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词汇 example_english_dark-matter
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Examples of dark matter


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In particular, the concepts of darkmatter, dark energy, and cosmic star formation history will be discussed, and their relation to the existence of intelligent life will be explored.
The missing component is known as darkmatter and its nature is unknown.
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Despite not solving the darkmatter problem, microlensing has been shown to be a useful tool for many applications.
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The third peak can be used to get information about the darkmatter density.
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These are not particles in the particle physics sense each particle represents approximately a billion solar masses of darkmatter.
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During matter domination, all causal darkmatter perturbations grow through gravitational clustering.
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At this stage, luminous, baryonic matter is expected to simply mirror the evolution of the dark matter, and their distributions should closely trace one another.
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By mapping the distorted light created by gravitational lensing, astronomers can trace how darkmatter is distributed in the cluster.
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They are not composed of darkmatter; rather, they are much less luminous than a star.
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The tanker collides with an iceberg, and spills darkmatter across the landscape.
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Crystals of high purity germanium are used in detectors for gamma spectroscopy and the search for darkmatter.
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Recent studies have indicated that the galaxy may potentially hold large amounts of darkmatter.
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In the 1980s it was proposed that these may be the explanation for the darkmatter thought to exist in the universe.
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If the two crystals are brought together, they will render all darkmatter useless.
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The centre focuses on research into the nature of darkmatter and dark energy.
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The darkmatter halo separates it from other high velocity clouds which are not so embedded.
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Examples include darkmatter and low-density plasmas subjected to high magnetic fields.
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The motions of more than 60 million particles which represented darkmatter and galactic gas were simulated for a period of 13 billion years.
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In the modern cosmological models, most energy in the universe is in forms that have never been detected directly, namely dark energy and darkmatter.
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Astrometric results are the basis used to calculate the distribution of darkmatter in the galaxy.
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Scientists theorize that the galaxy is held together by huge quantities of darkmatter.
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This is due to the possibility that at this low mass they would behave as expected of other particle candidates for darkmatter.
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The four possible types of matter are known as cold darkmatter, warm darkmatter, hot darkmatter, and baryonic matter.
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Current observations indicate that the dark energy density is already greater than the mass-energy density of radiation and matter (including darkmatter).
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His fields of specialty include low surface brightness galaxies, galaxy formation and evolution, tests of darkmatter and alternative hypotheses, and measurements of cosmological parameters.
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This not only alters the understanding of black holes, but has the potential to explain the dark energy and darkmatter that are indirectly observed.
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Hot darkmatter may include (massive) neutrinos, but observations imply that only a small fraction of darkmatter can be hot.
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There are places where darkmatter seems to be a small component or totally absent.
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Dark fluid combines darkmatter and dark energy in a single energy field that produces different effects at different scales.
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These extra positrons could be produced by darkmatter annihilation, but may also come from pulsars.
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Other ellipticals have low velocities in their outskirts (tracked for example by planetary nebulae) and were interpreted as not having darkmatter haloes.
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There are several powerful experimental reasons to expect new physics, including darkmatter and neutrino mass.
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Lensing mass maps can also potentially reveal dark clusters, clusters containing overdense concentrations of darkmatter but relatively insignificant amounts of baryonic matter.
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This type of darkmatter was postulated to resolve a number of conflicts between observations and simulations on the galactic scale and smaller.
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In theories where supersymmetry is a global symmetry, the goldstino is an ordinary particle (possibly the lightest supersymmetric particle, responsible for darkmatter).
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It has also been suggested that the darkmatter halo can pull the galaxy, thus stopping disk contraction.
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These particles are heavier than warm darkmatter and hot darkmatter, but are lighter than the traditional forms of cold darkmatter.
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A viable way of building light darkmatter models is thus by postulating new light bosons.
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The two factions are in a never-ending war for a rare material called darkmatter.
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In particular, they made the proposal that exotic smoothness structures can be resolve some of the problems in cosmology like darkmatter or dark energy.
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This included star formations, the structure of galaxies, interstellar space, black holes and darkmatter.
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His calculations suggested that there must be more mass in the universe than those apparent in the observable galaxies, and called this darkmatter.
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The gravitational effects of darkmatter are well understood, as it behaves like a cold, non-radiative fluid that forms haloes around galaxies.
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Such rings help in understanding the distribution of darkmatter, dark energy, the nature of distant galaxies, and the curvature of the universe.
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The measured orbital velocities of galaxies within galactic clusters have been found to be consistent with darkmatter observations.
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Another class of theories that unifies darkmatter and dark energy are suggested to be covariant theories of modified gravities.
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Before that, it is thought that the expansion was decelerating, due to the attractive influence of darkmatter and baryons.
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A paranormal phenomenon is different from hypothetical concepts such as darkmatter and dark energy.
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The infalling material (which contains galaxies, gas and darkmatter) gains kinetic energy as it falls into the cluster's gravitational potential well.
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Other areas are darkmatter, cosmology, astrodynamics, binary stars, solar neighborhood, solar physics and astrobiology.
