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| dc.contributor.author | I. Wanas, M. | |
| dc.contributor.author | Melek, M. | |
| dc.contributor.author | E. Kahil, M. | |
| dc.date.accessioned | 2020-01-18T08:19:47Z | |
| dc.date.available | 2020-01-18T08:19:47Z | |
| dc.date.issued | 2002 | |
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| dc.identifier.uri | https://arxiv.org/pdf/gr-qc/0306086.pdf | |
| dc.description | MSA Google Scholar | |
| 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 |
| dc.description.sponsorship | The Ninth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity, Gravitation and Relativistic Field Theories (In 3 Volumes) | en_US |
| dc.language.iso | en | en_US |
| dc.publisher | The 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.ispartofseries | The Ninth Marcel Grossmann Meeting;pages : 1100-1105 | |
| dc.subject | University of Photons, neutrinos, gravitons | en_US |
| dc.title | SN1987A: temporal models | en_US |
| dc.type | Article | en_US |
| dc.Affiliation | October University for modern sciences and Arts (MSA) |
