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Measuring an annual modulation in a direct Dark Matter detection experiment is not only a proof of the existence of WIMPs but can also tell us more about their interaction with standard matter and maybe even their density and velocity in…

仪器与探测器 · 物理学 2019-08-13 Francis Froborg

We experimentally demonstrate optical spectroscopy of magnetically trapped atoms on an atom chip. High resolution optical spectra of individual trapped clouds are recorded within a few hundred milliseconds. Detection sensitivities close to…

量子物理 · 物理学 2008-09-16 A. Günther , H. Bender , A. Stibor , J. Fortágh , C. Zimmermann

Various theories of dark matter predict distinctive astrophysical signatures in gravitational-wave sources that could be observed by ground- and space-based laser interferometers. Different candidates-including axions, dark photons,…

高能天体物理现象 · 物理学 2026-01-01 Andrew L. Miller

The weakly interacting massive particles (WIMPs) have been the most popular particle dark matter (DM) candidate for the last several decades, and it is well known that WIMP can be probed via the direct, indirect and collider experiments.…

高能物理 - 唯象学 · 物理学 2022-03-21 Jia Liu , Xiao-Ping Wang , Ke-Pan Xie

The existence of dark matter as evidenced by numerous indirect observations is one of the most important indications that there must be physics beyond the Standard Model of particle physics. This article reviews the concepts of direct…

宇宙学与河外天体物理 · 物理学 2019-11-26 Marc Schumann

While it is straightforward to count laser-cooled trapped ions by fluorescence imaging, detecting the number of dark ions embedded and sympathetically cooled in a mixed ion crystal is more challenging. We demonstrate a method to track the…

Weakly interacting massive particles (WIMPs) are one of the leading candidates for Dark Matter. So far we can use direct Dark Matter detection to estimate the mass of halo WIMPs only by fitting predicted recoil spectra to future…

高能物理 - 唯象学 · 物理学 2011-11-10 Chung-Lin Shan , Manuel Drees

A weakly interacting massive particle (WIMP) is a leading candidate of the dark matter. The WIMP dark matter abundance is determined by the freeze-out mechanism. Once we know the property of the WIMP particle such as the mass and…

高能物理 - 唯象学 · 物理学 2020-08-19 Ken'ichi Saikawa , Satoshi Shirai

We propose an alternate, calculable mechanism of dark matter genesis, "thermal freeze-in," involving a Feebly Interacting Massive Particle (FIMP) interacting so feebly with the thermal bath that it never attains thermal equilibrium. As with…

高能物理 - 唯象学 · 物理学 2014-11-20 Lawrence J. Hall , Karsten Jedamzik , John March-Russell , Stephen M. West

We present nanoscale explosives as a novel type of dark matter detector and study the ignition properties. When a Weakly Interacting Massive Particle WIMP from the Galactic Halo elastically scatters off of a nucleus in the detector, the…

天体物理仪器与方法 · 物理学 2014-04-15 Alejandro Lopez , Andrzej Drukier , Katherine Freese , Cagliyan Kurdak , Gregory Tarle

Direct detection of WIMP dark matter candidates has to face many difficult challenges. In particular, it requires an extremely high level of background rejection. The only way out seems to be particle identification which, for experiments…

高能物理 - 实验 · 物理学 2007-05-23 Luis Gonzalez-Mestres

Astrophysical observations and cosmological data have led to the conclusion that nearly one quarter of the Universe consists of dark matter. Under certain assumptions, an observable signature of dark matter is the annual modulation of the…

Dark matter candidates comprising several sub-states separated by a small mass gap, and coupled to the Standard Model by (sub-)GeV force carriers, can exhibit non-trivial scattering interactions in direct detection experiments. We analyze…

高能物理 - 唯象学 · 物理学 2009-07-09 Brian Batell , Maxim Pospelov , Adam Ritz

We present a halo-independent analysis of direct detection data on "light WIMPs," i.e. weakly interacting massive particles with mass close to or below 10 GeV/c^2. We include new results from silicon CDMS detectors (bounds and excess…

高能物理 - 唯象学 · 物理学 2015-06-15 Eugenio Del Nobile , Graciela B. Gelmini , Paolo Gondolo , Ji-Haeng Huh

Weakly Interacting Massive Particles (WIMPs) are candidates for non-baryonic Dark Matter. WIMPs are supposed to interact with baryonic matter via scattering off nuclei producing a nuclear recoil with energies up to a few 10 keV with a very…

An ever-increasing body of evidence suggests that weakly interacting massive particles (WIMPs) constitute the bulk of the matter in the Universe. We illustrate how experimental data, dimensional analysis and Standard Model particle physics…

天体物理学 · 物理学 2007-05-23 F. Halzen

The 'WIMP miracle' for the relic abundance of thermal dark matter motivates weak scale dark matter with renormalizable couplings to standard model particles. We study minimal models with such couplings that explain dark matter as a thermal…

高能物理 - 唯象学 · 物理学 2014-01-22 Spencer Chang , Ralph Edezhath , Jeffrey Hutchinson , Markus Luty

Describing experimental signatures of quantum spin ice has been the focus of many theoretical efforts, as definitive experimental verification of this candidate quantum spin liquid is yet to be achieved. Gapped excitations known as visons…

强关联电子 · 物理学 2020-09-16 M. P. Kwasigroch

Utilizing single-photon photoassociation, we have achieved ultracold rubidium molecules with a high number density that provides a new efficient approach toward molecular quantum degeneracy. A new detection mechanism for ultracold molecule…

原子物理 · 物理学 2015-06-12 Jun-Ren Chen , Cheng-Yang Kao , Hung-Bin Chen , Yi-Wei Liu

At present there is an effort to reconcile the results of the DAMA experiment with those from other Dark Matter experiments such as CoGeNT, CRESST, CDMS, and all LXe experiments. The author suggests a new model describing the Dark Matter…

星系天体物理 · 物理学 2016-11-26 J. Va'vra