Refinement of the Proposed Gamma-Ray Burst Time Delay Model
| dc.contributor.author | Abbey, G.F. | |
| dc.contributor.author | Simfukwe, J. | |
| dc.contributor.author | Simpemba, P.C. | |
| dc.contributor.author | Phiri, S.P. | |
| dc.contributor.author | Srivastava, A. | |
| dc.contributor.author | Nyambuya, G.G. | |
| dc.date.accessioned | 2025-07-07T14:14:16Z | |
| dc.date.available | 2025-07-07T14:14:16Z | |
| dc.date.issued | 2024-06-28 | |
| dc.description.abstract | This paper is the second instalment in our study of the observed time delay in the arrival times of radio photons emanating from Gamma Ray Bursts (GRBs). The mundane assumption in contemporary physics as to the cause of these pondersome time delays is that they are a result of the photon being endowed with a non-zero mass. While we do not rule out the possibility of a non-zero mass for the photon, our working assumption is that the major cause of these time delays may very well be that these photons are travelling in a rarefied cosmic plasma in which the medium’s electrons interact with the electric component of the Photon, thus generating tiny currents that lead to dispersion, hence, a frequency-dependent speed of Light (FDSL). In the present instalment, we “improve” on the model presented in the first instalment by dropping the assumption that the resultant pairs of these radio photons leave the shock front simultaneously. The new assumption of a non-simultaneous— albeit systematic—emission of these photon pairs allows us to obtain a much more convincing and stronger correlation in the time delay. This new correlation allows us to build a unified model for the four GRBs in our sample using a relative distance correction mechanism. The new unified model allows us to obtain as our most significant result a value for the frequency equivalence of the interstellar medium (ISM)’s conductance ν* ~ 1.500 ± 0.009 Hz and also an independent distance measure to the GRBs where we obtain for our four GRB samples an average distance of: ~69.40 ± 0.10, 40.00 ± 0.00, 58.40 ± 0.40, and 86.00 ± 1.00 Mpc, for GRB 030329, 980425, 000418 and 021004 respectively. | |
| dc.description.sponsorship | Financial support was obtained from Education, Audio and Culture Executive Agency of the European Commission through the Pan-African Planetary and Space Science Network under funding agreement number 6242.24-PANAF-12020-1-BW-PANAF-MOBAF. | |
| dc.identifier.citation | Abbey, G.F., Simfukwe, J., Simpemba, P.C., Phiri, S.P., Srivastava, A. and Nyambuya, G.G. (2024) Refinement of the Proposed Gamma-Ray Burst Time Delay Model. International Journal of Astronomy and Astrophysics, 14, 120-147. https://doi.org/10.4236/ijaa.2024.142008 | |
| dc.identifier.issn | 2161-4725 | |
| dc.identifier.uri | http://196.220.97.103:4000/handle/123456789/926 | |
| dc.language.iso | en | |
| dc.publisher | International Journal of Astronomy and Astrophysics | |
| dc.title | Refinement of the Proposed Gamma-Ray Burst Time Delay Model | |
| dc.type | Article |