03.07.2013 Views

Primordial Black Holes and Cosmological Phase Transitions Report ...

Primordial Black Holes and Cosmological Phase Transitions Report ...

Primordial Black Holes and Cosmological Phase Transitions Report ...

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

PBHs <strong>and</strong> <strong>Cosmological</strong> <strong>Phase</strong> <strong>Transitions</strong> 82<br />

cs 2<br />

0.3<br />

0.2<br />

0.1<br />

0<br />

t1<br />

t t<br />

-6 -5.5 -5 -4.5 -4 -3.5<br />

Log 10t1s<br />

Figure 30: The sound speed c 2 s(t) for the QCD phase transition according to the<br />

Lattice Fit with Tc = 170 MeV. During the coexistence phase, which occurs<br />

between the instants t− =9.37×10 −5 s <strong>and</strong> t+ =1.08×10 −4 s the sound speed<br />

drops to zero (dark gray zone). For t1 =5.1 × 10 −7 s the sound speed equals<br />

95% of its ‘background’ value. The dashed line represents the ideal gas case for<br />

which c 2 s =1/3.<br />

cs 2<br />

0.4<br />

0.3<br />

0.2<br />

0.1<br />

t<br />

t1<br />

t<br />

-4.4 -4.2 -4 -3.8 -3.6<br />

Log 10t1s<br />

Figure 31: The sound speed c 2 s (t) for the QCD phase transition in the case<br />

of a Crossover with a reference temperature Tc = 170 MeV <strong>and</strong> ∆T =0.1Tc.<br />

The dashed lines represent, for reference, the location of the first–order phase<br />

transition according to the Bag Model (t− =6.25 × 10 −5 s, t+ =1.08 × 10 −4 s).<br />

Between the instants t1 ≈ 7.1 × 10 −5 s <strong>and</strong> t2 ≈ 1.96 × 10 −4 s the sound speed<br />

stays below 95% of its ‘background’ value (c 2 s,0 =1/3).<br />

t2

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!