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相关论文: Some Properties of Multi-Component Axion Dark Matt…

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A multi-component weakly-interacting dark matter scenario is analyzed, where the candidate dark matter states arise from the $SU(2)_{D}\to Z_{3}^{D}\times Z_{2}^{\text{acc}}$ symmetry breaking triggered by a VEV-developing scalar in the…

高能物理 - 唯象学 · 物理学 2025-05-16 Carlos Alvarado , Alfredo Aranda , Cesar Bonilla , Carlos Ramos Portalatino

We review how axion-like particles (ALPs) naturally emerge in the low-energy effective field theory of string compactifications. We focus on the study of their mass spectrum and couplings, stressing that they depend on the mechanism used to…

高能物理 - 理论 · 物理学 2013-09-27 Michele Cicoli

The baryonic and cold dark matter are reviewed in the context of cosmological models. The theoretical search for the particle candidates is limited by supersymmetric extension of the Standard Model. Generically in such models there are just…

天体物理学 · 物理学 2007-05-23 V. Berezinsky

We present a systematic cosmological study of a universe in which the visible sector is coupled, albeit very weakly, to a hidden sector comprised of its own set of particles and interactions. Assuming that dark matter (DM) resides in the…

高能物理 - 唯象学 · 物理学 2015-03-17 Clifford Cheung , Gilly Elor , Lawrence J. Hall , Piyush Kumar

The Axion is a particle arising from the Peccei-Quinn solution to the strong CP problem. Peccei-Quinn symmetry breaking in the early universe could produce a large number of axions which would still be present today, making the axion a…

宇宙学与河外天体物理 · 物理学 2011-12-07 Dmitry Lyapustin

We show that very compact axion mini-clusters can form in models where axion-like-particle (ALP) dark matter is produced via the kinetic misalignment mechanism, which is well-motivated in pre-inflationary $U(1)$ symmetry breaking scenarios.…

高能物理 - 唯象学 · 物理学 2024-05-06 Cem Eröncel , Géraldine Servant

We introduce and study a model designed to simultaneously shed light on the mysteries connected with Baryogenesis, Dark Matter and Dark Energy. The model describes a self-interacting complex axion field whose imaginary part, a pseudo-scalar…

高能物理 - 理论 · 物理学 2021-04-21 Robert Brandenberger , Jürg Fröhlich

We demonstrate that nuclear magnetic resonance based searches for dark matter (DM) have intrinsic and powerful sensitivity to dark photons and the axion-photon coupling. The reason is conceptually straightforward. An instrument such as…

高能物理 - 唯象学 · 物理学 2025-05-23 Carl Beadle , Sebastian A. R. Ellis , Jacob M. Leedom , Nicholas L. Rodd

The asymmetric dark matter (ADM) scenario can solve the coincidence problem between the baryon and the dark matter (DM) abundance when the DM mass is of ${\cal O}(1)\,$GeV. In the ADM scenarios, composite dark matter is particularly…

高能物理 - 唯象学 · 物理学 2020-02-06 Masahiro Ibe , Shin Kobayashi , Ryo Nagai , Wakutaka Nakano

Despite considerable experimental progress large parts of the axion-like particle (ALP) parameter space remain difficult to probe in terrestrial experiments. In some cases, however, small-scale structure of the ALP dark matter (DM)…

宇宙学与河外天体物理 · 物理学 2020-02-18 Nikita Blinov , Matthew J. Dolan , Patrick Draper

We point out that a well known axion model with an explicit Z(N) symmetry breaking term predicts both dark energy and cold dark matter. We estimate the parameters of this model which fit the observed densities of the dark components of the…

高能物理 - 唯象学 · 物理学 2009-11-10 Pankaj Jain

Nearly all astrophysical and cosmological data point convincingly to a large component of cold dark matter in the Universe. The axion particle, first theorized as a solution to the strong charge-parity problem of quantum chromodynamics, has…

仪器与探测器 · 物理学 2017-01-09 I. Stern

An ultralight scalar boson with mass $m_1 \simeq 10^{-22}$ eV is gaining credence as a Dark Matter (DM) candidate that explains the dark cores of dwarf galaxies as soliton waves. Such a boson is naturally interpreted as an axion generic in…

星系天体物理 · 物理学 2021-02-24 Hoang Nhan Luu , S. -H. Henry Tye , Tom Broadhurst

A light hidden photon or axion-like particle is a good dark matter candidate and they are often associated with the spontaneous breaking of dark global or gauged U(1) symmetry. We consider the dark Higgs dynamics around the phase transition…

高能物理 - 唯象学 · 物理学 2021-10-27 Kazunori Nakayama , Wen Yin

The extragalactic background light is comprised of the cumulative radiation from all galaxies across the history of the universe. The angular power spectrum of the anisotropies of such a background at near-infrared (IR) frequencies lacks of…

宇宙学与河外天体物理 · 物理学 2021-05-20 Andrea Caputo , Andrea Vittino , Nicolao Fornengo , Marco Regis , Marco Taoso

The axion-like particles (ALPs) are very good candidates of the cosmological dark matter, which can exist in many extensions of the standard model (SM). The mass range of the ALPs as the dark matter can extend from a sub-eV scale to almost…

高能物理 - 唯象学 · 物理学 2018-12-05 Guo-yuan Huang , Newton Nath

We study a two component dark matter candidate inspired by the Minimal Walking Technicolor model. Dark matter consists of a dominant SIMP-like dark atom component made of bound states between primordial helium nuclei and a doubly charged…

高能天体物理现象 · 物理学 2015-09-02 K. Belotsky , M. Khlopov , C. Kouvaris , M. Laletin

We demonstrate that enhanced early galaxy formation can generically arise in axion-like particle (ALP) dark matter (DM) models with a delayed onset of axion field oscillation. In these models, the formation of localized massive objects…

高能物理 - 唯象学 · 物理学 2024-10-16 Simeon Bird , Chia-Feng Chang , Yanou Cui , Daneng Yang

In interacting multi-component dark matter (DM) models, if the DM components are nearly degenerate in mass and the interactions between them are strong enough, the relatively heavy DM components can be converted into lighter ones at late…

高能物理 - 唯象学 · 物理学 2015-06-03 Ze-Peng Liu , Yue-Liang Wu , Yu-Feng Zhou

The dark dimension scenario, which is motivated from Swampland principles and predicts a single micron scale extra dimension, suggests a consistent framework for the dark sector of the universe. We consider the implications of this scenario…

高能物理 - 理论 · 物理学 2024-07-18 Naomi Gendler , Cumrun Vafa