Charged cosmic rays deflected by magnetic fields. Neutrinos can be ... Neutralinos self annihilate into fermions or combinations of gauge and Higgs bosons ...
Searches for Charginos and Neutralinos (RPC) Searches for Charginos, ... (mSUGRA) Gauge mediated model ( GMSB ) (new chiral supermultiplets: messengers) ...
Cosmology and Collider Physics - Focus on Neutralino Dark Matter - Masahiro ... Cosmology in ... Interesting interplay between cosmology and collider physics ...
Ramage,GGR. KK state. For some compactifications LKP stable ... Cryptons,... Indirect detection. Direct detection possible. CMSSM. Ramage, GGR. SO(10) ...
You get this by trying ALL POSSIBLE neutralino momenta, k, consistent with ... For each of these momenta, k, 'that might have been' there is an 'mslepton(k) ...
QCD events( ) with fake due to energy mismeasurement - EWK process with real (mostly , ... Central Photon ID cuts. No photons matched to phoenix track. Phoenix ...
powers of (low momenta)/(big mass scales) by this argument, gravity should be irrelevant ... then Kaluza-Klein parity (i.e. KK momentum) is conserved. ...
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 ...
Prospects depend on both the characteristics of the dark matter particle and its ... (Draco, Sagittarius, etc.) Little is known for certain about the halo ...
Possible problems: perturbation of asteroids and validity of Gould approximations. ... Guess: No, the asteroid orbits are very special and in general WIMP orbits are ...
High energy physicists study the smallest, most fundamental objects and the forces ... The 'Hydra' Galactic Cluster. Wmatter ~ 0.3 from galactic clusters ...
Very close to the EGRET upper limit for a cluster @ 100Mpc. Many positional coincidence between clusters and un-ID EGRET sources (e.g. Reimer et al. 2003) ...
Title: Ong page 1 of VHE astro Author: Trial User Last modified by: Trial User Created Date: 8/5/2004 1:23:59 PM Document presentation format: On-screen Show
Dark Matter Phenomenology of sub-GUT SUSY Breaking. Pearl Sandick. University of Minnesota ... SUSY must be broken, so introduce soft SUSY-breaking parameters ...
Problem 2: Halo substructure. N-body simulations show more than 10 ... find very dense dark halo with profile r-1.2, with very stringent constraints to core. ...
Southern University and A&M College, Baton Rouge, USA. Universite Libre de ... University of Canterbury, Christchurch, NZ. ANTARCTICA. The IceCube Collaboration ...
... magnet (BL2= 0.85 Tm2) Silicon Tracker (rigidity, charge) ... AMS on the International Space Station will provide enough statistics to perform a multi ...
Title: PowerPoint Presentation Last modified by: Hep Group Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles
Early Universe dense and hot; WIMPs in thermal equilibrium ... Need precise predictions within models of SUSY breaking. WHEPP-9 Bhubaneswar. 44. S. Kraml ...
Two iso-doublets Hu , Hd and one scalar S. l. After spontaneous EW U(1)X symmetry breaking by. the doublet higgsino mass and higgsino-singlino mass terms are ...
Dark Puzzles of the Universe. 4. How do we measure the content of the Universe? ... Dark Puzzles of the Universe. 5. CMB was emitted when the Universe was only ...
Why we like SUSY. Solves the Naturalness Problem. Gauge coupling unification (GUTs) ... Below some critical Min (dependent on tan( ) and other factors), all of nearly ...
Title: Supersymmetry searches at coliders Author: pape Last modified by: pape Created Date: 8/30/2003 4:28:41 PM Document presentation format: On-screen Show
(Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such objects ... Halo profile (inhomogeneities?) Boundary conditions ...
Flavour Physics and Dark Matter Introduction Selected Experimental Results Impact on Dark Matter Searches Conclusion Matthew Herndon University of Wisconsin
... on Physics and ... Facility Projects in Physics. The first large NSF facility in physics ... Perspectives: Physics. 3. Research in Fundamental Physics ...
Parts (QED) in extremely good agreement with experiment even with ... Something's coming, something good, (West Side Story) Progress in the last Century ...
DarkSUSY is a set of Fortran routines for calculations of relic densities and ... The quark and spin content of the nucleons can be changed by the user. ...
... from the galactic halo. gamma rays from the galactic halo ... synchrotron radiation from the galactic center / galaxy clusters. gammas from around the sun ...
Radiative corrections to Higgs acquire SUSY corrections: No fine-tuning required ... Data mass distribution agrees with SM expectation: mvis 120 GeV: 8.4 0.9 ...
What prospects for Supersymmetry at the Large Hadron Collider ? Some ... (Baryon number violating) RPV. RPV (Lepton number violating) RPC ... 2: Baryon number ...
Less dependent on understanding of halo profile, diffusion parameters ... (Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such ...
Spiral galaxies consist of a central bulge and a very thin disc, and surrounded ... It can survive from the Big Bang. and form the Dark matter in the Universe. 29 ...
involves s-channel /Z exchange, which depends on the field content, ... Main backgrounds: WW, WZ, W , a bit of bb. Altogether: 2 events observed vs 0.9 0.5 expected ...
The Observational Case For 7-8 GeV Dark Matter: Fermi, CoGeNT and DAMA Dan Hooper Fermilab/University of Chicago University of California Santa Barbara