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  2. Gyromagnetic ratio - Wikipedia

    en.wikipedia.org/wiki/Gyromagnetic_ratio

    Here, ⁠ 1 / 2 ⁠ σ μν and F μν stand for the Lorentz group generators in the Dirac space, and the electromagnetic tensor respectively, while A μ is the electromagnetic four-potential. An example for such a particle [9] is the spin ⁠ 1 / 2 ⁠ companion to spin ⁠ 3 / 2 ⁠ in the D (½,1) ⊕ D (1,½) representation space of the ...

  3. Gravitational lensing formalism - Wikipedia

    en.wikipedia.org/wiki/Gravitational_lensing...

    In general relativity, a point mass deflects a light ray with impact parameter by an angle approximately equal to α ^ = 4 G M c 2 b {\displaystyle {\hat {\alpha }}={\frac {4GM}{c^{2}b}}} where G is the gravitational constant , M the mass of the deflecting object and c the speed of light .

  4. List of gravitationally rounded objects of the Solar System

    en.wikipedia.org/wiki/List_of_gravitationally...

    ^ Density derived from the mass divided by the volume. ^ Surface gravity derived from the mass m, the gravitational constant G and the radius r: Gm/r 2. ^ Escape velocity derived from the mass m, the gravitational constant G and the radius r: √ (2Gm)/r.

  5. Radial distribution function - Wikipedia

    en.wikipedia.org/wiki/Radial_distribution_function

    This similarity is not accidental; indeed, substituting in the relations above for the thermodynamic parameters (Equations 7, 9 and 10) yields the corresponding virial expansions. [7] The auxiliary function () is known as the cavity distribution function. [5]:

  6. Specific angular momentum - Wikipedia

    en.wikipedia.org/wiki/Specific_angular_momentum

    In celestial mechanics, the specific relative angular momentum (often denoted or ) of a body is the angular momentum of that body divided by its mass. [1] In the case of two orbiting bodies it is the vector product of their relative position and relative linear momentum, divided by the mass of the body in question.

  7. Distribution function (physics) - Wikipedia

    en.wikipedia.org/wiki/Distribution_function...

    Distribution functions may also feature non-isotropic temperatures, in which each term in the exponent is divided by a different temperature. Plasma theories such as magnetohydrodynamics may assume the particles to be in thermodynamic equilibrium. In this case, the distribution function is Maxwellian. This distribution function allows fluid ...

  8. Specific modulus - Wikipedia

    en.wikipedia.org/wiki/Specific_modulus

    Young's modulus per density; specific stiffness (10 6 m 2 s −2) Young's modulus per density squared (10 3 m 5 kg −1 s −2) Young's modulus per density cubed (m 8 kg −2 s −2) Reference Latex foam, low density, 10% compression [4] 5.9 × 10 ^ −7: 0.06: 9.83 × 10 ^ −6: 0.000164: 0.00273: Reversible Assembled Cellular Composite ...

  9. Dimensionless numbers in fluid mechanics - Wikipedia

    en.wikipedia.org/wiki/Dimensionless_numbers_in...

    Dimensionless numbers (or characteristic numbers) have an important role in analyzing the behavior of fluids and their flow as well as in other transport phenomena. [1] They include the Reynolds and the Mach numbers, which describe as ratios the relative magnitude of fluid and physical system characteristics, such as density, viscosity, speed of sound, and flow speed.

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    gnc mass x density divided by radius 2 and angle 7 is known as one