dark energy


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Related to dark energy: dark matter, black hole

dark energy,

repulsive force that opposes the self-attraction of matter (see gravitationgravitation,
the attractive force existing between any two particles of matter. The Law of Universal Gravitation

Since the gravitational force is experienced by all matter in the universe, from the largest galaxies down to the smallest particles, it is often called
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) and causes the expansion of the universe to accelerate. The search for dark energy was triggered by the discovery (1998) in images from the Hubble Space TelescopeHubble Space Telescope
(HST), the first large optical orbiting observatory. Built from 1978 to 1990 at a cost of $1.5 billion, the HST (named for astronomer E. P. Hubble) was expected to provide the clearest view yet obtained of the universe from a position some 350 mi (560 km)
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 of a distant supernova that implied an accelerating, expanding universe, which in turn required a new cosmological model (see cosmologycosmology,
area of science that aims at a comprehensive theory of the structure and evolution of the entire physical universe. Modern Cosmological Theories
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). Although dark energy is predicted in particle physics, it has never been directly observed. It is generally agreed, however, that dark energy dominates the universe, which is estimated to have a composition of about 68–70% dark energy, 26–27% dark matterdark matter,
material that is believed to make up nearly 27% of the mass of the universe but is not readily visible because it neither emits nor reflects electromagnetic radiation, such as light or radio signals.
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, and 4–5% normal visible matter such as stars. By 2006, astronomers using the space telescope to examine more distant supernovas had found evidence of the effects of dark energy dating to 9 billion years ago. Observations with the Chandra X-ray Observatory, published in 2008, indicate that dark energy is also retarding the growth of distant galaxy clusters.

The concept of dark energy was first proposed, and then discarded, by Albert Einstein early in the 20th cent. His theory of general relativityrelativity,
physical theory, introduced by Albert Einstein, that discards the concept of absolute motion and instead treats only relative motion between two systems or frames of reference.
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 implied that the pull of gravity would make the universe collapse, but, like many scientists of his time, he assumed the universe to be static and unchanging. To make his equations fit these assumptions, Einstein added a "cosmological constant" whose effect was repulsive. When American astronomer Edwin HubbleHubble, Edwin Powell,
1889–1953, American astronomer, b. Marshfield, Mo. He did research (1914–17) at Yerkes Observatory, and joined (1919) the staff of Mt. Wilson Observatory, Pasadena, Calif., of which he became director. Building on V. M.
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 discovered that the universe was expanding, it was assumed that the universe must be slowing down because of gravity and might even come to a halt. This led Einstein to remove the cosmological constant from his equations and to say that it had been the biggest blunder of his career.

dark energy

The energy associated with the acceleration of the expansion of the Universe. About three-quarters of the energy of the Universe exists in the form of dark energy. The existence of dark energy can be taken into account using a nonzero value for the cosmological constant but the nature of this energy is not understood at the present time.
References in periodicals archive ?
Beutler et al., "The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations," Monthly Notices of the Royal Astronomical Society, vol.
Some physicists propose dark energy is a 'fifth' force that acts on matter, beyond the four already known - gravitational, electromagnetic, and the strong and weak nuclear forces.
"It tells us what dark energy has been doing during that time, as well as other things like the curvature of space - which is what gets us cosmologists excited."
More evidence for dark energy came from clever experiments looking at deep space and echoes of the Big Bang, as well as observing minute oscillations in gravitational waves on Earth, but none of these showed what dark energy looked like or what its physical state might be.
For 15 years, there have been models in string theory that have been thought to give rise to dark energy. However, these have come in for increasingly harsh criticism, and several researchers are now asserting that none of the models proposed to date are workable.
Tegmark claims that only superintelligence can reengineer the universe to make enough gravity to grapple with dark energy so as to prevent the end of the universe.
The energy conservation equation for dark energy fluid, [T.sup.ij(de).sub.;j] = 0, yields
In this case, we consider that the universe is filled with dark matter ([[rho].sub.m]) and dark energy ([[rho].sub.[LAMBDA]]).
Researchers from the universities of Portsmouth and Rome have found indications that dark matter, the cosmic scaffolding on which the universe is built, is being slowly erased by dark energy.
To help uncover the mystery of dark energy, WFIRST will make incredibly precise measurements of the universe.
In this paper one considers only the role of the matter (baryonic and non-baryonic) and the dark energy.
Projects selected include: using a geochemical clock to predict volcanic eruptions, exploring the effects of Dark Matter and Dark Energy on gravitational theory, checking responsibility, liability and risk in situations where tasks are delegated to intelligent systems, and investigating the role of genetic and environmental factors in embryo brain wiring.