2 import matplotlib.pyplot
as plt
3 import py_cosmo_mad
as csm
16 pcs.background_set(cpar[
'om'],cpar[
'ol'],cpar[
'ob'],cpar[
'w0'],cpar[
'wa'],cpar[
'hh'],TCMB)
17 pcs.set_linear_pk(
'BBKS',-3,LKMAX,0.01,cpar[
'ns'],cpar[
's8'])
19 r_arr=np.array([pcs.M2R(m)
for m
in m_arr])
20 sm_arr=np.sqrt(np.array([pcs.sig0_L(r,r,
'TopHat',
'TopHat')
for r
in r_arr]))
23 plt.plot(m_arr,sm_arr)
24 plt.xlabel(
'$M\\,[M_{\\odot}\\,h^{-1}]$',fontsize=FS)
25 plt.ylabel(
'$\\sigma(M)$',fontsize=FS)
26 plt.gca().set_xscale(
'log');
27 plt.gca().set_yscale(
'log');
31 np.savetxt(prefix+
"_sm.txt",np.transpose([m_arr,sm_arr]),header=
"[1] M (M_sun/h), [2] sigma(M)")
33 z_arr=np.array([0.,1.,2.,3.,4.,5.])
34 lm_arr=6.+2*np.arange(6)
37 cpar_model1={
'om': 0.3,
'ol': 0.7,
'ob':0.05,
'hh': 0.7,
's8': 0.8,
'ns': 0.96,
'w0': -1.0,
'wa': 0.0}
38 cpar_model2={
'om': 0.3,
'ol': 0.7,
'ob':0.05,
'hh': 0.7,
's8': 0.8,
'ns': 0.96,
'w0': -0.9,
'wa': 0.0}
39 cpar_model3={
'om': 0.3,
'ol': 0.7,
'ob':0.05,
'hh': 0.7,
's8': 0.8,
'ns': 0.96,
'w0': -0.9,
'wa': 0.1}
41 do_all(m_arr,cpar_model1,
"model1")
42 do_all(m_arr,cpar_model2,
"model2")
43 do_all(m_arr,cpar_model3,
"model3")
def do_all(m_arr, cpar, prefix)