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Theories unifying gravity and other interactions suggest the possibility of spatial and temporal variation of physical ``constants'' in the Universe. Detection of high-redshift absorption systems intersecting the sight lines towards distant…

原子物理 · 物理学 2009-08-18 V. A. Dzuba , V. V. Flambaum , J. K. Webb.

One of the main problems in Particle Physics is to understand the origin and nature of Dark Matter. An exciting possibility is to consider that the Dark Matter belongs to a new complex but hidden sector. In this paper, we assume the…

高能物理 - 唯象学 · 物理学 2019-05-24 Constanza Callender , Alfonso R. Zerwekh

A direction sensitive dark matter detector using organic crystals is being developed. It exploits the anisotropic scintillation efficiency of organic crystals with respect to the direction of nuclear recoils relative to crystallographic…

天体物理学 · 物理学 2016-12-07 H. Sekiya , M. Minowa , Y. Shimizu , W. Suganuma , Y. Inoue

Ultralight dark matter induces time-dependent perturbations in the spacetime metric, enabling its gravitational direct detection. In this work, we propose using astrometry to detect dark matter. After reviewing the calculation of the metric…

高能物理 - 唯象学 · 物理学 2025-08-06 Jeff A. Dror , Sarunas Verner

Many modern theories predict that the fundamental constants depend on time, position, or the local density of matter. We develop a spectroscopic method for pulsed beams of cold molecules, and use it to measure the frequencies of microwave…

An ultralight scalar field is one of the dark matter candidates. If it couples with Standard Model particles, it oscillates mirrors in gravitational-wave detectors and generates detectable signals. We study the spectra of the signals taking…

高能物理 - 唯象学 · 物理学 2019-12-18 Soichiro Morisaki , Teruaki Suyama

In this Letter we put forward a novel phenomenological paradigm in which particle physics beyond the Standard Model may be tested by radio astronomy if they are related to a first order phase transition in the early Universe. For this type…

高能物理 - 唯象学 · 物理学 2018-06-20 Andrea Addazi , Yi-Fu Cai , Antonino Marciano

We review various issues related to the direct detection of constituents of dark matter, which are assumed to be Weakly Interacting Massive Particles (WIMPs). We specifically consider heavy WIMPs such as: 1) The lightest supersymmetric…

核理论 · 物理学 2017-08-23 J. D. Vergados

In the framework of an nonuniversal $U(1)'$ extension of the standard model, we propose an scalar candidate for cold dark matter which exhibits interactions with ordinary matter through Higgs and gauge bosons. Using limits from low energy…

高能物理 - 唯象学 · 物理学 2014-11-07 R. Martinez , J. Nisperuza , F. Ochoa , J. P. Rubio

Experiments aimed at detecting ultralight dark matter typically rely on resonant effects, which are sensitive to the dark matter mass that matches the resonance frequency. In this study, we investigate the nucleon couplings of ultralight…

高能物理 - 唯象学 · 物理学 2024-07-12 Zitong Xu , Xiaolin Ma , Kai Wei , Yuxuan He , Xing Heng , Xiaofei Huang , Tengyu Ai , Jian Liao , Wei Ji , Jia Liu , Xiao-Ping Wang , Dmitry Budker

Exotic dark matter together with the vacuum energy (associated with the cosmological constant) seem to dominate in the Universe. Thus its direct detection is central to particle physics and cosmology. Supersymmetry provides a natural dark…

天体物理学 · 物理学 2009-11-07 J. D. Vergados

The nature of the dark matter remains a mystery. The possibility of an unstable dark matter particle decaying to invisible daughter particles has been explored many times in the past few decades. Meanwhile, weak gravitational lensing shear…

宇宙学与河外天体物理 · 物理学 2010-12-24 Mei-Yu Wang , Andrew R. Zentner

For nearly 40 years, dark matter has been widely assumed to be cold and collisionless. Cold dark matter models make fundamental predictions for the behavior of dark matter on small (<10 kpc) scales. These predictions include cuspy density…

Current dark matter detection strategies are based on the assumption that the dark matter is a gas of non-interacting particles with a reasonably large number density. This picture is dramatically altered if there are significant self…

高能物理 - 唯象学 · 物理学 2018-12-19 Dorota M Grabowska , Tom Melia , Surjeet Rajendran

While the direct detection of the dark-matter particle remains very challenging, the nature of dark matter could be possibly constrained by comparing the observed abundance and properties of small-scale sub-galactic mass structures with…

星系天体物理 · 物理学 2023-05-17 D. Bayer , L. V. E. Koopmans , J. P. McKean , S. Vegetti , T. Treu , C. D. Fassnacht , K. Glazebrook

The observed accelerating universe indicates the presence of Dark Energy which is probably interpreted in terms of an extremely light gravitational scalar field. We suggest a way to probe this scalar field which contributes to optical…

广义相对论与量子宇宙学 · 物理学 2011-11-03 Yasunori Fujii , Kensuke Homma

We propose new signals for the direct detection of ultralight dark matter such as the axion. Axion or axion like particle (ALP) dark matter may be thought of as a background, classical field. We consider couplings for this field which give…

高能物理 - 唯象学 · 物理学 2013-09-11 Peter W. Graham , Surjeet Rajendran

Inelastic dark matter reconciles the DAMA anomaly with other null direct detection experiments and points to a non-minimal structure in the dark matter sector. In addition to the dominant inelastic interaction, dark matter scattering may…

高能物理 - 唯象学 · 物理学 2015-03-13 Mariangela Lisanti , Jay G. Wacker

Recent high-quality observations of dwarf and low surface brightness (LSB) galaxies have shown that their dark matter (DM) halos prefer flat central density profiles. On the other hand the standard cold dark matter model simulations predict…

星系天体物理 · 物理学 2021-02-17 T. Matos , Victor H. Robles

We propose a search for low mass dark matter particles through momentum recoils caused by their scattering from trapped, nm-scale objects. Our projections show that even with a modest array of fg-mass sensors, parameter-space beyond the…

仪器与探测器 · 物理学 2022-03-10 Gadi Afek , Daniel Carney , David C. Moore