It is accepted now that dark matter is observed(SN1,WMAP). There are several particle physics ... compared to X-ray images(red) Gravitational lensing ...
Ramage,GGR. KK state. For some compactifications LKP stable ... Cryptons,... Indirect detection. Direct detection possible. CMSSM. Ramage, GGR. SO(10) ...
Prospects depend on both the characteristics of the dark matter particle and its ... (Draco, Sagittarius, etc.) Little is known for certain about the halo ...
Early Universe dense and hot; WIMPs in thermal equilibrium ... Need precise predictions within models of SUSY breaking. WHEPP-9 Bhubaneswar. 44. S. Kraml ...
The redshifted 21 cm background and particle decays. Evgenii O. ... baryon density fluctuations. density-velocity cross spectrum. velocity fluctuations ...
... Dec 2006. The Quest for SUSY : issues for collider physics and cosmology ... The cosmology connection. Dark matter. EW phase transition and baryon ... cosmology ...
subdominant candidates variety is common in Nature. may be easier to detect ... thermal (ma 10-3 eV, subdominant) otherwise: smaller ma possible [Tegmark, ...
Right-handed sneutrino. as cold dark matter. of the universe. Takehiko Asaka ... Subdominant modes: hadronic branching ratio is small. Stau. Main decay mode: ...
Less dependent on understanding of halo profile, diffusion parameters ... (Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such ...
Monument is now fully funded to complete construction of the Selinsing gold mine ... Appoints Kevin J. Wright, ACSM mining and mineral processing engineer, as ...
This presentation includes certain estimates, projections and 'forward looking ... Within the shear zone the breccia and cataclasite are widely noted and show ...
... underlying theory of this phenomenology, moduli. Comments on LHC ... sometimes new collider phenomenology new light vector bosons with mass 1 GeV, ...
Depuis les ann es 60 les Quasars sont connus comme des sources la fois ... Travail de Yann Cl net (Cl net et al., accept ) Mesures 1.7 m (H), 2.2 m (K) et 3.8 m ' ...
A hyperfine transition is one that takes. place due to a change in the spin of an electron ... Neutral particles (uncharged) Very light, but containing mass ...
As a result of the thermal freeze-out process, a relic density of WIMPs is left behind: ... LHC Relic Density. Studying SUSY with the LHC and Astrophysics ...
The Universe is the equivalent of a baby of 13 months, just old enough to begin ... illustrates how X-rays from a distant quasar dim as they pass through a cloud ...
DE can be explained with the introduction of a slowly evolving scalar field called quintessence. ... The quintessence field satisfies the equation: and. The ...
(Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such objects ... Halo profile (inhomogeneities?) Boundary conditions ...
We can't see neither Dark Matter nor Dark Energy. Then why do we talk about it? ... Isotropy and Homogeneity. maximally symmetric space. Flat Euclidean space R3 ...
Direct detection experiments will continue providing data in the near future. ... The relation between the gravitino mass and the rest of the soft masses depends ...