Results of the Dark Matter Sun analysis with 2007- 2008 data (Official Plots) Guillaume Lambard IFIC (Valencia, Spain) 06/06/2012.

Slides:

Advertisements

Similar presentations

Measurement of Relic Density at the LHC1 Bhaskar Dutta Texas A&M University Bhaskar Dutta Texas A&M University Measurement of Relic Density at the LHC.

Advertisements

Quark Compositeness Search with γ +Jet Final State at the LHC Satyaki Bhattacharya, Sushil S. Chauhan, Brajesh Choudhary, Debajyoti Choudhury Department.

Constraining CMSSM dark matter with direct detection results Chris Savage Oskar Klein Centre for Cosmoparticle Physics Stockholm University with Yashar.

Combined Energy Spectra of Flux and Anisotropy Identifying Anisotropic Source Populations of Gamma-rays or Neutrinos Sheldon Campbell The Ohio State University.

Limits on the spin-dependent scattering cross section from IceCube Joakim Edsjö Presented by Carlos de los Heros.

Intro to neutralino dark matter Pearl Sandick University of Minnesota.

Zhiqing Zhang (LAL, Orsay) 30/5-3/6/ SM Background Contributions Revisited for SUSY DM Stau Analyses Based on 1.P. Bambade, M. Berggren,

Masato Yamanaka (ICRR, University of Tokyo) Collaborators Junji Hisano, Kazunori Nakayama Shohei Sugiyama, Tomohiro Takesako.

T2K neutrino experiment at JPARC Approved since 2003, first beam in April Priorities : 1. search for, and measurement of,   e appearance  sin.

B. Dutta Texas A&M University Phys.Rev.Lett.99:261301, 2007; To appear Inflation, Dark Matter and Neutrino Masses Collaborators: Rouzbeh Allahverdi, Anupam.

I.1 ii.2 iii.3 iv.4 1+1=. i.1 ii.2 iii.3 iv.4 1+1=

21-25 January 2002 WIN 2002 Colin Okada, LBNL for the SNO Collaboration What Else Can SNO Do? Muons and Atmospheric Neutrinos Supernovae Anti-Neutrinos.

Energy Reconstruction Algorithms for the ANTARES Neutrino Telescope J.D. Zornoza 1, A. Romeyer 2, R. Bruijn 3 on Behalf of the ANTARES Collaboration 1.

I.1 ii.2 iii.3 iv.4 1+1=. i.1 ii.2 iii.3 iv.4 1+1=

MACRO Atmospheric Neutrinos Barry Barish 5 May 00 1.Neutrino oscillations 2.WIMPs 3.Astrophysical point sources.

Paris 22/4 UED Albert De Roeck (CERN) 1 Identifying Universal Extra Dimensions at CLIC  Minimal UED model  CLIC experimentation  UED signals & Measurements.

Particle Physics and Cosmology cosmological neutrino abundance.

EuroGDR, 13 th December 2003 Dan Tovey CERN, 18/03/2004 G. Bélanger 1 Uncertainties in the relic density calculations in mSUGRA B. Allanach, G. Bélanger,

1Alan Barr PASCOS 09 PASCOS 2009 DESY 9 July 2009 …AT THE LHC DARK MATTER … Alan Barr University of Oxford On behalf of the ATLAS and CMS collaborations.

Atmospheric Neutrino Oscillations in Soudan 2

Supersymmetry Without Prejudice 第二部分 KITPC 2008 C.F. Berger, J. Gainer, JLH, T. Rizzo Coming soon to an ArXiv near you.

Powerpoint Templates Page 1 Powerpoint Templates Looking for a non standard supersymmetric Higgs Guillaume Drieu La Rochelle, LAPTH.

Simona Toscano IFIC (Instituto de Física Corpuscular) CSIC-Universitat de València, Spain on behalf of the ANTARES collaboration on behalf of the ANTARES.

J. Barrios, S. Schulte, J.P. Gómez-González. Outline Introduction Data selection and processing MC production Data/MC comparison Event selection Detector.

Neutrino oscillation physics II Alberto Gago PUCP CTEQ-FERMILAB School 2012 Lima, Perú - PUCP.

4. Einstein Angle and Magnification The angular deflection for a relativistic neutrino with mass m ʋ that passes by a compact lens of mass M with impact.

Singlet Dark Matter, Type II Seesaw and Cosmic Ray Signals Nobuchika Okada Miami Fort Fauderdale, Dec , 2009 University of Alabama, Tuscaloosa.

Neutralino Dark Matter in Light Higgs Boson Scenario (LHS) The scenario is consistent with  particle physics experiments Particle mass b → sγ Bs →μ +

Dark Matter Particle Physics View Dmitri Kazakov JINR/ITEP Outline DM candidates Direct DM Search Indirect DM Search Possible Manifestations DM Profile.

8.1.4 Can it still be factored? Factoring Completely I can factor out a common factor.

Lepton Flavor violation study In Muon-neutrino to Tau direct coupling Very preliminary estimations Nakamura M. August 2009.

The ANTARES neutrino telescope is located on the bottom of the Mediterranean Sea, 40 km off the French coast. The detector is installed at a depth of 2.5.

Detection of Neutralino WIMP Yeong Gyun Kim (Korea Univ.) I.Evidence for Dark Matter II.Dark Matter Candidates III.Direct Detection of Neutralino WIMP.

Nuclearite search with the ANTARES neutrino telescope Vlad Popa, for the ANTARES Collaboration Institute for Space Sciences, Bucharest – Magurele, Romania.

