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A low pressure time projection chamber for the detection of WIMPs is discussed. Discrimination against Compton electron background in such a device should be very good, and directional information about the recoil atoms would be obtainable.…

天体物理学 · 物理学 2007-05-23 M. J. Lehner , K. Griest , C. J. Martoff , G. E. Masek , T. Ohnuki , D. Snowden-Ifft , N. J. C. Spooner

Directional detection is a promising search strategy to discover galactic Dark Matter. Taking advantage on the rotation of the Solar system around the Galactic center through the Dark Matter halo, it allows to show a direction dependence of…

宇宙学与河外天体物理 · 物理学 2010-09-14 J. Billard , F. Mayet , D. Santos

Weakly Interacting Massive Particle (WIMP) direct detection experiments are just reaching the sensitivity required to detect Galactic dark matter in the form of neutralinos (or indeed any stable weakly interacting particle). Detection…

天体物理学 · 物理学 2007-05-23 Anne M Green

The direction dependence of the WIMP direct detection rate provides a powerful tool for distinguishing a WIMP signal from possible backgrounds. We study the the number of events required to discriminate a WIMP signal from an isotropic…

天体物理学 · 物理学 2009-11-13 Ben Morgan , Anne M. Green

Next-generation dark matter (DM) detectors searching for weakly interacting massive particles (WIMPs) will be sensitive to coherent scattering from solar neutrinos, demanding an efficient background-signal discrimination tool. Directional…

New techniques for the laboratory direct detection of dark matter weakly interacting massive particles (WIMPs) are sensitive to the recoil direction of the struck nuclei. We compute and compare the directional recoil rates…

天体物理学 · 物理学 2008-11-26 Moqbil S. Alenazi , Paolo Gondolo

Directional detection can provide unambiguous observation of Dark Matter interactions even in presence of insidious backgrounds. The DM-TPC collaboration is developing a detector with the goal of measuring the direction and sense of nuclear…

Present and planned dark matter detection experiments search for WIMP-induced nuclear recoils in poorly known background conditions. In this environment, the maximum gap statistical method provides a way of setting more sensitive cross…

天体物理学 · 物理学 2008-11-26 Shawn Henderson , Jocelyn Monroe , Peter Fisher

Directional detection is a promising direct Dark Matter (DM) search strategy. The angular distribution of the nuclear recoil tracks from WIMP events should present an anisotropy in galactic coordinates. This strategy requires both a…

Directional detection can provide unambiguous observation of Dark Matter interactions even in presence of insidious backgrounds. The DM-TPC collaboration is developing a detector with the goal of measuring the direction and sense of nuclear…

The direction dependence of the event rate in WIMP direct detection experiments provides a powerful tool for distinguishing WIMP events from potential backgrounds. We use a variety of (non-parametric) statistical tests to examine the number…

天体物理学 · 物理学 2010-11-19 Ben Morgan , Anne M. Green , Neil J. C. Spooner

There is a worldwide effort toward the development of a large TPC (Time Projection Chamber) devoted to directional Dark Matter detection. All current projects are being designed to fulfill a unique goal : identifying weakly interacting…

宇宙学与河外天体物理 · 物理学 2012-04-12 J. Billard , F. Mayet , D. Santos

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…

宇宙学与河外天体物理 · 物理学 2012-05-04 Samuel K. Lee , Annika H. G. Peter

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,…

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…

天体物理仪器与方法 · 物理学 2012-12-04 Laura Baudis

Distinguishing the signals due to scattering of WIMP dark matter off of nuclear targets from those due to background noise is a major challenge. The Earth's motion relative to the galactic halo should produce halo-dependent seasonal…

高能物理 - 唯象学 · 物理学 2009-10-31 Craig J. Copi , Junseong Heo , Lawrence M. Krauss

In this paper, as the third part of the third step of our study on developing data analysis procedures for using 3-dimensional information offered by directional direct Dark Matter detection experiments in the future, we introduce a…

高能天体物理现象 · 物理学 2021-03-15 Chung-Lin Shan

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

A generic weakly interacting massive particle (WIMP) is one of the most attractive candidates to account for the cold dark matter in our Universe, since it would be thermally produced with the correct abundance to account for the observed…

宇宙学与河外天体物理 · 物理学 2021-10-13 David G. Cerdeno , Anne M. Green

Directional detection is a promising Dark Matter search strategy. Indeed, WIMP-induced recoils present a direction dependence toward the Cygnus constellation, while background-induced recoils exhibit an isotropic distribution in the…

宇宙学与河外天体物理 · 物理学 2015-05-27 J. Billard , F. Mayet , C. Grignon , D. Santos