Universe - the definitive visual guide Gen ed Martin Rees Dark matter and dark energy DK 2012
There is far more dark matter in the Universe than that contained in stars and other visible objects. The invisible mass is called "dark matter". Its composition is unknown. Some might take the form of MACHOs (massive compact objects) - dark planet-like bodies - or WIMPs (weakly interacting massive particles) - exotic subatomic entities that scarcely interact with ordinary matter. . . . . . . . . . Cosmologists have proposed the existence of "dark energy", a force that counteracts gravity and causes the Universe to expand faster. The exact nature of dark energy is still speculative."
The Theory of (nearly) Everything BBC Focus Ed Daniel Bennett Searching for dark matter 2016
In terms of mass-energy "the Universe is 68% dark energy, 27% dark matter and 5% baryonic. If we discount the energy part, the numbers revert to - 85% dark matter (and) 15% baryonic matter."
"Has dark matter got anything to do with dark energy?
No. Dark energy is the name given to the mysterious entity thought to be accelerating the overall expansion of the Universe - a sort of anti-gravity. In contrast, dark matter can be thought of as gravitational glue that helps bind galaxies and clusters of galaxies together. We're literally in the dark as to what they are."
"Could dark matter be something else?
So far we've been assuming that dark matter is tangible, something that truly exists. But what if it doesn't . . . - a symptom of the fact that we don't understand gravity properly? That's exactly what proponents of a theory called Modified Newtonian Dynamics (MOND) advocate. . . . dark matter was introduced to account for the fact that stars in the Milky Way don't slow down the further they are from the galactic centre, unlike the planets of our Solar System. . . . . . . . . . The idea was first put forward by . . . Mordehai Milgrom in 1983. He suggested that the strength of gravity could become stronger where acceleration levels are small."
Astronomy Simulations zoom in on dark matter by Mark Zastrow February 2021
"Dark matter is a mysterious material that makes up more than 80% of all matter in the universe, This strange stuff permeates and surrounds every galaxy, and clumps of dark matter, called halos, are where galaxies tend to form. Now, supercomputer simulations have found that these cosmic clumps of dark matter look surprisingly alike, no matter their size - whether they encompass monstrous galaxy clusters or are mini-blobs the size of Earth. . . . . . . . . . While dark matter does not react with normal matter, it should give off a burst of gamma-ray light when it collides with its antimatter equivalent and the particles annihilate each other."
Endless Universe - beyond the big bang by Steinhardt and Turok Doubleday 2007
" . . . . . . dark matter and dark energy, rather unimaginative names for the two most surprising and enigmatic constituents of the Universe. The nomenclature is actually confusing because it suggests that the two are related, whereas the only thing they have in common is that they do not absorb or scatter light. Otherwise, their physical properties are completely different. And their roles in this history of the Universe. Dark matter dominated the past; dark energy will shape the future." . . . . . . . . .
"Most physicists think that dark matter consists of an ocean of elementary particles that are electrically neutral, so that they interact very weakly with ordinary matter, and do not scatter or absorb light. This would explain why the particles are not noticed even though the Earth is constantly moving through a sea of dark matter as it orbits the Sun."
The State of the Universe by Pedro G Ferreira Phoenix 2007
Dark and Exotic Matter
"Two main types of candidate for the missing matter have been proposed . . . . . . very heavy clumps of ordinary matter . . . and an altogether different kind of matter that does not emit or interact with radiation. (The neutrino - a failed candidate for dark matter.) . . . so we have to consider completely new types of particles . . . ." . . . . . . . . .
"The favoured candidate for dark matter drawn from supersymmetry theories is called the neutralino, a heavy, long-lived particle. Such particles would have to be heavy enough that even a small number of them would make an appreciable contribution to the mass density of the Universe. . . . . . . Neutralinos would be very weakly interacting and, if they existed, they would be constantly streaming through normal matter." . . . . . .
