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omega | ||||
subject | fact |
omega | has definition Heavy short-lived baryon. | |
has definition The ratio of the average density of mass in the universe to the critical mass density, the latter being the density of mass needed to eventually halt the outward expansion of the universe. In an open universe, omega is always less than 1; in a closed universe, it is always greater than 1; in a flat universe it is always exactly equal to 1. Unless omega is exactly equal to 1, it changes in time, constantly decreasing in an open universe and constantly increasing in a closed universe. Omega has been measured to be about 0.1, although such measurements are difficult and uncertain. (See critical mass density; closed universe; flat universe; open universe.) | ||
is an instance of hyperon | ||
is an instance of astronomical constant | ||
hyperon | has lifetime 10-8 to 10-10 seconds | |
has spin 1/2 or 3/2 | ||
baryon | has number of quarks 3 | |
radioactive particle | has desintegration energy the total energy produced when the particle decays | |
has decay products the products produced immediately after decay | ||
number | has value | |
fermion | has quantum behavior Fermi-Dirac statistics | |
obeys exclusion principle | ||
particle | obeys uncertainty principle | |
has frequency inversely proportional to the wavelength | ||
has wavelength inversely proportional to its momentum | ||
has charge | ||
has mass | ||
physical object | has location or center of gravity | |
has angular momentum | ||
has velocity | ||
has momentum | ||
has temperature | ||
has volume | ||
has extent | ||
has material |
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