Planck scale black hole dark matter from Higgs inflation

被引:70
作者
Rasanen, Syksy [1 ,2 ,3 ]
Tomberg, Eemeli [1 ,2 ]
机构
[1] Univ Helsinki, Dept Phys, POB 64, FIN-00014 Helsinki, Finland
[2] Univ Helsinki, Helsinki Inst Phys, POB 64, FIN-00014 Helsinki, Finland
[3] Birzeit Univ, Dept Phys, POB 14, Birzeit, West Bank, Palestine
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2019年 / 01期
关键词
dark matter theory; inflation; particle physics; cosmology connection; GR black holes; PALATINI VARIATIONAL PRINCIPLE; EXTENDED INFLATION; INITIAL CONDITIONS; PERTURBATIONS; RELICS; BOSON; CONSTRAINTS; EINSTEIN; GRAVITY; JORDAN;
D O I
10.1088/1475-7516/2019/01/038
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the production of primordial black hole (PBH) dark matter in the case when the Standard Model Higgs coupled non-minimally to gravity is the inflaton. PBHs can be produced if the Higgs potential has a near-critical point due to quantum corrections. In this case the slow-roll approximation may be broken, so we calculate the power spectrum numerically. We consider both the metric and the Palatini formulation of general relativity. Combining observational constraints on PBHs and on the CMB spectrum we find that PBHs can constitute all of the dark matter only if they evaporate early and leave behind Planck mass relics. This requires the potential to have a shallow local minimum, not just a critical point. The initial PBH mass is then below 10(6) g, and predictions for the CMB observables are the same as in tree-level Higgs inflation, n(s) = 0.96 and r = 5 x 10(-3) (metric) or r = 4 x 10(-8) ... 2 x 10(-7) (Palatini).
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页数:36
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