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Hidden photon and axion-like dark matter may be detected using spherical reflective surfaces such as dish antenna setups converting some of the dark matter particles into photons and concentrating them on a detector. These setups may be…

高能物理 - 唯象学 · 物理学 2017-02-16 Joerg Jaeckel , Stefan Knirck

We propose a method to identify the direction of an incident Weakly Interacting Massive Particle (WIMP) via induced nuclear recoil. Our method is based on spectroscopic interrogation of quantum defects in macroscopic solid-state crystals .…

高能物理 - 唯象学 · 物理学 2017-08-23 Surjeet Rajendran , Nicholas Zobrist , Alexander O. Sushkov , Ronald Walsworth , Mikhail Lukin

Among the many experimental techniques available, those providing directional information have the potential of yielding an unambiguous observation of WIMPs even in the presence of insidious backgrounds. A measurement of the distribution of…

天体物理学 · 物理学 2014-11-18 Gabriella Sciolla

Directional detection of WIMPs, in which the energies and directions of the recoiling nuclei are measured, currently presents the only prospect for probing the local velocity distribution of Galactic dark matter. We investigate the extent…

宇宙学与河外天体物理 · 物理学 2014-12-11 Ciaran A. J. O'Hare , Anne M. Green

Velocity distribution of dark matter is supposed to be isotropic Maxwell-Boltzmann distribution in most cases, however, other distribution models including anisotropic one are suggested by simulations. Directional direct detection of dark…

宇宙学与河外天体物理 · 物理学 2019-09-20 Keiko I. Nagao

Directional detection of galactic Dark Matter is a promising search strategy for discriminating geniune WIMP events from background ones. We present technical progress on gaseous detectors as well as recent phenomenological studies,…

Directional detection of Dark Matter particles (DM) in the MeV mass range could be accomplished by studying electron recoils in large arrays of parallel carbon nanotubes. In a scattering process with a lattice electron, a DM particle might…

高能物理 - 唯象学 · 物理学 2018-01-17 G. Cavoto , F. Luchetta , A. D. Polosa

We present the first method to probabilistically predict 3D direction in a deep neural network model. The probabilistic predictions are modeled as a heteroscedastic von Mises-Fisher distribution on the sphere $\mathbb{S}^2$, giving a simple…

数据分析、统计与概率 · 物理学 2024-07-15 Majd Ghrear , Peter Sadowski , Sven Einar Vahsen

The Dark Matter Time Projection Chamber (DMTPC) is a low pressure (75 Torr CF4) 10 liter detector capable of measuring the vector direction of nuclear recoils with the goal of directional dark matter detection. In this paper we present the…

Directional detection of galactic Dark Matter offers a unique opportunity to identify Weakly Interacting Massive Particle (WIMP) events as such. Depending on the unknown WIMP-nucleon cross section, directional detection may be used to :…

宇宙学与河外天体物理 · 物理学 2013-12-30 F. Mayet , J. Billard

Recoil-imaging gaseous time projection chambers (TPCs) with directional sensitivity are attractive for dark matter (DM) searches. Detectors capable of reconstructing 3D nuclear recoil directions would be uniquely sensitive to the predicted…

仪器与探测器 · 物理学 2022-06-23 J. Schueler , M. Ghrear , S. E. Vahsen , P. Sadowski , C. Deaconu

Dark matter with MeV scale mass is difficult to detect with standard direct search detectors. However, they can be searched for by considering the up-scattering of kinetic energies by cosmic rays. Because the dark matter density is higher…

宇宙学与河外天体物理 · 物理学 2023-08-01 Keiko I. Nagao , Satoshi Higashino , Tatsuhiro Naka , Kentaro Miuchi

Details about the velocity distribution of weakly interacting massive particle (WIMP) dark matter in our galaxy may be revealed by nuclear-recoil detectors with directional sensitivity. Previous studies have assumed that the velocity…

宇宙学与河外天体物理 · 物理学 2015-06-18 Samuel K. Lee

Directional detection of nuclear recoils is broadly desirable in nuclear and particle physics. At low recoil energies, this capability may be used to confirm the cosmological origin of a dark matter signal, to penetrate the so-called…

