International audienceThe nature of the most abundant components of the Universe, dark energy and dark matter, is still to be uncovered. I tackle this subject considering a novel cosmological probe: the neutral hydrogen emitted 21cm radiation, observed with the intensity mapping technique. I analyse competitive and realistic dark energy and dark matter models and show how they produce distinctive and detectable effects on the 21cm signal. Moreover, I provide radio telescope forecasts showing how these models will be distinguishable in an unprecedented way
Line-intensity mapping of the 21cm line is a powerful probe of large scale structure at z<6, tracing...
We investigate the effects of warm dark matter (WDM) on the cosmic 21-cm signal. If dark matter exis...
Imaging the Universe during the first hundreds of millions of years remains one of the exciting chal...
International audienceThe nature of the most abundant components of the Universe, dark energy and da...
The nature of the most abundant components of the Universe, dark energy and dark matter, is still to...
In this thesis we make progress toward establishing the observational method of 21 cm intensity mapp...
3D mapping of matter distribution in the universe through the 21 cm radio emission of atomic hydroge...
International audience21cm Intensity Mapping (IM) has been proposed about 15 years ago as a cost eff...
We investigate the impact that warm dark matter (WDM) has in terms of 21 cm intensity mapping in the...
This white paper envisions a revolutionary post-DESI, post-LSST dark energy program based on intensi...
This white paper envisions a revolutionary post-DESI, post-LSST dark energy program based on intensi...
We describe how the high-redshift 21-cm background can be used to improve both our understanding of ...
We are witnessing exciting times in the field of cosmology. Current and future experiments and surve...
We present a framework for forecasting cosmological constraints from future neutral hydrogen intensi...
We investigate the feasibility of measuring weak gravitational lensing using 21 cm intensity mapping...
Line-intensity mapping of the 21cm line is a powerful probe of large scale structure at z<6, tracing...
We investigate the effects of warm dark matter (WDM) on the cosmic 21-cm signal. If dark matter exis...
Imaging the Universe during the first hundreds of millions of years remains one of the exciting chal...
International audienceThe nature of the most abundant components of the Universe, dark energy and da...
The nature of the most abundant components of the Universe, dark energy and dark matter, is still to...
In this thesis we make progress toward establishing the observational method of 21 cm intensity mapp...
3D mapping of matter distribution in the universe through the 21 cm radio emission of atomic hydroge...
International audience21cm Intensity Mapping (IM) has been proposed about 15 years ago as a cost eff...
We investigate the impact that warm dark matter (WDM) has in terms of 21 cm intensity mapping in the...
This white paper envisions a revolutionary post-DESI, post-LSST dark energy program based on intensi...
This white paper envisions a revolutionary post-DESI, post-LSST dark energy program based on intensi...
We describe how the high-redshift 21-cm background can be used to improve both our understanding of ...
We are witnessing exciting times in the field of cosmology. Current and future experiments and surve...
We present a framework for forecasting cosmological constraints from future neutral hydrogen intensi...
We investigate the feasibility of measuring weak gravitational lensing using 21 cm intensity mapping...
Line-intensity mapping of the 21cm line is a powerful probe of large scale structure at z<6, tracing...
We investigate the effects of warm dark matter (WDM) on the cosmic 21-cm signal. If dark matter exis...
Imaging the Universe during the first hundreds of millions of years remains one of the exciting chal...