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Aspen 2013 - Closing in on Dark Matter

US/Mountain
Flug Forum (Aspen Center for Physics)

Flug Forum

Aspen Center for Physics

700 W. Gillespie Street Aspen, CO 81611
Anyes TAFFARD (University of California Irvine (US)), Jason KUMAR (University of Hawaii), Jennifer SIEGAL-GASKINS, Jodi COOLEY (SMU), Manoj KAPLINGHAT, Stefan FUNK
Description
Dark matter is a cornerstone of the cosmological Standard Model, but we only have evidence for it through its gravitational effects. Experimental results to date have provided inconclusive but tantalizing evidence for the particle nature of dark matter. In the coming months, experimental developments are expected to shed light on some of its fundamental properties. A significant advance in our understanding may follow. The complementary approaches to detecting dark matter are reaching sensitivities which will probe many dark matter theories. At the same time, there has been exciting new research elucidating the possible theoretical frameworks for dark matter. This Aspen Winter Workshop will focus on synthesizing these latest experimental results and theoretical developments, determining the implications for dark matter properties, and pinpointing future directions in this rapidly evolving field.
    • 17:00 19:00
      Registration Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 08:00 09:35
      Overview Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 08:00
        Welcome 5m
        Speaker: Jodi Cooley
      • 08:05
        Direct Detection 30m
        Speaker: Patrick Decowski
        Slides
      • 08:35
        Indirect Detection 30m
        Speaker: Dan Hooper
        Slides
      • 09:05
        Theory and Phenomenology 30m
        Speaker: Bhaskar Dutta
        Slides
    • 09:35 09:55
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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 09:55 11:10
      Direct Detection: 1 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 09:55
        XENON 25m
        Speaker: Emilija Pantic
        Slides
      • 10:20
        SuperCDMS 25m
        Speaker: Jeter Hall
        Slides
    • 11:10 16:30
      Break 5h 20m Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 16:30 17:45
      Theory-Pheno: 1 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 16:30
        Complementarity of Searches for Dark Matter 25m
        I'll discuss perspectives on how different types of searches for particle dark matter (direct, indirect, and production at colliders) are complementary, with emphasis on how theoretical descriptions of dark matter interactions with the Standard Model can help clarify the inter-relation of various search strategies.
        Speaker: Tim Tait
        Slides
      • 16:55
        On the annual modulations in direct-detection experiments and the DAMA results 25m
        In this talk I will discuss recent results concerning the annual modulations expected in experiments looking for dark matter recoils in the lab. I will begin by describing the general properties of this problem including some new tools. I will then focus on the DAMA result and its relation to the modulations of cosmic muons. I will end by discussing the relation between the modulated and unmodulated parts of a putative signal and how it applies to the signal seen by DAMA.
        Speaker: Itay Yavin
        Slides
      • 17:20
        Importance of upgraded energy reconstruction for direct dark matter searches with liquid xenon detectors 25m
        Speaker: Peter Sorensen
        Slides
    • 17:45 18:15
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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 18:15 19:30
      Indirect Detection: 1 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 18:15
        The Density & Velocity Structure of Dark Matter Halos 25m
        Speaker: Risa Wechsler
        Slides
      • 18:40
        Astrophysical simulations with baryons 25m
        Speaker: Justin Read
        Slides
      • 19:05
        Current and future insights on dark matter particle properties through strong gravitational lensing observations 25m
        Speaker: Leonidas Moustakas
        Slides
    • 08:00 09:15
      Direct Detection: 2 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 08:00
        Neutrino Backgrounds to Large Scale Dark Matter Detectors 25m
        Speaker: Tali Figueroa
        Slides
      • 08:25
        LUX 25m
        Speaker: Rick Gaitskell
        Slides
      • 08:50
        XENON 1T 25m
        Speaker: Rafeal Lang
        Slides
    • 09:15 09:45
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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 09:45 11:50
      Indirect Detection: 2 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 09:45
        Indirect Searches for Dark Matter with the Fermi LAT 25m
        Since its launch in 2008, the Fermi LAT has made significant progress towards constraining the standard “WIMP miracle” dark matter scenario. In this talk, I will review recent results from the LAT with a focus on current constraints, tentative signals, and associated uncertainties. I will discuss how an improved understanding the LAT instrument and gamma-ray astrophysics will help to disentangle dark matter signals from a complex gamma-ray sky.
        Speaker: Alex Drlica-Wagner
        Slides
      • 10:10
        Searches for TeV-scale dark matter 25m
        Speaker: Sasha Belikov
        Slides
      • 10:35
        Signals from Dark Matter Annihilation at the Galactic Center 25m
        Speaker: Tim Linden
        Slides
      • 11:00
        Joint dataset analysis and dark matter constraints from dwarf galaxies 25m
        I will discuss recent work on statistical methods that can be used to test the hypothesis of extremely faint dark matter signals contained in gamma-ray data. I will also discuss recent results on searches for dark matter annihilation emission from dwarf galaxies using data from Fermi and VERITAS
        Speaker: Savvas Koushiappas
        Slides
      • 11:25
        Cold Dark Matter vs Galactic Dynamics 25m
        Speaker: Matthew Walker
        Slides
    • 11:50 16:30
      Break 4h 40m Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 16:30 17:30
      Physics Cafe Wheeler Opera House

