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We examine dark matter production rates in supersymmetric axion models typified by the mass hierarchy m_gravitino << m_neutralino << m_axino. In such models, one expects the dark matter to be composed of an axion/gravitino admixture. After…

高能物理 - 唯象学 · 物理学 2015-04-20 Kyu Jung Bae , Howard Baer , Eung Jin Chun , Chang Sub Shin

The axion has emerged in recent years as a leading particle candidate to provide the mysterious dark matter in the cosmos, as we review here for a general scientific audience. We describe first the historical roots of the axion in the…

高能物理 - 唯象学 · 物理学 2022-10-18 Francesca Chadha-Day , John Ellis , David J. E. Marsh

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

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 calculate the rate for thermal production of axions via scattering of quarks and gluons in the primordial quark-gluon plasma. To obtain a finite result in a gauge-invariant way that is consistent to leading order in the strong gauge…

高能物理 - 唯象学 · 物理学 2011-04-21 Peter Graf , Frank Daniel Steffen

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

Axions, if realized in nature, can be copiously produced in the early universe via thermal processes, contributing to the mass-energy density of thermal hot relics. In light of the most recent cosmological observations, we analyze two…

宇宙学与河外天体物理 · 物理学 2021-05-27 William Giarè , Eleonora Di Valentino , Alessandro Melchiorri , Olga Mena

One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysical observations provide ample evidence for the existence of an invisible and dominant mass component in the observable universe, from the…

宇宙学与河外天体物理 · 物理学 2015-09-04 Laura Baudis

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

Recent work from the last years has raised the possibility that a portion of Dark Matter could consist of exotic particles, such as axion (anti)quark nuggets (AQN, A\bar{Q}N). After a brief review outlining the main features of axion…

高能物理 - 唯象学 · 物理学 2024-05-22 Ionel Lazanu , Mihaela Parvu

Axions are produced during a period of dilaton-driven inflation by amplification of quantum fluctuations. We show that for some range of string cosmology parameters and some range of axion masses, primordial axions may constitute a large…

高能物理 - 唯象学 · 物理学 2009-10-31 Ram Brustein , Merav Hadad

Axions as dark matter is an increasingly important subject in astrophysics and cosmology. Experimental and observational searches are mounting across the mass spectrum of axion-like particles, many of which require detailed knowledge of…

宇宙学与河外天体物理 · 物理学 2019-03-13 Erik W. Lentz , Thomas R. Quinn , Leslie J Rosenberg

We study a dark matter (DM) model offering a very natural explanation of two (naively unrelated) problems in cosmology: the observed relation $\Omega_{\rm DM}\sim\Omega_{\rm visible}$ and the observed asymmetry between matter and antimatter…

高能物理 - 唯象学 · 物理学 2018-02-21 Shuailiang Ge , Xunyu Liang , Ariel Zhitnitsky

Diluted axion star, a self-gravitating object with the quantum pressure balancing gravity, has been predicted in many models with a QCD axion or axion-like particle. It can be formed in the early universe and composes a sizable fraction of…

宇宙学与河外天体物理 · 物理学 2022-02-02 Yang Bai , Xiaolong Du , Yuta Hamada

Hot axions are produced in the early Universe via their interactions with Standard Model particles, contributing to dark radiation commonly parameterized as $\Delta N_{\text{eff}}$. In standard QCD axion benchmark models, this contribution…

高能物理 - 唯象学 · 物理学 2024-03-12 Marcin Badziak , Keisuke Harigaya , Michał Łukawski , Robert Ziegler

Recent work has shown that axions can be efficiently produced via non-stationary pair plasma discharges in the polar cap region of pulsars. Here, we point out that for axion masses $10^{-9} \, {\rm eV} \lesssim m_a \lesssim 10^{-4} \, \rm…

高能物理 - 唯象学 · 物理学 2024-10-08 Dion Noordhuis , Anirudh Prabhu , Christoph Weniger , Samuel J. Witte

Sterile neutrinos can be generated in the early universe through oscillations with active neutrinos and represent a popular and well-studied candidate for our universe's dark matter. Stringent constraints from X-ray and gamma-ray line…

高能物理 - 唯象学 · 物理学 2017-04-19 Asher Berlin , Dan Hooper

Axions may be produced thermally inside the cores of neutron stars (NSs), escape the stars due to their feeble interactions with matter, and subsequently convert into X-rays in the magnetic fields surrounding the stars. We show that a…

高能物理 - 唯象学 · 物理学 2021-03-03 Malte Buschmann , Raymond T. Co , Christopher Dessert , Benjamin R. Safdi

We demonstrate that ultralight axion dark matter with a coupling to photons induces an oscillating global terrestrial magnetic field signal in the presence of the background geomagnetic field of the Earth. This signal is similar in…

高能物理 - 唯象学 · 物理学 2022-05-25 Ariel Arza , Michael A. Fedderke , Peter W. Graham , Derek F. Jackson Kimball , Saarik Kalia

Relativistic axions are good candidates for the dark radiation for which there are mounting observational hints. The primordial decays of heavy fields produce axions which are ultra-energetic compared to thermalised matter and inelastic…

高能物理 - 唯象学 · 物理学 2015-06-15 Joseph P. Conlon , M. C. David Marsh