Taking a Razor to Dark Matter Parameter Space (at the LHC) Chiu-Tien Yu (UW-Madison/Fermilab) with Paddy Fox, Roni Harnik, and Reinard Primulando arXiv:

IceCube Galactic Halo Analysis Carsten Rott Jan-Patrick Huelss CCAPP Mini Workshop Columbus OH August 6, m 2450 m August 6, 20091CCAPP DM Miniworkshop.

ORCA simulations - First steps J. Brunner 06/09/2012.

1 Gauge-singlet dark matter in the left-right symmetric model with spontaneous CP violation 郭万磊中国科学院理论物理研究所 CPS 2008, JiNan ， W.L. Guo, L.M.

Overview of Supersymmetry and Dark Matter

V. Bertin - CPPM - MANTS Paris - Sept'10 Indirect search of Dark Matter with the ANTARES Neutrino Telescope Vincent Bertin - CPPM-Marseille on behalf.

Dark matter and hidden U(1) X (Work in progress, In collaboration with E.J. Chun & S. Scopel) Park, Jong-Chul (KIAS) August 10, 2010 Konkuk University.

Indirect detection of Dark Matter with the ANTARES Neutrino Telescope Miguel Ardid on behalf of the ANTARES Collaboration Rome – September 2015.

1 Constraining ME Flux Using ν + e Elastic Scattering Wenting Tan Hampton University Jaewon Park University of Rochester.

Abstract Several models of elementary particle physics beyond the Standard Model, predict the existence of neutral particles that can decay in jets of.

Type II Seesaw Portal and PAMELA/Fermi LAT Signals Toshifumi Yamada Sokendai, KEK In collaboration with Ilia Gogoladze, Qaisar Shafi (Univ. of Delaware)

V. Bertin - CPPM - PONT Avignon - April'14 Indirect search for Dark Matter with the ANTARES Neutrino Telescope Vincent Bertin - CPPM-Marseille on behalf.

ORCA from ANTARES modules J. Brunner 06/10/2012. Detector Hexagonal layout a la IceCube 37 lines, distance 20m 25 ANTARES storeys  z = 4.5m Equipped.

Global Analysis, Combination & Complementarity The vision: explore 10 TeV scale directly (100 TeV pp) + indirectly (e + e - )

Xenon100 collaboration gives a stringent constraint on spin-independent elastic WIMP-nucleon scattering cross section. Ton-scale detectors for direct detection.

Higgs Recoil Mass Measurement and ZH Cross Section Tim Barklow, Awatif Belymam SLAC Feb 24, 2009.

Studies of Systematics for Dark Matter Observations John Carr 1.

Roma International Conference on Astroparticle Physics Rome, May 2013 Juan de Dios Zornoza (IFIC – Valencia) in collaboration with G. Lambard (IFIC) on.

Sergio Palomares-Ruiz June 30, 2008 Intermediate γ β-beam neutrino experiment with long baseline NuFact08 Valencia (Spain) June 30-July 5, 2008 See Christopher.

Systematics Sanghoon Jeon.

Indirect search for Dark Matter with neutrino telescopes

DM searches with the ANTARES neutrino telescope

Dark Matter Search in the Galactic Center with ANTARES

An interesting candidate?

Optimization studies of a tower based km3 detector

Dark Matter Phenomenology of the GUT-less CMSSM

Search for point-like source in ANTARES

Search for Dark Matter physics 805 fall 2008.

MC studies of the KM3NeT physics performance Rezo Shanidze

Claudio Bogazzi * - NIKHEF Amsterdam ICRC 2011 – Beijing 13/08/2011

We-Fu Chang, Wei-Ping Pan

7. Internal structure. II.

Solving Equations 3x+7 –7 13 –7 =.

P. Sapienza, R. Coniglione and C. Distefano

Intae Yu Sungkyunkwan University (SKKU), Korea KNO 2nd KNU, Nov

Presentation transcript:

Results of the Dark Matter Sun analysis with data (Official Plots) Guillaume Lambard IFIC (Valencia, Spain) 06/06/2012

Official plots Unblinding results I Data versus estimated background (derivative) BBFit reconstructed data && estimated background (from the scrambled data) && Feldman- Cousins statistical approach

06/06/2012Official plots Unblinding results I Data versus estimated background (derivative) BBFit reconstructed data && estimated background (from the scrambled data) && Feldman- Cousins statistical approach

06/06/2012Official plots Unblinding results II Neutrino + anti-neutrino flux limit from ANTARES Effective area to be estimated for different sets (Q,cone)

06/06/2012Official plots Unblinding results II Neutrino + anti-neutrino flux limit from ANTARES Optimum cone angles around the Sun

06/06/2012Official plots Unblinding results II Neutrino + anti-neutrino flux limit from ANTARES Neutrino + anti-neutrino flux limit ANTARES

06/06/2012Official plots Unblinding results III Muons flux limit from ANTARES Muon flux limit for ANTARES in the CMSSM framework

06/06/2012Official plots Unblinding results III Muons flux limit from ANTARES Muon flux limit for ANTARES in the mUED framework

06/06/2012Official plots Unblinding results IV Cross-section limits from ANTARES Spin-dependent cross-section limit for ANTARES in CMSSM Compare SUSY predictions to observables as sparticles masses, collider observables, dark matter relic density, direct detection cross-sections, … SuperBayes (arXiv: ) E μ >1 GeV

06/06/2012Official plots Unblinding results IV Cross-section limits from ANTARES Spin-independent cross-section limit for ANTARES in CMSSM Compare SUSY predictions to observables as sparticles masses, collider observables, dark matter relic density, direct detection cross-sections, … SuperBayes (arXiv: ) E μ >1 GeV

06/06/2012Official plots Unblinding results IV Cross-section limits from ANTARES Spin-dependent cross-section limit for ANTARES 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, (2011)) E μ >1 GeV