enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Kinetic energy - Wikipedia

    en.wikipedia.org/wiki/Kinetic_energy

    For example, for a speed of 10 km/s (22,000 mph) the correction to the non-relativistic kinetic energy is 0.0417 J/kg (on a non-relativistic kinetic energy of 50 MJ/kg) and for a speed of 100 km/s it is 417 J/kg (on a non-relativistic kinetic energy of 5 GJ/kg). The relativistic relation between kinetic energy and momentum is given by

  3. Tests of relativistic energy and momentum - Wikipedia

    en.wikipedia.org/wiki/Tests_of_relativistic...

    Kinetic energy in special relativity and Newtonian mechanics. Relativistic kinetic energy increases to infinity when approaching the speed of light, thus no massive body can reach this speed. Tests of relativistic energy and momentum are aimed at measuring the relativistic expressions for energy, momentum, and mass.

  4. Energy–momentum relation - Wikipedia

    en.wikipedia.org/wiki/Energy–momentum_relation

    For photons, this is the relation, discovered in 19th century classical electromagnetism, between radiant momentum (causing radiation pressure) and radiant energy. If the body's speed v is much less than c, then reduces to E = ⁠ 1 / 2 ⁠ m 0 v 2 + m 0 c 2; that is, the body's total energy is simply its classical kinetic energy (⁠ 1 / 2 ...

  5. Proper velocity - Wikipedia

    en.wikipedia.org/wiki/Proper_velocity

    The dashed red curve is γ − 1 (kinetic energy K/mc 2), while the dashed magenta curve is the relativistic Doppler factor. In relativity , proper velocity (also known as celerity ) w of an object relative to an observer is the ratio between observer-measured displacement vector x {\displaystyle {\textbf {x}}} and proper time τ elapsed on the ...

  6. List of relativistic equations - Wikipedia

    en.wikipedia.org/wiki/List_of_relativistic_equations

    In this context, "speed of light" really refers to the speed supremum of information transmission or of the movement of ordinary (nonnegative mass) matter, locally, as in a classical vacuum. Thus, a more accurate description would refer to c 0 {\displaystyle c_{0}} rather than the speed of light per se.

  7. Ultrarelativistic limit - Wikipedia

    en.wikipedia.org/wiki/Ultrarelativistic_limit

    The energy of an ultrarelativistic particle is almost completely due to its kinetic energy = (). The total energy can also be approximated as E = γ m c 2 ≈ p c {\displaystyle E=\gamma mc^{2}\approx pc} where p = γ m v {\displaystyle p=\gamma mv} is the Lorentz invariant momentum .

  8. Mass–energy equivalence - Wikipedia

    en.wikipedia.org/wiki/Mass–energy_equivalence

    The same relations in different notation were used by Lorentz in 1913 and 1914, though he placed the energy on the left-hand side: ε = Mc 2 and ε 0 = mc 2, with ε being the total energy (rest energy plus kinetic energy) of a moving material point, ε 0 its rest energy, M the relativistic mass, and m the invariant mass.

  9. Relativistic mechanics - Wikipedia

    en.wikipedia.org/wiki/Relativistic_mechanics

    In physics, relativistic mechanics refers to mechanics compatible with special relativity (SR) and general relativity (GR). It provides a non-quantum mechanical description of a system of particles, or of a fluid, in cases where the velocities of moving objects are comparable to the speed of light c.