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Recently there has been interest in the physical properties of dark matter axion condensates. Due to gravitational attraction and self-interactions, they can organize into spatial localized clumps, whose properties were examined by us in…

高能物理 - 唯象学 · 物理学 2018-11-08 Mark P. Hertzberg , Enrico D. Schiappacasse

Motivated by the SU(2)$_{\rm CMB}$ modification of the cosmological model $\Lambda$CDM, we consider isolated fuzzy-dark-matter lumps, made of ultralight axion particles whose masses arise due to distinct SU(2) Yang-Mills scales and the…

高能物理 - 唯象学 · 物理学 2021-06-17 Janning Meinert , Ralf Hofmann

Existence of dark matter indicates the presence of unknown fundamental laws of nature. Ultralight axion-like particles are well-motivated dark matter candidates, emerging naturally from theories of physics at ultrahigh energies. We report…

高能物理 - 实验 · 物理学 2021-01-11 Alexander V. Gramolin , Deniz Aybas , Dorian Johnson , Janos Adam , Alexander O. Sushkov

We consider the hypothesis that galactic dark matter is composed of ultra-light scalar particles and use internal properties of dwarf spheroidal galaxies to establish a preferred range for the mass m of these bosonic particles. We…

星系天体物理 · 物理学 2015-05-30 V. Lora , Juan Magana , Argelia Bernal , F. J. Sanchez-Salcedo , E. K. Grebel

The axion is arguably one of the best motivated candidates for dark matter. For a decay constant greater than about 10^9 GeV, axions are dominantly produced non-thermally in the early universe and hence are "cold", their velocity dispersion…

高能物理 - 唯象学 · 物理学 2016-12-30 Andreas Ringwald

A number of proposed and ongoing experiments search for axion dark matter with a mass nearing the limit set by small scale structure (${\cal O} ( 10 ^{ - 21 } {\rm eV} ) $). We consider the late universe cosmology of these models, showing…

高能物理 - 唯象学 · 物理学 2021-01-11 Jeff A. Dror , Jacob M. Leedom

We search for ultra-light axions as dark matter (DM) and dark energy particle candidates, for axion masses $10^{-32}\,\mathrm{eV} \leq m_\mathrm{a} \leq 10^{-24}\,\mathrm{eV}$, by a joint analysis of cosmic microwave background (CMB) and…

Although the standard {\Lambda}CDM model describes the cosmic microwave background radiation and the large scale structure of the Universe with great success, it has some tensions with observations in the effective number of neutrino…

高能物理 - 唯象学 · 物理学 2012-11-26 Kiwoon Choi , Ki-Young Choi , Chang Sub Shin

Structure formation simulations of ultralight bosonic dark matter, ruled by the Gross-Pitaevskii-Poisson (GPP) system of equations, show that dark matter clumps to form structures with density profiles consisting of a core surrounded by a…

宇宙学与河外天体物理 · 物理学 2019-04-17 F. S. Guzman

We present forecasts on the detectability of Ultra-light axion-like particles (ULAP) from future 21cm radio observations around the epoch of reionization (EoR). We show that the axion as the dominant dark matter component has a significant…

宇宙学与河外天体物理 · 物理学 2022-01-19 Cristiano G. Sabiu , Kenji Kadota , Jacobo Asorey , Inkyu Park

Dark matter (DM) can be composed of a collection of axions, or axion-like particles (ALPs), whose existence is due to the spontaneous breaking of the Peccei-Quinn $U(1)$ symmetry which is the most compelling solution of the strong…

高能物理 - 唯象学 · 物理学 2023-06-16 Bryan Cordero-Patino , Álvaro Duenas-Vidal , Jorge Segovia

The axion is a long-postulated boson that can simultaneously solve two fundamental problems of modern physics: the charge-parity symmetry problem in the strong interaction and the enigma of dark matter. In this work we estimate, by means of…

It is known that a coherently oscillating axion field is a candidate of the dark matter. In the presence of the oscillating axion, the photon can be resonantly produced through the parametric amplification. In the universe, there also exist…

高能物理 - 唯象学 · 物理学 2020-02-12 Emi Masaki , Arata Aoki , Jiro Soda

Axion-like fields are naturally generated by a mechanism of anomaly cancellation of one or more anomalous gauge abelian symmetries at the Planck scale, emerging as duals of a two-form from the massless bosonic sector of string theory. This…

高能物理 - 唯象学 · 物理学 2018-07-04 Claudio Coriano , Paul H. Frampton

The QCD axion was originally predicted as a dynamical solution to the strong CP problem. Axion like particles (ALPs) are also a generic prediction of many high energy physics models including string theory. Theoretical models for axions are…

高能物理 - 唯象学 · 物理学 2017-12-11 David J. E. Marsh

Theories with several hundred axion fields have enormous numbers of distinct meta-stable minima. A small fraction of these local minima have vacuum energy compatible with current measurements of dark energy. The potential also contains…

高能物理 - 理论 · 物理学 2019-02-19 Thomas C. Bachlechner , Kate Eckerle , Oliver Janssen , Matthew Kleban

We consider the long time behavior of solutions to scalar field models appearing in the theory of cosmological inflation (oscillons) and cold dark matter, in presence or absence of the cosmological constant. These models are not included in…

偏微分方程分析 · 数学 2023-06-26 Matías Morales , Claudio Muñoz

Axions are hypothetical particles related to the violation of the charge-parity symmetry, being the most prone candidates for dark matter. Multiple attempts to prove their existence are currently performed in different physical systems.…

高能物理 - 唯象学 · 物理学 2018-05-09 H. Terças , J. D. Rodrigues , J. T. Mendonça

The axion is a light pseudoscalar particle postulated to solve issues with the Standard Model, including the strong CP problem and the origin of dark matter. In recent years, there has been remarkable progress in the physics of axions in…

高能物理 - 唯象学 · 物理学 2021-11-03 Kiwoon Choi , Sang Hui Im , Chang Sub Shin

The supersymmetrized DFSZ axion model is highly motivated not only because it offers solutions to both the gauge hierarchy and strong CP problems, but also because it provides a solution to the SUSY mu problem which naturally allows for a…

高能物理 - 唯象学 · 物理学 2015-06-22 Kyu Jung Bae , Howard Baer , Andre Lessa , Hasan Serce