      Wheeler Opera House

      Conveners: Kimberly Palladino, Risa Wechsler
    • 17:30 19:00
      Public Lecture Wheeler Opera House

      Wheeler Opera House

      • 17:30
        Searching for Dark Matter 1h
        Speaker: Jim Peebles
    • 08:00 09:15
      Direct Detection: 3 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 08:00
        DAMA/LIBRA 25m
        Speaker: Periluigi Belli
        Slides
      • 08:25
        KIMS 25m
        Speaker: Youngduk Kim
        Slides
      • 08:50
        DM-ICE 25m
        Speaker: Reina Maruyama
        Slides
    • 09:15 09:45
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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 09:45 11:00
      Indirect Detection: 3 Flug Forum

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      700 W. Gillespie Street Aspen, CO 81611
    • 11:00 16:30
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      700 W. Gillespie Street Aspen, CO 81611
    • 16:30 17:45
      Theory-Pheno: 3 Flug Forum

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      700 W. Gillespie Street Aspen, CO 81611
      • 16:30
        The Search for Dark Matter Debris 25m
        Speaker: Mariangela Lisanti
        Slides
      • 16:55
        Flavored Dark Matter: Direct Detection and Collider Signals 25m
        I consider theories where the dark matter particle carries flavor quantum numbers, and has renormalizable contact interactions with the Standard Model fields. The phenomenology of this scenario depends sensitively on whether dark matter carries lepton flavor, quark flavor or its own internal flavor quantum numbers. I show that each of these possibilities is associated with a characteristic type of vertex, has different implications for direct detection experiments and gives rise to distinct collider signatures. The region of parameter space where dark matter has the right abundance to be a thermal relic is shown to be within reach of current direct detection experiments. I focus on a class of models where dark matter carries tau flavor, and show that the collider signals of these models include events with four or more isolated leptons and missing energy. A full simulation of the signal and backgrounds, including detector effects, shows that in a significant part of parameter space these theories can be discovered above Standard Model backgrounds at the Large Hadron Collider.
        Speaker: Zacharia Chacko
        Slides
      • 17:20
        Dark Dynamics in Theory Space and Their Signals in Anomaly Space 25m
        Speaker: Neal Weiner
        Slides
    • 17:45 18:15
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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 18:15 19:30
      Indirect Detection: 4 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 18:15
        IceCube + Neutrino Searches 25m
        Speaker: Carsten Rott
        Slides
      • 18:40
        HAWC 25m
        Speaker: John Pretz
        Slides
      • 19:05
        AMS-02 25m
        Speaker: Andrei Kounine
        Slides
    • 19:30 21:00
      Conference Dinner Aspen Meadows

