SN1987A: temporal models

dc.AffiliationOctober University for modern sciences and Arts (MSA)
dc.contributor.authorI. Wanas, M.
dc.contributor.authorMelek, M.
dc.contributor.authorE. Kahil, M.
dc.date.accessioned2020-01-18T08:19:47Z
dc.date.available2020-01-18T08:19:47Z
dc.date.issued2002
dc.descriptionMSA Google Scholar
dc.description.abstractIt 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
dc.description.sponsorshipThe Ninth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories (In 3 Volumes)en_US
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dc.identifier.urihttps://arxiv.org/pdf/gr-qc/0306086.pdf
dc.language.isoenen_US
dc.publisherThe Ninth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories (In 3 Volumes)en_US
dc.relation.ispartofseriesThe Ninth Marcel Grossmann Meeting;pages : 1100-1105
dc.subjectUniversity of Photons, neutrinos, gravitonsen_US
dc.titleSN1987A: temporal modelsen_US
dc.typeArticleen_US

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