Commit ab1642d3d920456597a888bd830409f26547b70c
1 parent
4448ea24
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master
Add usefull integrand in Constantes.py
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5 changed files
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34 additions
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23 deletions
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Angle_distribution.py
... | ... | @@ -33,8 +33,8 @@ def fit_theta(E,B): |
33 | 33 | delta=Dic0/(2*RL0)*((Esource/2)**2 *Eic/E-1) |
34 | 34 | return abs(arcsin(delta_to_theta*sin(delta))*degre) |
35 | 35 | |
36 | -#fig2 = plt.figure() | |
37 | -#ax2 = fig2.add_subplot(111) | |
36 | +fig2 = plt.figure() | |
37 | +ax2 = fig2.add_subplot(111) | |
38 | 38 | |
39 | 39 | fig1 = plt.figure() |
40 | 40 | gs = gridspec.GridSpec(2, 1, height_ratios=[4,1]) |
... | ... | @@ -59,7 +59,7 @@ for fileId in argv[2:]: |
59 | 59 | diry=diry/hyp |
60 | 60 | dirz=dirz/hyp |
61 | 61 | costheta=dirx*posx+diry*posy+dirz*posz |
62 | - cond=(costheta<=1)&(costheta>=-1)&(charge==0) | |
62 | + cond=(costheta<=1)&(costheta>=-1) | |
63 | 63 | theta = arccos(costheta[cond])*degre |
64 | 64 | weight= weight[cond] |
65 | 65 | energy= energy[cond] |
... | ... | @@ -80,26 +80,29 @@ for fileId in argv[2:]: |
80 | 80 | #ax11.plot(energy,theta,'.'+color[ind],label="$10^{-%.0f"%float(fileId)+"}$Gauss - MC") |
81 | 81 | B=10**(-float(fileId)) |
82 | 82 | yfit = fit_theta(enercenter,B) |
83 | - ax11.plot(enercenter,yfit,'--'+color[ind+1],linewidth=2,label="$10^{-%.0f"%float(fileId)+"}$Gauss - analytic") | |
83 | + ax11.plot(enercenter,yfit,'--'+color[ind],linewidth=2,label="$10^{-%.0f"%float(fileId)+"}$Gauss - analytic") | |
84 | 84 | elif argv[1] == "EBL": |
85 | 85 | ax11.plot(enercenter,angle,'.'+color[ind],label=Model[int(fileId)-1]) |
86 | 86 | if ind==0: |
87 | 87 | yfit = fit_theta(enercenter,B) |
88 | - ax11.plot(enercenter,yfit,'--'+color[ind+1],linewidth=2,label="$10^{-15}$Gauss - analytic") | |
88 | + ax11.plot(enercenter,yfit,'--'+color[ind],linewidth=2,label="$10^{-15}$Gauss - analytic") | |
89 | 89 | |
90 | 90 | error=angle/yfit-1 |
91 | 91 | ax12.plot(enercenter,error,'+'+color[ind]) |
92 | 92 | |
93 | 93 | # figure: radial distribution |
94 | 94 | #============================= |
95 | - #nbBins = 20 | |
96 | - #theta = log10(theta) | |
97 | - #nb,angle1=histogram(theta, nbBins, weights=weight) | |
95 | + nbBins = 20 | |
96 | + theta = theta[theta!=0] | |
97 | + weight=weight[theta!=0] | |
98 | + #theta = log10(theta**2) | |
99 | + nb,angle1=histogram(theta**2,nbBins, range=[0,1],weights=weight) | |
98 | 100 | #angle1=10**angle1 |
99 | - #anglecenter=(angle1[1:nbBins+1]+angle1[0:nbBins])/2 | |
100 | - #binSize=angle1[1:nbBins+1]-angle1[0:nbBins] | |
101 | - #ax2.plot(anglecenter,nb,'-'+color[ind],label="$10^{-%.0f"%float(fileId)+"}$Gauss - MC") | |
102 | - #ax2.hist(theta, nbBins, weights=weight,log=True, | |
