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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

We revisit the simplest model for dark matter. In this context the dark matter candidate is a real scalar field which interacts with the Standard Model particles through the Higgs portal. We discuss the relic density constraints as well as…

高能物理 - 唯象学 · 物理学 2016-06-29 Michael Duerr , Pavel Fileviez Perez , Juri Smirnov

We attempt to estimate the uncertainty in the constraints on the spin independent dark matter-nucleon cross section due to our lack of knowledge of the dark matter phase space in the galaxy. We fit the density of dark matter before…

宇宙学与河外天体物理 · 物理学 2015-06-05 Malcolm Fairbairn , Tom Douce , Jace Swift

We consider the prospects for multiple dark matter direct detection experiments to determine if the interactions of a dark matter candidate are isospin-violating. We focus on theoretically well-motivated examples of isospin-violating dark…

高能物理 - 唯象学 · 物理学 2018-03-09 Chris Kelso , Jason Kumar , Danny Marfatia , Pearl Sandick

In this paper we complete formulae for the elastic cross section of general vector dark matter with nucleon in the direct detection at the leading order of the strong coupling constant, assuming that the dark matter is composed of vector…

高能物理 - 唯象学 · 物理学 2015-09-08 Junji Hisano , Koji Ishiwata , Natsumi Nagata , Masato Yamanaka

We propose new concepts for experiments in which intense high energy photon or muon beams are employed parasitically to detect scattering by cosmic heavy weakly interacting dark matter (DM) particles. We show that the scattering…

高能物理 - 唯象学 · 物理学 2026-03-04 A. Acar , M. Bashkanov , D. P. Watts

Direct detection of dark matter (DM) requires an interaction of dark matter particles with nucleons. The same interaction can lead to dark matter pair production at a hadron collider, and with the addition of initial state radiation this…

高能物理 - 唯象学 · 物理学 2011-01-05 Yang Bai , Patrick J. Fox , Roni Harnik

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

Owing to its low electronic noise and flexible target materials, the Spherical Proportional Counter (SPC) with a single electron detection threshold can be utilized to search for sub-GeV dark matter (DM). In this work, we investigate the…

高能物理 - 唯象学 · 物理学 2023-09-19 Yuchao Gu , Jie Tang , Lei Wu , Bin Zhu

Direct searches for light dark matter particles (mass $<10$ GeV) are especially challenging because of the low energies transferred in elastic scattering to typical heavy nuclear targets. We investigate the possibility of using liquid…

天体物理仪器与方法 · 物理学 2015-06-12 Wei Guo , Daniel N. McKinsey

Dark matter (DM) direct detection experiments which are directionally-sensitive may be the only method of probing the full velocity distribution function (VDF) of the Galactic DM halo. We present an angular basis for the DM VDF which can be…

高能物理 - 唯象学 · 物理学 2015-07-14 Bradley J. Kavanagh

Directional detection is a promising search strategy to discover galactic Dark Matter. We present a Bayesian analysis framework dedicated to Dark Matter phenomenology using directional detection. The interest of directional detection as a…

天体物理仪器与方法 · 物理学 2015-05-30 J. Billard , F. Mayet , D. Santos

Particles weakly interacting with ordinary matter, with an associated mass of the order of an atomic nucleus (WIMPs), are plausible candidates for Dark Matter. The direct detection of an elastic collision of a target nuclei induced by one…

天体物理仪器与方法 · 物理学 2016-08-01 C. Couturier , O. Guillaudin , F. Naraghi , Q. Riffard , D. Santos , N. Sauzet , P. Colas , E. Ferrer Ribas , I. Giomataris , J. Busto , D. Fouchez , C. Tao , N. Zhou

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

We propose a novel dark matter (DM) detection strategy for the models with non-minimal dark sector. The main ingredients in the underlying DM scenario are a boosted DM particle and a heavier dark sector state. The relativistic DM impinged…

高能物理 - 唯象学 · 物理学 2017-10-25 Doojin Kim , Jong-Chul Park , Seodong Shin

Exotic dark matter together with the vacuum energy or cosmological constant seem to dominate in the Universe. An even higher density of such matter seems to be gravitationally trapped in the Galaxy. Thus its direct detection is central to…

高能物理 - 唯象学 · 物理学 2014-11-17 J. D. Vergados

The traditional methods of estimating the Dark Matter (DM) mass scale crucially depend on the assumptions about the interaction mechanism between the DM and the Standard Model (SM) sectors, making it challenging to achieve precise mass…

高能物理 - 唯象学 · 物理学 2025-05-27 Bibhabasu De

We present MadDM v.3.0, a numerical tool to compute particle dark matter observables in generic new physics models. The new version features a comprehensive and automated framework for dark matter searches at the interface of collider…

We propose and experimentally demonstrate a method for detection of light scalar Dark Matter (DM), through probing temporal oscillations of fundamental constants in an atomic optical transition. Utilizing the quantum information notion of…

高能物理 - 唯象学 · 物理学 2021-04-28 Shahaf Aharony , Nitzan Akerman , Roee Ozeri , Gilad Perez , Inbar Savoray , Ravid Shaniv

Direct detection experiments are poised to detect dark matter in the form of weakly interacting massive particles (WIMPs). The signals expected in these experiments depend on the ultra-local WIMP density and velocity distribution. Firstly…

宇宙学与河外天体物理 · 物理学 2012-02-14 Anne M. Green