SciPy

darkhistory.history.tla.get_history

darkhistory.history.tla.get_history(rs_vec, init_cond=None, baseline_f=False, inj_particle=None, f_H_ion=None, f_H_exc=None, f_heating=None, DM_process=None, mDM=None, sigmav=None, lifetime=None, struct_boost=None, injection_rate=None, reion_switch=False, reion_rs=None, photoion_rate_func=None, photoheat_rate_func=None, xe_reion_func=None, helium_TLA=False, f_He_ion=None, mxstep=1000, rtol=0.0001)

Returns the ionization and thermal history of the IGM.

Parameters:
rs_vecndarray

Abscissa for the solution.

init_condarray, optional

Array containing [initial temperature, initial xHII, initial xHeII, initial xHeIII]. Defaults to standard values if None.

baseline_fbool

If True, uses the baseline f values with no backreaction returned by f_std(). Default is False.

inj_particle{‘elec’, ‘phot’}, optional

Specifies which set of f to use: electron/positron or photon.

f_H_ionfunction or float, optional

f(rs, x_HI, x_HeI, x_HeII) for hydrogen ionization. Treated as constant if float.

f_H_excfunction or float, optional

f(rs, x_HI, x_HeI, x_HeII) for hydrogen Lyman-alpha excitation. Treated as constant if float.

f_heatingfunction or float, optional

f(rs, x_HI, x_HeI, x_HeII) for heating. Treated as constant if float.

DM_process{‘swave’, ‘decay’}, optional

Dark matter process to use. Default is None.

sigmavfloat, optional

Thermally averaged cross section for DM_process == 'swave'. Default is None.

lifetimefloat, optional

Decay lifetime for DM_process == 'decay'. Default is None.

struct_boostfunction, optional

Energy injection boost factor due to structure formation. Default is None.

injection_ratefunction or float, optional

Injection rate of DM as a function of redshift. Treated as constant if float. Default is None.

reion_switchbool

Reionization model included if True.

reion_rsfloat, optional

Redshift 1+z at which reionization effects turn on.

photoion_rate_functuple of functions, optional

Functions take redshift 1+z as input, return the photoionization rate in s^-1 of HI, HeI and HeII respectively. If not specified, defaults to darkhistory.history.reionization.photoion_rate.

photoheat_rate_functuple of functions, optional

Functions take redshift 1+z as input, return the photoheating rate in s^-1 of HI, HeI and HeII respectively. If not specified, defaults to darkhistory.history.reionization.photoheat_rate.

xe_reion_funcfunction, optional

Specifies a fixed ionization history after reion_rs.

helium_TLAbool, optional

Specifies whether to track helium before reionization.

f_He_ionfunction or float, optional

f(rs, x_HI, x_HeI, x_HeII) for helium ionization. Treated as constant if float. If None, treated as zero.

mxstepint, optional

The maximum number of steps allowed for each integration point. See scipy.integrate.odeint for more information.

rtolfloat, optional

The relative error of the solution. See scipy.integrate.odeint for more information.

Returns:
list of ndarray

[temperature solution (in eV), xHII solution, xHeII, xHeIII].

Notes

The actual differential equation that we solve is expressed in terms of y = arctanh(f*(x - f)), where f = 0.5 for x = xHII, and f = nHe/nH * 0.5 for x = xHeII or xHeIII, where nHe/nH is approximately 0.083.

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