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Primordial Black Holes and Cosmological Phase Transitions Report ...

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PBHs <strong>and</strong> <strong>Cosmological</strong> <strong>Phase</strong> <strong>Transitions</strong> viii<br />

29 The sound speed for the QCD phase transition according to the<br />

Bag Model. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 81<br />

30 The sound speed for the QCD phase transition according to the<br />

Lattice Fit. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82<br />

31 The sound speed for the QCD phase transition in the case of a<br />

Crossover. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 82<br />

32 The width of the QCD Crossover in terms of temperature as a<br />

function of the parameter ∆T . . . . . . . . . . . . . . . . . . . . 84<br />

33 The width of the QCD Crossover in terms of time as a function<br />

of the parameter ∆T . . . . . . . . . . . . . . . . . . . . . . . . . 85<br />

34 <strong>Phase</strong> diagram for the EW phase transition. . . . . . . . . . . . . 87<br />

35 The EW <strong>and</strong> QCD phase diagrams in terms of temperature <strong>and</strong><br />

the relevant chemical potentials. . . . . . . . . . . . . . . . . . . 88<br />

36 Evolution of the Higgs scalar potential V for different values of<br />

temperature. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 91<br />

37 The sound speed for the EW Crossover as a function of temperature. 94<br />

38 The minimum value attained by the sound speed as a function of<br />

the parameter ∆T (EW Crossover <strong>and</strong> QCD Crossover). . . . . . 95<br />

39 The sound speed for the EW Crossover as a function of time. . . 95<br />

40 The EoS with in the case of an EW first–order phase transition<br />

<strong>and</strong> with two metastable branches. . . . . . . . . . . . . . . . . . 97<br />

41 The sound speed for the EW phase transition according to the<br />

Bag Model. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99<br />

42 The sound speed during the electron–positron annihilation as a<br />

function of temperature. . . . . . . . . . . . . . . . . . . . . . . . 104<br />

43 The sound speed during the electron–positron annihilation as a<br />

function of time. . . . . . . . . . . . . . . . . . . . . . . . . . . . 104<br />

44 The function x(t) for the QCD Bag Model. . . . . . . . . . . . . 112<br />

45 Regions in the (δ, log 10 x) plane corresponding to different classes<br />

of perturbations for the QCD Bag Model. . . . . . . . . . . . . . 115<br />

46 Regions in the (δ, log 10 x) plane corresponding to different classes<br />

of perturbations for the QCD Lattice Fit. . . . . . . . . . . . . . 116<br />

47 The function x(t) for the EW Bag Model. . . . . . . . . . . . . . 118<br />

48 Formation of a PBH from a fluctuation for which δk =0.535. . . 123<br />

49 A zoom into the upper left region of Figure 48. . . . . . . . . . . 123<br />

50 PBH formation during the QCD transition according to the Bag<br />

Model for the case x = 2 <strong>and</strong> δc =1/3. . . . . . . . . . . . . . . . 125<br />

51 PBH formation during the QCD transition according to the Bag<br />

Model for the cases x = 15, x = 30, <strong>and</strong> x = 90 when δc =1/3. . 127<br />

52 The curve in the (x, δ) plane indicating which values lead to collapse<br />

to a BH, according to the QCD Bag Model, when x>1<br />

<strong>and</strong> δc =1/3. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 129<br />

53 PBH formation during the QCD transition, according to the Bag<br />

Model, for the cases x = 2, x = 15, <strong>and</strong> x = 30 when δc assumes<br />

different values. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 130

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