Why does dark matter behave differently in small galaxies than in large ones?

The most important characteristic of dark matter is that it interacts only by way of gravity. And as the only one of the four fundamental forces, gravity is always attractive. Therefore, no matter where it occurs, dark matter must always collect at the mass center of the respective structure, regardless of whether it is a small galaxy or a giant galaxy cluster.

But in reality, things look quite different: in galaxy clusters, dark matter exhibits the expected behavior, but in smaller galaxies it is distributed much more widely than it should be. This arrangement could be explained in that the dark matter particles bounce off each other like billiard balls, scattering them. The result of this scattering process is a much wider distribution.

But why does this happen only in dwarf galaxies? Researchers at the Kavli Institute for the Physics and Mathematics of the Universe (IPMU) believe that they have discovered the answer. Their idea: in a dwarf galaxy, dark matter moves more slowly; it has less energy. In a galaxy cluster, in contrast, it is faster and has more energy. Apparently, the particles must meet each other with very specific energy levels for scattering to occur, and these resonance conditions occur only in small galaxies. Elsewhere, dark matter is too fast (or too slow) to bounce off each other.

Such resonance conditions are not uncommon in the universe. They might also reveal something about dark matter itself, of which we know precious little. «It may also be a sign that our world has more dimensions than we can see,” says the Chinese physicist Xiaoyong Chu. “If a particle moves in extra dimensions, it therefore has additional energy. For us, who don’t see the extra dimension, this additional energy appears as mass according to Einstein’s E=mc2. Maybe some particles move twice as fast in the extra dimension, so that their mass is exactly twice the mass of the dark matter.”

Normally, particles of dark matter influence each other only by means of their mass (picture: Kavli IPMU)
Under certain conditions, they interact with each other in resonance and are then scattered (picture: Kavli IPMU)
Why does dark matter clump together in large galaxy clusters, but spreads out in smaller galaxies? (picture: Kavli IPMU – Kavli IPMU / NASA, STScI)

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  • BrandonQMorris
  • Brandon Q. Morris es físico y especialista en el espacio. Lleva mucho tiempo preocupado por las cuestiones espaciales, tanto a nivel profesional como privado, y aunque quería ser astronauta, tuvo que quedarse en la Tierra por diversas razones. Le fascina especialmente el "qué pasaría si" y a través de sus libros pretende compartir historias convincentes de ciencia ficción dura que podrían suceder realmente, y que algún día podrían suceder. Morris es autor de varias novelas de ciencia ficción de gran éxito de ventas, como la serie Enceladus.

    Brandon es un orgulloso miembro de la Science Fiction and Fantasy Writers of America y de la Mars Society.