AbstractWe calculate the fluxes of 511 keV photons from the galactic bulge caused by positrons produced in the decays of relic particles with masses less than 100 MeV. In particular, we tighten the constraints on sterile neutrinos over a large domain of the mass-mixing angle parameter space, where the resulting photon flux would significantly exceed the experimental data. At the same time, the observed photon fluxes can be easily caused by decaying sterile neutrinos in the mass range 1<msterile≲50 MeV with the cosmological abundance typically within 10−9≲Ωsterile≲10−5, assuming that Ωsterile comes entirely from the conversion of active neutrinos in the early universe. Other candidates for decaying relics such as neutral (pseudo)scalar parti...
We analyze the most recent cosmological data, including Planck, taking into account the possible exi...
International audienceContext. The Galaxy hosts a widespread population of low-energy positrons reve...
International audienceWe devise a new semi-analytical method dedicated to the propagation of Galacti...
AbstractWe calculate the fluxes of 511 keV photons from the galactic bulge caused by positrons produ...
International audienceFeebly interacting particles with masses with O(10–100) MeV can be copiously ...
There has recently been renewed interest in massive neutral dark-matter particle candidates with mas...
In this paper, we calculate the relic abundance of the dark matter particles when they can annihilat...
The observed 511 keV line from the Galactic Bulge is a real challenge for theoretical astrophysics: ...
The authors examine a mechanism which can lead to flavor transformation of neutrino-antineutrino asy...
AbstractAlthough Planck data supports the standard ΛCDM model, it still allows for the presence of D...
We present constraints on the mass of warm dark matter (WDM) particles from a combined analysis of t...
We derive constraints on the relic abundance of a generic particle of mass $\sim~1-10^{14}$ TeV whic...
International audienceThe first γ-ray line originating from outside the Solar System that was ever d...
Although Planck data supports the standard ΛCDM model, it still allows for the presence of Dark Radi...
The annihilation of positrons in the Milky Way Galaxy has been observed for ∼50 years; however, the ...
We analyze the most recent cosmological data, including Planck, taking into account the possible exi...
International audienceContext. The Galaxy hosts a widespread population of low-energy positrons reve...
International audienceWe devise a new semi-analytical method dedicated to the propagation of Galacti...
AbstractWe calculate the fluxes of 511 keV photons from the galactic bulge caused by positrons produ...
International audienceFeebly interacting particles with masses with O(10–100) MeV can be copiously ...
There has recently been renewed interest in massive neutral dark-matter particle candidates with mas...
In this paper, we calculate the relic abundance of the dark matter particles when they can annihilat...
The observed 511 keV line from the Galactic Bulge is a real challenge for theoretical astrophysics: ...
The authors examine a mechanism which can lead to flavor transformation of neutrino-antineutrino asy...
AbstractAlthough Planck data supports the standard ΛCDM model, it still allows for the presence of D...
We present constraints on the mass of warm dark matter (WDM) particles from a combined analysis of t...
We derive constraints on the relic abundance of a generic particle of mass $\sim~1-10^{14}$ TeV whic...
International audienceThe first γ-ray line originating from outside the Solar System that was ever d...
Although Planck data supports the standard ΛCDM model, it still allows for the presence of Dark Radi...
The annihilation of positrons in the Milky Way Galaxy has been observed for ∼50 years; however, the ...
We analyze the most recent cosmological data, including Planck, taking into account the possible exi...
International audienceContext. The Galaxy hosts a widespread population of low-energy positrons reve...
International audienceWe devise a new semi-analytical method dedicated to the propagation of Galacti...