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  2. Ultrabright electron - Wikipedia

    en.wikipedia.org/wiki/Ultrabright_electron

    An ultrabright electron beam has been defined as having >10 A/cm^2 with spatial coherence of >1 nm. [1] This level of energy in that small of a coherence is a large technical problem, not only in the production of such a beam, but also how to use the beam without destroying the sample in the process of characterization. [1]

  3. Electron - Wikipedia

    en.wikipedia.org/wiki/Electron

    The electron has an intrinsic angular momentum or spin of ⁠ ħ / 2 ⁠. [80] This property is usually stated by referring to the electron as a spin-1/2 particle. [79] For such particles the spin magnitude is ⁠ ħ / 2 ⁠, [84] while the result of the measurement of a projection of the spin on any axis can only be ± ⁠ ħ / 2 ⁠.

  4. Luminosity - Wikipedia

    en.wikipedia.org/wiki/Luminosity

    The apparent magnitude is the observed visible brightness from Earth which depends on the distance of the object. The absolute magnitude is the apparent magnitude at a distance of 10 pc (3.1 × 10 17 m), therefore the bolometric absolute magnitude is a logarithmic measure of the bolometric luminosity.

  5. Magnitude (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Magnitude_(astronomy)

    Magnitude values do not have a unit. The scale is logarithmic and defined such that a magnitude 1 star is exactly 100 times brighter than a magnitude 6 star. Thus each step of one magnitude is times brighter than the magnitude 1 higher. The brighter an object appears, the lower the value of its magnitude, with the brightest objects reaching ...

  6. Apparent magnitude - Wikipedia

    en.wikipedia.org/wiki/Apparent_magnitude

    For example, a magnitude 2.0 star is 2.512 times as bright as a magnitude 3.0 star, 6.31 times as magnitude 4.0, and 100 times magnitude 7.0. The brightest astronomical objects have negative apparent magnitudes: for example, Venus at −4.2 or Sirius at −1.46.

  7. Elementary charge - Wikipedia

    en.wikipedia.org/wiki/Elementary_charge

    The elementary charge, usually denoted by e, is a fundamental physical constant, defined as the electric charge carried by a single proton (+1 e) or, equivalently, the magnitude of the negative electric charge carried by a single electron, which has charge −1 e. [2] [a]

  8. Mass–luminosity relation - Wikipedia

    en.wikipedia.org/wiki/Mass–luminosity_relation

    Since matter is fully ionized in the star core (as well as where the temperature is of the same order of magnitude as inside the core), photons collide mainly with electrons, and so λ satisfies = Here is the electron density and: = is the cross section for electron-photon scattering, equal to Thomson cross-section. α is the fine-structure ...

  9. Atomic units - Wikipedia

    en.wikipedia.org/wiki/Atomic_units

    A set of base units in the atomic system as in one proposal are the electron rest mass, the magnitude of the electronic charge, the Planck constant, and the permittivity. [6] [9] In the atomic units system, each of these takes the value 1; the corresponding values in the International System of Units [10]: 132 are given in the table.