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  2. Dark energy - Wikipedia

    en.wikipedia.org/wiki/Dark_energy

    The density of dark matter in an expanding universe decreases more quickly than dark energy, and eventually the dark energy dominates. Specifically, when the volume of the universe doubles, the density of dark matter is halved, but the density of dark energy is nearly unchanged (it is exactly constant in the case of a cosmological constant).

  3. Electron - Wikipedia

    en.wikipedia.org/wiki/Electron

    The energy change E 2 − E 1 determines the frequency f of the emitted photon. Photons mediate electromagnetic interactions between particles in quantum electrodynamics. An isolated electron at a constant velocity cannot emit or absorb a real photon; doing so would violate conservation of energy and momentum. Instead, virtual photons can ...

  4. Cosmological constant - Wikipedia

    en.wikipedia.org/wiki/Cosmological_constant

    A positive vacuum energy density resulting from a cosmological constant implies a negative pressure, and vice versa. If the energy density is positive, the associated negative pressure will drive an accelerated expansion of the universe, as observed. (See Dark energy and Cosmic inflation for details.)

  5. Dark energy does not exist, some scientists have claimed – which could help get rid of one of the universe’s biggest mysteries. For a century, scientists have thought that the universe was ...

  6. This new cosmological map shines some light on dark energy

    www.aol.com/cosmological-map-shines-light-dark...

    Dark energy is one of the greatest mysteries in science today. One of the simplest explanations is that it is a “cosmological constant” – a result of the energy of empty space itself – an ...

  7. List of particles - Wikipedia

    en.wikipedia.org/wiki/List_of_particles

    The field equations of condensed matter physics are remarkably similar to those of high energy particle physics. As a result, much of the theory of particle physics applies to condensed matter physics as well; in particular, there are a selection of field excitations, called quasi-particles , that can be created and explored.

  8. Dirac equation - Wikipedia

    en.wikipedia.org/wiki/Dirac_equation

    The infinitely negative contributions from the sea of negative-energy electrons have to be canceled by an infinite positive "bare" energy and the contribution to the charge density and current coming from the sea of negative-energy electrons is exactly canceled by an infinite positive "jellium" background so that the net electric charge density ...

  9. Antiparticle - Wikipedia

    en.wikipedia.org/wiki/Antiparticle

    While the electron has a negative electric charge, the positron has a positive electric charge, and is produced naturally in certain types of radioactive decay. The opposite is also true: the antiparticle of the positron is the electron. Some particles, such as the photon, are their own antiparticle. Otherwise, for each pair of antiparticle ...