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- W3104768158 abstract "We performed accurate numerical calculations of angle-, time-, and frequency-dependent radiative transfer for the relativistic motion of matter in gamma-ray burst (GRB) models. Our technique for solving the transfer equation, which is based on the method of characteristics, can be applied to the motion of matter with a Lorentz factor up to 1000. The effect of synchrotron self-absorption is taken into account. We computed the spectra and light curves from electrons with a power-law energy distribution in an expanding relativistic shock and compare them with available analytic estimates. The behavior of the optical afterglows from GRB 990510 and GRB 000301c is discussed qualitatively." @default.
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- W3104768158 date "2003-06-01" @default.
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- W3104768158 title "Spectra and light curves of GRB afterglows" @default.
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- W3104768158 doi "https://doi.org/10.1134/1.1579780" @default.
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