An unidentified 3.5 keV line from X-ray observations of galaxy clusters has been reported recently. Although still under scrutiny, decaying dark matter could be responsible for this signal. We investigate whether an axino with a mass of 7 keV could explain the line, keeping the discussion as model independent as possible. We point out several obstacles, which were overlooked in the literature, and which make the axino an unlikely candidate. The only viable scenario predicts a light metastable neutralino, with a mass between 0.1 and 10 GeV and a lifetime between 10−3 and 104 s
In the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitino mass i...
AbstractIn the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitin...
The recently reported X-ray line signal at Eγ≃3.5keV from a stacked spectrum of various galaxy clust...
An unidentified 3.5 keV line from X-ray observations of galaxy clusters has been reported recently. ...
Axino as the superpartner of axion that solves the strong CP problem can be a good candidate of dark...
AbstractRecently a weak X-ray emission around Eγ≃3.5 keV was detected in the Andromeda galaxy and va...
Recently, indications for an emission line at 3.55 keV have been found in the combined spectra of a ...
AbstractWe consider axino warm dark matter in a supersymmetric axion model with R-parity violation. ...
Recently a weak X-ray emission around <math altimg="si1.gif" xmlns="http://www.w3.org/1998/Math/Math...
We propose a scenario where the saxion dominates the energy density of the Universe and reheats the ...
Recently, indications for an emission line at 3.55 keV have been found in the combined spectra of a ...
Recently, indications for an emission line at 3.55 keV have been found in the combined spectra of a ...
The recently reported X-ray line signal at Eγ ' 3.5keV from a stacked spectrum of various galax...
AbstractWe propose a scenario where the saxion dominates the energy density of the Universe and rehe...
Galaxy clusters can efficiently convert axion-like particles (ALPs) to photons. We propose that the ...
In the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitino mass i...
AbstractIn the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitin...
The recently reported X-ray line signal at Eγ≃3.5keV from a stacked spectrum of various galaxy clust...
An unidentified 3.5 keV line from X-ray observations of galaxy clusters has been reported recently. ...
Axino as the superpartner of axion that solves the strong CP problem can be a good candidate of dark...
AbstractRecently a weak X-ray emission around Eγ≃3.5 keV was detected in the Andromeda galaxy and va...
Recently, indications for an emission line at 3.55 keV have been found in the combined spectra of a ...
AbstractWe consider axino warm dark matter in a supersymmetric axion model with R-parity violation. ...
Recently a weak X-ray emission around <math altimg="si1.gif" xmlns="http://www.w3.org/1998/Math/Math...
We propose a scenario where the saxion dominates the energy density of the Universe and reheats the ...
Recently, indications for an emission line at 3.55 keV have been found in the combined spectra of a ...
Recently, indications for an emission line at 3.55 keV have been found in the combined spectra of a ...
The recently reported X-ray line signal at Eγ ' 3.5keV from a stacked spectrum of various galax...
AbstractWe propose a scenario where the saxion dominates the energy density of the Universe and rehe...
Galaxy clusters can efficiently convert axion-like particles (ALPs) to photons. We propose that the ...
In the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitino mass i...
AbstractIn the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitin...
The recently reported X-ray line signal at Eγ≃3.5keV from a stacked spectrum of various galaxy clust...