" . . . the WIMP (Weakly Interacting Massive Particles) candidate is in fact incredibly light, with a mass of less than one millionth that of the electron. Such a candidate, the axion, was postulated to solve a problem in the theory of strong interactions. . . . . . . . . . As with all other dark matter candidates, the mildness of the axion's interactions makes it incredibly difficult to detect." . . . . . . . . .
"The presence of dark matter is one of the main unsolved problems in cosmology. We are quite convinced that it exists, but we have no real idea of what it is or how to see it."
All About Space Issue 112 Dark Matter by Kulvinder Singh Chadha January 2021
"Dark Matter - where did it come from?
"Fritz Zwicky was a Swiss astronomer . . . . . . averaging the rotations of galaxies in the Coma Cluster . . . Zwicky noticed that their speeds were excessive . . . so much so, that the galaxies should have flown apart. there wasn't enough visible matter to gravitationally bind each galaxy together . . . he concluded that there must be a 'dark matter' component to them. . . . Six years later . . . Horace Babcock showed dark matter present in the Andromeda Galaxy . . . was more concentrated in the periphery of the disc . . . . . . the first indication that galaxies had dark matter haloes. . . . in the late 1970s, Rubin and Ford showed . . . that galaxies contained between 5 and 10 times more dark matter than luminous matter."
"The term 'dark matter' is a slight misnomer. It simply isn't dark; it's completely invisible, no matter which part of the electromagnetic spectrum it's observed in. Its only observed effect is gravitational . . . but this gives dark matter a dramatic character, one predicted by Einstein . . . ".
"No one has yet been successful in detecting dark matter, so how would someone look for dark matter filtered by cosmic bubbles? 'We consider the best prospects for finding evidence for our proposal are collider searches for the new [phi] particle, detection of dark matter annihilation products or detection of background gravitational waves."
"The puzzle of dark matter forces us to think in new ways, and even if these ideas turn out to be unrelated, they could provide the key to understanding some of the deepest mysteries in the Universe."
Work in progress. Last edit 14.00 BST June 14th 2021.
There is far more dark matter in the Universe than that contained in stars and other visible objects. The invisible mass is called "dark matter". Its composition is unknown. Some might take the form of MACHOs (massive compact objects) - dark planet-like bodies - or WIMPs (weakly interacting massive particles) - exotic subatomic entities that scarcely interact with ordinary matter. . . . . . . . . . Cosmologists have proposed the existence of "dark energy", a force that counteracts gravity and causes the Universe to expand faster. The exact nature of dark energy is still speculative."
The Theory of (nearly) Everything BBC Focus Ed Daniel Bennett Searching for dark matter 2016
In terms of mass-energy "the Universe is 68% dark energy, 27% dark matter and 5% baryonic. If we discount the energy part, the numbers revert to - 85% dark matter (and) 15% baryonic matter."
"Has dark matter got anything to do with dark energy?
No. Dark energy is the name given to the mysterious entity thought to be accelerating the overall expansion of the Universe - a sort of anti-gravity. In contrast, dark matter can be thought of as gravitational glue that helps bind galaxies and clusters of galaxies together. We're literally in the dark as to what they are."
"Could dark matter be something else?
So far we've been assuming that dark matter is tangible, something that truly exists. But what if it doesn't . . . - a symptom of the fact that we don't understand gravity properly? That's exactly what proponents of a theory called Modified Newtonian Dynamics (MOND) advocate. . . . dark matter was introduced to account for the fact that stars in the Milky Way don't slow down the further they are from the galactic centre, unlike the planets of our Solar System. . . . . . . . . . The idea was first put forward by . . . Mordehai Milgrom in 1983. He suggested that the strength of gravity could become stronger where acceleration levels are small."
