Changeset 6270
- Timestamp:
- 02/04/05 19:58:37 (20 years ago)
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trunk/MagicSoft/GRB-Proposal/Timing.tex
r6267 r6270 20 20 \item Regarding the fireball model~\cite{REES1,REES2}, 21 21 two efficient mechanisms are available for the generation of VHE photons~\cite{DERISHEV}. 22 (1) The prompt emission of $\sim$100\,GeV photons is expected before and during the keV-MeV peak. 22 23 \begin{enumerate} 24 \item The prompt emission of $\sim$100\,GeV photons is expected before and during the keV-MeV peak. 23 25 This emission should have their highest luminosity together with the main GRB peak. 24 (2)VHE photons generated due to inverse Compton (IC) scattering in relativistic shocks26 \item VHE photons generated due to inverse Compton (IC) scattering in relativistic shocks 25 27 are strongly absorbed by infrared background radiation and 26 28 cannot be observed from cosmological distances. 29 \end{enumerate} 30 27 31 With the presence of a dense ambient medium close to the GRB, 28 32 the UHE photons will be reprocessed into a softer spectral range. … … 99 103 %%% mode: latex 100 104 %%% TeX-master: "GRB_proposal_2005" 105 %%% TeX-master: "Timing" 101 106 %%% End:
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