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Related papers: Dark matter directional detection with MIMAC

200 papers

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…

Cosmology and Nongalactic Astrophysics · Physics 2014-12-11 Ciaran A. J. O'Hare , Anne M. Green

We study the possibility of identifying dark matter properties from direct (XENON100) and indirect (GLAST) detection experiments. In the same way, we examine the perspectives given by the next generation of colliders (ILC). All this…

High Energy Physics - Phenomenology · Physics 2008-05-16 Nicolas Bernal

Understanding the ability to measure and discriminate particle events at the lowest possible energy is an essential requirement in developing new experiments to search for weakly interacting massive particle (WIMP) dark matter. In this…

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

We report a systematic study on the directional sensitivity of a direct dark matter detector that detects the polar angle of a recoiling nucleus. A weakly interacting massive particle (WIMP)-mass independent method is used to obtain the…

High Energy Physics - Phenomenology · Physics 2015-09-02 Jin Li

Direct dark matter searches are promising techniques to identify the nature of dark matter particles. I describe the future of this field of research, focussing on the question of what can be achieved in the next decade. I will present the…

Instrumentation and Methods for Astrophysics · Physics 2012-12-04 Laura Baudis

Cosmological observations and the dynamics of the Milky Way provide ample evidence for an invisible and dominant mass component. This so-called dark matter could be made of new, colour and charge neutral particles, which were…

Instrumentation and Methods for Astrophysics · Physics 2014-08-20 Laura Baudis

Astrophysical and cosmological observations suggest the existence of beyond standard model ingredient known as dark matter (DM). One of the most supported class of theories suggests that DM is composed of weakly interactive massive…

Instrumentation and Detectors · Physics 2025-07-04 Giorgio Dho

Over the past decades, several ideas and technologies have been developed to directly detect WIMP from the galactic halo. All these detection strategies share the common goal of discriminating a WIMP signal from the residual backgrounds. By…

Instrumentation and Detectors · Physics 2015-06-23 J. Billard

Dark Matter experiments are recently focusing their detection techniques in low-mass WIMPs, which requires the use of light elements and low energy threshold. In this context, we present the TREX-DM experiment, a low background…

Weakly Interacting Massive Particles (WIMPs) are leading candidates for the dominant part of the mass density of the Universe. Here we will review direct WIMP detection techniques by giving examples of currently running experiments, and…

Astrophysics · Physics 2007-05-23 Laura Baudis , H. V. Klapdor-Kleingrothaus

We explore the ability of directional nuclear-recoil detectors to constrain the local velocity distribution of weakly interacting massive particle (WIMP) dark matter by performing Bayesian parameter estimation on simulated recoil-event data…

Cosmology and Nongalactic Astrophysics · Physics 2012-05-04 Samuel K. Lee , Annika H. G. Peter

Directional detection is a promising Dark Matter search strategy. Even though it could accommodate to a sizeable background contamination, electron/recoil discrimination remains a key and challenging issue as for direction-insensitive…

Instrumentation and Methods for Astrophysics · Physics 2015-06-05 J. Billard , F. Mayet , D. Santos

Searches for WIMP dark matter will in the near future be sensitive to solar neutrinos. Directional detection offers a method to reject solar neutrinos and improve WIMP searches, but reaching that sensitivity with existing directional…

Instrumentation and Detectors · Physics 2021-03-05 Mason C. Marshall , Matthew J. Turner , Mark J. H. Ku , David F. Phillips , Ronald L. Walsworth

The potentialities of MIMAC-He3, a MIcro-tpc MAtrix of Chambers of Helium 3, for supersymmetric dark matter search are discussed within the framework of effective MSSM models without gaugino mass unification at the GUT scale. A…

Astrophysics · Physics 2011-07-19 E. Moulin , F. Mayet , D. Santos

The nature of dark matter is still an open problem, but there is evidence that a large part of the dark matter in the universe is non-baryonic, non-luminous and non-relativistic and hypothetical Weakly Interacting Massive Particles (WIMPs)…

Instrumentation and Detectors · Physics 2009-07-03 Ionel Lazanu , Sorina Lazanu

The Time Projection Chamber (TPC) has been recognized as a potentially powerful detector for the search of WIMPs by measuring the directions of nuclear recoils, in which the most convincing signature of WIMPs, caused by the Earth's motion…

The Dark Matter Time Projection Chamber (DMTPC) collaboration is developing a low pressure gas TPC for detecting Weakly Interacting Massive Particle (WIMP)-nucleon interactions. Optical readout with CCD cameras allows for the detection of…

The measurement of the direction of WIMP-induced nuclear recoils is a compelling but technologically challenging strategy to provide an unambiguous signature of the detection of Galactic dark matter. Most directional detectors aim to…

Multiply-interacting massive particles (MIMPs) are heavy (>10^10 GeV/c^2) dark matter particles that interact strongly with regular matter, but may have evaded detection due to the low number density required to make up the local dark…

High Energy Physics - Phenomenology · Physics 2022-01-12 Michael Clark , Amanda Depoian , Bahaa Elshimy , Abigail Kopec , Rafael F. Lang , Shengchao Li , Juehang Qin
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