The best-known theories of this class are MOND and its relativistic generalization tensorvectorscalar gravity (TeVeS),[173] f(R) gravity,[174] negative mass, dark fluid,[175][176][177] and entropic gravity. [70][71], If dark matter does not exist, then the next most likely explanation must be that general relativity the prevailing theory of gravity is incorrect and should be modified. They travel around the cosmos conquering planets by poisoning the atmosphere with their mind-controlling clouds. Although WIMPs have been the main search candidates,[15] axions have drawn renewed attention, with the Axion Dark Matter Experiment (ADMX) searches for axions and many more planned in the future. [66][67], The observed CMB angular power spectrum provides powerful evidence in support of dark matter, as its precise structure is well fitted by the Lambda-CDM model,[67] but difficult to reproduce with any competing model such as modified Newtonian dynamics (MOND).[67][68]. Darkness is mostly used to cloud everything into total darkness, but can also be channeled to a variety of effects, both as an absence of light and a solid substance: one can also control and manipulate the beings that exist there, create and dispel shields and areas of total darkness, create constructs and weapons, teleport one's self through massive distances via shadows, etc. This is the focus for dark matter research, as hot dark matter does not seem capable of supporting galaxy or galaxy cluster formation, and most particle candidates slowed early. The constituents of cold dark matter are unknown. Aoi Fukasaku (Coppelion) possesses an energy field for various powers that are related to manipulating dark matter. [d] From Kepler's Second Law, it is expected that the rotation velocities will decrease with distance from the center, similar to the Solar System. Instituto de Astrofsica de Canarias (IAC). Wisely Kamelot's Dark Matter is in his Demon Eye which he can read the minds of othersand force people to relive memories explode/implode the brains of his targets. Summary Dark Matter Manipulation is the ability to control Dark Matter, which is a hypothetical form of matter that gets it's name from the fact it can't be interacted with electromagnetic radiation, such as light. These maps are slightly distorted because distances are estimated from observed redshifts; the redshift contains a contribution from the galaxy's so-called peculiar velocity in addition to the dominant Hubble expansion term. Deletions from the Genome, End for Indus Megacities: Prolonged Droughts. In 1972, David Rogstad and Seth Shostak[45] published H-I rotation curves of five spirals mapped with the Owens Valley interferometer; the rotation curves of all five were very flat, suggesting very large values of mass-to-light ratio in the outer parts of their extended H-I disks. Dark matter does not interact directly with radiation, but it does affect the cosmic microwave background (CMB) by its gravitational potential (mainly on large scales) and by its effects on the density and velocity of ordinary matter. Candidate particles can be grouped into three categories on the basis of their effect on the fluctuation spectrum (Bond et al. The different scale factors for matter and radiation are a consequence of radiation redshift: for example, after gradually doubling the diameter of the observable Universe via cosmic expansion in General Relativity, a has been doubled. It is fatal to the touch, disintegrating the unfortunate victim completely, and even eating holes in space. Opposite of Mirror Matter Manipulation and Matter Manipulation . Opposite of Mirror Matter Manipulation and Matter Manipulation. It allows us to be honest with ourselves, to express those values that we would disavow in the light. User can create, shape and manipulate Dark Matter, a hypothetical type of matter distinct from baryonic matter (ordinary matter such as protons and neutrons), neutrinos and dark energy. [154][155][156], Many experimental searches have been undertaken to look for such emission from dark matter annihilation or decay, examples of which follow. The mass-to-light ratios correspond to dark matter densities predicted by other large-scale structure measurements. Instead, they may be matter or energy of varying properties, depending on the manufacturing process, such as being outside the boundaries of the laws of physics, or granting abilities and even bodies. You could, in principle, manipulate dark matter using gravitational forces. As more sensitive receivers became available, Morton Roberts and Robert Whitehurst[44] were able to trace the rotational velocity of Andromeda to 30 kpc, much beyond the optical measurements. Lord Kelvin concluded "Many of our supposed thousand million stars, perhaps a great majority of them, may be dark bodies". ScienceDaily. Because a dark matter particle should have negligible interactions with normal visible matter, it may be detected indirectly as (large amounts of) missing energy and momentum that escape the detectors, provided other (non-negligible) collision products are detected. [2], The primary evidence for dark matter comes from calculations showing