The production of high energy neutrinos by big bing particles is revie
wed. The big bang particles are divided into two categories: dark matt
er particles (DMP), i.e. those with the critical mass density (rho(X)
= rho(c)) at present, and the exotic relics whose mass density can be
smaller than the critical one. For the case of DMP the neutralino and
the gravitino are considered. High energy neutrinos can be produced du
e to the capture of the neutralinos in the earth and the sun, with the
subsequent annihilation of these particles there. If R-parity is weak
ly violated, the neutralino decay can be a source of high energy neutr
inos. The gravitino as DMP is unobservable directly, unless R-parity i
s violated and the gravitino decays. For thermal exotic relics a very
general conclusion is reached: the detectable neutrino flux can be pro
duced only by long-lived particles with tau(X) > t(o) where t(o) is th
e age of the Universe (the exceptional case is the decay only to the n
eutrinos). Very large neutrino fluxes can be produced by superheavy (U
p to approximately 10(18) GeV) metastable relics in the particular cos
mological scenario where the violent entropy production occurs.