Non-Gaussian stochastic gravitational waves from phase transitions
Abstract Cosmological phase transitions in the primordial universe can produce anisotropic stochastic gravitational wave backgrounds (GWB), similar to the cosmic microwave background (CMB). For adiabatic perturbations, the fluctuations in GWB follow those in the CMB, but if primordial fluctuations c...
Главные авторы: | Soubhik Kumar, Raman Sundrum, Yuhsin Tsai |
---|---|
Формат: | Статья |
Язык: | English |
Опубликовано: |
SpringerOpen
2021-11-01
|
Серии: | Journal of High Energy Physics |
Предметы: | |
Online-ссылка: | https://doi.org/10.1007/JHEP11(2021)107 |
Схожие документы
-
Cosmological particle production and pairwise hotspots on the CMB
по: Jeong Han Kim, и др.
Опубликовано: (2021-11-01) -
Electroweak phase transition and gravitational waves in a two-component dark matter model
по: Ahmad Mohamadnejad
Опубликовано: (2022-03-01) -
Gravitational wave signatures from domain wall and strong first-order phase transitions in a two complex scalar extension of the Standard Model
по: Avik Paul, и др.
Опубликовано: (2021-05-01) -
Seeing higher-dimensional grand unification in primordial non-gaussianities
по: Soubhik Kumar, и др.
Опубликовано: (2019-04-01) -
Manifestly causal in-in perturbation theory about the interacting vacuum
по: Matthew Baumgart, и др.
Опубликовано: (2021-03-01)