Carol
09-13-2008, 03:58 AM
I'm not sure where to put this info as it's more science related but this seems good enough unless someone comes up with a better suggestion. Mahalo Nui Loa
'Missing' Dark Matter Is Really There, Says Hebrew University Cosmologist
September 28, 2005
A new analysis that refutes challenges to the existence of dark matter in certain galaxies appears in an article published this week in the journal Nature. Leading author of the article is Avishai Dekel, professor of physics at the Hebrew University of Jerusalem.
Accepted cosmological theory postulates that every observable galaxy in the universe (each made up of billions of stars similar to our sun) is embedded in a massive “halo" of dark matter. Though unseen, dark matter can be clearly detected indirectly by observing its tremendous gravitational effects on visible objects.
This common understanding faced a severe challenge when a team of astronomers, writing in Science in 2003, reported a surprising absence of dark matter in one type of galaxy – “elliptical" (rounded) galaxies. Their theory was based on observations that stars located at great distances from the center in such galaxies move at very slow speeds, as opposed to the great speed one would have expected from the heavy gravitational pull exerted by dark matter.
The new analysis in Nature provides a simple explanation for these observations. “In fact,” says Dekel, “our analysis fits comfortably with the standard picture in which elliptical galaxies also reside in massive dark matter halos.
"A dearth of dark matter in elliptical galaxies is especially puzzling in the context of the common theory of galaxy formation, which assumes that ellipticals originate from mergers of disk galaxies," added Dekel. "Massive dark-matter halos are clearly detected in disk galaxies, so where did they disappear to during the mergers?" asks Dekel.
The Nature article is based on simulations of galaxy mergers run on a supercomputer by graduate student Thomas J. Cox, supervised by Joel Primack, a professor of physics at the University of California, Santa Cruz. The simulations were analyzed by Dekel and collaborators Felix Stoehr and Gary Mamon at the Institute of Astrophysics in Paris, where Dekel is the incumbent of the Blaise Pascal International Chair of Research at the Ecole Normale Superieure.
The simulations show that the observations reported in Science are a predictable consequence of the violent collision and merger of the spiral galaxies that lead to the formation of the elliptical galaxies.
Evidence for dark matter halos around spiral galaxies comes from studying the circular motions of stars in these galaxies. Because most of the visible mass in a galaxy is concentrated in the central region, stars at great distances from the center would be expected to move more slowly than stars closer in. Instead, observations of spiral galaxies show that the rotational speed of stars in the outskirts of the disk remains constant as far out as astronomers can measure it.
The reason for this, according to the dark matter theory, is the presence of an enormous halo of unseen dark matter in and around the galaxy, which exerts its gravitational influence on the stars. Additional support for dark matter halos has come from a variety of other observations.
In elliptical galaxies, however, it has been difficult to study the motions of stars at great distances from the center. The scientists writing in Science found a decrease in the velocities with increasing distance from the center of the galaxy, which is inconsistent with simple models of the gravitational effects of dark matter halos.
Part of the explanation for that phenomenon, put forth in the new Nature paper, lies in the fact that the velocities in the earlier study were measured along the line of sight. "You cannot measure the absolute speeds of the stars, but you can measure their relative speeds along the line of sight, because if a star is moving toward us its light is shifted to shorter wave lengths, and if it is moving away from us its light is shifted to longer wave lengths," Primack explained.
This limitation would not be a problem if the orbits of the observed stars were randomly oriented with respect to the line of sight, According to Cox's simulations, however, the stars in elliptical galaxies that are farthest from the center are likely to be moving in elongated, eccentric orbits such that most of their motion is perpendicular to the line of sight. Therefore, they could be moving at high velocities without exhibiting much motion toward or away from the observers.
Why this is so is traceable to the processes whereby disk galaxies merge to form elliptical galaxies. "In the merger process that produces these galaxies, a lot of the stars get flung out to fairly large distances, and they end up in highly elongated orbits that take them far away and then back in close to the center," explained Dekel.
"If we see a star at a large distance from the center of the galaxy, that star is going to be mostly moving either away from the center or back toward the center. Almost certainly, most of its motion is perpendicular to our line of sight," Dekel said. Under such circumstances, the star would appear to be moving quite slowly, when in fact this is not the case, based upon the models of simulated galaxy mergers studied by the Hebrew University-UCSC-Paris team.
