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On the origin of primordial black holes

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1 On the origin of primordial black holes
Zong-Kuan Guo 引力与宇宙学研讨会(大同)

2 Inflation CMB 1st WAMP Planck 2013 SNe GWs 1982 1998 2003 2013 2016

3 1. Motivations  a candidate for cold dark matter [ ]  to provide seeds for supermassive BHs [ , ]  to provide seeds for cosmic structures [ ]  to account for LIGO events [astro-ph/ , ] 2. Constraints on the PBH abundance [ ] 3. Discriminating PBHs from astrophysical BHs [ , ] 4. The origin of primordial balk holes 1) from early universe phase transition  Q-balls [ ]  vacuum bubbles [hep-ph/ , , ] 2) from preheating after inflation  preheating [hep-ph/ ]  tachyonic preheating [hep-ph/ ]  oscillons [ ] 3) from large perturbations on small scales produced during inflation

4 from large perturbations on small scales produced during inflation
 multiple-field inflation [astro-ph/ , ]  single-field inflation with an inflection point [ , ] critical Higgs inflation [ , , ] axion inflation [ , ] supergravity [ ]  a scalar field non-minimally coupled to gravity [ , ]  the growth of perturbations on super-Hubble scales [ ]  particle production during inflation [ , ]  a contracting universe [ ]  quantum diffusion during inflation [ , , ]

5 Credit: arXiv: microlensing of stars femtolensing of γ-ray burst effects on CMB extragalactic γ-rays

6 1/(𝑎𝐻) 1/𝑘 ln 𝑎 ∗ ln 𝑎 𝑒 ln 𝑎 eq 𝑀=𝛾 4𝜋 3 𝜌 𝐻 −3 =𝛾4𝜋 𝑀 pl 2 𝐻 −1
𝛽 𝑀 = 𝛿 𝑐 ∞ 𝑑𝛿 2𝜋 𝜎 𝑒 − 𝛿 2 2 𝜎 2 1/𝑘 𝛽 𝑀, 𝑡 eq = 𝑎( 𝑡 eq ) 𝑎( 𝑡 PBH ) 𝛽 𝑀 Ω PBH ( 𝑡 eq )= 𝑑 ln 𝑀 𝛽(𝑀, 𝑡 eq ) ln 𝑎 ∗ ln 𝑎 𝑒 ln 𝑎 eq the threshold 𝛿 𝑐 =1/3 ? the efficiency factor 𝛾~𝒪(1) ? 𝑓 PBH (𝑀)≡ Ω PBH (𝑀) Ω CDM

7 new physics? 𝑘 PBH

8 𝑉(𝜙) 𝜙 𝜙 PBH 𝜙 ∗ 𝑢 𝑘 ′′ + 𝑘 2 − 𝑧 ′′ 𝑧 𝑢 𝑘 =0 50< 𝑁 ∗ <60
𝑢 𝑘 ′′ + 𝑘 2 − 𝑧 ′′ 𝑧 𝑢 𝑘 =0 𝑉(𝜙) 50< 𝑁 ∗ <60 𝒫 ℛ = 1 12 𝜋 2 𝑀 pl 6 𝑉 3 𝑉 𝜙 2 𝑁 𝜙 = 1 𝑀 pl 2 𝜙 𝑒 𝜙 𝑉 𝑉 𝜙 𝑑𝜙 𝜙 𝜙 PBH 𝜙 ∗ 𝐴 𝑠 =(2.10±0.03)× 10 −9 𝑛 𝑠 =0.9649±0.0044 𝛼=−0.0065±0.0066 𝑟<0.07

9 𝑉(𝜙) 𝜙 𝜙 PBH 𝜙 ∗ T.J. Gao, ZKG, arXiv:1806.09320
𝑉= 𝑒 𝐾 [ 𝐷 𝑖 𝑊 𝐾 −1 𝑖 𝑗 (𝐷 𝑗 𝑊) ∗ −3 |𝑊| 2 ] 𝐷 𝑖 𝑊= 𝜕 𝑖 𝑊+ 𝜕 𝑖 𝐾 𝑊 𝐾 𝑖 𝑗 = 𝜕 2 𝐾 𝜕 Φ 𝑖 𝜕 Φ 𝑗 𝜙 𝜙 PBH 𝜙 ∗ 𝐾=𝑖𝑐 Φ− Φ − Φ− Φ 2 − 𝜁 4 (Φ− Φ ) 4 𝑊= 𝑎 0 (1+ 𝑎 1 𝑒 − 𝑏 1 Φ + 𝑎 2 𝑒 − 𝑏 2 Φ + 𝑎 3 𝑒 − 𝑏 3 Φ )

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12 Thanks for your attention!

13 不忘初心,继续前行


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