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By Thomas ( Ed. ) Abbondi

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There are several problems with such a notion, one being the adiabatic losses on the way from close to the pulsar out to the interstellar gas, and another one the sky distribution, which should be very anisotropic given the distribution and strength of galactic magnetic fields. On the other hand, if this concept could be proven, it would certainly provide a very easy expla- nation for why there are particles beyond the GZK cutoff: for galactic particles the interaction with the microwave background is totally irrelevant, and so no GZK cutoff is expected.

Examples include measurements of the solar neutrino flux which challenge our understanding of energy generation in the stars and attempts to detect the superpartners, axions, strings, and other exotic objects predicted by various models in highenergy physics and possible solutions to the missing-mass problem. The standard theoretical model in cosmology for the past several decades has been based on Einstein’s general theory of relativity, supplemented by assumptions about the homogeneity and isotropy of space–time, and data from spectroscopy, consistent with understanding gained from nuclear physics, about the distribution of ordinary matter among various species.

67 × 1027 g. 15 × 107 . 5 × 1010 years; our galaxy is younger than the universe, but we do not know the two ages well enough to determine the difference with any reliability. • Units: energy. 6 × 10−12 erg; 1 MeV = 106 eV, 1 GeV = 109 eV, 1 TeV = 1012 eV, 1 PeV = 1015 eV, 1 EeV = 1015 eV. • Elementary particles. The natural constituents of matter are the proton, neutron, and electron. 511 MeV. This is in energy units using Einstein’s equivalence E = mc2 , where E is the energy, m the rest mass, and c the speed of light.

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