All Tables

Table 1: Input parameters and results for all simulation runs. Input parameters are: electron initial Lorentz factor $\gamma _0$ , number density in the beam n in terms of Goldreich-Julian density at the pulsar surface $n_{{\rm GJ}\ast }$ , dimensionless wiggler strength K, wiggler wavelength $\lambda _{{\rm w}}$ , dimensionless wiggler phase speed $\beta _{{\rm w}}$ and (uniform) background magnetic field B₀. Results from the numerical simulations are: central frequency $\nu _{{\rm cen}}$ , FWHM bandwidth of the radiation $\Delta \nu$ , peak power of the light pulse $P_{{\rm max}}$ , and brightness temperature corresponding to the peak power $T_{{\rm b}}$ . The last four entries are the energy density of each ingredient in the simulation: beam $\epsilon _{{\rm b}}$ , wiggler $\epsilon _{{\rm w}}$ , background magnetic field $\epsilon _{{\rm b0}}$ and pulse $\epsilon _{{\rm p}}$ . Note that every time "-'' appears, it means the entry has the value as in run 1. In run 5, n appears for $\nu _{{\rm res}}$ , $\Delta \nu$ and $T_{{\rm b}}$ , which means, that for those cases, the spectra are flat, no peaks are seen, and also the brightness temperatures which depend on the bandwidths are not calculated.
Table A.1: The range of opening angles $\phi$ for different z₀ and wavelengths between 3 cm and 30 m according to Eq. (A.20).