Feedback in the dark: a critical examination of CMB bounds on primordial black holes

被引:12
作者
Agius, Dominic [1 ]
Essig, Rouven [2 ]
Gaggero, Daniele [3 ]
Scarcella, Francesca [4 ,5 ]
Suczewski, Gregory [2 ]
Valli, Mauro [6 ]
机构
[1] Univ Valencia, CSIC, Inst Fis Corpuscular, C Catedrat Jose Beltran 2, E-46980 Paterna, Spain
[2] SUNY Stony Brook, CN Yang Inst Theoret Phys, 100 Nicolls Rd, Stony Brook, NY 11794 USA
[3] INFN, Sez Pisa, Largo B Pontecorvo 3, I-56127 Pisa, Italy
[4] Univ Montpellier, Lab Univers & Particules Montpellier LUPM, Pl Eugene Bataillon, Montpellier F-34095, France
[5] CNRS, Pl Eugene Bataillon, F-34095 Montpellier, France
[6] INFN, Sez Roma, Piazzale Aldo Moro 2, I-00185 Rome, Italy
关键词
accretion; cosmological parameters from CMBR; dark matter theory; primordial black holes; BONDI ACCRETION; MATTER;
D O I
10.1088/1475-7516/2024/07/003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
If present in the early universe, primordial black holes (PBHs) would have accreted matter and emitted high-energy photons, altering the statistical properties of the Cosmic Microwave Background (CMB). This mechanism has been used to constrain the fraction of dark matter that is in the form of PBHs to be much smaller than unity for PBH masses well above one solar mass. Moreover, the presence of dense dark matter mini -halos around the PBHs has been used to set even more stringent constraints, as these would boost the accretion rates. In this work, we critically revisit CMB constraints on PBHs taking into account the role of the local ionization of the gas around them. We discuss how the local increase in temperature around PBHs can prevent the dark matter mini -halos from strongly enhancing the accretion process, in some cases significantly weakening previously derived CMB constraints. We explore in detail the key ingredients of the CMB bound and derive a conservative limit on the cosmological abundance of massive PBHs.
引用
收藏
页码:1 / 36
页数:36
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