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  2. Radiation pressure - Wikipedia

    en.wikipedia.org/wiki/Radiation_pressure

    The radiation pressure force of the light circulating in the cavity can damp or amplify the oscillation of the mirror on the spring. Main articles: Cavity optomechanics and Laser cooling The reflection of a laser pulse from the surface of an elastic solid can give rise to various types of elastic waves that propagate inside the solid or liquid.

  3. Beam emittance - Wikipedia

    en.wikipedia.org/wiki/Beam_emittance

    The normalized emittance does not change as a function of energy and so can be used to indicate beam degradation if the particles are accelerated. For speeds close to the speed of light, where = / is close to one, the emittance is approximately inversely proportional to the energy. In this case, the physical width of the beam will vary ...

  4. Optical lift - Wikipedia

    en.wikipedia.org/wiki/Optical_lift

    Optical lift is a component of force imparted from uniform light. First CP1 fabricated flying carpets. The ability of light to apply pressure to objects is known as radiation pressure, which was first postulated in 1619 and proven in 1900. This is the principle behind the solar sail, which uses light radiation pressure to move through space.

  5. Angular momentum of light - Wikipedia

    en.wikipedia.org/wiki/Angular_momentum_of_light

    Light, or more generally an electromagnetic wave, carries not only energy but also momentum, which is a characteristic property of all objects in translational motion. The existence of this momentum becomes apparent in the "radiation pressure " phenomenon, in which a light beam transfers its momentum to an absorbing or scattering object, generating a mechanical pressure on it in the process.

  6. Heat transfer physics - Wikipedia

    en.wikipedia.org/wiki/Heat_transfer_physics

    The macroscopic energy equation for infinitesimal volume used in heat transfer analysis is [6] = +, ˙, where q is heat flux vector, −ρc p (∂T/∂t) is temporal change of internal energy (ρ is density, c p is specific heat capacity at constant pressure, T is temperature and t is time), and ˙ is the energy conversion to and from thermal ...

  7. Optical force - Wikipedia

    en.wikipedia.org/wiki/Optical_force

    The optical force is a phenomenon whereby beams of light can attract and repel each other. The force acts along an axis which is perpendicular to the light beams. Because of this, parallel beams can be induced to converge or diverge. The optical force works on a microscopic scale, and cannot currently be detected at larger scales.

  8. Poynting vector - Wikipedia

    en.wikipedia.org/wiki/Poynting_vector

    However, any type of energy has its direction of movement in space, as well as its density, so energy flux vectors can be defined for other types of energy as well, e.g., for mechanical energy. The Umov–Poynting vector [11] discovered by Nikolay Umov in 1874 describes energy flux in liquid and elastic media in a completely generalized view.

  9. Beer–Lambert law - Wikipedia

    en.wikipedia.org/wiki/Beer–Lambert_law

    There are two factors that determine the degree to which a medium containing particles will attenuate a light beam: the number of particles encountered by the light beam, and the degree to which each particle extinguishes the light. [15] Assume that a beam of light enters a material sample. Define z as an axis parallel to the direction of the ...

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