In the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitino mass is around keV, we show that the 3.5 keV X-ray lines can be explained naturally through several different mechanisms: (I) a keV scale dark gaugino plays the role of sterile neutrino in the presence of bilinear R -parity violation. Because the light dark gaugino obtains Majorana mass only via gravity mediation, it is a decaying warm dark matter (DM) candidate; (II) the compressed cold DM states, whose mass degeneracy is broken by gravity mediated SUSY breaking, emit such a line via the heavier one decay into the lighter one plus photon(s). A highly supersymmetric dark sector may readily provide such kind of system; (III) the light axino, whose m...
We show that a couplet, a pair of closely spaced photon lines, in the X-ray spectrum is a distinctiv...
We consider a local U(1) B − L extension of Zee-Babu model to explain the recently observed 3.5 keV ...
We study the phenomenology of a keV sterile neutrino in a supersymmetric model with U(1) R -lepton n...
AbstractIn the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitin...
In the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitino mass i...
We present some R-parity conserving supersymmetric models which can accommodate the 3.5 keV X-ray li...
We present a simple model of weak-scale thermal dark matter that gives rise to X-ray lines. Dark mat...
A recent analysis of XXM-Newton data reveals the possible presence of an X-ray line at approximately...
AbstractWe consider some implications of X-ray lines from certain astronomical objects as potential ...
The recent observation of an X-ray line at an energy of 3.5 keV mainly from galaxy clusters has init...
AbstractThe recent observation of an X-ray line at an energy of 3.5 keV mainly from galaxy clusters ...
The 3.5 keV line recently detected in the X-ray spectra of certain galaxy clusters may have had a da...
We study an exciting dark matter scenario in a radiative neutrino model to explain the X-ray line si...
AbstractWe consider axino warm dark matter in a supersymmetric axion model with R-parity violation. ...
An unidentified 3.5 keV line from X-ray observations of galaxy clusters has been reported recently. ...
We show that a couplet, a pair of closely spaced photon lines, in the X-ray spectrum is a distinctiv...
We consider a local U(1) B − L extension of Zee-Babu model to explain the recently observed 3.5 keV ...
We study the phenomenology of a keV sterile neutrino in a supersymmetric model with U(1) R -lepton n...
AbstractIn the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitin...
In the supersymmetric models with low scale supersymmetry (SUSY) breaking where the gravitino mass i...
We present some R-parity conserving supersymmetric models which can accommodate the 3.5 keV X-ray li...
We present a simple model of weak-scale thermal dark matter that gives rise to X-ray lines. Dark mat...
A recent analysis of XXM-Newton data reveals the possible presence of an X-ray line at approximately...
AbstractWe consider some implications of X-ray lines from certain astronomical objects as potential ...
The recent observation of an X-ray line at an energy of 3.5 keV mainly from galaxy clusters has init...
AbstractThe recent observation of an X-ray line at an energy of 3.5 keV mainly from galaxy clusters ...
The 3.5 keV line recently detected in the X-ray spectra of certain galaxy clusters may have had a da...
We study an exciting dark matter scenario in a radiative neutrino model to explain the X-ray line si...
AbstractWe consider axino warm dark matter in a supersymmetric axion model with R-parity violation. ...
An unidentified 3.5 keV line from X-ray observations of galaxy clusters has been reported recently. ...
We show that a couplet, a pair of closely spaced photon lines, in the X-ray spectrum is a distinctiv...
We consider a local U(1) B − L extension of Zee-Babu model to explain the recently observed 3.5 keV ...
We study the phenomenology of a keV sterile neutrino in a supersymmetric model with U(1) R -lepton n...