arXiv:1904.02129 Solvay Workshop, 4th April 2019
Juan García-Bellido IFT-UAM/CSIC Madrid
A common origin of Baryons and Dark Matter via gravitational - - PowerPoint PPT Presentation
A common origin of Baryons and Dark Matter via gravitational collapse of Primordial Black Holes arXiv:1904.02129 Solvay Workshop, 4 th April 2019 Juan Garca-Bellido IFT-UAM/CSIC Madrid Outline Introduction - LIGO Gravitational Waves
arXiv:1904.02129 Solvay Workshop, 4th April 2019
Juan García-Bellido IFT-UAM/CSIC Madrid
Hot Spot EW baryogenesis at QCD
LVC (2018)
If LIGO detects a single BH with M < 1Msun it will necessarily be
Given the present rate O1-O2 R ~ 20-120 events/yr/Gpc3 soon O3 will have MANY events. Will test lognormal distribution. Observed rate of events is OK with clustered wide-mass distr. Chirp mass
Clesse & JGB (2016-18)
Effective aligned spin Effective precession spin
GW170817 GW170608 GW151226 GW151012 GW170104 GW170814 GW170809 GW170818 GW150914 GW170823 GW170729
0.00 0.25 0.50 0.75 1.00 χp
G W 1 7 8 1 7 G W 1 7 6 8 G W 1 5 1 2 2 6 G W 1 5 1 1 2 G W 1 7 1 4 G W 1 7 8 1 4 G W 1 7 8 9 G W 1 7 8 1 8 G W 1 5 9 1 4 G W 1 7 8 2 3 G W 1 7 7 2 9
−1.0 −0.5 0.0 0.5 1.0 χeff
LVC (2018) LVC (2018)
N=ln a/aend N=0
1/(aH) a0 rec eq BBN QCD PBH 1/(aH) Inflation Radiation Matter Horizon crossing
1/k comoving scale EW
LIGO range!
Byrnes et al. (2018) Jedamzik (1997)
Out-of-equilibrium gravitational collapse
Asaka et al. (2004)
0 two-fold 1 two-fold 2 two-folds 3 two-folds 4 two-folds 5 two-folds 6 two-folds 7 two-folds 8 two-folds 9 two-folds
Evolution of the stochastic spectator field (eg. QCD axion) in our patch:
T=150 MeV T=125 MeV T=100 MeV
1¥1018 2¥1018 0.0000 0.00002 0.00004 0.00006 0.00008 0.0001 a @GeVD VHaL @GeV4 D
a(x) hai
hai ' aend
slow-roll region
These regions will collapse and form PBH with different masses Coarse-grained multiverse
hai ' aend
no Dark Matter Universe Universe with 2 inflation phases
0.01 0.10 1 10 100 10-5 10-4 0.001 0.010 0.100 1 MPBH (MΘ) fPBH
20 MeV 120 MeV 1 GeV
Axion dominance PBH=DM collapse 200 MeV quark-hadron transition Baryogenesis hot-spot EWB 100 MeV baryon diffusion light elements 10 MeV 1 MeV Nucleosynthesis
Hubble domains that collapse to form PBH.
collapse of PBH and BAU via “Hot spot” EWB.
could be measured by LIGO/Virgo in the near future.