"Our conclusion is that what the cosmologists described in 2003 is exactly what the dark matter model would predict," he said, “Our findings remove a problem which bothered them and make it possible to better understand the processes involved in creation of new galaxies in the universe.”
Source: Hebrew University of Jerusalem
A Primer on Dark Matter
FIGURE: Superposed on an optical picture of a group of galaxies is an X-ray image taken by ROSAT. The image shows confined hot gas (which produces X-rays) highlighted in false red color. The presence of this confined gas indicates that the gravity exerted in groups and clusters of galaxies is larger than that expected from the observed galaxies.
There are many reasons to believe that the universe is full of "dark matter", matter that influences the evolution of the universe gravitationally, but is not seen directly in our present observations. The adjacent image exhibits one recent piece of evidence for undetected matter: the hot gas seen in the X-ray spectrum would have dispersed if it were held in place only the by gravity of the mass that is producing light in this image (the so-called "luminous mass").
The nature of this dark matter, and the associated "missing mass problem", is one of the fundamental cosmological issues of modern astrophysics. The following is a brief tutorial on this issue extracted from an informal email message:
1 If inflation is correct then, since luminous stars and galaxies only contribute 0.5% of the closure density, then 99% of the Universe is in the form of dark matter and this, no doubt, must be a particle. There are always candidates. Neutrinoes have never been a viable candidate for a fairly simple reason. Neutrinoes are relativistic (e.g. hot dark matter) and therefore they erase fluctuations on small scales (they free stream and fill the horizon in the early universe). Thus the only fluctuations that can still exist in a neutrino dominated Universe are on a very large scale. These will cool and form structure but only on largescales, you will never form galaxies in this manner.
2 On smaller scales, such as galaxies and clusters of galaxies, dynamical estimates of the mass, based on either rotation curves of galaxies or velocity dispersions of galaxies indicate that 90% (not 99% which is another order of magnitude) of the total mass is sub-lumnous. This isn't so bad as it implies the mass density of the Universe is 10% of the closure density. In this case, the sub-luminous mass could very well be normal (baryonic) and be locked up in stellar remnants (white dwarfs, neutron stars, black holes) or just in very dim stars called "Brown Dwarfs". There is recent evidence for possible observation of one of these very dim Brown Dwarfs. Some of this is being tested with the microlensing experiments currently underway in australia (you can actually find some of what I am talking about at http://zebu.uoregon.edu/cosmo.html) and there are positive detections but the selection function is unknown at present and so the lensing population is also unknown.
3 Although inflation demands that the Universe has a density equal to its critical density (and inflation is necessary to solve the horizon problem) there has never been any observational evidence to support this high of mass density. Most dynamical studies suggest values of 10-20% of closure density. These studies are based on large scale deviations from hubble expansion velocities (so called peculiar velocities).
4 Large scale structure (e.g. the distribution of galaxies) is very hard to understand, particularly in light of the relatively smooth microwave background as measured by the COBE satellite. There is way too much power on large scales. One way to accomodate this is to go to a mixed dark matter model in which you have some hot dark matter (for the large scale power) and some cold dark matter (wimps, axions, photinos, supersymmetric particles, etc) to act as a seed for galaxy formation. None of those models, however, fit the data using the critical density. The best models to date (you can see a diagram in the http document referenced above) suggest mixed dark matter and an overall cosmological mass density of 20-30% of closure. Hence, to retain inflation, with its inescapable prediction that the Universe must be flat, requires re-invoking Einstein's cosmological constant - meaning the universe has vacuum energy (negative pressure) and is currently accelerating. This makes our cosmology complicated but much data is pointing this way.
5 Finally, there have been speculative papers that if the dark matter is really something toally new and mysterious then maybe it communicates with itself over some long range force (either attractive or repulsive). An intriguing idea as that would mess up all the comoslogical dynamics - but given the really surprising nature of the galaxy distribution - something clearly very funny is going on.
6 Supernova 1987a neutrino time of flight studies as well as the Solar Neutrino experiment are consistent with the neutrino having a mass, but a very small mass, not one that can cosmologically dominate. As for seeing particles in other ways - well since the SSC won't be built we can not do an accelerator test for seeing supersymmetric particles which would only be created at very high energy (e.g. the early universe) - so there remain many viable potential particles that are consistent with the Standard MOdel of particles (e.g. 3 generations of neutrinoes, 6 quarks) and which would remain unnoticed in any accelerator experiments.
