Primordial Gravitational Waves are the next target of modern cosmology. They represent a window on the early Universe and the only probe of the physics and microphysics of the inflationary period. When the production of GWs happens in scenarios richer than the standard single-field slow-roll, the GW signal becomes potentially detectable also on scales smaller than the Cosmic Microwave Background. LISA will be extremely complementary to CMB experiments to extract information about primordial inflationary models and in particular to probe phases of the inflationary period for which we have very poor knowledges.acceptedVersio
The idea that primordial black holes (PBHs) can comprise most of the dark matter of the Universe has...
Abstract: A toy-model is studied, which considers two flat directions meeting at an enhanced symmetr...
International audienceIn this contribution we discuss the possibility of generating an observable gr...
Any inflationary model predicts the production of a stochastic gravitational-wave background. Such a ...
Forthcoming advances in direct gravitational wave detection from kilohertz to nanohertz frequencies ...
The idea that primordial black holes (PBHs) can comprise most of the dark matter of the Universe has...
The stochastic gravitational wave background (SGWB) offers a new opportunity to observe signals of p...
The stochastic gravitational wave background (SGWB) offers a new opportunity to observe signals of p...
The stochastic gravitational wave background (SGWB) offers a new opportunity to observe signals of p...
There has recently been renewed interest in the possibility that the dark matter in the Universe con...
A primordial spectrum of gravitational waves serves as a backlight to the relativistic degrees of fr...
There has recently been renewed interest in the possibility that the dark matter in the Universe con...
A primordial spectrum of gravitational waves serves as a backlight to the relativistic degrees of fr...
A primordial spectrum of gravitational waves serves as a backlight to the relativistic degrees of fr...
Abstract: A toy-model is studied, which considers two flat directions meeting at an enhanced symmetr...
The idea that primordial black holes (PBHs) can comprise most of the dark matter of the Universe has...
Abstract: A toy-model is studied, which considers two flat directions meeting at an enhanced symmetr...
International audienceIn this contribution we discuss the possibility of generating an observable gr...
Any inflationary model predicts the production of a stochastic gravitational-wave background. Such a ...
Forthcoming advances in direct gravitational wave detection from kilohertz to nanohertz frequencies ...
The idea that primordial black holes (PBHs) can comprise most of the dark matter of the Universe has...
The stochastic gravitational wave background (SGWB) offers a new opportunity to observe signals of p...
The stochastic gravitational wave background (SGWB) offers a new opportunity to observe signals of p...
The stochastic gravitational wave background (SGWB) offers a new opportunity to observe signals of p...
There has recently been renewed interest in the possibility that the dark matter in the Universe con...
A primordial spectrum of gravitational waves serves as a backlight to the relativistic degrees of fr...
There has recently been renewed interest in the possibility that the dark matter in the Universe con...
A primordial spectrum of gravitational waves serves as a backlight to the relativistic degrees of fr...
A primordial spectrum of gravitational waves serves as a backlight to the relativistic degrees of fr...
Abstract: A toy-model is studied, which considers two flat directions meeting at an enhanced symmetr...
The idea that primordial black holes (PBHs) can comprise most of the dark matter of the Universe has...
Abstract: A toy-model is studied, which considers two flat directions meeting at an enhanced symmetr...
International audienceIn this contribution we discuss the possibility of generating an observable gr...