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  2. First observation of gravitational waves - Wikipedia

    en.wikipedia.org/wiki/First_observation_of...

    Indirect observation. [] Evidence of gravitational waves was first deduced in 1974 through the motion of the double neutron star system PSR B1913+16, in which one of the stars is a pulsar that emits electro-magnetic pulses at radio frequencies at precise, regular intervals as it rotates.

  3. Binary black hole - Wikipedia

    en.wikipedia.org/wiki/Binary_black_hole

    The star field behind the black holes is being heavily distorted and appears to rotate and move, due to extreme gravitational lensing, as space-time itself is distorted and dragged around by the rotating black holes. [1] A binary black hole ( BBH ), or black hole binary, is a system consisting of two black holes in close orbit around each other.

  4. Planck's law - Wikipedia

    en.wikipedia.org/wiki/Planck's_law

    The cgs units of spectral radiance B ν are erg·s −1 ·sr −1 ·cm −2 ·Hz −1. The terms B and u are related to each other by a factor of ⁠ 4π / c ⁠ since B is independent of direction and radiation travels at speed c. The spectral radiance can also be expressed per unit wavelength λ instead of per unit frequency. In addition, the ...

  5. Schrödinger equation - Wikipedia

    en.wikipedia.org/wiki/Schrödinger_equation

    e. Schrödinger's equation inscribed on the gravestone of Annemarie and Erwin Schrödinger. ( Newton's dot notation for the time derivative is used.) The Schrödinger equation is a partial differential equation that governs the wave function of a quantum-mechanical system. [1] : 12 Its discovery was a significant landmark in the development ...

  6. Polarization (waves) - Wikipedia

    en.wikipedia.org/wiki/Polarization_(waves)

    However, in many instances the more relevant figure of merit is the polarizer's degree of polarization or extinction ratio, which involve a comparison of g 1 to g 2. Since Jones vectors refer to waves' amplitudes (rather than intensity), when illuminated by unpolarized light the remaining power in the unwanted polarization will be (g 2 /g 1) 2 ...

  7. Particle in a box - Wikipedia

    en.wikipedia.org/wiki/Particle_in_a_box

    The states (B,C,D) are energy eigenstates, but (E,F) are not. In quantum mechanics, the particle in a box model (also known as the infinite potential well or the infinite square well) describes the movement of a free particle in a small space surrounded by impenetrable barriers. The model is mainly used as a hypothetical example to illustrate ...

  8. Unruh effect - Wikipedia

    en.wikipedia.org/wiki/Unruh_effect

    Unruh effect. The Unruh effect (also known as the Fulling–Davies–Unruh effect) is a theoretical prediction in quantum field theory that an observer who is uniformly accelerating through empty space will perceive a thermal bath. This means that even in the absence of any external heat sources, an accelerating observer will detect particles ...

  9. Phase (waves) - Wikipedia

    en.wikipedia.org/wiki/Phase_(waves)

    Plot of one cycle of a sinusoidal function. The phase for each argument value, relative to the start of the cycle, is shown at the bottom, in degrees from 0° to 360° and in radians from 0 to 2π. In physics and mathematics, the phase (symbol φ or ϕ) of a wave or other periodic function of some real variable (such as time) is an angle -like ...