Source: http://zebu.uoregon.edu/text/darkmatter.txt
Explanation: What type of matter makes up most of the universe? This question is arguably the most perplexing astronomical mystery of our time. A leading candidate is a type of dim, low mass star called a "brown dwarf" star. Our universe could contain more brown dwarfs than any other type of star - but they are so dim they have so far escaped detection. The dramatic photograph above, taken in October 1994, sheds new light on this "dark matter" problem. The seemingly inconspicuous companion to the right of the overexposed image of a normal star is thought to be an elusive brown dwarf. Now that the existence of brown dwarfs has been demonstrated, a key remaining question is their abundance.
Here are links to two experimental searches for Dark Matter candidates:
• The MACHO (MAssive Compact Halo Objects) Dark Matter Search Project
• The Optical Gravitational Lensing Experiment (OGLE)
Dark Matter Mystery
While carefully measuring the speed of rotation of galaxies, astronomers stumbled upon a profound cosmic mystery.
They could estimate what the rotation speed should be by calculating the mass of all the visible stars and gas, thereby determining the gravity of the galaxy. Much to their surprise, the measurements showed that most galaxies are rotating faster than they should. Not a little faster. Much faster! More than twice as fast. This meant that, according to Einstein's theory of gravity, these galaxies should be flying apart. Yet clearly, they are not.
Scientists are considering a number of possibilities. Candidates for dark matter include MACHOS, WIMPS and GAS. A "Good News" and "Bad News" analysis is given below for each of the candidates.
MACHOS (Massive Compact Halo Objects) Examples: brown dwarfs, white dwarfs, neutron stars, black holes.
What can the answer be? Is it possible that most galaxies are surrounded by some "dark" form of matter that cannot be observed by radio, infrared, optical, ultraviolet, X-ray, or gamma-ray telescopes? Could Einstein's theory of gravity, which has proved to be correct in all cases so far, be somehow wrong?
X-ray telescopes have discovered vast clouds of multimillion degree gas in clusters of galaxies. These hot gas clouds increase the mass of the cluster, but not enough to solve the mystery. In fact they provide an independent measurement of dark matter. The measurement shows that there must be at least four times as much dark matter as all the stars and gas we observe, or the hot gas would escape the cluster.
What can the dark matter be?
Brown Dwarf stars have a mass that is less than eight percent of the mass of the Sun--too low to produce the nuclear reactions that make stars shine.
Good News: Recently, astronomers have found some objects that are either brown dwarf stars or very large planets around other stars. Observations of the brightening and then dimming of distant stars--thought to be due to the gravitational lens effect of a foreground star-- may also provide further evidence for a large population of brown dwarfs in our galaxy.
Bad News: There is as yet no evidence that brown dwarfs are anywhere near as abundant as they would have to be to account for the dark matter in our galaxy.
White Dwarfs are the final condensed states of small to medium sized stars.
Good News: White dwarfs are known to exist and to be plentiful. Maybe they could be plentiful enough to explain the dark matter if young galaxies produced white dwarfs that cool more rapidly than present theory predicts.
Bad News: No good alternative to the present theory exists. Also the production of large numbers of white dwarfs implies the production of a large amount of helium, which is not observed.
Neutron Stars or Black Holes are the final condensed states of large and very large stars.
Good News: They can be dark, especially black holes, which are totally dark, except for a negligible amount of so-called Hawking radiation. See http://chandra.harvard.edu/resources/faq/black_hole/bhole-31.html
Bad News: These objects are expected to be much scarcer than white dwarfs. Also, the processes that produce these objects release a lot of energy and heavy elements; there is no evidence of such a release.
WIMPS (Weakly Interacting Massive Particles) Examples: Exotic Subatomic Particles such as axions, massive neutrinos, and photinos.
Good News: Theoretically, WIMPS could have been produced in the Big Bang origin of the universe in the right amounts and with the right properties to explain the dark matter.
Bad News: No one has ever observed even one of these particles, let alone enough of them to explain the dark matter.
Hydrogen Gas
Good News: Seventy to seventy-five percent of the visible matter in the universe is in the form of hydrogen, the simplest element. It may be possible that the dark matter is numerous small clouds of hydrogen gas.
