Dark matter in galaxies cannot be made of neutrinos because neutrinos are too light and move too quickly to account for the gravitational effects observed in galaxies. Neutrinos also interact weakly with other particles, making them unlikely candidates for the majority of dark matter in the universe.
Neutrinos are important in the search for dark matter because they are weakly interacting particles that can provide clues about the presence of dark matter. By studying neutrinos and their interactions, scientists can gather information about the distribution and behavior of dark matter in the universe.
Dark matter is a mysterious substance that does not interact with regular matter, so it is unlikely you would be able to walk through a wall made of dark matter. Our current understanding of dark matter is that it exists in a halo around galaxies and does not clump together like regular matter to form solid structures like walls.
Dark matter does not directly affect humans as it does not interact with us on a daily basis. It primarily influences the behavior of galaxies and the universe on a larger scale, but its impact on human life is minimal.
Dark matter is believed to have been created shortly after the Big Bang. It does not emit, absorb, or reflect light, making it invisible and difficult to detect. Dark matter interacts with gravity and is thought to make up about 27 of the universe, influencing the formation and structure of galaxies and other cosmic structures.
Neutrinos are interesting because they are extremely light, neutral particles that interact very weakly with matter, making them difficult to detect. They can provide valuable insights into fundamental physics and help scientists better understand processes in the universe, such as those occurring in stars and supernovae. Studying neutrinos can also shed light on the properties of dark matter and the early universe.
Neutrinos are important in the search for dark matter because they are weakly interacting particles that can provide clues about the presence of dark matter. By studying neutrinos and their interactions, scientists can gather information about the distribution and behavior of dark matter in the universe.
Dark matter MIGHT be made of neutrinos. Problem is, we can't be certain because of two gaps in our knowledge: 1) how much mass is in one neutrino? We have an upper limit for its mass (about 1 eV) and we have a lower limit for its mass (about 0.04 eV); but we don't know any better than that. 2) how many neutrinos are out there? We can make a general estimate of how many neutrinos existed near the start of the Big Bang, but even this has some variation. Then we must ask what percentage of neutrinos have decayed in the last 13.7 billion years. Again, we know that neutrinos decay, but we don't have a good idea of how often they do so. As we get a better idea of the answer to (1) and (2), we might be able to either conclude that neutrinos account for almost all of the dark matter, or that they account for very little. Until then, we're just multiplying a speculative number times a speculative number times a speculative number.
By definiton, "dark" matter neither emits or absorbs light. Thus, it does not effect the brightness of galaxies.
most of the mass in a cluster of galaxies is invisible, which provides astronomers with the strongest evidence that the universe contains a great amount of DARK MATTER
most of the mass in a cluster of galaxies is invisible, which provides astronomers with the strongest evidence that the universe contains a great amount of DARK MATTER
Neutrinos are attractive candidates for dark matter because they are known to interact weakly with other particles, making them difficult to detect. They are also abundant in the universe and have non-zero mass, which could contribute to the overall mass content of the universe. However, current evidence suggests that the combined mass of neutrinos is not enough to account for all of dark matter.
We do not know as we have not found any dark matter to examine. The only way we detect it and know it exists is due to its gravitational attraction of the ordinary matter we can see. One speculation when neutrinos were discovered to have tiny nonzero masses was that dark matter might be neutrinos. Another speculation is that dark matter is only ordinary matter, but its in another separate universe in a shared higher dimensional spacetime. Nobody knows.
Probably not. Dark matter is not believed to concentrate well in or around masses the size of stars. But it does concentrate well around galaxies and clusters of galaxies. Most of the mass of a galaxy like ours is believed to be in a sphere of dark matter in the galaxy's spherical halo.
Yes. All hypotheses about the nature of dark matter assume it will accelerate, just like baryonic matter does in a gravitational field. In fact, one hypothesis is that dark matter consists of neutrinos, which move at near the speed of light.
Components of the universe include dark energy, dark matter, luminous matter, and other compounds that are non-luminous. Sub-components include photons, atoms, neutrinos, and dark matter.
Components of the universe include dark energy, dark matter, luminous matter, and other compounds that are non-luminous. Sub-components include photons, atoms, neutrinos, and dark matter.
Robert Alexander Swaters has written: 'Dark matter in late-type dwarf galaxies' -- subject(s): Dissertations, Dwarf galaxies, Dark matter (Astronomy)