Download presentation
Presentation is loading. Please wait.
Published byAmi Wilkinson Modified over 9 years ago
1
Results of the Dark Matter Sun analysis with 2007- 2008 data (Official Plots) Guillaume Lambard IFIC (Valencia, Spain) 06/06/2012
2
Official plots 20122 Unblinding results I Data 2007-2008 versus estimated background (derivative) BBFit reconstructed data 2007-2008 && estimated background (from the scrambled data) && Feldman- Cousins statistical approach
3
06/06/2012Official plots 20123 Unblinding results I Data 2007-2008 versus estimated background (derivative) BBFit reconstructed data 2007-2008 && estimated background (from the scrambled data) && Feldman- Cousins statistical approach
4
06/06/2012Official plots 20124 Unblinding results II Neutrino + anti-neutrino flux limit from ANTARES 2007-2008 Effective area to be estimated for different sets (Q,cone)
5
06/06/2012Official plots 20125 Unblinding results II Neutrino + anti-neutrino flux limit from ANTARES 2007-2008 Optimum cone angles around the Sun
6
06/06/2012Official plots 20126 Unblinding results II Neutrino + anti-neutrino flux limit from ANTARES 2007-2008 Neutrino + anti-neutrino flux limit ANTARES 2007-2008
7
06/06/2012Official plots 20127 Unblinding results III Muons flux limit from ANTARES 2007-2008 Muon flux limit for ANTARES 2007-2008 in the CMSSM framework
8
06/06/2012Official plots 20128 Unblinding results III Muons flux limit from ANTARES 2007-2008 Muon flux limit for ANTARES 2007-2008 in the mUED framework
9
06/06/2012Official plots 20129 Unblinding results IV Cross-section limits from ANTARES 2007-2008 Spin-dependent cross-section limit for ANTARES 2007-2008 in CMSSM Compare SUSY predictions to observables as sparticles masses, collider observables, dark matter relic density, direct detection cross-sections, … SuperBayes (arXiv:1101.3296) E μ >1 GeV
10
06/06/2012Official plots 201210 Unblinding results IV Cross-section limits from ANTARES 2007-2008 Spin-independent cross-section limit for ANTARES 2007-2008 in CMSSM Compare SUSY predictions to observables as sparticles masses, collider observables, dark matter relic density, direct detection cross-sections, … SuperBayes (arXiv:1101.3296) E μ >1 GeV
11
06/06/2012Official plots 201211 Unblinding results IV Cross-section limits from ANTARES 2007-2008 Spin-dependent cross-section limit for ANTARES 2007-2008 in mUED Compare mUED predictions to observables as KK masses, collider observables, relic density, direct detection cross- sections, … SuperBayes modified version (Physical Review D 83, 036008 (2011)) E μ >1 GeV
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.