Bad News: It is very difficult to hide hydrogen gas from the probing, sensitive eyes of radio, infrared, optical, ultraviolet, and X-ray telescopes.
'Missing' Dark Matter Is Really There, Says Hebrew University Cosmologist
September 28, 2005
A new analysis that refutes challenges to the existence of dark matter in certain galaxies appears in an article published this week in the journal Nature. Leading author of the article is Avishai Dekel, professor of physics at the Hebrew University of Jerusalem.
Accepted cosmological theory postulates that every observable galaxy in the universe (each made up of billions of stars similar to our sun) is embedded in a massive “halo" of dark matter. Though unseen, dark matter can be clearly detected indirectly by observing its tremendous gravitational effects on visible objects.
This common understanding faced a severe challenge when a team of astronomers, writing in Science in 2003, reported a surprising absence of dark matter in one type of galaxy – “elliptical" (rounded) galaxies. Their theory was based on observations that stars located at great distances from the center in such galaxies move at very slow speeds, as opposed to the great speed one would have expected from the heavy gravitational pull exerted by dark matter.
The new analysis in Nature provides a simple explanation for these observations. “In fact,” says Dekel, “our analysis fits comfortably with the standard picture in which elliptical galaxies also reside in massive dark matter halos.
"A dearth of dark matter in elliptical galaxies is especially puzzling in the context of the common theory of galaxy formation, which assumes that ellipticals originate from mergers of disk galaxies," added Dekel. "Massive dark-matter halos are clearly detected in disk galaxies, so where did they disappear to during the mergers?" asks Dekel.
The Nature article is based on simulations of galaxy mergers run on a supercomputer by graduate student Thomas J. Cox, supervised by Joel Primack, a professor of physics at the University of California, Santa Cruz. The simulations were analyzed by Dekel and collaborators Felix Stoehr and Gary Mamon at the Institute of Astrophysics in Paris, where Dekel is the incumbent of the Blaise Pascal International Chair of Research at the Ecole Normale Superieure.
The simulations show that the observations reported in Science are a predictable consequence of the violent collision and merger of the spiral galaxies that lead to the formation of the elliptical galaxies.
Evidence for dark matter halos around spiral galaxies comes from studying the circular motions of stars in these galaxies. Because most of the visible mass in a galaxy is concentrated in the central region, stars at great distances from the center would be expected to move more slowly than stars closer in. Instead, observations of spiral galaxies show that the rotational speed of stars in the outskirts of the disk remains constant as far out as astronomers can measure it.
The reason for this, according to the dark matter theory, is the presence of an enormous halo of unseen dark matter in and around the galaxy, which exerts its gravitational influence on the stars. Additional support for dark matter halos has come from a variety of other observations.
In elliptical galaxies, however, it has been difficult to study the motions of stars at great distances from the center. The scientists writing in Science found a decrease in the velocities with increasing distance from the center of the galaxy, which is inconsistent with simple models of the gravitational effects of dark matter halos.
Part of the explanation for that phenomenon, put forth in the new Nature paper, lies in the fact that the velocities in the earlier study were measured along the line of sight. "You cannot measure the absolute speeds of the stars, but you can measure their relative speeds along the line of sight, because if a star is moving toward us its light is shifted to shorter wave lengths, and if it is moving away from us its light is shifted to longer wave lengths," Primack explained.
This limitation would not be a problem if the orbits of the observed stars were randomly oriented with respect to the line of sight, According to Cox's simulations, however, the stars in elliptical galaxies that are farthest from the center are likely to be moving in elongated, eccentric orbits such that most of their motion is perpendicular to the line of sight. Therefore, they could be moving at high velocities without exhibiting much motion toward or away from the observers.
Why this is so is traceable to the processes whereby disk galaxies merge to form elliptical galaxies. "In the merger process that produces these galaxies, a lot of the stars get flung out to fairly large distances, and they end up in highly elongated orbits that take them far away and then back in close to the center," explained Dekel.
"If we see a star at a large distance from the center of the galaxy, that star is going to be mostly moving either away from the center or back toward the center. Almost certainly, most of its motion is perpendicular to our line of sight," Dekel said. Under such circumstances, the star would appear to be moving quite slowly, when in fact this is not the case, based upon the models of simulated galaxy mergers studied by the Hebrew University-UCSC-Paris team.
