Nota de FísicaPublicado
Weak-Scale Hidden Sector and Energy Transport in Fireball Models of Gamma-Ray Bursts
Durmus A. Demir; Herman J. Mosquera Cuesta
2000
Datos de la publicación
- Autores
- Durmus A. Demir; Herman J. Mosquera Cuesta
- Tipo
- Nota de Física
- Estado
- Publicado
- Fecha de publicación
- 2000
- Descripción
- The annihilation of pairs of very weakly interacting particles in the neibourghood of gamma-ray sources is introduced here as a plausible mechanism to overcome the baryon load problem. This way we can explain how these very high energy gamma-ray bursts can be powered at the onset of very energetic events like supernovae (collapsars) explosions or coalescences of binary neutron stars. Our approach uses the weak-scale hidden sector models in which the Higgs sector of the standard model is extended to include a gauge singlet that only interacts with the Higgs particle. These particles would be produced either during the implosion of the red supergiant star core or at the aftermath of a neutron star binary merger. The whole energetics and timescales of the relativistic blast wave, the fireball, are reproduced.
- Año
- 2000
- Número
- CBPF-NF-079/00
- Vínculo con tesis
- No
- Vínculo con beca
- No