Astronomy Simulations zoom in on dark matter by Mark Zastrow February 2021
"Dark matter is a mysterious material that makes up more than 80% of all matter in the universe, This strange stuff permeates and surrounds every galaxy, and clumps of dark matter, called halos, are where galaxies tend to form. Now, supercomputer simulations have found that these cosmic clumps of dark matter look surprisingly alike, no matter their size - whether they encompass monstrous galaxy clusters or are mini-blobs the size of Earth. . . . . . . . . . While dark matter does not react with normal matter, it should give off a burst of gamma-ray light when it collides with its antimatter equivalent and the particles annihilate each other."
Endless Universe - beyond the big bang by Steinhardt and Turok Doubleday 2007
" . . . . . . dark matter and dark energy, rather unimaginative names for the two most surprising and enigmatic constituents of the Universe. The nomenclature is actually confusing because it suggests that the two are related, whereas the only thing they have in common is that they do not absorb or scatter light. Otherwise, their physical properties are completely different. And their roles in this history of the Universe. Dark matter dominated the past; dark energy will shape the future." . . . . . . . . .
"Most physicists think that dark matter consists of an ocean of elementary particles that are electrically neutral, so that they interact very weakly with ordinary matter, and do not scatter or absorb light. This would explain why the particles are not noticed even though the Earth is constantly moving through a sea of dark matter as it orbits the Sun."
The State of the Universe by Pedro G Ferreira Phoenix 2007
Dark and Exotic Matter
"Two main types of candidate for the missing matter have been proposed . . . . . . very heavy clumps of ordinary matter . . . and an altogether different kind of matter that does not emit or interact with radiation. (The neutrino - a failed candidate for dark matter.) . . . so we have to consider completely new types of particles . . . ." . . . . . . . . .
"The favoured candidate for dark matter drawn from supersymmetry theories is called the neutralino, a heavy, long-lived particle. Such particles would have to be heavy enough that even a small number of them would make an appreciable contribution to the mass density of the Universe. . . . . . . Neutralinos would be very weakly interacting and, if they existed, they would be constantly streaming through normal matter." . . . . . .
" . . . the WIMP (Weakly Interacting Massive Particles) candidate is in fact incredibly light, with a mass of less than one millionth that of the electron. Such a candidate, the axion, was postulated to solve a problem in the theory of strong interactions. . . . . . . . . . As with all other dark matter candidates, the mildness of the axion's interactions makes it incredibly difficult to detect." . . . . . . . . .
"The presence of dark matter is one of the main unsolved problems in cosmology. We are quite convinced that it exists, but we have no real idea of what it is or how to see it."
All About Space Issue 112 Dark Matter by Kulvinder Singh Chadha January 2021
"Dark Matter - where did it come from?
"Fritz Zwicky was a Swiss astronomer . . . . . . averaging the rotations of galaxies in the Coma Cluster . . . Zwicky noticed that their speeds were excessive . . . so much so, that the galaxies should have flown apart. there wasn't enough visible matter to gravitationally bind each galaxy together . . . he concluded that there must be a 'dark matter' component to them. . . . Six years later . . . Horace Babcock showed dark matter present in the Andromeda Galaxy . . . was more concentrated in the periphery of the disc . . . . . . the first indication that galaxies had dark matter haloes. . . . in the late 1970s, Rubin and Ford showed . . . that galaxies contained between 5 and 10 times more dark matter than luminous matter."
"The term 'dark matter' is a slight misnomer. It simply isn't dark; it's completely invisible, no matter which part of the electromagnetic spectrum it's observed in. Its only observed effect is gravitational . . . but this gives dark matter a dramatic character, one predicted by Einstein . . . ".
"No one has yet been successful in detecting dark matter, so how would someone look for dark matter filtered by cosmic bubbles? 'We consider the best prospects for finding evidence for our proposal are collider searches for the new [phi] particle, detection of dark matter annihilation products or detection of background gravitational waves."
"The puzzle of dark matter forces us to think in new ways, and even if these ideas turn out to be unrelated, they could provide the key to understanding some of the deepest mysteries in the Universe."
Work in progress. Last edit 14.00 BST June 14th 2021.
Last edited: