PQ-invariant multi-singlet NMSSM with anomalous U(1) gauge symmetry Kiwoon Choi The IBS Center for Theoretical Physics of the Universe KIAS-NCTS Workshop.
Signatures of Energy Injection in the CMB Rutgers University High Energy Theory Seminar 10/18/2011 Tracy Slatyer, Institute for Advanced Study based on.
Future large scale accelerator projects for particle phys
Dark matter candidates from particle physics and methods of detection
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Dark Matter cannot be seen directly with telescopes; it neither emits nor absorbs light; estimated to constitute 84.5% of the total matter in the universe.
1 Observationally Verifiable Predictions of Modified Gravity Talk given at Topical Conference on Elementary Particles, Astrophysics, and Cosmology, Miami.
Aldo Morselli INFN, Sezione di Roma 2 & Università di Roma Tor Vergata 1 Report from Italy A. Morselli, A. Lionetto, A. Cesarini, F.Fucito, P.Ullio* INFN,
Form Factor Dark Matter
Chapter 24 Or, how the scale factor grew in the past and will change in the future….
A P REDECESSOR TO A S CREENER OF U LTRA- L OW- L EVEL R ADIATION: THE P ROTOTYPE
2005. 2. 16 - 19 Changbom Park (Korea Institute for Advanced Study)
