gnei, vgnei: collisional plasma, non-equilibrium, temperature evolution
Non-equilibrium ionization collisional plasma model. This is a generalization of the nei model where the temperature is allowed to have been different in the past i.e. the ionization timescale averaged temperature is not necessarily equal to the current temperature. For example, in a standard Sedov model with equal electron and ion temperatures, the ionization timescale averaged temperature is always higher than the current temperature for each fluid element. The references for this model can be found under the description of the equil model. Several versions are available. To switch between them use the xset neivers command. xset neivers 1.0 gives the version from xspec v11.1, xset neivers 1.1 uses updated calculations of ionization fractions using dielectronic recombination rates from Mazzotta et al (1988), and xset neivers 2.0 uses the same ionization fractions as 1.1 but uses APED to calculate the resulting spectrum. Note that versions 1.x have no emission from Ar. The default is version 1.1.
The vgnei variant allows the user to set the abundances of the model.
For the gnei model the parameters are:
par1 |
plasma temperature (keV) |
par2 |
Metal abundances (He fixed at cosmic). The elements included are C, N, O, Ne, Mg, Si, S, Ar, Ca, Fe, Ni. Abundances are given by the Anders & Grevesse mixture |
par3 |
Ionization timescale in units of s cm–3. |
par4 |
Ionization timescale averaged plasma temperature (keV) |
par5 |
(fixed) redshift |
norm |
where DA is the angular size distance to the source (cm), ne and nH (cm-3) are the electron and hydrogen densities respectively. |
For vgnei the parameters are:
par1 |
plasma temperature (keV) |
par2-par13 |
(Fixed) Abundances for He, C, N, O, Ne, Mg, Si, S, Ar, Ca, Fe, Ni wrt Solar (given by the Anders & Grevesse mixture) |
par14 |
Ionization timescale in units of s cm–3. |
par15 |
Ionization timescale averaged plasma temperature (keV) |
par16 |
(fixed) redshift |
norm |
where DA is the angular size distance to the source (cm), and ne , nH (cm-3) are the electron and hydrogen densities respectively. |