Add to ORKGWe present constraints on the mass of warm dark matter (WDM) particles derived from the Lyman-alpha flux power spectrum of 55 high-resolution HIRES spectra at 2.0~1.2 keV (2sigma) if the WDM consists of early decoupled thermal relics and mWDM>~5.6 keV (2sigma) for sterile neutrinos. Adding the Sloan Digital Sky Survey Lyman-alpha flux power spectrum, we get mWDM>~4 keV and mWDM>~28 keV (2sigma) for thermal relics and sterile neutrinos. These results improve previous constraints by a factor of 2
The observed Lyman-α flux power spectrum (FPS) is suppressed on scales below ∼ 30 km s−1. This cutof...
Warm dark matter (WDM) has been invoked to resolve apparent conflicts of cold dark matter (CDM) mode...
International audienceWe use the large BOSS DR9 sample of quasar spectra to constrain two cases of n...
We present constraints on the mass of warm dark matter (WDM) particles derived from the Lyman-alpha ...
We present constraints on the mass of warm dark matter (WDM) particles derived from the Lyman-alpha ...
The flux power spectrum of the high resolution Lyman-$\alpha$ forest data exhibits suppression at sm...
We present constraints on the mass of Warm Dark Matter (WDM) particles from a combined analysis of t...
We present new measurements of the free-streaming of warm dark matter (WDM) from Lyman-α flux-power ...
We present new measurements of the free-streaming of warm dark matter (WDM) from Lyman-α flux-power ...
We investigate the mass range and the corresponding free-streaming length scale of dark matter produ...
We present constraints on the masses of extremely light bosons dubbed fuzzy dark matter from Lyman- ...
This study introduces novel constraints on the free-streaming of thermal relic warm dark matter (WDM...
International audienceWe revisit Lyman-alpha bounds on the dark matter mass in Lambda Warm DarkMatte...
This study introduces novel constraints on the free streaming of thermal relic warm dark matter (WDM...
The matter power spectrum at comoving scales of (1-40)h-1 Mpc is very sensitive to the presence of W...
The observed Lyman-α flux power spectrum (FPS) is suppressed on scales below ∼ 30 km s−1. This cutof...
Warm dark matter (WDM) has been invoked to resolve apparent conflicts of cold dark matter (CDM) mode...
International audienceWe use the large BOSS DR9 sample of quasar spectra to constrain two cases of n...
We present constraints on the mass of warm dark matter (WDM) particles derived from the Lyman-alpha ...
We present constraints on the mass of warm dark matter (WDM) particles derived from the Lyman-alpha ...
The flux power spectrum of the high resolution Lyman-$\alpha$ forest data exhibits suppression at sm...
We present constraints on the mass of Warm Dark Matter (WDM) particles from a combined analysis of t...
We present new measurements of the free-streaming of warm dark matter (WDM) from Lyman-α flux-power ...
We present new measurements of the free-streaming of warm dark matter (WDM) from Lyman-α flux-power ...
We investigate the mass range and the corresponding free-streaming length scale of dark matter produ...
We present constraints on the masses of extremely light bosons dubbed fuzzy dark matter from Lyman- ...
This study introduces novel constraints on the free-streaming of thermal relic warm dark matter (WDM...
International audienceWe revisit Lyman-alpha bounds on the dark matter mass in Lambda Warm DarkMatte...
This study introduces novel constraints on the free streaming of thermal relic warm dark matter (WDM...
The matter power spectrum at comoving scales of (1-40)h-1 Mpc is very sensitive to the presence of W...
The observed Lyman-α flux power spectrum (FPS) is suppressed on scales below ∼ 30 km s−1. This cutof...
Warm dark matter (WDM) has been invoked to resolve apparent conflicts of cold dark matter (CDM) mode...
International audienceWe use the large BOSS DR9 sample of quasar spectra to constrain two cases of n...