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  2. Quadrupole formula - Wikipedia

    en.wikipedia.org/wiki/Quadrupole_formula

    After a long history of debate on its physical correctness, observations of energy loss due to gravitational radiation in the Hulse–Taylor binary discovered in 1974 confirmed the result, with agreement up to 0.2 percent (by 2005). [2]

  3. Tired light - Wikipedia

    en.wikipedia.org/wiki/Tired_light

    The simplest form of a tired light theory assumes an exponential decrease in photon energy with distance traveled: = ⁡ where () is the energy of the photon at distance from the source of light, is the energy of the photon at the source of light, and is a large constant characterizing the "resistance of the space".

  4. Radiative transfer - Wikipedia

    en.wikipedia.org/wiki/Radiative_transfer

    Radiative transfer (also called radiation transport) is the physical phenomenon of energy transfer in the form of electromagnetic radiation.The propagation of radiation through a medium is affected by absorption, emission, and scattering processes.

  5. Stellar structure - Wikipedia

    en.wikipedia.org/wiki/Stellar_structure

    For energy transport refer to Radiative transfer.. The different transport mechanisms of high-mass, intermediate-mass and low-mass stars. Different layers of the stars transport heat up and outwards in different ways, primarily convection and radiative transfer, but thermal conduction is important in white dwarfs.

  6. Glossary of astronomy - Wikipedia

    en.wikipedia.org/wiki/Glossary_of_astronomy

    A-type star In the Harvard spectral classification system, a class of main-sequence star having spectra dominated by Balmer absorption lines of hydrogen. Stars of spectral class A are typically blue-white or white in color, measure between 1.4 and 2.1 times the mass of the Sun, and have surface temperatures of 7,600–10,000 kelvin.

  7. Spectral energy distribution - Wikipedia

    en.wikipedia.org/wiki/Spectral_Energy_Distribution

    The SED of M51 (upper right) obtained by combining data at many different wavelengths, e.g. UV, visible, and infrared (left). A spectral energy distribution (SED) is a plot of energy versus frequency or wavelength of light (not to be confused with a 'spectrum' of flux density vs frequency or wavelength). [1]

  8. Reionization - Wikipedia

    en.wikipedia.org/wiki/Reionization

    As a consequence, Population III stars are currently considered the most likely energy source to initiate the reionization of the universe, [60] though other sources are likely to have taken over and driven reionization to completion. In June 2015, astronomers reported evidence for Population III stars in the Cosmos Redshift 7 galaxy at z = 6.60.

  9. Matter power spectrum - Wikipedia

    en.wikipedia.org/wiki/Matter_power_spectrum

    Let () represent the matter overdensity, a dimensionless quantity defined as: = ¯ ¯, where ¯ is the average matter density over all space.. The power spectrum is most commonly understood as the Fourier transform of the autocorrelation function, , mathematically defined as: = (′) = (), for = ′.