AbstractIn this paper we investigate di-atomic molecules embedded in ice crystals under strain. In this environment coherent vibrations of many OH-bonds may be generated by one WIMP collision. The detection of such multiple-photon signals may provide a signature of a 100 GeV/c2 WIMP. To do a proper lab test of “WIMP-induced” multi-photon emission is very difficult. We suggest that Ice Cube make a search for multi-photon events, and investigate whether the rate of such events exhibits yearly modulation
Context. Many interstellar molecules are thought to form on dust grains. In particular, hydrogenatio...
We show that a two-excitation process in superfluid helium, combined with sensitivity to meV energy ...
The interstellar medium (ISM) is the place surrounding the stars. It is constituted of gas and dust ...
In this paper we investigate di-atomic molecules embedded in ice crystals under strain. In this envi...
AbstractIn this paper we investigate di-atomic molecules embedded in ice crystals under strain. In t...
We believe that the Dark Matter (DM) search should be expanded into the domain of detectors sensitiv...
Direct detection of nuclear scatterings of sub-GeV Dark Matter (DM) particles favors low-Z nuclei. H...
International audienceThe present study measures the sticking probability of heavy water (D2O) on H2...
AbstractWe believe that the Dark Matter (DM) search should be expanded into the domain of detectors ...
Intermolecular reactions in and on icy films on silicate and carbonaceous grains constitute a major...
Context. The vacuum-UV (VUV) absorption cross sections of most molecular solids present in...
Carbon dioxide has been produced from the impact of a monoenergetic O(P-3) beam upon a surface coole...
The deposition of energy in the form of electronic excitations in molecules condensed on cold surfac...
Recent detections of Complex Organic Molecules (COMs) in the cold regions of the interstellar medium...
Context. In cold regions of the interstellar medium with intense ultraviolet radiation fields, photo...
Context. Many interstellar molecules are thought to form on dust grains. In particular, hydrogenatio...
We show that a two-excitation process in superfluid helium, combined with sensitivity to meV energy ...
The interstellar medium (ISM) is the place surrounding the stars. It is constituted of gas and dust ...
In this paper we investigate di-atomic molecules embedded in ice crystals under strain. In this envi...
AbstractIn this paper we investigate di-atomic molecules embedded in ice crystals under strain. In t...
We believe that the Dark Matter (DM) search should be expanded into the domain of detectors sensitiv...
Direct detection of nuclear scatterings of sub-GeV Dark Matter (DM) particles favors low-Z nuclei. H...
International audienceThe present study measures the sticking probability of heavy water (D2O) on H2...
AbstractWe believe that the Dark Matter (DM) search should be expanded into the domain of detectors ...
Intermolecular reactions in and on icy films on silicate and carbonaceous grains constitute a major...
Context. The vacuum-UV (VUV) absorption cross sections of most molecular solids present in...
Carbon dioxide has been produced from the impact of a monoenergetic O(P-3) beam upon a surface coole...
The deposition of energy in the form of electronic excitations in molecules condensed on cold surfac...
Recent detections of Complex Organic Molecules (COMs) in the cold regions of the interstellar medium...
Context. In cold regions of the interstellar medium with intense ultraviolet radiation fields, photo...
Context. Many interstellar molecules are thought to form on dust grains. In particular, hydrogenatio...
We show that a two-excitation process in superfluid helium, combined with sensitivity to meV energy ...
The interstellar medium (ISM) is the place surrounding the stars. It is constituted of gas and dust ...