that many galaxies would behave quite differently if they did not contain a large amount of unseen matter. [65], The CMB anisotropy was first discovered by COBE in 1992, though this had too coarse resolution to detect the acoustic peaks. Contents 1 Also Called 2 Capabilities 2.1 Universal Differences 2.2 Other 3 Applications 4 Techniques 5 Variations 6 Associations 7 Limitations 8 Known Users Power/Ability to: Manipulate darkness. The user can create, shape and manipulate Dark Matter, a hypothetical type of matter distinct from baryonic matter (ordinary matter such as protons and neutrons), neutrinos and dark energy. Nonetheless, Zwicky did correctly conclude from his calculation that the bulk of the matter was dark. Number 95: Galaxy Eyes Dark Matter Dragon (Yu-Gi-Oh!) Directional dark matter experiments include DMTPC, DRIFT, Newage and MIMAC. There are many candidates for CDM including supersymmetric particles. Shadow Matter | X Men Destiny Wiki | Fandom [15] Dark matter is classified as "cold", "warm", or "hot" according to its velocity (more precisely, its free streaming length). Some researchers consider this a better fit to observations. Questions? Most of the ordinary matter familiar to astronomers, including planets, brown dwarfs, red dwarfs, visible stars, white dwarfs, neutron stars, and black holes, is called baryonic matter (referring to the baryons that dominate the mass of most ordinary matter). Contents 1 History 1.1 Dark Elf Conflict 1.1.1 Preparing Algrim's Mission 1.1.2 Sacking of Asgard 1.2 Alternate Universe Versions 1.2.1 Used by the Collector 2 Capabilities 3 Gallery 4 References History Dark Elf Conflict Preparing Algrim's Mission ", "First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5350GeV", "First Result from the Alpha Magnetic Spectrometer Experiment", "Scientists find hint of dark matter from cosmos", "Alpha Magnetic Spectrometer zeroes in on dark matter", "NASA TV Briefing Discusses Alpha Magnetic Spectrometer Results", "New Clues to the Mystery of Dark Matter", "The dark matter problem from f(R) gravity viewpoint", "Bringing balance to the universe: New theory could explain missing 95 percent of the cosmos", "New theory of gravity might explain dark matter", "Verlinde's new theory of gravity passes first test", "First test of rival to Einstein's gravity kills off dark matter", "Unique prediction of 'modified gravity' challenges dark matter", "Dark matter vs. modified gravity: A trialogue", "Incandescent: Light Bulbs and Conspiracies", "The X-Files/Millennium: "F. Emasculata"/"Soft Light"/"Our Town"/"Anasazi", "First 3D map of the Universe's dark matter scaffolding", "Dark matter maps reveal cosmic scaffolding", "News CFHT - Astronomers reach new frontiers of dark matter", "CFHTLenS: the CanadaFranceHawaii Telescope Lensing Survey: CFHTLenS", "Gravitational lensing analysis of the Kilo-Degree Survey", "Hyper Suprime-Cam Survey Maps Dark Matter in the Universe - News - Carnegie Mellon University", "Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data", "Dark Energy Survey Year 3 results: Curved-sky weak lensing mass map reconstruction", "The most detailed 3D map of the Universe ever made", Missing Dark Matter in a far-away galaxy, "Helmholtz Alliance for Astroparticle Physics", "Astronomers claim first 'dark galaxy' find", "Astronomers' doubts about the Dark Side ", "The physicist who denies that dark matter exists", What is Dark Matter Puzzling Missing Mass of the Universe, Mathematical formulation of the Standard Model, Religious interpretations of the Big Bang, https://en.wikipedia.org/w/index.php?title=Dark_matter&oldid=1152169363, Short description is different from Wikidata, Pages using sidebar with the child parameter, Articles with unsourced statements from April 2016, Wikipedia articles needing clarification from September 2018, Wikipedia articles needing clarification from September 2021, Pages displaying wikidata descriptions as a fallback via Module:Annotated link, Pages displaying short descriptions of redirect targets via Module:Annotated link, Creative Commons Attribution-ShareAlike License 3.0, From the scatter in radial velocities of the galaxies within clusters. Dark Energy Physics Manipulation Capabilities The user can create, shape and manipulate dark energy, usually drawn from inter-dimensional or other similar sources. Primordial density fluctuations smaller than this length get washed out as particles spread from overdense to underdense regions, while larger fluctuations are unaffected; therefore this length sets a minimum scale for later structure formation. Prior to structure formation, the Friedmann solutions to general relativity describe a homogeneous universe. He estimated the cluster had about 400 times more mass than was visually observable. The categories are set with respect to the size of a protogalaxy (an object that later evolves into a dwarf galaxy): Dark matter particles are classified as cold, warm, or hot according to their FSL; much smaller (cold), similar to (warm), or much larger (hot) than a protogalaxy. In parallel, the use of interferometric arrays for extragalactic H-I spectroscopy was being developed. [82] Combining