#+ # VIDE -- Void IDentification and Examination -- ./python_tools/vide/apTools/chi2/cosmologyTools.py # Copyright (C) 2010-2014 Guilhem Lavaux # Copyright (C) 2011-2014 P. M. Sutter # # This program is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; version 2 of the License. # # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License along # with this program; if not, write to the Free Software Foundation, Inc., # 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301 USA. #+ # a suite of functions to compute expansion rates, angular diameter # distances, and expected void stretching import numpy as np import scipy.integrate as integrate import os #from backend import * __all__=['expansion', 'comovingDistance', 'aveExpansion'] # returns 1/E(z) for the given cosmology def expansion(z, Om = 0.27, Ot = 1.0, w0 = -1.0, wa = 0.0): ez = Om * (1+z)**3 + (Ot-Om)# * (1+z)**(3.+3*wz) #ez = Om * (1+z)**3 + (Ot-Om)# * integrade.quad(eosDE, 0.0, z, args=(w0,wa))[0] ez = 1./np.sqrt(ez) return ez # returns DE value at redshift z def eosDE(z, w0 = -1.0, wa = 0.0): return w0 + wa*z/(1+z) # returns the comoving distance for the given cosmology def comovingDistance(z, Om = 0.27, Ot = 1.0, w0 = -1.0, wa = 0.0): da = integrate.quad(expansion, 0.0, z, args=(Om, Ot, w0, wa))[0] return da # ----------------------------------------------------------------------------- # returns average expected expansion for a given redshift range def aveExpansion(zStart, zEnd, Om = 0.27, Ot = 1.0, w0 = -1.0, wa = 0.0): if zStart == 0.0: zStart = 1.e-6 ave = integrate.quad(expansion, zStart, zEnd, args=(Om, Ot, w0, wa))[0] ave = (zEnd-zStart)/ave return ave