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SIMPle Dark Matter

In Dark Matter by Brian Koberlein

Dark matter remains an enigma of modern cosmology. We have indirect evidence of its existence, and even some evidence of its characteristics, but we have yet to detect dark matter directly. This puts us in a kind of middle ground where there’s enough evidence to support dark matter, but not enough to define it, which is the perfect playground for theorists to try new ideas. This week in Physical Review Letters, just such a new idea has been presented.

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On X-rays and Axions

In Dark Matter by Brian Koberlein

There’s been a few articles in the popular press recently announcing the discovery of dark matter particles coming from the Sun. This is not the case. No science team is claiming they’ve discovered dark matter. The story traces it origin to a paper being published in MNRAS, which could be an indirect detection of dark matter, but could also be a few other things. It is an interesting paper, nonetheless.

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Profile Matching

In Dark Matter by Brian Koberlein

As I’ve written about before, the existence of dark matter is well supported by observational evidence. There isn’t much debate in the astronomical community on the existence of dark matter and the fact that it makes up a large part of the mass of galaxies. We’d still like to have a direct observation of dark matter to be certain sure, but there is general consensus on dark matter.

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Modified Dark Matter

In Dark Matter by Brian Koberlein

Dark matter is an aspect of the universe we still don’t fully understand. We have lots of evidence pointing to its existence (as I outlined in a series of posts a while back), and the best evidence we have points toward a specific type of matter known as cold dark matter (CDM). One big downside is that we have yet to find any direct detection of dark matter particles. In fact, many of the likely candidates for dark matter have been all but eliminated. Another is that cold dark matter doesn’t agree with our observations of dwarf galaxies. Now a new paper presents a solution to the second problem that might even help with the first.

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We Already Know Quite a Bit

In Dark Matter by Brian Koberlein

In this series we started with the basic observations of stellar motion in a galaxy, and how that led to the idea of some kind of dark matter. We saw that modified gravity models couldn’t explain things like the Bullet Cluster, while dark matter could. We also saw that dark matter must be something other than the normal matter that makes up you and me. It must be non-baryonic, weakly interacting with light, and make up a goodly portion of galaxies. Then again, our best candidate for dark matter is a hypothetical particle based on a particle physics model that is quite probably wrong.

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Known Dark Matter Isn’t Enough

In Dark Matter by Brian Koberlein

Last time we saw that while alternative gravity models don’t agree with galactic stellar motion and gravitational lensing, the dark matter model does. While some of that dark matter is likely regular (baryonic) matter such as MACHOs (brown dwarfs, neutron stars, etc.), such objects cannot make up the majority of dark matter in the universe.

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The Dark Matter Model Works

In Dark Matter by Brian Koberlein

Yesterday we looked at alternative gravitational models (specifically Modified Newtonian Dynamics) as a solution to the problem of gravitational lensing and stellar motion not matching the observed masses of galaxies. We saw that observations of colliding galaxies such as the Bullet Cluster show that the mass distributions observed directly don’t agree with the distributions calculated by gravitational lensing. This pretty much kills the alternative gravity models, because you wouldn’t expect the two results to be radically different if they are both due to the same mass.

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Other Gravitational Models Don’t Work

In Dark Matter by Brian Koberlein

Last time we talked about where the problem lies. When we map the distribution of visible mass in a galaxy and calculate what the motion of stars should be in that galaxy, it doesn’t match the motion we see. The stars in a galaxy move as if there is ten times the mass we observe. Observations of the cosmic microwave background indicate that our measurement of galactic mass should be correct, but observations of gravitational lensing by galaxies agree with stellar motion. Something just doesn’t add up.

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The Old Model Doesn’t Work

In Dark Matter by Brian Koberlein

Astrophysics is mainly about gravity. Yes, it also depends upon chemistry, nuclear physics, optics and the like, but gravity is the overarching force. Gravity drives stars to shine, it drives black holes to form, and it drives the motion of stars and planets. So a good understanding of the universe depends upon a good understanding of gravity.