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The 14th International Workshop Dark Side Of the Universe

25–29 juin 2018
Annecy-le-Vieux, France
Fuseau horaire Europe/Paris

Session

Parallel II

25 juin 2018, 15:20
Auditorium (Annecy-le-Vieux, France)

Auditorium

Annecy-le-Vieux, France

9 chemin de Bellevue

Présidents de session

Parallel II: Dark Matter models

  • Bryan Zaldivar (LAPTh, Annecy-le-Vieux)

Parallel II: Dark Matter models

  • Bryan Zaldivar (LAPTh, Annecy-le-Vieux)

Parallel II: Indirect dark matter searches

  • Francesca Calore (LAPTh, CNRS)

Parallel II: Dark matter direct detection

  • Hyun Min Lee

Documents de présentation

Korsmeier_DSU18.pdf
  1. 41. Supersymmetric dark matter by GAMBIT
    Csaba Balazs (Monash University)
    25/06/2018 15:20
    Dark matter models
    Contributed talk

    Is supersymmetry loosing ground as a compelling explanation for dark matter? Or is there still enough experimental evidence to support our faith in supersymmetric dark matter? In search of quantitative answers, focusing on dark matter properties, I review the latest GAMBIT results for various supersymmetric models covering the CMSSM, NUHM1 and 2, MSSM7 and MSSM9.

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  2. 67. LHC and dark matter signals motivated by the $\mu\nu$SSM
    Daniel Lopez-Fogliani
    25/06/2018 15:40
  3. 13. Radiative corrections to the Relic Density in the IDM
    Guillaume Chalons (LPSC-IN2P3-CNRS)
    25/06/2018 16:30
    Dark matter models
    Contributed talk

    The current experimental precision from PLANCK on the extraction of the relic abundance of Dark Matter calls for very precise prediction from the theory side to be able to extract meaningful information. In this study we compute the full set of radiative corrections entering the calculation of the relic density of Dark Matter in the Inert Doublet Model and weigh their impact on its prediction...

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  4. 53. Moduli Portal Dark Matter
    Debtosh Chowdhury (CPHT, Ecole Polytechnique)
    25/06/2018 16:50
    Dark matter models
    Contributed talk

    Supergravity and string theories usually have particles, such as a modulus, with only gravitational interactions. These moduli fields arise due to the flat directions in the above theories. We inspect the possibility that these moduli fields acting as a mediator between the dark sector and the Standard Model, from an effective field theory perspective. We show that in this scenario, dark...

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  5. 68. Dynamical EW symmetry breaking via multiple bosonic seesaw
    Shohei Okawa (TUM, Munich)
    25/06/2018 17:10
  6. 26. SuperIso Relic new extensions for direct and indirect detection
    Glenn Robbins (CRAL)
    25/06/2018 17:30
    Indirect detection
    Contributed talk

    SuperIso Relic is a public computing program for the calculation of flavour observables and relic density in supersymmetry (MSSM and NMSSM). We present new extensions of the code dedicated to the calculation of dark matter direct and indirect detection constraints from the latest experiment results. After presenting the new features of the program in particular the treatment of the relevant...

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  7. 117. Dark matter searches with cosmic-ray antideuteron and antihelium
    Michael Korsmeier
    25/06/2018 17:50
    Contributed talk
  8. 49. Constraining Galactic dark matter with gamma-ray pixel counts statistics
    Silvia Manconi (University of Turin)
    26/06/2018 16:30
    Indirect detection
    Contributed talk

    The investigation of the composition of the extra-galactic gamma-ray background (EGB) is a powerful tool to search for dark matter signals in the gamma-ray sky. In the last few years, statistical analysis methods have been demonstrated to outperfom classic detection methods in decomposing the EGB. In particular, the 1-point photon counts statistics (1pPDF) permits to resolve the population of...

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  9. 43. Probing the Nature of Dark Matter with Gamma Rays: Prospects for the Cherenkov Telescope Array at the Galactic Center
    Christopher Eckner (University of Nova Gorica), for the CTA Consortium
    26/06/2018 16:50
    Indirect detection
    Contributed talk

    Revealing the nature of dark matter is one of the most riveting open tasks of modern astronomy and cosmology. To this end, observing and analyzing high-energy gamma-rays provides a promising and highly-effective tool which is, in particular, well-suited to constrain Weakly Interacting Massive Particle (WIMP) models.
    Being currently in its pre-construction phase, the Cherenkov Telescope Array...

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  10. 28. Constraining TeV-scale dark matter with cosmic-ray antiprotons
    Dr Jan Heisig (RWTH Aachen University)
    26/06/2018 17:10
    Indirect detection
    Contributed talk

    osmic-ray observations provide a powerful probe of dark matter annihilation in the Galaxy. In this paper we derive constraints on heavy dark matter from the recent precise AMS-02 antiproton data. We consider all possible annihilation channels into pairs of standard model particles. Furthermore, we interpret our results in the context of minimal dark matter, including higgsino, wino and...

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  11. 22. Astrophysical background and dark matter implication based on latest AMS-02 data
    Hong-Bo Jin (National Astronomical Observatories, Chinese Academy of Sciences)
    26/06/2018 17:30
    Indirect detection
    Contributed talk

    The cosmic ray(CR) positrons and antiprotons are often regarded as the products of collisions of CR nucleons with the interstellar medium. However this conclusion is challenged by recent experimental data. In this work, we choose the latest AMS-02 data to analyze the astrophysical background of CR positrons and antiprotons based on the GALPROP code for CR propagation and QGSJET-II-04 for ...

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  12. 102. One loop direct detection
    Natsumi Nagata
    28/06/2018 16:40
  13. 36. Direct detection of exothermic dark matter with light mediator
    Dr Da Huang (University of Warsaw)
    28/06/2018 17:00
    Direct detection
    Contributed talk

    In this talk, we study the possible models trying to reconcile the tension between the CDMS-Si signals and null experiments. In particular, we focus on the models with the following properties: isospin-violating couplings, exothermic scatterings, and/or a light mediator. In the light of the latest constraints from LUX, PandaX-II, XENON1T, CDMSlite and PICO-60, we find that, for almost all the...

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  14. 103. Boosted dark matter and surface detector
    Jong-Chul Park
    28/06/2018 17:20
  15. 104. Direct detection of mirror dark matter
    Robert Foot
    28/06/2018 17:40
  16. 20. Surrogate Models for Direct Dark Matter Detection
    Andrew Cheek (Durham, IPPP)
    28/06/2018 18:00
    Contributed talk

    This talk will introduce the use of surrogate model techniques for direct detection of dark matter. We have developed a tool, RAPIDD, that replaces the exact calculation of the dark matter differential rate (which in general involves up to three nested integrals) with a much faster parametrization in terms of ordinary polynomials of the dark matter mass and couplings, obtained in an initial...

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  17. 113. Inelastic boosted dark matter at protoDUNE
    Doojin Kim
    28/06/2018 18:20
    Contributed talk
  18. 70. Moduli portal DM
    D. Choudhury
  19. 29. Observable windows for the QCD axion as a hot relic
    Alessio Notari
    Contributed talk

    I will discuss the possibility of detecting the QCD axion as a hot relic from the early universe, if it is directly coupled to quarks, such as in DFSZ models. For sufficiently low decay constant the dominant production mechanism at temperatures 1GeV≲T≲100GeV is obtained via scatterings with heavy quarks. This leads to a contribution to the effective neutrino number, $N_eff$, which is larger...

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  20. 69. Sneutrino DM in non-minimal SUSY
    S. Khalil
Ordre du jour en construction...