We discuss four approaches to the determination of absolute neutrino mass.
These are the measurement of the zero-neutrino double beta decay rate, of t
he tritium decay end-point spectrum, of the cosmic ray spectrum above the G
ZK cutoff (in the Z-burst model), and the cosmological measurement of the p
ower spectrum governing the CMB and large scale structure. The first two ap
proaches are sensitive to the mass eigenstates coupling to the electron neu
trino, whereas the latter two are sensitive to the heavy component of the c
osmic neutrino background. All mass eigenstates are related by the deltam(2
)'s inferred from neutrino oscillation data. Consequently, the potential fo
r the absolute mass determination of each of the four approaches is correla
ted with the other three, in ways that we point out.