‘Dark matter’ forms a ghost universe that mirrors the observable one, says Berkeley astronomy professor
‘The dark world has a dynamic life of its own,’ asserts Chung-Pei Ma
| 20 November 2003
The “dark matter” that comprises a still-undetected one-quarter of the universe is not a uniform cosmic fog, says a Berkeley astrophysicist, but instead forms dense clumps that move about like dust motes dancing in a shaft of light.
In a paper submitted earlier this month to Physical Review D, Chung-Pei Ma, an associate professor of astronomy at Berkeley, and Edmund Bertschinger of the Massachusetts Institute of Technology (MIT), prove that the motion of dark-matter clumps can be modeled in a way similar to the Brownian motion of airborne dust or pollen.
Their findings should provide astrophysicists with a new way to calculate the evolution of this ghost universe of dark matter and reconcile it with the observable universe, Ma says.
A persistent problem
Dark matter has been a nagging problem for astronomy for more than 30 years. Stars within galaxies and galaxies within clusters move in a way that indicates there is more matter there than we can see. This unseen matter seems to be in a spherical halo that extends probably 10 times farther than the visible stellar halo around galaxies. Early proposals that the invisible matter is comprised of burnt-out stars or heavy neutrinos have not panned out, and the current favorite candidates are exotic “supersymmetric particles” variously called neutrilinos or axions. Because these exotic particles interact with ordinary matter through gravity only, not via electromagnetic waves, they emit no light.
“We’re only seeing half of all particles,” Ma says. “They’re too heavy to produce now in accelerators, so half of the world we don’t know about.”
The picture only got worse four years ago when “dark energy” was found to be even more prevalent than dark matter. The cosmic account now pegs dark energy at about 69 percent of the universe, exotic dark matter at 27 percent, mundane dark matter — dim, unseen stars — at 3 percent, and what we actually see at a mere 1 percent.
Based on computer models of how dark matter would move under the force of gravity, Ma says that dark matter is not a uniform mist enveloping clusters of galaxies. Instead, dark matter forms smaller clumps that look superficially like the galaxies and globular clusters we see in our luminous universe. The dark matter has a dynamic life independent of luminous matter, she says.
“The cosmic microwave background shows the early effects of dark-matter clumping, and these clumps grow under gravitational attraction,” Ma says. “But each of these clumps, the halo around galaxy clusters, was thought to be smooth. People were intrigued to find that high-resolution simulations show they are not smooth, but instead have intricate substructures. The dark world has a dynamic life of its own.”
Ma, Bertschinger, and Berkeley graduate student Michael Boylan-Kolchin performed some of these simulations themselves. Several other groups over the past two years have also showed similar clumping.
The ghost universe of dark matter is a template for the visible universe, says Ma. Dark matter is 25 times more abundant than mere visible matter, so visible matter should cluster wherever dark matter clusters.
Searching for equivalencies
Therein lies the problem. Computer simulations of the evolution of dark matter predict far more clumps of dark matter in a region than there are clumps of luminous matter we can see. If luminous matter follows dark matter, there should be nearly equivalent numbers of each.
“Our galaxy, the Milky Way, has about a dozen satellites, but in simulations we see thousands of satellites of dark matter,” says Ma. “Dark matter in the Milky Way is a dynamic, lively environment in which thousands of smaller satellites of dark matter clumps are swarming around a big parent dark matter halo, constantly interacting with and disturbing each other.”
In addition, astrophysicists modeling the motion of dark matter were puzzled to see that each clump had a density that peaked in the center and fell off toward the edges in the exact same way, independent of its size. This universal density profile, however, appears to be in conflict with observations of some dwarf galaxies made by Ma’s colleague, Berkeley professor of astronomy Leo Blitz, and his research group, among others.
Ma hopes that a new way of looking at the motion of dark matter will resolve these problems and square theory with observation. In her submission to Physical Review she proved that the motion of dark matter can be modeled much like the Brownian motion that botanist Robert Brown described in 1828 and Albert Einstein explained in a seminal 1905 paper that helped garner him the 1921 Nobel Prize in Physics.
Brownian motion was first described as the zigzag path traveled by a grain of pollen floating in water, pushed about by water molecules colliding with it. The phenomenon refers equally to the motion of dust in air and dense clumps of dark matter in the dark matter universe, says Ma.
This insight “lets us use a different language, a different point of view than the standard view,” to investigate the movement and evolution of dark matter, Ma says.
Other astronomers, such as Berkeley emeritus professor of astronomy Ivan King, have used the theory of Brownian motion to model the movement of hundreds of thousands of stars within star clusters, but this, Ma says, “is the first time it has been applied rigorously to large cosmological scales. The idea is that we don’t care exactly where the clumps are, but rather, how clumps behave statistically in the system, how they scatter gravitationally.”
Ma notes that the Brownian motion of clumps is governed by an equation, the Fokker-Planck equation, that is used to model many stochastic or random processes, including the stock market. Ma and her collaborators are currently working on solving this equation for cosmological dark matter.
“It is surprising and delightful that the evolution of dark matter, the evolution of clumps, obeys a simple, 90-year-old equation,” she says.
A video simulation of the evolution of dark matter is available on Ma’s website, astron.berkeley.edu/~cpma/.