"Our conclusion is that what the cosmologists described in 2003 is exactly what the dark matter model would predict," he said, “Our findings remove a problem which bothered them and make it possible to better understand the processes involved in creation of new galaxies in the universe.”
Source: Hebrew University of Jerusalem
A Primer on Dark Matter
FIGURE: Superposed on an optical picture of a group of galaxies is an X-ray image taken by ROSAT. The image shows confined hot gas (which produces X-rays) highlighted in false red color. The presence of this confined gas indicates that the gravity exerted in groups and clusters of galaxies is larger than that expected from the observed galaxies.
There are many reasons to believe that the universe is full of "dark matter", matter that influences the evolution of the universe gravitationally, but is not seen directly in our present observations. The adjacent image exhibits one recent piece of evidence for undetected matter: the hot gas seen in the X-ray spectrum would have dispersed if it were held in place only the by gravity of the mass that is producing light in this image (the so-called "luminous mass").
The nature of this dark matter, and the associated "missing mass problem", is one of the fundamental cosmological issues of modern astrophysics. The following is a brief tutorial on this issue extracted from an informal email message:
1 If inflation is correct then, since luminous stars and galaxies only contribute 0.5% of the closure density, then 99% of the Universe is in the form of dark matter and this, no doubt, must be a particle. There are always candidates. Neutrinoes have never been a viable candidate for a fairly simple reason. Neutrinoes are relativistic (e.g. hot dark matter) and therefore they erase fluctuations on small scales (they free stream and fill the horizon in the early universe). Thus the only fluctuations that can still exist in a neutrino dominated Universe are on a very large scale. These will cool and form structure but only on largescales, you will never form galaxies in this manner.
2 On smaller scales, such as galaxies and clusters of galaxies, dynamical estimates of the mass, based on either rotation curves of galaxies or velocity dispersions of galaxies indicate that 90% (not 99% which is another order of magnitude) of the total mass is sub-lumnous. This isn't so bad as it implies the mass density of the Universe is 10% of the closure density. In this case, the sub-luminous mass could very well be normal (baryonic) and be locked up in stellar remnants (white dwarfs, neutron stars, black holes) or just in very dim stars called "Brown Dwarfs". There is recent evidence for possible observation of one of these very dim Brown Dwarfs. Some of this is being tested with the microlensing experiments currently underway in australia (you can actually find some of what I am talking about at http://zebu.uoregon.edu/cosmo.html) and there are positive detections but the selection function is unknown at present and so the lensing population is also unknown.
3 Although inflation demands that the Universe has a density equal to its critical density (and inflation is necessary to solve the horizon problem) there has never been any observational evidence to support this high of mass density. Most dynamical studies suggest values of 10-20% of closure density. These studies are based on large scale deviations from hubble expansion velocities (so called peculiar velocities).
4 Large scale structure (e.g. the distribution of galaxies) is very hard to understand, particularly in light of the relatively smooth microwave background as measured by the COBE satellite. There is way too much power on large scales. One way to accomodate this is to go to a mixed dark matter model in which you have some hot dark matter (for the large scale power) and some cold dark matter (wimps, axions, photinos, supersymmetric particles, etc) to act as a seed for galaxy formation. None of those models, however, fit the data using the critical density. The best models to date (you can see a diagram in the http document referenced above) suggest mixed dark matter and an overall cosmological mass density of 20-30% of closure. Hence, to retain inflation, with its inescapable prediction that the Universe must be flat, requires re-invoking Einstein's cosmological constant - meaning the universe has vacuum energy (negative pressure) and is currently accelerating. This makes our cosmology complicated but much data is pointing this way.
5 Finally, there have been speculative papers that if the dark matter is really something toally new and mysterious then maybe it communicates with itself over some long range force (either attractive or repulsive). An intriguing idea as that would mess up all the comoslogical dynamics - but given the really surprising nature of the galaxy distribution - something clearly very funny is going on.
6 Supernova 1987a neutrino time of flight studies as well as the Solar Neutrino experiment are consistent with the neutrino having a mass, but a very small mass, not one that can cosmologically dominate. As for seeing particles in other ways - well since the SSC won't be built we can not do an accelerator test for seeing supersymmetric particles which would only be created at very high energy (e.g. the early universe) - so there remain many viable potential particles that are consistent with the Standard MOdel of particles (e.g. 3 generations of neutrinoes, 6 quarks) and which would remain unnoticed in any accelerator experiments.
