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Hints of direct dark matter detection coming from the DAMA, CoGeNT experiments point toward light dark matter with isospin-violating and possibly inelastic couplings. However an array of astrophysical constraints are rapidly closing the…

高能物理 - 唯象学 · 物理学 2015-05-30 James M. Cline , Andrew R. Frey

Supersymmetry can explain the observed dark matter relic density with a neutralino dark matter particle and a coannihilating, almost mass-degenerate sparticle. If this were the case in nature, a linear electron positron collider like the…

高能物理 - 唯象学 · 物理学 2016-02-29 Suvi-Leena Lehtinen , Mikael Berggren , Jenny List

We propose a new out-of-equilibrium production mechanism of light dark matter: resonance scanning. If the dark matter mass evolved in the early Universe, resonant production may have occurred for a wide range of light dark matter masses…

高能物理 - 唯象学 · 物理学 2021-01-01 Djuna Croon , Gilly Elor , Rachel Houtz , Hitoshi Murayama , Graham White

We study the freeze-in of gravitationally interacting dark matter in extra dimensions. Focusing on a minimal dark matter candidate that only interacts with the SM via gravity in a five-dimensional model we find that a large range of dark…

高能物理 - 唯象学 · 物理学 2023-04-26 Arturo de Giorgi , Stefan Vogl

We consider the possibility of interpreting the recently reported diphoton excess at 750 GeV as a spin-two massive particle (such as a Kaluza-Klein graviton in warped extra-dimensions) which serves as a mediator to Dark Matter via its…

高能物理 - 唯象学 · 物理学 2016-03-07 Chengcheng Han , Hyun Min Lee , Myeonghun Park , Veronica Sanz

We demonstrate that if the dark matter (DM) in the Universe contains multiple components,the interactions between the DM components may induce DM conversions. It is then possible that the lightest DM component with an annihilation cross…

高能物理 - 唯象学 · 物理学 2011-10-11 Ze-Peng Liu , Yue-Liang Wu , Yu-Feng Zhou

We know from cosmological and astrophysical observations that more than 80% of the matter density in the Universe is non-luminous, or dark. This non-baryonic dark matter could be composed of neutral, heavy particles, which were…

天体物理学 · 物理学 2007-11-27 Laura Baudis

Dark and baryonic matter contribute comparable energy density to the present Universe. The dark matter may also be responsible for the cosmic positron/electron excesses. We connect these phenomena with Dirac seesaw for neutrino masses. In…

高能物理 - 唯象学 · 物理学 2009-10-29 Pei-Hong Gu , Utpal Sarkar , Xinmin Zhang

We studied the dilaton cosmology based on Weyl-Scaled induced gravity. The potential of dilaton field is taken as exponential form. An analytical solution of Einstein equation is found. The dilaton can be a candidate for dark energy that…

高能物理 - 理论 · 物理学 2007-05-23 H. Q. Lu , Z. G. Huang , W. Fang , K. F. Zhang

The majority of the matter in the universe is still unidentified and under investigation by both direct and indirect means. Many experiments searching for the recoil of dark-matter particles off target nuclei in underground laboratories…

高能物理 - 唯象学 · 物理学 2015-10-28 Michael Klasen , Martin Pohl , Günter Sigl

Both axion and dark photon dark matter are among the most promising candidates of dark matter. What we know with some confidence is that they exhibit a small velocity distribution $\delta v\lesssim v\sim 10^{-3}$c. In addition, their mass…

高能物理 - 唯象学 · 物理学 2025-08-12 Puxian Wei , Ruifeng Zheng , Qiaoli Yang

According to a scenario in string cosmology, a relic background of light dilatons can be a significant component of the dark matter in the Universe. A new approach of searching for such a dilatonic background by observing Earth's surface…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Sachie Shiomi

Cosmological and astrophysical measurements indicate that the universe contains a large amount of dark matter. A number of weak scale dark matter candidates have been proposed in extensions of the standard model. The potential to discover…

高能物理 - 唯象学 · 物理学 2009-12-17 G. Bélanger

One of the most promising strategies to identify the nature of dark matter consists in the search for new particles at accelerators and with so-called direct detection experiments. Working within the framework of simplified models, and…

We present a novel way of probing non-gravitational dark matter interactions: dark astronomy, which leverages the dark radiation emitted by dissipative dark sectors. If the mediator of the dark matter self interactions is a dark photon with…

宇宙学与河外天体物理 · 物理学 2024-12-11 Gonzalo Alonso-Álvarez , David Curtin

Dark matter is one of the greatest unsolved mysteries in cosmology at the present time. About 80% of the universe's gravitating matter is non-luminous, and its nature and distribution are for the most part unknown. In this paper, we will…

高能物理 - 唯象学 · 物理学 2011-02-01 Katherine Garrett , Gintaras Duda

We explore the viability of laboratory-scale mechanical resonators as detectors for ultralight scalar dark matter. The signal we investigate is an atomic strain due to modulation of the fine structure constant and the lepton mass at the…

天体物理仪器与方法 · 物理学 2020-04-22 Jack Manley , Russell Stump , Dalziel Wilson , Daniel Grin , Swati Singh

We present a new mechanism for producing the correct relic abundance of dark photon dark matter over a wide range of its mass, extending down to $10^{-20}\,\mathrm{eV}$. The dark matter abundance is initially stored in an axion which is…

高能物理 - 唯象学 · 物理学 2019-12-11 Prateek Agrawal , Naoya Kitajima , Matthew Reece , Toyokazu Sekiguchi , Fuminobu Takahashi

Dark matter (DM) is currently searched for with a variety of detection strategies. Accelerator searches are particularly promising, but even if Weakly Interacting Massive Particles (WIMPs) are found at the Large Hadron Collider (LHC), it…

高能物理 - 唯象学 · 物理学 2010-10-13 Gianfranco Bertone , David G. Cerdeno , Mattia Fornasa , Roberto Ruiz de Austri , Roberto Trotta

Cosmological axions/axion-like particles can compose a significant part of dark matter; however, the uncertainty of their mass is large. Here, we propose to search the axions using a cylindrical capacitor, in which the static electric field…

高能物理 - 唯象学 · 物理学 2024-06-21 Wenming Chen , Yu Gao , Qiaoli Yang