Primordial Black Holes and Cosmological Phase Transitions Report ...

More documents

Recommendations

Info

$Kawasaki dynamic in continuum Math. Encounters XXXV ... - CCM$

PBHs and Cosmological Phase Transitions 190 Table 46: The contribution to β from the QCD Crossover. In yellow we show the cases for which there is a non–negligible contribution to β from the QCD Crossover. For more details see Tables 41 and 42. nmax log10(t+/1s) 1.28 1.30 1.32 1.34 1.36 1.38 1.40 1.42 1.44 1.46 1.48 1.50 1.52 1.54 1.56 1.58 1.60 1.62 1.64 -11 R R R R -10 R R R -9 R R R -8 R R R R -7 R R R RC -6 R RC RC RC -5 RC RC RC RC Fig. 106d -4 RC RC RC RC RC RC Fig. 106a Fig. 104 -3 RC RC RC RC RC RC* Fig. 106e Fig. 105 -2 RC RC RC RC RCea RCea Fig. 106f -1 R R Rea RCea RCea RCea RCea 0 R Rea Rea Rea Rea Rea Rea Rea
PBHs and Cosmological Phase Transitions 191 log 10Βtk 0 -20 -40 -60 -80 n1.48, log 10t1s4 -8 -6 -4 -2 log10 tk 1 s Figure 104: The fraction of the universe going into PBHs in a universe with a running–tilt power spectrum when n+ =1.48 and t+ = 10 −4 s. The dark curve represents the radiation contribution and the maroon line the observational constraints. The other curves represent the contribution from the QCD phase transition: Crossover (green), Lattice Fit (magenta) and Bag Model (blue). The latter two models for the QCD transition are excluded, due to observational constraints. log 10Βtk 0 -2.5 -5 -7.5 -10 -12.5 -15 -17.5 n1.52, log 10t1s3 -7 -6 -5 -4 -3 -2 -1 0 log10 tk 1 s Figure 105: The fraction of the universe going into PBHs in a universe with a running–tilt power spectrum when n+ =1.52 and t+ = 10 −3 s (see Figure 104 for more details). Whatever the model adopted for the QCD transition this case must be excluded, due to observational constraints.
Page 1:
CCM-Centro de Ciências Matemática
Page 4 and 5:
Contents List of Figures vii List o
Page 6 and 7:
PBHs and Cosmological Phase Transit
Page 8 and 9:
Page 10 and 11:
Page 12 and 13:
List of Tables 1 The Universe timel
Page 14 and 15:
Page 16 and 17:
Page 19 and 20:
Page 21 and 22:
Page 23 and 24:
Page 25 and 26:
Page 27 and 28:
Page 29 and 30:
Page 31 and 32:
Page 33 and 34:
Page 35 and 36:
Page 37 and 38:
Page 39 and 40:
Page 41 and 42:
Page 43 and 44:
Page 45 and 46:
Page 47 and 48:
Page 49 and 50:
Page 51 and 52:
Page 53 and 54:
Page 55 and 56:
Page 57 and 58:
Page 59 and 60:
Page 61 and 62:
Page 63 and 64:
Page 65 and 66:
Page 67 and 68:
Page 69 and 70:
Page 71 and 72:
Page 73 and 74:
Page 75 and 76:
Page 77 and 78:
Page 79 and 80:
Page 81 and 82:
Page 83 and 84:
Page 85 and 86:
Page 87 and 88:
Page 89 and 90:
Page 91 and 92:
Page 93 and 94:
Page 95 and 96:
Page 97 and 98:
Page 99 and 100:
Page 101 and 102:
Page 103 and 104:
Page 105 and 106:
Page 107 and 108:
Page 109 and 110:
Page 111 and 112:
Page 113 and 114:
Page 115 and 116:
Page 117 and 118:
Page 119 and 120:
Page 121 and 122:
Page 123 and 124:
Page 125 and 126:
Page 127 and 128:
Page 129 and 130:
Page 131 and 132:
Page 133 and 134:
Page 135 and 136:
Page 137 and 138:
Page 139 and 140:
Page 141 and 142:
Page 143 and 144:
Page 145 and 146:
Page 147 and 148:
Page 149 and 150:
Page 151 and 152:
Page 153 and 154:
Page 155 and 156:
Page 157 and 158: PBHs and Cosmological Phase Transit
Page 207: PBHs and Cosmological Phase Transit
Page 221 and 222: Table 49 (continued). PBHs and Cosm
Page 223 and 224: Table 49 (continued). Radiation EW
show all

Primordial Black Holes and Cosmological Phase Transitions Report ...

Create successful ePaper yourself

Delete template?

Save as template?