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100 _a20210428a2020 k y0engy50 ba
101 0 _aeng
135 _adrcn ---uucaa
181 0 _ai
182 0 _ab
200 1 _aPrimordial black holes from modified supergravity
_fE. Aldabergenov, A. Addazi, S. V. Ketov
203 _aText
_celectronic
300 _aTitle screen
320 _a[References: 68 tit.]
330 _aThe modified supergravity approach is applied to describe a formation of Primordial Black Holes (PBHs) after Starobinsky inflation. Our approach naturally leads to the two-(scalar)-field attractor-type double inflation, whose first stage is driven by scalaron and whose second stage is driven by another scalar field which belongs to a supergravity multiplet. The scalar potential and the kinetic terms are derived, the vacua are studied, and the inflationary dynamics of those two scalars is investigated. We numerically compute the power spectra and we find the ultra-slow-roll regime leading to an enhancement (peak) in the scalar power spectrum. This leads to an efficient formation of PBHs. We estimate the masses of PBHs and we find their density fraction (as part of Dark Matter). We show that our modified supergravity models are in agreement with inflationary observables, while they predict the PBH masses in a range between 1016 g and 1020 g. In this sense, modified supergravity provides a natural top-down approach for explaining and unifying the origin of inflation and the PBHs Dark Matter.
461 _tThe European Physical Journal C
463 _tVol. 80, iss. 10
_v[917, 20 p.]
_d2020
610 1 _aэлектронный ресурс
610 1 _aтруды учёных ТПУ
610 1 _aсупергравитация
610 1 _aтемная материя
610 1 _aчерные дыры
700 1 _aAldabergenov
_bE.
_gErmek
701 1 _aAddazi
_bA.
_gAndrea
701 1 _aKetov
_bS. V.
_cphysicist
_cProfessor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences
_f1960-
_gSergey Vladimirovich
_2stltpush
_3(RuTPU)RU\TPU\pers\36631
712 0 2 _aНациональный исследовательский Томский политехнический университет
_bИсследовательская школа физики высокоэнергетических процессов
_c(2017- )
_h8118
_2stltpush
_3(RuTPU)RU\TPU\col\23551
801 2 _aRU
_b63413507
_c20210428
_gRCR
856 4 _uhttps://doi.org/10.1140/epjc/s10052-020-08506-6
942 _cCF