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  2. Stability of matter - Wikipedia

    en.wikipedia.org/wiki/Stability_of_matter

    Classical physics predicts that such systems should be inherently unstable due to attractive and repulsive electrostatic forces between charges, and thus the stability of matter was a theoretical problem that required a quantum mechanical explanation.

  3. Pauli exclusion principle - Wikipedia

    en.wikipedia.org/wiki/Pauli_exclusion_principle

    In 1995 Elliott Lieb and coworkers showed that the Pauli principle still leads to stability in intense magnetic fields such as in neutron stars, although at a much higher density than in ordinary matter. [19] It is a consequence of general relativity that, in sufficiently intense gravitational fields, matter collapses to form a black hole.

  4. Elliott H. Lieb - Wikipedia

    en.wikipedia.org/wiki/Elliott_H._Lieb

    Lieb has been awarded several prizes in mathematics and physics, including the Heineman Prize for Mathematical Physics of the American Physical Society and the American Institute of Physics (1978), [9] the Max Planck Medal of the German Physical Society (1992), [10] the Boltzmann medal of the International Union of Pure and Applied Physics (1998), [11] the Schock Prize (2001), [12] the Henri ...

  5. Island of stability - Wikipedia

    en.wikipedia.org/wiki/Island_of_stability

    In nuclear physics, the island of stability is a predicted set of isotopes of superheavy elements that may have considerably longer half-lives than known isotopes of these elements. It is predicted to appear as an "island" in the chart of nuclides , separated from known stable and long-lived primordial radionuclides .

  6. Topological defect - Wikipedia

    en.wikipedia.org/wiki/Topological_defect

    The existence of a topological defect can be demonstrated whenever the boundary conditions entail the existence of homotopically distinct solutions. Typically, this occurs because the boundary on which the conditions are specified has a non-trivial homotopy group which is preserved in differential equations; the solutions to the differential equations are then topologically distinct, and are ...

  7. Degenerate matter - Wikipedia

    en.wikipedia.org/wiki/Degenerate_matter

    Degenerate matter occurs when the Pauli exclusion principle significantly alters a state of matter at low temperature. The term is used in astrophysics to refer to dense stellar objects such as white dwarfs and neutron stars , where thermal pressure alone is not enough to prevent gravitational collapse .

  8. Floquet theory - Wikipedia

    en.wikipedia.org/wiki/Floquet_theory

    Floquet theory shows stability in Hill differential equation (introduced by George William Hill) approximating the motion of the moon as a harmonic oscillator in a periodic gravitational field. Bond softening and bond hardening in intense laser fields can be described in terms of solutions obtained from the Floquet theorem.

  9. Earnshaw's theorem - Wikipedia

    en.wikipedia.org/wiki/Earnshaw's_theorem

    Informally, the case of a point charge in an arbitrary static electric field is a simple consequence of Gauss's law.For a particle to be in a stable equilibrium, small perturbations ("pushes") on the particle in any direction should not break the equilibrium; the particle should "fall back" to its previous position.