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The model does not contain any viable darkmatter particle that possesses all of the required properties deduced from observational cosmology.
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Indirect evidence for darkmatter comes from its gravitational influence on other matter, as no darkmatter particles have been observed in laboratories.
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Furthermore, cosmological experiments also suggest the existence of darkmatter, supposedly composed of fundamental particles outside the scheme of the standard model.
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These events could include darkmatter, low energy solar neutrinos, double beta decay or rare radioactive decay.
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Analysis concluded that this was a giant cloud of hydrogen gas falling onto a clump of darkmatter in the early universe, creating a protogalaxy.
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This has proven to be very controversial since it implies the non-existence of the non-baryonic darkmatter that is central to physical cosmology.
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In particular, the potential for a tremendous discovery surrounding darkmatter is possible over the next several years.
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Gravitationally, the universe will be dominated by darkmatter, electrons, and positrons (not protons).
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When the deviations from homogeneity are small, the darkmatter may be treated as a pressureless fluid and evolves by very simple equations.
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These searches have ruled out the possibility that these objects make up a significant fraction of darkmatter in our galaxy.
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Cosmologists doubt they make up a majority of darkmatter because the black holes are at isolated points of the galaxy.
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It is designed to measure antimatter in cosmic rays and search for evidence of darkmatter.
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Dubbed dark energy by analogy with darkmatter, it is believed to account for roughly 70% of the universe's energy content.
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While mapping the darkmatter, astronomers found a dark-matter ring near the cluster's center (although this is disputed by other independent studies).
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The ring's discovery is among the strongest evidence that darkmatter exists.
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It has been proposed as a candidate particle to explain the darkmatter content of the universe.
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This provides support for the idea that most of the mass in the cluster pair is in the form of collisionless darkmatter.
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Observational data that is taken as evidence for dark energy and darkmatter could indicate the need for new physics.
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A possible explanation of darkmatter comes from particle physics.
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Research shows that this filament only contains about 20 percent of normal matter, the rest is assumed to be darkmatter.
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Darkmatter is matter that can not be detected by electromagnetic radiation, hence "dark".
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The darkmatter density drops off with distance from the galactic center.
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According to the team, the universe is 13.798 0.037 billion years old, and contains 4.9% ordinary matter, 26.8% darkmatter and 68.3% dark energy.
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It is currently theorised that these ripples gave rise to the present vast cosmic web of galactic clusters and darkmatter.
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According to the team, the universe is 13.7980.037 billion years old, and contains 4.9% ordinary matter, 26.8% darkmatter and 68.3% dark energy.
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Matter distribution throughout the cosmos is also discussed, and the concepts of darkmatter and dark energy come full circle.
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Rather, it implies the presence of a darkmatter halo with tens of billions of solar masses.
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A possible explanation for this problem is the non-luminous darkmatter.
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Since his discovery, astronomers have determined that a large portion of galaxies (and most of the universe) is made up of darkmatter.
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More simply, the question is whether the darkmatter has pressure, and thus can be described as a perfect fluid.
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From these figures, matter accounts for 31.7% of the mass-energy content of the universe, and 84.5% of the matter is darkmatter.
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Instead, the existence and properties of darkmatter are inferred from its gravitational effects on visible matter, radiation, and the large-scale structure of the universe.
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Ordinary (baryonic) matter interacts strongly with radiation whereas, by definition, darkmatter does not.
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Darkmatter acts as a compactor of structure.
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Exceptions to this general picture of darkmatter haloes for galaxies appear to be galaxies with mass-to-light ratios close to that of stars.
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This matter is composed partly of visible galaxies but it is mostly darkmatter.
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Early in the universe, galaxies were composed mostly of gas and darkmatter.
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The theory predicts that in the long term protons or neutrons can be destroyed by interactions with darkmatter.
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It has not yet been determined how the darkmatter and galaxies were separated.
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Fundamental to the structure of the universe is the existence of darkmatter and dark energy.
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Darkmatter gravitationally attracts baryonic matter, and it is this normal matter that astronomers see forming long, thin walls of super-galactic clusters.
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These darkmatter clumps then formed the scaffolding around galaxies and galactic clusters.
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The darkmatter halo is estimated to have 10 times the mass of the stars in the galaxy.
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The galaxy is one of the few elliptical galaxies proven to have significant amounts of darkmatter.
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This mass has been given the name darkmatter.
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The results seem to support the theory that both visible and darkmatter are clumped into web like structures.
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The post-war setting complements the protagonist's presence in the novel, and increases the intensity as he masters the void and all darkmatter.
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However, one may calculate the density of gravitinos and it turns out to be much higher than the observed darkmatter density.
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Darkmatter makes up around 75 percent of the cluster's mass.
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This is inconsistent with predictions from most models of darkmatter sources, in which the positron and antiproton excesses are correlated.
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These examples are from corpora and from sources on the web. Any opinions in the examples do not represent the opinion of the Cambridge Dictionary editors or of Cambridge University Press or its licensors.
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