Mystery in the Perseus Cluster
science.nasa.gov
science.nasa.gov
We'll have to wait to see if this result can be replicated by others and we'll look at the results from ASTRO-H when it launches. If you examine at the original paper (http://arxiv.org/abs/1402.2301), it's certainly not cut and dried dark matter emission (yet).
It may be worth noting the significance of ASTRO-H to this kind of science (full disclaimer: it's a long time since I did any astrophysics so I am liable to get things wrong). The attraction of ASTRO-H is not just newer == better. In fact in several ways it's worse than existing X-ray satellites, for example it won't have the angular resolution of Chandra (so no pretty pictures) or the sensitivity of XMM-Newton (so bad for looking at very faint objects). Where it is designed to excel, however, is in spectral resolution, where it is about an order of magnitude better than the other observatories. This means it's going to be great at measuring the precise energy of incoming X-rays, which is essential for studying emission lines like this. If your spectral resolution is too low you'll find it difficult to detect weak lines at all because they get averaged over such a big energy range that they end up just looking like the background emission from the hot plasma in the cluster.
Once you have established that there is a line in the emission, good spectral resolution is also critical to determining which models are compatible with it. There's almost certainly a lot of ideas people can dream up that will fit "a vauge bump around 3.55keV", many of which will be eliminated once you have a better idea of the shape of the line. This is the sort of science that ASTRO-H should be good at.
Hopefully someone will correct me if I made any egregious errors.
Absolutely right - ASTRO-H brings new capabilities - high spectral resolution in X-rays which we don't have now. It's pretty exciting.
Beyond that, here in Europe, the European Space Agency has now approved our proposal for Athena (http://www.mpe.mpg.de/Athena), which should provide a large collecting area, high spectral resolution and pretty good spatial resolution. It's going to be a large technical challenge, which unfortunately means we'll have to wait until 2028 for launch. It requires development of a new mirror technology (based on stacks of silicon chip wafers!), development of a cryogenic X-IFU (X-ray integral field unit), which is going to provide spatially-resolve high spectral resolution X-ray spectroscopy. There's also a wide field imager, capable of mapping large areas of the sky quickly.
It's been a long time since High School chemistry class, but as I remember it, spectral emission lines are caused by electrons changing orbital levels and thereby releasing a photon. So dark matter has electrons? Er, would that mean that it's not dark? Why wouldn't this just mean that we've missed an orbital level somewhere?
The suggestion of dark energy comes from some theories where postulated dark matter particles can annihilate if they hit another dark matter particle. In these theories, the result is emission of high energy photons with an energy which is related to the mass of the individual dark matter particle. Basically E=mc^2. So it is still an emission line, but not one that arises from an election transition in an atom or molecule.
So a novel photon interaction in intergalactic space would be huge news even if it doesn't map directly to dark matter.
[0] https://en.wikipedia.org/wiki/Atacama_Large_Millimeter_Array
Anyone interested in the universe should take a quick gander at this massive, massive scientific wonder.
New physics!
I'm imagining a boiling ocean, covered in volcanoes, with a nuclear bomb going off in the middle of it.
http://science.nasa.gov/science-news/science-at-nasa/2014/24...
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A commonly used secondary definition of menagerie is "a strange or diverse collection of people or things."
FE I is not ionized Fe (26 protons, 26 electrons, 0 net charge)
FE II is ionized Fe (26 protons, 25 electrons, +1 net charge)
FE III is not ionized Fe (26 protons, 24 electrons, +2 net charge)
...
FE XXV has (26 protons, 2 electrons, +24 net charge)
FE XXVI has (26 protons, 1 electron, +25 net charge)
--
This is not the standard chemical notation. In chemistry:
FE II is ionized Fe++ (26 protons, 24 electrons, +2 net charge)
FE III is ionized Fe+++ (26 protons, 23 electrons, +3 net charge)
George Gamow, his advisor, thought it would be funny to include Hans Bethe as a coauthor for Alpher's original research, just for the author list "Alpher, Bethe, Gamow". Bethe was not involved in anyway in that piece of research.
More here http://en.wikipedia.org/wiki/Ralph_Asher_Alpher#Big_Bang_nuc...
If you have not read Gamow's popular science writings.... highly recommended.
As Alpher also showed that the universal ratio of hydrogen and helium isotopes can be explained by nucleosynthesis in the big bang, he seems to have been seriously overlooked.
'The menagerie of dark matter candidates that might produce this kind of line include axions, sterile neutrinos, and "moduli dark matter" that may result from the curling up of extra dimensions in string theory.'
