Search for a Scalar Induced Stochastic Gravitational Wave Background in the Third LIGO-Virgo Observing Run

被引：34

作者：

Romero-Rodriguez, Alba ^{[1
]}

Martinez, Mario ^{[1
,2
]}

Pujolas, Oriol ^{[1
]}

Sakellariadou, Mairi ^{[3
]}

Vaskonen, Ville ^{[1
]}

机构：

[1] Barcelona Inst Sci & Technol, Inst Fis Altes Energies IFAE, E-08193 Barcelona, Spain

[2] Catalan Inst Res & Adv Studies ICREA, E-08010 Barcelona, Spain

[3] Univ London, Kings Coll London, Phys Dept, Theoret Particle Phys & Cosmol Grp, London WC2R 2LS, England

来源：

PHYSICAL REVIEW LETTERS | 2022年 / 128卷 / 05期

基金：

美国国家科学基金会;

关键词：

PRIMORDIAL BLACK-HOLES; COLLAPSE; COALESCENCES;

D O I：

10.1103/PhysRevLett.128.051301

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The formation of primordial black holes from inflationary fluctuations is accompanied by a scalar induced gravitational wave background. We perform a Bayesian search of such background in the data from Advanced LIGO and Virgo's first, second, and third observing runs, parametrizing the peak in the curvature power spectrum by a log-normal distribution. The search shows no evidence for such a background. We place 95% confidence level upper limits on the integrated power of the curvature power spectrum peak which, for a narrow width, reaches down to 0.02 at 10(17) Mpc(-1). The resulting constraints are stronger than those arising from big bang nucleosynthesis or cosmic microwave background observations. In addition, we find that the constraints from LIGO and Virgo, at their design sensitivity, and from the Einstein Telescope can compete with those related to the abundance of the formed primordial black holes.

引用

页数：7

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