Changeset 6270


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Timestamp:
02/04/05 19:58:37 (20 years ago)
Author:
gaug
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*** empty log message ***
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1 edited

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  • trunk/MagicSoft/GRB-Proposal/Timing.tex

    r6267 r6270  
    2020\item Regarding the fireball model~\cite{REES1,REES2},
    2121two 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.
    2325This 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 shocks
     26\item VHE photons generated due to inverse Compton (IC) scattering in relativistic shocks
    2527are strongly absorbed by infrared background radiation and
    2628cannot be observed from cosmological distances.
     29\end{enumerate}
     30
    2731With the presence of a dense ambient medium close to the GRB,
    2832the UHE photons will be reprocessed into a softer spectral range.
     
    99103%%% mode: latex
    100104%%% TeX-master: "GRB_proposal_2005"
     105%%% TeX-master: "Timing"
    101106%%% End:
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