1) Assumption of dark matter 2) String theory
It's never hard to find a group of theoretical physicists willing to tag anything currently, poorly misunderstood as most likely an effect of dark matter and string theory.
And, of course, this will require a new observatory.
Also, a new observatory is a good thing. Bring it on.
There's the usual stuff about galaxy rotation curves, there's the http://en.wikipedia.org/wiki/Bullet_Cluster which people consider to be more of a smoking gun, but then there's also evidence from http://en.wikipedia.org/wiki/Baryon_acoustic_oscillations visible in the CMB. That last one's slightly over my head, but apparently cosmologists find it extremely convincing, especially when combined with the other evidence. The wiki page talks about dark energy, but the subject has significance for dark matter too. Let me see if I can find the relevant plot...
At the end of the day it's just another weakly interacting particle. Last time we discovered one of those was the neutrino in the 50s, it's not an outlandish thing to think about.
EDIT: here's the BAO stuff: http://ned.ipac.caltech.edu/level5/Sept09/Einasto/Einasto6.h...
Of course, quite a bit of it might turn out to be exotic new types of particles, but that's a question for theory and experiment.
The precedent here is quite strong, incidentally, on a few counts.
We have high confidence in our understanding of gravity on the macro scale, and that understanding has survived some crises. For example, the orbit of the planet Uranus, as originally calculated, was "wrong" -- it did not appear to be conforming to the understood behavior of gravity. One theory which was developed to explain this, and which could at the time have been criticized in the style of your comment, was that there must be another planet further out, whose gravity was perturbing Uranus' orbit. Calculating backwards from Uranus' behavior, this theory predicted the location in the sky of the additional planet... which was then promptly observed via telescope (this was the discovery of Neptune).
Similarly, we have high confidence that weakly-interacting particles -- undiscovered variants of which are a popular candidate for examples of dark matter -- exist. The neutrino is the classic example: a particle which was posited by theory as "this is the only thing that makes sense given what we see", but which would necessarily be incredibly difficult to detect on account of barely if ever interacting with anything (and thus, again, would be open to your criticism). Of course, the neutrino was eventually detected and its existence confirmed.
So there is nothing wrong or arbitrary or unusual, in terms of the history of physics, in positing something like dark matter.
I've often wondered about this(and don't know any physicists so would really love some insight on this), why do we assume that there's additional matter rather than question whether our models are correct at that scale?
There are also physicists that question the models. Some scientists follow a path of inquiry based on assumptions that Einstein's theory is mostly correct -- hence a postulation of "dark matter" which leads to searching for the existence of it(1). But there are other physicists that assume there's something missing in the accepted equations that would explain the galaxy rotation speeds without any need for "dark matter".
Each competing theory tries to accumulate more and more evidence for their case until one "wins" (scientific consensus)(2). Right now, the "dark matter" line of inquiry has more scientists, more papers, and more press coverage.
(1)direct instead of indirect observation
(2)Some might say Dark Matter theory has already "won" in the marketplace of ideas
As for dismissing God, I don't see why, we just need to come up with some signature that would differ between a designed universe and an accidental one and apply for observation time on a suitable instrument.
1. Huh, those are some weird observations. What could explain it? 2. Maybe it's X? That could explain it. 3. So could Y? 4. Here's an experiment we could do to rule out Y! 5. Hmm, actually the result of that experiment was consistent with Y, but constrains some of its free parameters. And Y could still be false.
And so on.
Science doesn't require that you have something in a lab, just that you make hypotheses which are testable by some sort of observation. Otherwise we'd have to throw out nearly all of cosmology.
There are competing hypotheses still with respect to dark matter (e.g. that the force of gravity works differently than we thought over long distances), precisely because we haven't yet figured out how to do the experiments to rule out all but one hypothesis. But that's why it's called a hypothesis. We haven't yet figured out the answer! That's the beauty of science.
Closest references I could find: http://phys.org/news/2013-02-dark-galaxies-ways-collision-he...
"In the Bullet Cluster, a collision between two galaxy clusters appears to have caused a separation of dark matter and baryonic matter." - https://en.wikipedia.org/wiki/Dark_Matter
http://www.lsst.org/lsst/science/scientist_dark_matter
http://scienceblogs.com/startswithabang/2011/04/20/how-gravi...
http://www.ifa.hawaii.edu/~ger/ASTRO-110_sp08/Lecture28_Dark...
Also, despite the name "dark energy" has no relation to dark matter and the evidence for either does not overlap. Moreover, the inability of one theory to explain everything else in the universe does not invalidate that theory. The theory of biological evolution fails to explain the existence of neutron stars, yet it is still a valid theory.