仪器与探测器 · 物理学 2021-10-13 Majd Ghrear , Sven E. Vahsen , Cosmin Deaconu

Now that conventional weakly interacting massive particle (WIMP) dark matter searches are approaching the neutrino floor, there has been a resurgence of interest in detectors with sensitivity to nuclear recoil directions. A large-scale…

We demonstrate a new type of analysis for the DRIFT-IId directional dark matter detector using a machine learning algorithm called a Random Forest Classifier. The analysis labels events as signal or background based on a series of selection…

Weakly Interacting Massive Particles (WIMPs) may constitute most of the matter in the Universe. The ability to detect the directionality of recoil nuclei will considerably facilitate detection of WIMPs. In this paper we propose a novel type…

天体物理仪器与方法 · 物理学 2015-01-13 Andrzej Drukier , Katherine Freese , Alejandro Lopez , David Spergel , Charles Cantor , George Church , Takeshi Sano

A convincing identification of dark matter (DM) particles can probably be achieved only through a combined analysis of different detections strategies, which provides an effective way of removing degeneracies in the parameter space of DM…

高能天体物理现象 · 物理学 2014-11-21 Pasquale D. Serpico , Gianfranco Bertone

We present the case for a dark matter detector with directional sensitivity. This document was developed at the 2009 CYGNUS workshop on directional dark matter detection, and contains contributions from theorists and experimental groups in…

宇宙学与河外天体物理 · 物理学 2014-11-20 S. Ahlen , N. Afshordi , J. B. R. Battat , J. Billard , N. Bozorgnia , S. Burgos , T. Caldwell , J. M. Carmona , S. Cebrian , P. Colas , T. Dafni , E. Daw , D. Dujmic , A. Dushkin , W. Fedus , E. Ferrer , D. Finkbeiner , P. H. Fisher , J. Forbes , T. Fusayasu , J. Galan , T. Gamble , C. Ghag , I. Giomataris , M. Gold , H. Gomez , M. E. Gomez , P. Gondolo , A. Green , C. Grignon , O. Guillaudin , C. Hagemann , K. Hattori , S. Henderson , N. Higashi , C. Ida , F. J. Iguaz , A. Inglis , I. G. Irastorza , S. Iwaki , A. Kaboth , S. Kabuki , J. Kadyk , N. Kallivayalil , H. Kubo , S. Kurosawa , V. A. Kudryavtsev , T. Lamy , R. Lanza , T. B. Lawson , A. Lee , E. R. Lee , T. Lin , D. Loomba , J. Lopez , G. Luzon , T. Manobu , J. Martoff , F. Mayet , B. Mccluskey , E. Miller , K. Miuchi , J. Monroe , B. Morgan , D. Muna , A. St. J. Murphy , T. Naka , K. Nakamura , M. Nakamura , T. Nakano , G. G. Nicklin , H. Nishimura , K. Niwa , S. M. Paling , J. Parker , A. Petkov , M. Pipe , K. Pushkin , M. Robinson , A. Rodriguez , J. Rodriguez-Quintero , T. Sahin , R. Sanderson , N. Sanghi , D. Santos , O. Sato , T. Sawano , G. Sciolla , H. Sekiya , T. R. Slatyer , D. P. Snowden-Ifft , N. J. C. Spooner , A. Sugiyama , A. Takada , M. Takahashi , A. Takeda , T. Tanimori , K. Taniue , A. Tomas , H. Tomita , K. Tsuchiya , J. Turk , E. Tziaferi , K. Ueno , S. Vahsen , R. Vanderspek , J. Vergados , J. A. Villar , H. Wellenstein , I. Wolfe , R. K. Yamamoto , H. Yegoryan

We discuss the relevance of directional detection experiments in the post-discovery era and propose a method to extract the local dark matter phase space distribution from directional data. The first feature of this method is a…

星系天体物理 · 物理学 2016-04-18 Daniele S. M. Alves , Sonia El Hedri , Jay G. Wacker