SN1987A: Temporal Models
General Relativity and Quantum Cosmology
2007-05-23 v1 Astrophysics
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.
Cite
@article{arxiv.gr-qc/0306086,
title = {SN1987A: Temporal Models},
author = {M. I. Wanas and M. Melek and M. E. Kahil},
journal= {arXiv preprint arXiv:gr-qc/0306086},
year = {2007}
}
Comments
7 pages LaTex file, published in the Proceedings of MG IX, Vol. 2, p.1100, World Scientific Pub.(2002)