Andere Kunden interessierten sich auch für
![Search for ¿-mesic helium via dd¿3Henpi0 reaction at WASA-at-COSY]( "Search for ¿-mesic helium via dd¿3Henpi0 reaction at WASA-at-COSY")
Search for ¿-mesic helium via dd¿3Henpi0 reaction at WASA-at-COSY32,99 €![Unification of Science]( "Unification of Science")
Unification of Science15,99 €![Synthesis of Silver Nanoparticles via Chemical and Green Routes]( "Synthesis of Silver Nanoparticles via Chemical and Green Routes")
Synthesis of Silver Nanoparticles via Chemical and Green Routes42,99 €![A search for proton decay via p ¿ ¿+K0 in Super Kamiokande I]( "A search for proton decay via p ¿ ¿+K0 in Super Kamiokande I")
A search for proton decay via p ¿ ¿+K0 in Super Kamiokande I44,99 €![New Look to the World of Dark Energy and Materials]( "New Look to the World of Dark Energy and Materials")
New Look to the World of Dark Energy and Materials39,99 €![Joint search for gravitational waves and High-energy neutrinos]( "Joint search for gravitational waves and High-energy neutrinos")
Joint search for gravitational waves and High-energy neutrinos42,99 €![In Search of Asteroids: Orbit Calculation and Citizen Science]( "In Search of Asteroids: Orbit Calculation and Citizen Science")
In Search of Asteroids: Orbit Calculation and Citizen Science29,99 €
Dark matter is a non-baryonic type of matter that accounts for the total amount of mass in the Universe. After many observations, starting with the pioneering ones, of Jan Oort in 1932 and Fritz Zwicky in 1933, physicists have discovered that a large mass constitute of the Universe exists in a non-luminous and non-absorbing form. The evidence of the missing mass came up by observing the rotation curves and orbital velocities of stars in the Milky Way, as also the orbital velocities of galaxies in clusters of galaxies. The velocities of various luminous objects (stars, gas clouds or entire galaxies) reveal that these objects move faster than expected if they only felt the gravitational attraction of other visible objects. The existence of Dark Matter (DM) became plausible after the observed gravitational lensing of background objects by galaxy clusters, the temperature distribution of hot gas in galaxies and clusters of galaxies and recently the pattern of anisotropies in the cosmic microwave background. This book reveal the way of the axion research at CERN with the axion telescope. The research is focused on the axion particle as a strong DM candidate.