ueb12e - time period to signicantly detect te source. How...

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Astroparticle physics, 2011 Problem 12 Problem 12: In class we discussed the evolution of an electron spectrum under the influence of synchrotron losses and escape, assuming the initial spectrum was a power law. The emission of sources is often so weak, that detectors need to integrate over a substantial
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Unformatted text preview: time period to signicantly detect te source. How would you calculate the time-integrated spectrum for the time interval T i ? Can you estimate asymptotic spectra a very small and very high energies?...
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