      Aspen Meadows

    • 08:00 09:15
      Direct Detection: 4 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 08:00
        Axion Overview 25m
        Speaker: David Tanner
        Slides
      • 08:25
        ADMX 25m
        Speaker: Gianpaolo Carosi
        Slides
      • 08:50
        CAST 25m
        Speaker: Jaime Ruz Armendariz
        Slides
    • 09:15 09:45
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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 09:45 11:00
      Theory-Pheno: 4 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 09:45
        Probing dark matter streams with direct detection experiments 25m
        Speaker: Aravind Natarajan
        Slides
      • 10:10
        Beyond Collisionless Dark Matter 25m
        Self-interacting dark matter has been proposed to solve small scale structure problems. In this talk, we will present a simple and generic self-interacting dark matter model where dark matter particles interact through a sub-GeV force carrier. We show that the simple model can accommodate all astrophysical bounds on self-interactions in dark matter halos and explain the observed relic density, through a single coupling constant.
        Speaker: Hai-bo Yu
        Slides
      • 10:35
        Beyond CDM: The Cosmology of Atomic Dark Matter 25m
        Speaker: Francis-Yan Cyr-Racine
        Slides
    • 11:00 16:30
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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 16:30 17:45
      Theory-Pheno: 5 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 16:30
        An Unexpected Journey: The Implications of the Detection of Continuum Energy Gamma-rays Consistent with Dark Matter Annihilation in the Galactic Center 25m
        It has been known for some time that the center of the Milky Way Galaxy would be the most luminous source of gamma-ray photons from dark matter annihilation. Our recent work shows that observations by the Fermi Gamma-ray Space Telescope reveal that Galactic Center (GC) has a source with large luminosity and high statistical significance that is consistent with extended emission from dark matter annihilation in three ways: (1) its spatial morphology is consistent with that expected from numerical simulations; (2) its luminosity is consistent with the expected thermal-production dark matter annihilation rate; and (3) its energy spectrum is consistent with annihilation into standard model quark channels for weak-scale dark matter particle masses. The very crowded region of the GC also harbors a high density of other astrophysical high-energy sources, including millisecond pulsars, that could mimic this signal. I will discuss the details of the observation, its several interpretations, its implications, and the potential future resolution of the nature of this source.
        Speaker: Kevork Abazajian
        Slides
      • 16:55
        Bubbles And Bumps: Disentangling Two Spectral Components In The Fermi Bubbles 25m
        Speaker: Tracy Slatyer
        Slides
      • 17:20
        Aspects of Iso-spin violating dark matter 25m
        Speaker: Danny Marfatia
        Slides
    • 17:45 18:15
      Break 30m Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 18:15 19:30
      Indirect Detection: 5 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 18:15
        Light dark matter: motivation, theory, ongoing search 25m
        I will review the motivation, the models, and some astrophysical clues for dark matter in the keV mass range, including sterile neutrinos and string/supersymmetry moduli. I will also discuss the results of an ongoing search for this form of dark matter using dedicated observations on all three X-ray telescopes: Chandra, Suzaku, and XMM-Newton.
        Speaker: Alex Kusenko
        Slides
      • 18:40
        Local Dark Matter Density 25m
        Speaker: Jo Bovy
        Slides
      • 19:05
        Tidal streams 25m
        Speaker: Raymond Carlberg
        Slides
    • 08:00 09:15
      Direct Detection: 5 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 08:00
        COUPP 25m
        Speaker: Russell Neilson
        Slides
      • 08:25
        PandaX 25m
        Speaker: Scott Stephenson
        Slides
      • 08:50
        DM-TPC 25m
        Speaker: James Battat
        Slides
    • 09:15 09:45
      Break 30m Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 09:45 11:00
      Indirect Detection: 6 Flug Forum

