I lift my arm, raise my thumb. We see evidence of this very often – directly from the sun during the day and reflecting off the moon at night. I. Overview of products and scientific results – Table 9", "First Planck results: the Universe is still weird and interesting", "Planck captures portrait of the young Universe, revealing earliest light", "Big-Bang Nucleosynthesis and the Baryon Density of the Universe", Monthly Notices of the Royal Astronomical Society, 10th PATRAS Workshop on Axions, WIMPs and WISPs, "The hidden lives of galaxies: Hidden mass", "The Mass Distribution in the Galactic Disc – Part III – the Local Volume Mass Density", "Some problems concerning the structure and dynamics of the galactic system and the elliptical nebulae NGC 3115 and 4494", "Vera Rubin, 88, Dies; Opened Doors in Astronomy, and for Women", "First observational evidence of dark matter", "A neutral hydrogen survey of the southern regions of the Andromeda nebula", "Dark matter may be smoother than expected – Careful study of large area of sky imaged by VST reveals intriguing result", "Scientists unveil the most detailed map of dark matter to date", "Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations", "Hubble snaps dark matter warping spacetime", "Intermediate Guide to the Acoustic Peaks and Polarization", "Hubble Maps the Cosmic Web of "Clumpy" Dark Matter in 3-D", "Constraints on the composite photon theory", "Science-in-progress: Did the Bullet Cluster withstand scrutiny?
Could Planet 9 be a primordial black hole? So why do scientists think it dominates?
", "Obviously, that's the real prize. [164][165][166], The prevailing opinion among most astrophysicists is while modifications to general relativity can conceivably explain part of the observational evidence, there is probably enough data to conclude there must be some form of dark matter.[167]. However, multiple lines of evidence suggest the majority of dark matter is not made of baryons: Candidates for non-baryonic dark matter are hypothetical particles such as axions, sterile neutrinos, weakly interacting massive particles (WIMPs), gravitationally-interacting massive particles (GIMPs), supersymmetric particles, or primordial black holes. Only about 4% of the total energy density in the universe (as inferred from gravitational effects) can be seen directly. She kisses me. In addition, if the particles of which it is composed are supersymmetric, they can undergo annihilation interactions with themselves, possibly resulting in observable by-products such as gamma rays and neutrinos (indirect detection).[98]. Examples of underground laboratories with direct detection experiments include the Stawell mine, the Soudan mine, the SNOLAB underground laboratory at Sudbury, the Gran Sasso National Laboratory, the Canfranc Underground Laboratory, the Boulby Underground Laboratory, the Deep Underground Science and Engineering Laboratory and the China Jinping Underground Laboratory. By examining the apparent shear deformation of the adjacent background galaxies, the mean distribution of dark matter can be characterized. Please try again. The excess can be explained by annihilations of dark matter particles with a mass between 31 and 40 billion electron volts, researchers said.
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