The GRB Rate At High Photon Energies
|
Descargar SCORM
¡Sea el primero en solicitar este recurso!
Para poder solicitar este recurso debe identificarse como usuario de la biblioteca
|
| |
Ver
Detalles del recurso
|
|
|
The GRB Rate At High Photon Energies
|
| Id. |
41559304 |
| Idioma |
inglés
|
| Titulo |
The GRB Rate At High Photon Energies |
| Autor(es) |
Burkhardt Funk,Karl Mannheim
|
| Localización |
http://citeseer.ist.psu.edu/125207.html
|
| Versión |
1.0 |
| Estado |
Final
|
| Descripción |
INTRODUCTION
The lack of a significant large scale anisotropy in the angular distribution
of GRBs argues in favor of their cosmological origin. Assuming they are all
standard candles, the observed number of bursts at a given flux directly relates
to a number of sources at a given redshift. The maximum redshift sampled
by BATSE under these assumptions is z max ¸ 2 (1). As a direct consequence
absorption of the high energy gamma rays by diffuse background radiation
becomes important at photon energies ?30 GeV.
In this work we calculate the expected burst rate as a function of photon
energy accounting for cosmic absorption and compare the result with experimental
limits. We will start with the computation of the gamma ray horizon
which in a second step will be used to determine the number of bursts at
a given detection threshold. Finally, we determine the experimental sensitivity
required for the detection of all GRBs within the gam
|
| Tipo |
ps
|
| Palabras clave |
Burkhardt Funk,Karl Mannheim The GRB Rate At High Photon Energies
|
| Tipo de Interactividad |
Expositivo
|
| Nivel de Interactividad |
muy bajo
|
| Audiencia |
Estudiante
Profesor
Autor
|
| Estructura |
Atomic |
| Coste |
no
|
| Copyright |
sí
|
|
unrestricted |
| Formatos |
ps
|
| Requerimientos técnicos |
Browser: Any
|
| Relación |
[IsBasedOn] http://wpos6.physik.uni-wuppertal.de:8080/postscript/hsv95.w2.grb.ps
|
| Fecha de contribución |
31-mar-2009 |
| Contacto |
|
|
|
|
|
Valoración de los usuarios
No hay ninguna valoración para este recurso. Sea el primero en
valorar este recurso.
|
|
|
|
