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  2. Lorentz factor - Wikipedia

    en.wikipedia.org/wiki/Lorentz_factor

    Definition of the Lorentz factor γ. The Lorentz factor or Lorentz term (also known as the gamma factor [1]) is a dimensionless quantity expressing how much the measurements of time, length, and other physical properties change for an object while it moves. The expression appears in several equations in special relativity, and it arises in ...

  3. Lorenz system - Wikipedia

    en.wikipedia.org/wiki/Lorenz_system

    Time t = 2: Time t = 3: These figures — made using ρ = 28, σ = 10 and β = ⁠ 8 / 3 ⁠ — show three time segments of the 3-D evolution of two trajectories (one in blue, the other in yellow) in the Lorenz attractor starting at two initial points that differ only by 10 −5 in the x-coordinate. Initially, the two trajectories seem ...

  4. File:Lorentz factor.svg - Wikipedia

    en.wikipedia.org/wiki/File:Lorentz_factor.svg

    21:45, 2 March 2010: 1,102 × 1,118 (17 KB) Trassiorf {{Information |Description=Lorentz factor as a function of velocity. Graph created with KmPlot, edited with Inkscape. This is well enough, but it takes more than 1000 segments to draw the curve. I simplify it to 4 bézier arcs. |So: 12:53, 6 October 2007: 1,102 × 1,118 (195 KB) Egg: 12:23 ...

  5. Classical electromagnetism and special relativity - Wikipedia

    en.wikipedia.org/wiki/Classical_electromagnetism...

    is called the Lorentz factor and c is the speed of light in free space. Lorentz factor (γ) is the same in both systems. The inverse transformations are the same except for the substitution v → −v. An equivalent, alternative expression is: [3]

  6. Lorentz transformation - Wikipedia

    en.wikipedia.org/wiki/Lorentz_transformation

    It may include a rotation of space; a rotation-free Lorentz transformation is called a Lorentz boost. In Minkowski space—the mathematical model of spacetime in special relativity—the Lorentz transformations preserve the spacetime interval between any two events. They describe only the transformations in which the spacetime event at the ...

  7. Ultrarelativistic limit - Wikipedia

    en.wikipedia.org/wiki/Ultrarelativistic_limit

    Below are few ultrarelativistic approximations when .The rapidity is denoted : ⁡ Motion with constant proper acceleration: d ≈ e aτ /(2a), where d is the distance traveled, a = dφ/dτ is proper acceleration (with aτ ≫ 1), τ is proper time, and travel starts at rest and without changing direction of acceleration (see proper acceleration for more details).

  8. Sprouts (game) - Wikipedia

    en.wikipedia.org/wiki/Sprouts_(game)

    A 2-spot game of Sprouts. The game ends when the first player is unable to draw a connecting line between the only two free points, marked in green. The game is played by two players, [2] starting with a few spots drawn on a sheet of paper. Players take turns, where each turn consists of drawing a line between two spots (or from a spot to ...

  9. Covariant formulation of classical electromagnetism - Wikipedia

    en.wikipedia.org/wiki/Covariant_formulation_of...

    The covariant formulation of classical electromagnetism refers to ways of writing the laws of classical electromagnetism (in particular, Maxwell's equations and the Lorentz force) in a form that is manifestly invariant under Lorentz transformations, in the formalism of special relativity using rectilinear inertial coordinate systems.