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      700 W. Gillespie Street Aspen, CO 81611
      • 09:45
        The Quest for Dark Matter Signals and the gamma-ray sky: the low energy window 25m
        To uncover the dark matter, to connect what is astrophysically observed to what will be seen as new particles produced in the LHC, we need new measurements. The Fermi Large Area Telescope is providing the measurements of high energy cosmic ray electrons, positrons and gammas with unprecedented accuracy. These measurements represent a unique probe for studying the origin and diffusive propagation of cosmic rays as well as for looking for possible evidences of Dark Matter. I will review recent results and future experiments at high energies (like CTA) and the plans to cover the low energy range between 10 and 50 MeV.
        Speaker: Aldo Morselli
        Slides
      • 10:10
        CTA 25m
        Speaker: Matthew Wood
        Slides
      • 10:35
        Dark Matter Search Perspectives with Gamma-400 25m
        Speaker: Alex Moiseev
        Slides
    • 11:00 16:30
      Break 5h 30m Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 16:30 17:55
      Theory-Pheno: 6 Flug Forum

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      700 W. Gillespie Street Aspen, CO 81611
      • 16:30
        Axion, WIMP and collider search complementarity 25m
        Speaker: Howie Baer
        Slides
      • 16:55
        Dark Matter at Colliders 25m
        Speaker: Lian-Tao Wang
        Slides
      • 17:20
        ATLAS 35m
        Speaker: Daniel Whiteson
        Slides
    • 17:55 18:15
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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
    • 18:15 19:30
      Direct Detection: 6 Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 18:15
        DEAP/CLEAN 25m
        Speaker: Kimberly Palladino
        Slides
      • 18:40
        Future with Liquid Noble Detectors 25m
        Speaker: Dan McKinsey
        Slides
      • 19:05
        Future with Solid State Devices 25m
        Speaker: Richard Schnee
        Slides
    • 08:30 09:50
      Collider Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 08:30
        Axions and Radio Telescopes 20m
        Speaker: Peter Quinn
        Slides
      • 08:50
        Dark matter searches at CMS 35m
        This presentation will summarize the results of dark matter searches in 5 ifb of proton-proton collision data at the center-of-mass energy 7 TeV collected with the CMS detector at Large Hadron Collider (LHC) in 2011. Dark matter particles, if produced in the collision, will be invisible to the CMS detector; their existence can be inferred by a large missing transverse momentum (MET). Supersymmetric (SUSY) models predict the existence of dark matter candidate particles. This presentation will show interpretations of the CMS SUSY searches in terms of Constrained minimum Supersymmetric extension of the Standard Model (CMSSM) and Simplified Model Spectra (SMS) with an emphasis on dark matter searches. Events with large MET and a single jet (monojet events) or events with large MET and a single photon (mono-photon events) can be final states of direct productions of dark matter particles after the initial-state radiation (ISR). This presentation will also show the upper limits on the dark matter-nucleon cross sections that the CMS monojet and mono-photon analyses placed.
        Speaker: Tai Sakuma
        Slides
      • 09:25
        Search for dark matter and dark forces at BaBar 25m
        Recent astrophysical observations have motivated interest in models with a dark sector with GeV-scale gauge and Higgs bosons. In such models, dark-sector photons typically mix with the standard-model photon, enabling their detection in e+e- collisions at BABAR, with very little background in some of the channels. We present searches for a dark-sector photon and a dark-sector Higgs boson and set stringent limits on the parameters of the model. Our limits on the SM-dark sector mixing parameter are tighter than previous limits by up to two orders of magnitude, depending on the masses of the dark Higgs and dark boson.
        Speaker: Bertrand Echenard
        Slides
    • 09:50 10:40
      Closing Flug Forum

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      Aspen Center for Physics

      700 W. Gillespie Street Aspen, CO 81611
      • 09:50
        Conference Highlights and Summary 35m
        Speaker: Bernard Sadoulet
        Slides