AbstractBayesian methods offer a coherent and efficient framework for implementing uncertainties into induction problems. In this article, we review how this approach applies to the analysis of dark matter direct detection experiments. In particular we discuss the exclusion limit of XENON100 and the debated hints of detection under the hypothesis of a WIMP signal. Within parameter inference, marginalizing consistently over uncertainties to extract robust posterior probability distributions, we find that the claimed tension between XENON100 and the other experiments can be partially alleviated in isospin violating scenario, while elastic scattering model appears to be compatible with the frequentist statistical approach. We then move to mode...
In this activity we try to reproduce the XENON100 direct dark matter search results from 224 live da...
A great number of astrophysical observations suggests that of the matter in our universe, only a six...
We examine the consequences of the effective field theory (EFT) of dark matter–nucleon scattering fo...
Bayesian methods offer a coherent and efficient framework for implementing uncertainties into induct...
In this paper we assess the present status of dark matter direct searches by means of Bayesian stati...
Abstract. Bayesian statistical methods offer a simple and consistent framework for incorporating unc...
International audienceThe experimental situation of Dark Matter Direct Detection has reached anexcit...
8 pages, 6 figuresMany experiments that aim at the direct detection of Dark Matter are able to disti...
Abstract. Recently there has been a huge activity in the dark matter direct detection field, with th...
The experimental situation of dark matter direct detection has reached an exciting crossroads, with ...
Cosmological and astronomical observations show that most of the matter in the Universe is dark. Thi...
Astronomical and cosmological observations on different scales point to the existence of dark matter...
We discuss irreducible statistical limitations of future ton-scale dark matter direct detection expe...
International audienceThe scattering of dark matter particles off nuclei in direct detection experim...
Identifying the true theory of dark matter depends crucially on accurately characterizing interactio...
In this activity we try to reproduce the XENON100 direct dark matter search results from 224 live da...
A great number of astrophysical observations suggests that of the matter in our universe, only a six...
We examine the consequences of the effective field theory (EFT) of dark matter–nucleon scattering fo...
Bayesian methods offer a coherent and efficient framework for implementing uncertainties into induct...
In this paper we assess the present status of dark matter direct searches by means of Bayesian stati...
Abstract. Bayesian statistical methods offer a simple and consistent framework for incorporating unc...
International audienceThe experimental situation of Dark Matter Direct Detection has reached anexcit...
8 pages, 6 figuresMany experiments that aim at the direct detection of Dark Matter are able to disti...
Abstract. Recently there has been a huge activity in the dark matter direct detection field, with th...
The experimental situation of dark matter direct detection has reached an exciting crossroads, with ...
Cosmological and astronomical observations show that most of the matter in the Universe is dark. Thi...
Astronomical and cosmological observations on different scales point to the existence of dark matter...
We discuss irreducible statistical limitations of future ton-scale dark matter direct detection expe...
International audienceThe scattering of dark matter particles off nuclei in direct detection experim...
Identifying the true theory of dark matter depends crucially on accurately characterizing interactio...
In this activity we try to reproduce the XENON100 direct dark matter search results from 224 live da...
A great number of astrophysical observations suggests that of the matter in our universe, only a six...
We examine the consequences of the effective field theory (EFT) of dark matter–nucleon scattering fo...