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相关论文: Implications of a Running Dark Photon Coupling

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We consider indirect detection signals of atomic dark matter, with a massive dark photon which mixes kinetically with hypercharge. In significant regions of parameter space, dark matter remains at least partially ionized today, and dark…

高能物理 - 唯象学 · 物理学 2015-04-29 Lauren Pearce , Kalliopi Petraki , Alexander Kusenko

Dark energy and dark matter are the dominant sources in the evolution of the late universe. They are currently only indirectly detected via their gravitational effects, and there could be a coupling between them without violating…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Christian G. Boehmer , Gabriela Caldera-Cabral , Ruth Lazkoz , Roy Maartens

Results are reported from a search for a class of composite dark matter models with feeble, long-range interactions with normal matter. We search for impulses arising from passing dark matter particles by monitoring the mechanical motion of…

高能物理 - 实验 · 物理学 2020-11-03 Fernando Monteiro , Gadi Afek , Daniel Carney , Gordan Krnjaic , Jiaxiang Wang , David C. Moore

In anomaly-mediated supersymmetry breaking, superpartners in a hidden sector have masses that are proportional to couplings squared, and so naturally freeze out with the desired dark matter relic density for a large range of masses. We…

高能物理 - 唯象学 · 物理学 2014-10-03 Jonathan L. Feng , Vikram Rentala , Ze'ev Surujon

Coupled dark matter-dark energy systems can suffer from non-adiabatic instabilities at early times and large scales. In these proceedings, we consider two parameterizations of the dark sector interaction. In the first one the…

宇宙学与河外天体物理 · 物理学 2014-11-20 L. Lopez Honorez , 0. Mena

We consider a model of dark photon which appears as a result of the successive symmetry breaking SU(2)$\,\to\,$U(1)$\,\to \mathbb{Z}_2$, where various types of topological defects appear in the dark sector. In this paper, we study the…

高能物理 - 唯象学 · 物理学 2023-09-07 Akifumi Chitose , Masahiro Ibe

We identify form-stable coupled excitations of light and matter (``dark-state polaritons'') associated with the propagation of quantum fields in Electromagnetically Induced Transparency. The properties of the dark-state polaritons such as…

量子物理 · 物理学 2009-11-06 M. Fleischhauer , M. D. Lukin

Large composite dark matter states source a scalar binding field that, when coupled to Standard Model nucleons, provides a potential under which nuclei recoil and accelerate to energies capable of ionization, radiation, and thermonuclear…

高能物理 - 唯象学 · 物理学 2022-02-08 Javier F. Acevedo , Joseph Bramante , Alan Goodman

Dark photons that are sufficiently light and/or weakly-interacting represent a compelling vision of dark matter. Dark photon decay into three photons, which we call the dark photon trident, can be the dominant channel when the dark photon…

高能物理 - 唯象学 · 物理学 2025-07-22 Tim Linden , Thong T. Q. Nguyen , Tim M. P. Tait

We study a simple model of vector dark matter that couples to Standard Model particles via magnetic dipole interactions. In this scenario, the cosmological abundance arises through the freeze-in mechanism and depends on the dipole coupling,…

高能物理 - 唯象学 · 物理学 2022-10-14 Gordan Krnjaic , Duncan Rocha , Anastasia Sokolenko

Recently, condensed matter and atomic experiments have reached a length-scale and temperature regime where new quantum collective phenomena emerge. Finding such physics in systems of photons, however, is problematic, as photons typically do…

其他凝聚态物理 · 物理学 2007-08-01 Andrew D. Greentree , Charles Tahan , Jared H. Cole , L. C. L. Hollenberg

We investigate an optomechanical system in which a cavity with a moving mirror is driven by two external fields. When the field frequencies match resonance conditions, we show that there exists a class of dark states of the moving mirror in…

量子物理 · 物理学 2013-06-05 Gao-Feng Xu , C. K. Law

Bulk dark energy properties are determined by the redshift evolution of its pressure-to-density ratio, $w_{de}(z)$. An experimental goal is to decide if the dark energy is dynamical, as in the quintessence (and phantom) models treated here.…

宇宙学与河外天体物理 · 物理学 2011-01-27 Zhiqi Huang , J. Richard Bond , Lev Kofman

We provide a systematic discussion of the phenomenology of Dark Photon iDM (A$^{\prime}$iDM) where the Standard Model (SM) is extended by a dark sector containing an additional $U(1)_D$ gauge symmetry under which all SM particles are…

高能物理 - 唯象学 · 物理学 2026-02-23 Abhishek Roy , Prasenjit Sanyal , Stefano Scopel

Recent work has shown the utility of examining background effects from ultralight dark matter on precision measurements. This effect enhances seemingly benign contributions to the level that experiments are sensitive to them. In this work,…

高能物理 - 唯象学 · 物理学 2024-10-15 Jason L. Evans , Jun-Yuan Lyu

Atmospheric collisions can copiously produce dark sector particles in the invisible dark photon model, leading to detectable signals in underground neutrino detectors. We consider the dark photon model with the mass mixing mechanism and use…

高能物理 - 唯象学 · 物理学 2025-09-11 Mingxuan Du , Rundong Fang , Zuowei Liu , Wenxi Lu , Zicheng Ye

A strongly interacting massive particle (SIMP) is an interesting candidate for dark matter (DM) because its self-interaction cross section can be naturally strong enough to address the astrophysical problem of small-scale structure…

高能物理 - 唯象学 · 物理学 2020-10-14 Ayuki Kamada , Masaki Yamada , Tsutomu T. Yanagida

The absolute stability of a dark matter (DM) particle is not a binding requirement. Here we suggest a few scenarios where the DM particle is liable to decay via extremely feeble interactions. This can happen via inexplicably small Yukawa…

高能物理 - 唯象学 · 物理学 2020-08-31 Laura Covi , Avirup Ghosh , Tanmoy Mondal , Biswarup Mukhopadhyaya

One of the interesting portals linking a dark sector and the standard model (SM) is the kinetic mixing between the SM $U(1)_Y$ field with a new dark photon $A'$ from a $U(1)_{A'}$ gauge interaction. Stringent limits have been obtained for…

高能物理 - 唯象学 · 物理学 2017-09-13 Min He , Xiao-Gang He , Cheng-Kai Huang

We show that an interaction between dark matter and dark energy generically results in an effective dark energy equation of state of w<-1. This arises because the interaction alters the redshift-dependence of the matter density. An observer…

天体物理学 · 物理学 2010-03-26 Subinoy Das , Pier Stefano Corasaniti , Justin Khoury