Astronomers Detect Cosmic 'Dark Energy' in Galaxies Nearest Earth

Jan 06, 2010
Plot of velocities versus distances for the Local Group central region and outlying members.The Mkpc units indicated on the horizontal axes are about 3 million light years each from the center. The zero acceleration transition radius region is indicated by a horizontal error bar. The vertical axis is Doppler shift radial velocity in km/s. Note the positive (outward) and negative (inward) velocities in the bound central region along with the dark energy accelerated recession with radius beyond the transition radius. Different Local Group masses in trillions of times the mass of our sun correspond to curved lines. The currently accepted value of dark energy is used to generate the sloping mass plot lines.

(PhysOrg.com) -- An international team of astronomers, including a University of Alabama researcher, have detected effects of "dark energy" within the Local Group of galaxies containing our own Milky Way Galaxy.

Astronomers use the term “” to describe the mysterious field they believe must be present in the mostly empty space of the Universe in order to cause galaxies’ accelerated movement away from each other.

The team, including Dr. Gene Byrd, professor emeritus of physics and astronomy at The University of Alabama, and researchers from Finland and Russia, presented the research today at the American Astronomical Society meeting in Washington D. C.

The research, published in the most recent issue of the European , shows dark energy’s accelerating effects act on “small” scales of millions of light years, in contrast to dark energy’s previous discovery at distances of billions of light years. A light year is a distance of about six trillion miles in length.

The universe is populated with multitudes of galaxies each containing billions of stars and other gravitational matter. The distribution of galaxies is clumpy with most galaxies in systems ranging from groups of a few dozen to rich clusters with thousands.

As a consequence of the Big Bang, these systems are observed, via the lengthening of their spectral wavelengths, known as redshift, to be flying away (receding) from one another, Byrd said. Faster galaxy recessions are seen at greater distances from Earth in the cosmological expansion of the universe.

Besides their cosmological redshifts, individual galaxies in groups show shorter and longer wavelength Doppler shifts because of their internal orbital motions. During the 1980s, team members Byrd, and Mauri Valtonen, of Finland, explained excess internal orbital Doppler member redshifts as resulting from more group members receding from the group centers rather than equal numbers orbiting inward and outward.

The explanation why these members were leaving the groups awaited a new discovery. Until the late 1990s, it was thought that the gravitation of the matter in the universe governed its fate by slowing the expansion, Byrd said.

Astronomers used exploding (supernova) stars to measure much larger distances to galaxies along with their cosmological redshifts. These distances and redshifts indicated an additional mysterious “dark energy” which actually accelerates the recession.

Byrd pointed out that, in contrast to gravity’s decrease in strength with increasing distance, the distant galaxy observations indicate that dark energy acceleration effect increases with increasing distance.

The observations also indicate that, because of the spreading out of gravitating matter as the galaxies recede from one another, since about 6 or 7 billion years ago, dark energy’s “repulsion” actually has dominated gravity.

Using the matter/energy equivalence (E=mc2) from Einstein’s theory of relativity, the relative density proportions today are 72 percent dark energy and only 28 percent gravitating matter.

The next step in understanding, according to Byrd, was soon after the dark energy discovery. Team members Arthur Chernin, of Russia, and Pekka Teerikorpi, of Finland, along with collaborator Yuri Baryshev, realized that dark energy could have effects on motions of galaxies among groups of galaxies at separations much smaller than billions of light years.

The research presented at the meeting takes advantage of the fact that recent Hubble Space Telescope observations give astronomers the individual Local Group members’ distances and Doppler shift velocities with improved accuracy, Byrd said.

At the meeting, Byrd presented plots of distances and Doppler shift velocity observations, showing that near the Local Group center, equal numbers of members approach and recede in orbits forming a bound system.

The Galaxy and the Andromeda Galaxy - 2.5 million light years away - dominate this central region comprising most of the gravitating mass. However, the team found that outside a 4.6 million light year transition radius gap, small Local Group members are all receding. At larger distances, the small members recede more rapidly.

The team points out that at the transitional radius gap, the inward gravitation and outward dark energy acceleration add to zero. The increase of recession beyond the transition radius indicates that over a several million light year distance, dark energy’s acceleration increases with distance. This increase is like that previously found from observations of billions of light years away.

From the results of this paper, Byrd emphasized that ideas on the nature of dark energy should now take into account its accelerating effects and distance dependence at scales 1/1000 those previously seen.

From the Local Group members’ velocities and distances, the transition radius and the age of the , the team finds that the “local” dark energy density is consistent with the large distance estimated value. Byrd also said that dark energy effects must be included in estimating the gravitating mass in galaxy groups, with revised estimates of about 4 trillion solar masses for the Local Group.

Explore further: New mass map of a distant galaxy cluster is the most precise yet

Provided by University of Alabama

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brant
5 / 5 (1) Jan 06, 2010
Definitely time for a new gravity model.
Parsec
3.7 / 5 (3) Jan 06, 2010
All those budding physicists that believe that dark matter and dark energy are both manifestations of flaws in Einstein's gravity equations could be right.

I suggest that proposing a set of equations that actually resolve them would be more persuasive however than flat rejection of either concept, or just assuming that this is the answer.

I myself have a gut level feeling that we are starting to create epicycles and that there is a simpler underlying reality, probably involving a theory that accounts for gravity at the quantum level. Unfortunately, physical reality doesn't often correspond with personal desire, and often violates gut-level intuition.
croghan26
not rated yet Jan 07, 2010
"As a consequence of the Big Bang, these systems are observed, via the lengthening of their spectral wavelengths, known as redshift, to be flying away (receding) from one another, Byrd said. Faster galaxy recessions are seen at greater distances from Earth in the cosmological expansion of the universe. "

In another thread about Hubble discovering the most distant galaxies yet, someone pointed out that they are not 'flying away from each other' but space/time is expanding - and so the actual distance between galaxies is growing.

Is this another example of this happening?
GPhillip
5 / 5 (2) Jan 07, 2010
All of our math models of the universe are just that, models. Few scientists now believe that the model General Relativity is totally complete. Hardly anyone believes that Quantum Mechanics is totally complete. Both are extremely accurate in their predictions, but they will be revised or improved upon as new data is collected. The same happened when Newton's laws of gravitation needed to be revised to account for the orbit of Mercury, which General Relativity calculates very well. In fact, we may never understand these things completely. It could be that they are really many orders of magnitude more complex than we suspect and that we will be revising and improving our models for all time. It's great science though, and congrats to U of A for the good work.