Michael R. Savoy

  • Citations Per Year
Learn More
  • Marc Gagné, G. Fehon, +19 authors Lida M. Oskinova
  • 2011
The Chandra Carina Complex contains 200 known Oand B-type stars. The Chandra survey detected 68 of the 70 O stars and 61 of 127 known B0–B3 stars. We have assembled a publicly available optical/X-ray database to identify OB stars that depart from the canonical LX/Lbol relation or whose average X-ray temperatures exceed 1 keV. Among the single O stars with(More)
By insisting on naturalness in both the electroweak and quantum chromodynamics (QCD) sectors of the minimal supersymmetric standard model (MSSM), the portrait for dark matter production is seriously modified from the usual weakly interacting massive particle (WIMP) miracle picture. In supersymmetry (SUSY) models with radiatively-driven naturalness(More)
Howard Baer, Vernon Barger, Michael Savoy, and Xerxes Tata Dept. of Physics and Astronomy, University of Oklahoma, Norman, OK, 73019, USA Dept. of Physics, University of Wisconsin, Madison, WI 53706 USA and Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106 USA Dept. of Physics and Astronomy, University of Hawaii,(More)
  • 1