150 citations
- J. Farine2 profiles7 · h 43
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- Evgeni Kharadze Georgian National Astrophysical ObservatoryGE7 papers
- Kansas State UniversityUS7 papers
- Colorado State UniversityUS5 papers
- SLAC National Accelerator LaboratoryUS5 papers
- Stanford UniversityUS5 papers
- Carleton UniversityCA4 papers
- Menlo SchoolUS4 papers
- University of AlabamaUS4 papers
- University of NeuchâtelCH4 papers
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- Queen's UniversityCA3 papers
- Stanford Synchrotron Radiation LightsourceUS3 papers
6 papers · 1 filter
New Insights into Particle Detection with Superheated Liquids
S. Archambault, F. Aubin, M. Auger +34
We report new results obtained in calibrations of superheated liquid droplet detectors used in dark matter searches with different radiation sources (n,,). In particular, det…
Vibrational density of states of silicon nanoparticles
R. Meyer, D. Comtesse
The vibrational density of states of silicon nanoparticles in the range from 2.3 to 10.3 nm is studied with the help of molecular-dynamics simulations. From these simulations the v…
Primordial magnetic field limits from cosmological data
Tina Kahniashvili, Alexander G. Tevzadze, Shiv K. Sethi +2
We study limits on a primordial magnetic field arising from cosmological data, including that from big bang nucleosynthesis, cosmic microwave background polarization plane Faraday…
A simple radionuclide-driven single-ion source
M. Montero Díez, K. Twelker, W. Fairbank +54
We describe a source capable of producing single barium ions through nuclear recoils in radioactive decay. The source is fabricated by electroplating 148Gd onto a silicon α-particl…
Deformed shell model results for two neutrino positron double beta decay of Sr
R. Sahu, V. K. B. Kota
Half-lives for two neutrino positron double beta decay modes EC/ECEC are calculated for Sr, a nucleus of current experimental interest, within the fram…
Numerical simulations of the decay of primordial magnetic turbulence
Tina Kahniashvili, Axel Brandenburg, Alexander G. Tevzadze +1
We perform direct numerical simulations of forced and freely decaying 3D magnetohydrodynamic turbulence in order to model magnetic field evolution during cosmological phase transit…