Source: http://zebu.uoregon.edu/text/darkmatter.txt
Explanation: What type of matter makes up most of the universe? This question is arguably the most perplexing astronomical mystery of our time. A leading candidate is a type of dim, low mass star called a "brown dwarf" star. Our universe could contain more brown dwarfs than any other type of star - but they are so dim they have so far escaped detection. The dramatic photograph above, taken in October 1994, sheds new light on this "dark matter" problem. The seemingly inconspicuous companion to the right of the overexposed image of a normal star is thought to be an elusive brown dwarf. Now that the existence of brown dwarfs has been demonstrated, a key remaining question is their abundance.
Here are links to two experimental searches for Dark Matter candidates:
• The MACHO (MAssive Compact Halo Objects) Dark Matter Search Project
• The Optical Gravitational Lensing Experiment (OGLE)
Dark Matter Mystery
While carefully measuring the speed of rotation of galaxies, astronomers stumbled upon a profound cosmic mystery.
They could estimate what the rotation speed should be by calculating the mass of all the visible stars and gas, thereby determining the gravity of the galaxy. Much to their surprise, the measurements showed that most galaxies are rotating faster than they should. Not a little faster. Much faster! More than twice as fast. This meant that, according to Einstein's theory of gravity, these galaxies should be flying apart. Yet clearly, they are not.
Scientists are considering a number of possibilities. Candidates for dark matter include MACHOS, WIMPS and GAS. A "Good News" and "Bad News" analysis is given below for each of the candidates.
MACHOS (Massive Compact Halo Objects) Examples: brown dwarfs, white dwarfs, neutron stars, black holes.
What can the answer be? Is it possible that most galaxies are surrounded by some "dark" form of matter that cannot be observed by radio, infrared, optical, ultraviolet, X-ray, or gamma-ray telescopes? Could Einstein's theory of gravity, which has proved to be correct in all cases so far, be somehow wrong?
X-ray telescopes have discovered vast clouds of multimillion degree gas in clusters of galaxies. These hot gas clouds increase the mass of the cluster, but not enough to solve the mystery. In fact they provide an independent measurement of dark matter. The measurement shows that there must be at least four times as much dark matter as all the stars and gas we observe, or the hot gas would escape the cluster.
What can the dark matter be?
Brown Dwarf stars have a mass that is less than eight percent of the mass of the Sun--too low to produce the nuclear reactions that make stars shine.
Good News: Recently, astronomers have found some objects that are either brown dwarf stars or very large planets around other stars. Observations of the brightening and then dimming of distant stars--thought to be due to the gravitational lens effect of a foreground star-- may also provide further evidence for a large population of brown dwarfs in our galaxy.
Bad News: There is as yet no evidence that brown dwarfs are anywhere near as abundant as they would have to be to account for the dark matter in our galaxy.
White Dwarfs are the final condensed states of small to medium sized stars.
Good News: White dwarfs are known to exist and to be plentiful. Maybe they could be plentiful enough to explain the dark matter if young galaxies produced white dwarfs that cool more rapidly than present theory predicts.
Bad News: No good alternative to the present theory exists. Also the production of large numbers of white dwarfs implies the production of a large amount of helium, which is not observed.
Neutron Stars or Black Holes are the final condensed states of large and very large stars.
Good News: They can be dark, especially black holes, which are totally dark, except for a negligible amount of so-called Hawking radiation. See http://chandra.harvard.edu/resources/faq/black_hole/bhole-31.html
Bad News: These objects are expected to be much scarcer than white dwarfs. Also, the processes that produce these objects release a lot of energy and heavy elements; there is no evidence of such a release.
WIMPS (Weakly Interacting Massive Particles) Examples: Exotic Subatomic Particles such as axions, massive neutrinos, and photinos.
Good News: Theoretically, WIMPS could have been produced in the Big Bang origin of the universe in the right amounts and with the right properties to explain the dark matter.
Bad News: No one has ever observed even one of these particles, let alone enough of them to explain the dark matter.
Hydrogen Gas
Good News: Seventy to seventy-five percent of the visible matter in the universe is in the form of hydrogen, the simplest element. It may be possible that the dark matter is numerous small clouds of hydrogen gas.
Bad News: It is very difficult to hide hydrogen gas from the probing, sensitive eyes of radio, infrared, optical, ultraviolet, and X-ray telescopes.