101 | + anglecenter=(angle1[1:nbBins+1]+angle1[0:nbBins])/2 | |
102 | + binSize=angle1[1:nbBins+1]-angle1[0:nbBins] | |
103 | + ax2.plot(anglecenter,nb,'-'+color[ind], | |
104 | + label="$10^{-%.0f"%float(fileId)+"}$Gauss - MC") | |
105 | + #ax2.hist(theta, nbBins, range=[0,0.5], weights=weight,log=True, | |
103 | 106 | # facecolor=color[ind],alpha=.5,label="$10^{-%.0f"%float(fileId)+"}$Gauss") |
104 | 107 | |
105 | 108 | ind=ind+1 |
... | ... | @@ -119,11 +122,11 @@ plt.ylim(min(error)-step, max(error)+step) |
119 | 122 | xticklabels = ax11.get_xticklabels() |
120 | 123 | plt.setp(xticklabels, visible=False) |
121 | 124 | |
122 | -#ax2.legend(loc="best") | |
125 | +ax2.legend(loc="best") | |
123 | 126 | #ax2.set_xscale('log') |
124 | -#ax2.set_yscale('log') | |
125 | -#ax2.grid(b=True,which='major') | |
126 | -#ax2.set_xlabel("$\\theta$ [degre]") | |
127 | -#ax2.set_ylabel("Nb events * weight") | |
127 | +ax2.set_yscale('log') | |
128 | +ax2.grid(b=True,which='major') | |
129 | +ax2.set_xlabel("$\\theta^2$ [degre]") | |
130 | +ax2.set_ylabel("Nb events * weight") | |
128 | 131 | |
129 | 132 | plt.show() | ... | ... |
Constantes.py
... | ... | @@ -64,3 +64,14 @@ Ethreshold_ic = Eic*Dic/RL # GeV |
64 | 64 | # Pair production |
65 | 65 | Ethreshold_gg=(me)**2/Eebl *1e-3 #GeV |
66 | 66 | lambda_gg=0.8 # (E_gamma/1TeV)^-1 Gpc (from Durrer and Neronov 2013) |
67 | + | |
68 | +# usefull integrand | |
69 | +def comobileTime(z): | |
70 | + return -1/(H0*(1+z)*sqrt(omegaM*(1+z)**3+omegaK*(1+z)**2+omegaL)) | |
71 | + | |
72 | +def distPhoton(z): | |
73 | + return -c/(H0*a0*sqrt(omegaM*(1+z)**3+omegaK*(1+z)**2+omegaL)) | |
74 | + | |
75 | +def distLepton(z,E): | |
76 | + beta = sqrt(1-m**2*c**4/E**2) | |
77 | + return -beta*c/(H0*a0*sqrt(omegaM*(1+z)**3+omegaK*(1+z)**2+omegaL)) | ... | ... |
Constantes.pyc
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Energy_distribution.py
... | ... | @@ -24,7 +24,7 @@ else: |
24 | 24 | |
25 | 25 | # figure: energy distribution |
26 | 26 | #============================= |
27 | -nbBins = 70 | |
27 | +nbBins = 100 | |
28 | 28 | convert= 180/np.pi |
29 | 29 | color=['b','r','g','c','m','y'] |
30 | 30 | |
... | ... | @@ -70,7 +70,7 @@ for fileId in argv[2:]: |
70 | 70 | |
71 | 71 | def fit(x,a,b,c): |
72 | 72 | return a* x**b +c |
73 | -a=1 | |
73 | +a=1/2.5 | |
74 | 74 | b=0.5 |
75 | 75 | c=0 |
76 | 76 | ... | ... |
Time_distribution.py
... | ... | @@ -35,10 +35,7 @@ color=['b','r','g','c','m','y'] |
35 | 35 | fig = plt.figure() |
36 | 36 | ax = fig.add_subplot(111) |
37 | 37 | |
38 | -def properTime(z): | |
39 | - return -1/(H0*(1+z)*sqrt(omegaM*(1+z)**3+omegaK*(1+z)**2+omegaL)) | |
40 | - | |
41 | -tlim = quad(properTime,zSource,0)[0]/s_to_yr | |
38 | +tlim = quad(comobileTime,zSource,0)[0]/s_to_yr | |
42 | 39 | print tlim |
43 | 40 | |
44 | 41 | time= loadtxt(fileName+argv[2]+"/Results_position",unpack=True,usecols=[0]) | ... | ... |