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Related papers: Directional Dark Matter Search and Velocity Distri…

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Direct detection experiments aim at the detection of dark matter in the form of weakly interacting massive particles (WIMPs) by searching for signals from elastic dark matter nucleus scattering. Additionally, inelastic scattering in which…

High Energy Physics - Phenomenology · Physics 2020-01-08 G. Arcadi , C. Döring , C. Hasterok , S. Vogl

We study the distribution of dark matter in dwarf spheroidal galaxies by modelling the moments of their line-of-sight velocity distributions. We discuss different dark matter density profiles, both cuspy and possessing flat density cores.…

Astrophysics · Physics 2009-11-07 Ewa L. Lokas

Dark matter detectors with directional sensitivity have the capability to distinguish dark matter induced nuclear recoils from isotropic backgrounds, thus providing a smoking gun signature for dark matter in the Galactic halo. Motivated by…

Instrumentation and Detectors · Physics 2019-07-05 Shang-Yung Wang

In this paper we review the theoretical issues involved in the direct detection of supersymmetric (SUSY) dark matter. After a brief discussion of the allowed SYSY parameter space we focus on the determination of the traditional neutralino…

Astrophysics · Physics 2007-05-23 J. D. Vergados

The magnetic inelastic dark matter (MiDM) model, in which dark matter inelastically scatters off nuclei through a magnetic dipole interaction, has previously been shown to reconcile the DAMA/LIBRA annual modulation signal with null results…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 Tongyan Lin , Douglas P. Finkbeiner

Dynamical dark matter (DDM) is an alternative framework for dark-matter physics in which the dark-matter candidate is an ensemble of constituent fields with differing masses, lifetimes, and cosmological abundances. In this framework, it is…

High Energy Physics - Phenomenology · Physics 2013-05-30 Keith R. Dienes , Jason Kumar , Brooks Thomas

Next-generation dark matter direct detection experiments will explore several orders of magnitude in the dark matter--nucleus scattering cross section below current upper limits. In case a signal is discovered the immediate task will be to…

High Energy Physics - Phenomenology · Physics 2019-10-14 Juan Herrero-Garcia , Yannick Müller , Thomas Schwetz

The measurement of an annual modulation in the event rate of direct dark matter detection experiments is a powerful tool for dark matter discovery. Indeed, several experiments have already claimed such a discovery in the past decade. While…

Cosmology and Nongalactic Astrophysics · Physics 2020-05-05 Francis Froborg , Alan R Duffy

Measurement of the direction of the elastic nuclear recoil track and ionization charge distribution along it, gives unique possibility for unambiguous detection of the dark matter WIMP particle. Within current radiation detection…

Instrumentation and Detectors · Physics 2017-08-23 N. J. C. Spooner , P. Majewski

Driven by the null results in the searches for dark matter, the field of direct dark matter detection is constantly evolving to push new frontiers. Ultimately, a vast parameter space for dark matter masses below a few GeV is yet to be…

High Energy Physics - Experiment · Physics 2025-12-18 Melih Solmaz

The future of direct terrestrial WIMP detection lies on two fronts: new, much larger low background detectors sensitive to energy deposition, and detectors with directional sensitivity. The former can large range of WIMP parameter space…

Astrophysics · Physics 2008-11-26 Craig J. Copi , Lawrence M. Krauss , David Simmons-Duffin , Steven R. Stroiney

Non-baryonic, or "dark," matter is believed to be a major component of the total mass budget of the universe. We review the candidates for particle dark matter and discuss the prospects for direct detection (via interaction of dark matter…

Astrophysics · Physics 2008-11-26 Gianfranco Bertone , David Merritt

Indirect detection is the search for the particle nature of dark matter with astrophysical probes. Manifestly, it exists right at the intersection of particle physics and astrophysics, and the discovery potential for dark matter can be…

High Energy Physics - Phenomenology · Physics 2018-05-21 Nicholas L. Rodd

We explore systematic biases in the identification of dark matter in future direct detection experiments and compare the reconstructed dark matter properties when assuming a self-consistent dark matter distribution function and the standard…

Cosmology and Nongalactic Astrophysics · Physics 2013-02-27 Miguel Pato , Louis E. Strigari , Roberto Trotta , Gianfranco Bertone

Directional detection of non-baryonic Dark Matter is a promising search strategy for discriminating WIMP events from background. However, this strategy requires both a precise measurement of the energy down to a few keV and 3D…

Dark matter candidates such as weakly-interacting massive particles are predicted to annihilate or decay into Standard Model particles leaving behind distinctive signatures in gamma rays, neutrinos, positrons, antiprotons, or even…

