikipedia.org/wiki/Noncommutative_quantum...

    On the other hand, according to the Heisenberg uncertainty principle, a measurement of a space-time separation causes an uncertainty in momentum inversely proportional to the extent of the separation. Thus energy whose scale corresponds to the uncertainty in momentum is localized in the system within a region corresponding to the uncertainty in ...

  5. Wave function collapse - Wikipedia

    en.wikipedia.org/wiki/Wave_function_collapse

    The concept of wavefunction collapse was introduced by Werner Heisenberg in his 1927 paper on the uncertainty principle, "Über den anschaulichen Inhalt der quantentheoretischen Kinematik und Mechanik", and incorporated into the mathematical formulation of quantum mechanics by John von Neumann, in his 1932 treatise Mathematische Grundlagen der ...

  6. Quantum harmonic oscillator - Wikipedia

    en.wikipedia.org/wiki/Quantum_harmonic_oscillator

    As an example, consider the 3-dimensional case: Define n = n 1 + n 2 + n 3. All states with the same n will have the same energy. For a given n, we choose a particular n 1. Then n 2 + n 3 = n − n 1. There are n − n 1 + 1 possible pairs {n 2, n 3}. n 2 can take on the values 0 to n − n 1, and for each n 2 the value of n 3 is fixed.

  7. Zero-point energy - Wikipedia

    en.wikipedia.org/wiki/Zero-point_energy

    It occurs when all of space is filled with a sea of particles which are charged and thus the field has a nonzero vacuum expectation value. Interaction with the vacuum energy filling the space prevents certain forces from propagating over long distances (as it does in a superconducting medium; e.g., in the Ginzburg–Landau theory).

  8. Virtual particle - Wikipedia

    en.wikipedia.org/wiki/Virtual_particle

    The strong nuclear force between quarks is the result of interaction of virtual gluons. The residual of this force outside of quark triplets (neutron and proton) holds neutrons and protons together in nuclei, and is due to virtual mesons such as the pi meson and rho meson. The weak nuclear force is the result of exchange by virtual W and Z bosons.

  9. Casimir effect - Wikipedia

    en.wikipedia.org/wiki/Casimir_effect

    In quantum field theory, the Casimir effect (or Casimir force) [1] is a physical force acting on the macroscopic boundaries of a confined space which arises from the quantum fluctuations of a field. The term Casimir pressure is sometimes used when it is described in units of force per unit area.