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en_US |
dc.description.abstract |
It is well known that carriers of astrophysical information are massless spinning
particles. These carriers are photons, neutrinos and, expectedly, gravitons. All these
particles are emitted during supernova events. Information carried by these particles
characterize their sources, but such information are affected by the trajectories
of the carriers. Recently, it is shown that these trajectories are spin dependent.
Knowing these trajectories and the arrival times of such particles to the detectors,
a spin dependent model is constructed and compared with the conventional spin
independent model. |
en_US |