SN1987A: Temporal Models

dc.creatorWanas, M. I.
dc.creatorMelek, M.
dc.creatorKahil, M. E.
dc.date2003-06-19
dc.date.accessioned2026-07-07T06:35:00Z
dc.date.available2026-07-07T06:35:00Z
dc.descriptionIt 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.
dc.description7 pages LaTex file, published in the Proceedings of MG IX, Vol. 2, p.1100, World Scientific Pub.(2002)
dc.identifierhttps://arxiv.org/abs/gr-qc/0306086
dc.identifierhttp://arxiv.org/abs/gr-qc/0306086
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/99691
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleSN1987A: Temporal Models
dc.typetext

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