Testing primordial black holes as dark matter in supergravity from gravitational waves; Physics Letters B; Vol. 814

Testing primordial black holes as dark matter in supergravity from gravitational waves; Physics Letters B; Vol. 814

Dades bibliogràfiques
Parent link:	Physics Letters B Vol. 814.— 2021.— [136069, 5 p.]
Autor principal:	Aldabergenov E. Ermek
Autor corporatiu:	Национальный исследовательский Томский политехнический университет Исследовательская школа физики высокоэнергетических процессов
Altres autors:	Addazi A. Andrea, Ketov S. V. Sergey Vladimirovich
Sumari:	Title screen We 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.
Idioma:	anglès
Publicat:	2021
Matèries:	электронный ресурс труды учёных ТПУ черные дыры темная материя супергравитация
Accés en línia:	http://earchive.tpu.ru/handle/11683/132663 https://doi.org/10.1016/j.physletb.2021.136069
Format:	Electrònic Capítol de llibre
KOHA link:	https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=664586

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