Showing papers in "Physics of the Dark Universe in 2015"
Academia Sinica1, Imperial College London2, CERN3, École normale supérieure de Lyon4, University of Lyon5, Tel Aviv University6, University of Southampton7, SLAC National Accelerator Laboratory8, Durham University9, University of Melbourne10, Rutgers University11, International School for Advanced Studies12, Chinese Academy of Sciences13, Université libre de Bruxelles14, University of California, Davis15, Vrije Universiteit Brussel16, University of Freiburg17, University of Geneva18, University of Bonn19, King's College London20, University of Maryland, College Park21, University of Oxford22, Argonne National Laboratory23, Fermilab24, University of Grenoble25, University of California, Santa Barbara26, University of Malaya27, University of Oregon28, Harvard University29, Royal Holloway, University of London30, University College London31, Ohio State University32, Texas Tech University33, Brown University34, University of Amsterdam35, University of Chicago36, Rutherford Appleton Laboratory37, University of California, Irvine38, KEK39, University of Glasgow40, University of California, Berkeley41, Lawrence Berkeley National Laboratory42, University of Zurich43, University of Toronto44, University of Oklahoma45, Max Planck Society46, Weizmann Institute of Science47, New York University48, McMaster University49, Perimeter Institute for Theoretical Physics50
TL;DR: In this paper, a set of simplified models for dark matter and its interactions with the Standard Model particles are presented, and the guiding principles underpinning these simplified models are spelled out, and some suggestions for implementation are presented.
318 citations
Imperial College London1, Durham University2, University of Amsterdam3, University of Southampton4, Rutherford Appleton Laboratory5, University of Bristol6, CERN7, SLAC National Accelerator Laboratory8, King's College London9, University of California, Santa Barbara10, Brown University11, Lawrence Berkeley National Laboratory12
TL;DR: In this article, the authors present a concrete proposal for the consistent interpretation of Dark Matter searches at colliders and in direct detection experiments based on a specific implementation of simplified models of vector and axial-vector mediator exchanges.
104 citations
TL;DR: In this paper, the authors applied the z-fiducialization technique to a directional dark matter search and achieved the first background-free operation of a directional detector, achieving a 1.1 pb exclusion curve for spin-dependent WIMP-proton interactions at 100GeV/c2.
91 citations
TL;DR: MadDM v20 as discussed by the authors is a numerical tool for dark matter physics in a generic model and is the next step towards the development of a fully automated framework for dark-matter searches at the interface of collider physics, astro-physics and cosmology.
70 citations
TL;DR: In this article, the authors summarize the many dark matter searches currently being pursued in each of these four approaches and highlight the complementarity of the four general approaches that are required to sustain a vital dark matter research program.
39 citations
TL;DR: In this paper, the authors calculate the expected rate of carbon ions channeled in single-wall nanotubes once extracted by the scattering with a massive dark matter particle, depending on its initial kinematic conditions, the ejected carbon ion may be trapped in the nanotube array or stop in the bulk.
33 citations
TL;DR: In this paper, a dipole moment operator and a small dark sector mass splitting is proposed to explain the gamma-ray excess in the direction of the Galactic Center. But the authors find that the line is suppressed only by the relative scales and couplings.
28 citations
TL;DR: The axion field equations in a voltage-driven Josephson junction environment allow for a nontrivial solution where the axion-induced electrical current manifests itself as an oscillating supercurrent as discussed by the authors.
26 citations
TL;DR: In this article, the power spectra of comoving curvature perturbation and primordial gravitational waves in the FLRW universes with K = + 1 and maximally symmetry spatial sections according to the slowly rolling inflationary scenario were derived.
12 citations
TL;DR: In this article, the theoretical value of the cosmological constant is consistent with its observational value, and the Freidmann-Lama-Robertson-Walker cosmology embedded isometrically in an 11-dimensional ambient is studied.
8 citations