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101 0 _aeng
135 _aarnn ---uucaa
181 0 _ai
182 0 _ab
200 1 _aTesting primordial black holes as dark matter in supergravity from gravitational waves
_fE. Aldabergenov, A. Addazi, S. V. Ketov
203 _aText
_celectronic
300 _aTitle screen
320 _a[References.: 27 tit.]
330 _aWe explore the Gravitational Waves (GW) phenomenology of a simple class of supergravity models that can explain and unify inflation and Primordial Black Holes (PBH) as Dark Matter (DM). Our (modified) supergravity models naturally lead to a two-field attractor-type double inflation, whose first stage is driven by Starobinsky scalaron and the second stage is driven by another scalar belonging to a supergravity multiplet. The PBHs formation in our supergravity models is efficient, compatible with all observational constraints, and predicts a stochastic GW background. We compute the PBH-induced GW power spectrum and show that GW signals can be detected within the sensitivity curves of the future space-based GW interferometers such as LISA, DECIGO, TAIJI and TianQin projects, thus showing predictive power of supergravity in GW physics and their compatibility.
461 _tPhysics Letters B
463 _tVol. 814
_v[136069, 5 p.]
_d2021
610 1 _aэлектронный ресурс
610 1 _aтруды учёных ТПУ
610 1 _aчерные дыры
610 1 _aтемная материя
610 1 _aсупергравитация
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/10.1016/j.physletb.2021.136069
942 _cCF