A dark matter candidate from extra dimensions. 1. Regis Marco (SISSA, Trieste) ... Dark matter candidate. Coannihilation process. Resonant channels. Results ...
In mSUGRA the only possibilities : coannihilation, Higgs resonance, or Higgsino ... One example: changing the gaugino mass relations at GUT scale. A0= -1700 GeV ...
The coannihilation point is in a region that is favored if SUSY is to ... The digitized data files located at /usatlas/magdacache001/ common/doyen/A9_digi ...
Possible problems: perturbation of asteroids and validity of Gould approximations. ... Guess: No, the asteroid orbits are very special and in general WIMP orbits are ...
subdominant candidates variety is common in Nature. may be easier to detect ... thermal (ma 10-3 eV, subdominant) otherwise: smaller ma possible [Tegmark, ...
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. ...
Possible solution to the Li ... Toshifumi Jittoh, Kazunori Kohri, Masafumi Koike, Joe Sato, Takashi Shimomura ... A nucleus has the Coulomb barrier. While ...
Dark Matter Phenomenology of sub-GUT SUSY Breaking. Pearl Sandick. University of Minnesota ... SUSY must be broken, so introduce soft SUSY-breaking parameters ...
Early Universe dense and hot; WIMPs in thermal equilibrium ... Need precise predictions within models of SUSY breaking. WHEPP-9 Bhubaneswar. 44. S. Kraml ...
m(l l-)max. Using other. observables like. Mllq Mlq, MT, it is ... Baer, Barger, Shaughnessy, Summy, Wang 07. Gluino decays into t t c0, t b c - (mostly) ...
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 ...
Discovering (and understanding) SUSY at the LHC Alan Barr University of Oxford an introduction (with apologies to the many people who s work I have included
Title: Prospects for SUSY at ATLAS and CMS Author: Dan Tovey Last modified by: Dan Tovey Created Date: 4/16/2004 10:36:09 AM Document presentation format
Prospects depend on both the characteristics of the dark matter particle and its ... (Draco, Sagittarius, etc.) Little is known for certain about the halo ...
... Dec 2006. The Quest for SUSY : issues for collider physics and cosmology ... The cosmology connection. Dark matter. EW phase transition and baryon ... cosmology ...
'SOMETHING' fills the Universe: it 'disturbs' Weak ... del polo (AMANDA), o sotto il mare ( ANTARES, Marsiglia, in futuro NEMO, Capo Passero, Sicilia) ...
... magnet (BL2= 0.85 Tm2) Silicon Tracker (rigidity, charge) ... AMS on the International Space Station will provide enough statistics to perform a multi ...
N. Arkani-Hamed, G.F.G., R. Rattazzi, in preparation ... Cancellation of Existence of. positron. charm. top. 10-3 eV?? CAVEAT EMPTOR. electron self-energy ...
data taking (although it will certainly work better if both machines are. alive simultaneously) ... ILC can predict chi03/chi04/chi 2 from chi01/chi02/chi 1 ...
Large Extra Dim Model. N.Okada. Indirect signal of KK gravitons. Angular distribution of ee- HH ... Large extra dim. Techni pion production. Techni-pion mass ...
Less dependent on understanding of halo profile, diffusion parameters ... (Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such ...
(Draco, Sagittarius, etc.) Little is known for certain about the halo profiles of such objects ... Halo profile (inhomogeneities?) Boundary conditions ...
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. ...
COS-B and EGRET (20keV~30GeV) observed diffuse gamma rays, measured its spectra. ... EGRET data requires the neutralino mass be in the range 40~50 GeV and DM ...
Search for Gamma Rays from. LKP Dark Matter in the. UED framework ... correlative observations of transient events. Orbit. 565 km, circular. periode ~95 mns ...
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 ...
... and governance issues as well as the pre-production of the telescope components ... UK: Univ. Aberdeen, Univ. Leeds, Univ. Liverpool, Univ. Sheffield ...
Enhanced flux possible thanks to halo density profile and substructure (as predicted by CDM) ... profile needed for DM substructure; some fine-tuning to get ...
Main asset of LHC: huge event statistics thanks to high s and L. Allows precision measurements/tests ... EDELWEISS 2. CRESST-II. ZEPLIN-I. EDELWEISS. CDMS. DAMA ...
Impacts of Supercritical String Cosmology at the Large Hadron Collider ... Supercritical String Cosmology (SSC) predicts a smoothly evolving Dark Energy. ...
Luminous matter does not account for enough mass to explain rotational velocities of galaxies ... Also groups pursuing Argon (WARP/ArDM), Helium (HERON), Neon (CLEAN) ...
Title: PowerPoint Presentation Last modified by: Tommaso Lari Created Date: 1/1/1601 12:00:00 AM Document presentation format: On-screen Show Other titles
Golden physics channel! d(1/p) = 7 x 10-5/GeV. 1/10 LEP !!! goal: dMmm 0.1x GZ ... between EM and hadronic showers. small X0/lhad. longitudinal segmentation ...
Chicago has been involved in the OPAL Higgs searches since day-1: ... Martina moving to CERN; devoting to SUSY Emiss analysis. Now primary activity for Oreglia ...
For these and other benchmark scenarios, boost factors needed to fit HEAT data ... Center) visible signal in cuspy profile scenarios or other boost factors. ...
Institute for Particle Physics Phenomenology ... EDELWEISS. 16-01-06 CICHEP Cairo ... EDELWEISS. Increase m and help avoiding UFB constraints. Can even be positive if ...