redshift oor Sweeds

redshift

naamwoord
en
(physics) A change in the wavelength of light, in which the wavelength is longer than when it was emitted at the source.

Vertalings in die woordeboek Engels - Sweeds

rödförskjutning

naamwoordalgemene
en
change in wavelength
Physicists call this phenomenon gravitational redshift.
Fysiker kallar detta fenomen relativistisk rödförskjutning.
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During the quasar controversies of the 1970s, these same astronomers were also of the opinion that quasars exhibited high redshifts not due to their incredible distance but rather due to unexplained intrinsic redshift mechanisms that would cause the periodicities and cast doubt on the Big Bang.
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The value of the Hubble constant is estimated by measuring the redshift of distant galaxies and then determining the distances to the same galaxies (by some other method than Hubble's law).
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Additionally, in an expanding universe, distant objects recede from us, which causes the light emanated from them to be redshifted and diminished in brightness by the time we see it.
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This expansion is consistent with the observation that the light from distant galaxies has been redshifted; the photons emitted have been stretched to longer wavelengths and lower frequency during their journey.
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To achieve this, the spacecraft will measure the redshift of galaxies at varying distances from Earth and investigate the relationship between distance and redshift.
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Light from an object that is moving away from an observer is reddish and is called redshifted.
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Gravitational redshift has been measured in the laboratory and using astronomical observations.
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Tolman's test compares the surface brightness of galaxies as a function of their redshift (measured as z).
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In 2013, the second true triplet quasars QQQ J1519+0627 was found with redshift z = 1.51 (approx 9 billion light-years) by an international team of astronomers led by Farina of the University of Insubria, the whole system is well accommodated within 25 (i.e., 200 kpc in projected distance).
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The link between galactic shapes and their corresponding redshift will give a look into how dark energy contributes to the increased acceleration of the universe.
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Physicists call this phenomenon gravitational redshift.
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Euclid will measure spectroscopic redshifts for 50 million objects.
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Euclid will probe the history of the expansion of the universe and the formation of cosmic structures by measuring the redshift of galaxies out to a factor of 2, which is equivalent to seeing back 10 billion years in the past.
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In contrast, the spectra of most other galaxies are redshifted.
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The first two were famous for suggesting that there were periodicities in the redshift distributions of galaxies and quasars.
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At the time of discovery and development of Hubble's law, it was acceptable to explain redshift phenomenon as a Doppler shift in the context of special relativity, and use the Doppler formula to associate redshift z with velocity.
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The light from very distant galaxies is significantly affected by the cosmological redshift.
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One of the most fundamental findings was the discovery of large numbers of galaxies with high redshift values.
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In reality we determine, say, a supernova brightness, which provides information about its distance, and the redshift z = ∆λ/λ of its spectrum of radiation.
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Currently, she is a professor emeritus of physics at UCSD and continues to be active in research, including non-standard cosmologies such as intrinsic redshift.
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Significantly, apart from a few nearby galaxies, all known galaxies have spectral lines that are redshifted.
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Examples of such differences include gravitational time dilation, gravitational lensing, the gravitational redshift of light, and the gravitational time delay.
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But using different assumptions about the special-relativistic frames (such as their being earth-fixed, or in free fall), one can derive different predictions for the gravitational redshift, that is, the way in which the frequency of light shifts as the light propagates through a gravitational field (cf. below).
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Spectroscopic measurements will permit measuring the redshifts of galaxies and determining their distances using the Hubble's Law.
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In its present incarnation (2015), a large fraction of its primary mission will be focused on probing the expansion history of the Universe and the growth of cosmic structure with multiple methods in overlapping redshift ranges, with the goal of precisely measuring the effects of dark energy, the consistency of general relativity, and the curvature of spacetime.
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