the CMB observations with BAO measurements from galaxy redshift surveys provides a precise estimate of the Hubble constant and the average matter density in the Universe. After the discovery of the first acoustic peak by the balloon-borne BOOMERanG experiment in 2000, the power spectrum was precisely observed by WMAP in 20032012, and even more precisely by the Planck spacecraft in 20132015. Darkforce | Marvel Cinematic Universe Wiki | Fandom But in spite of the essential role that this extra material plays, we know almost nothing about its nature, behaviour and composition, which is one of the basic problems of modern physics. [116] Nonetheless, research and theories proposing dense dark matter accounts for dark matter continue as of 2018, including approaches to dark matter cooling,[117][118] and the question remains unsettled. 1983). Thus dark matter may accumulate at the center of these bodies, increasing the chance of collision/annihilation. BAOs set up a preferred length scale for baryons. Advanced Umbrakinesis practitioners can actually cause entire cities or countries to fall into total darkness, just using the power of their mind. A darkness so dense it sucks in everything. Sufficient diffuse, baryonic gas or dust would be visible when backlit by stars. These are predicted to arise in the Lambda-CDM model due to acoustic oscillations in the photonbaryon fluid of the early universe, and can be observed in the cosmic microwave background angular power spectrum. Warm dark matter comprises particles with an FSL comparable to the size of a protogalaxy. If a character were able to have the power of dark matter manipulation Void Wind: The dark counterpart to the Sphere of the Gods which can snuff out magic and gods. The neutrino qualifies as such a particle. WIMPs coming from the direction in which the Sun travels (approximately towards Cygnus) may then be separated from background, which should be isotropic. [194][195], DM map by the CFHT Lensing Survey (CFHTLenS) using the CanadaFranceHawaii Telescope (2012). Following Babcock's 1939 report of unexpectedly rapid rotation in the outskirts of the Andromeda galaxy and a mass-to-light ratio of 50; in 1940 Jan Oort discovered and wrote about the large non-visible halo of NGC3115. A Level 4 Akuma (D.Gray-man) turning its arms into Gatling guns that fire deadly Dark Matter blood bullets that disintegrate any normal humans. Some galaxies would not have formed at all and others would not move as they currently do. The density of dark matter in the centres of galaxies has been a mystery for decades. Superpower Wiki is a FANDOM Anime Community. Note: Darkness Manipulation is essentially the same as Shadow Manipulation, in the sense that all of its applications would be identical. Real dark matter exists but doesn't affect normal matter, it can't be touched, it can't be seen, the user . Zero Point Energy Field Manipulator | Half-Life Wiki | Fandom Variation of Dark Matter Manipulation. [b] The primary candidate for dark matter is some new kind of elementary particle that has not yet been discovered, particularly weakly interacting massive particles (WIMPs). [65] The first peak mostly shows the density of baryonic matter, while the third peak relates mostly to the density of dark matter, measuring the density of matter and the density of atoms. Apathy Ability 1. Detailed analysis of the small irregularities (anisotropies) in the, This page was last edited on 28 April 2023, at 16:45. Because no one has directly observed dark matter yet assuming it exists it must barely interact with ordinary baryonic matter and radiation except through gravity. [27], In 1933, Swiss astrophysicist Fritz Zwicky, who studied galaxy clusters while working at the California Institute of Technology, made a similar inference. Various astrophysical observations - including gravitational . Strongest DARK MATTER users in the Universe - YouTube Contents You would need some kind of true sight or all knowing . Eshi (D.Gray-Man) forming chains out of Dark Matter, which allows him to manipulate the gravity field around anything the chains are bound to. Galaxy clusters are particularly important for dark matter studies since their masses can be estimated in three independent ways: Generally, these three methods are in reasonable agreement that dark matter outweighs visible matter by approximately 5 to 1.[54]. This effect is not detectable for any one structure since the true shape is not known, but can be measured by averaging over many structures. These processes could be detected indirectly through an excess of gamma rays, antiprotons or positrons emanating from high density regions in our galaxy or others. In 1939, Horace W. Babcock reported the rotation curve for the Andromeda nebula (known now as the Andromeda Galaxy), which suggested the mass-to-luminosity ratio increases radially. Context will usually indicate which meaning is intended. Possibilities range from large objects like MACHOs (such as black holes[127] and Preon stars[128]) or RAMBOs (such as clusters of brown dwarfs), to new particles such as WIMPs and axions.
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