High Energy Astrophysical Phenomena · Physics 2017-06-01 Jan Conrad , Olaf Reimer

The dark matter directional detection opens a new field in cosmology bringing the possibility to build a map of nuclear recoils that would be able to explore the galactic dark matter halo giving access to a particle characterization of such…

Recoil imaging entails the detection of spatially resolved ionization tracks generated by particle interactions. This is a highly sought-after capability in many classes of detector, with broad applications across particle and astroparticle…

Instrumentation and Detectors · Physics 2022-07-19 C. A. J. O'Hare , D. Loomba , K. Altenmüller , H. Álvarez-Pol , F. D. Amaro , H. M. Araújo , D. Aristizabal Sierra , J. Asaadi , D. Attié , S. Aune , C. Awe , Y. Ayyad , E. Baracchini , P. Barbeau , J. B. R. Battat , N. F. Bell , B. Biasuzzi , L. J. Bignell , C. Boehm , I. Bolognino , F. M. Brunbauer , M. Caamaño , C. Cabo , D. Caratelli , J. M. Carmona , J. F. Castel , S. Cebrián , C. Cogollos , D. Collison , E. Costa , T. Dafni , F. Dastgiri , C. Deaconu , V. De Romeri , K. Desch , G. Dho , F. Di Giambattista , D. Díez-Ibáñez , G. D'Imperio , B. Dutta , C. Eldridge , S. R. Elliott , A. C. Ezeribe , A. Fava , T. Felkl , B. Fernández-Domínguez , E. Ferrer Ribas , K. J. Flöthner , M. Froehlich , J. Galán , J. Galindo , F. García , J. A. García Pascual , B. P. Gelli , M. Ghrear , Y. Giomataris , K. Gnanvo , E. Gramellini , G. Grilli Di Cortona , R. Hall-Wilton , J. Harton , S. Hedges , S. Higashino , G. Hill , P. C. Holanda , T. Ikeda , I. G. Irastorza , P. Jackson , D. Janssens , B. Jones , J. Kaminski , I. Katsioulas , K. Kelly , N. Kemmerich , E. Kemp , H. B. Korandla , H. Kraus , A. Lackner , G. J. Lane , P. M. Lewis , M. Lisowska , G. Luzón , W. A. Lynch , G. Maccarrone , K. J. Mack , P. A. Majewski , R. D. P. Mano , C. Margalejo , D. Markoff , T. Marley , D. J. G. Marques , R. Massarczyk , G. Mazzitelli , C. McCabe , L. J. McKie , A. G. McLean , P. C. McNamara , Y. Mei , A. Messina , A. F. Mills , H. Mirallas , K. Miuchi , C. M. B. Monteiro , M. R. Mosbech , H. Muller , H. Natal da Luz , K. D. Nakamura , A. Natochii , T. Neep , J. L. Newstead , K. Nikolopoulos , L. Obis , E. Oliveri , G. Orlandini , A. Ortiz de Solórzano , J. von Oy , T. Papaevangelou , O. Pérez , Y. F. Perez-Gonzalez , D. Pfeiffer , N. S. Phan , S. Piacentini , E. Picatoste Olloqui , D. Pinci , S. Popescu , A. Prajapati , F. S. Queiroz , J. L. Raaf , F. Resnati , L. Ropelewski , R. C. Roque , E. Ruiz-Choliz , A. Rusu , J. Ruz , J. Samarati , E. M. Santos , J. M. F. dos Santos , F. Sauli , L. Scharenberg , T. Schiffer , S. Schmidt , K. Scholberg , M. Schott , J. Schueler , L. Segui , H. Sekiya , D. Sengupta , Z. Slavkovska , D. Snowden-Ifft , P. Soffitta , M. van Stenis , N. J. C. Spooner , L. Strigari , A. E. Stuchbery , X. Sun , S. Torelli , E. G. Tilly , A. W. Thomas , T. N. Thorpe , P. Urquijo , A. Utrobičić , S. E. Vahsen , R. Veenhof , J. K. Vogel , A. G. Williams , M. H. Wood , J. Zettlemoyer

Although many astrophysical and cosmological observations point towards the existence of Dark Matter (DM), the nature of the DM particle has not been clarified to date. In this paper, we investigate a minimal model with a vector DM (VDM)…

High Energy Physics - Phenomenology · Physics 2020-01-08 S. Glaus , M. Mühlleitner , J. Müller , S. Patel , R. Santos

Understanding the nature of dark matter is among the top priorities of modern physics. However, due to its inertness, detecting and studying it directly in terrestrial experiments is extremely challenging. Numerical N-body simulations…

Astrophysics of Galaxies · Physics 2024-03-06 Zhen Li , Steen H. Hansen