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Axion quark nuggets (AQNs) are hypothetical objects with a mass greater than a few grams and sub-micrometer size, formed during the quark-hadron transition. Originating from the axion field, they offer a possible resolution of the…

Macroscopic dark matter with dominating strong interactions, supposed to be composites, represents an alternative to the most popular WIMP particles. Predicted in various models as strangelets, nuclearites, nuggets, having different…

高能物理 - 唯象学 · 物理学 2026-04-01 Ionel Lazanu , Konstantin Zioutas

We review a testable, the axion quark nugget (AQN) model outside of the standard WIMP paradigm. The model was originally invented to explain the observed similarity between the dark and the visible components, $\Omega_{\rm DM}\approx…

高能物理 - 唯象学 · 物理学 2021-06-25 Ariel Zhitnitsky

Axion quark nuggets (AQNs) are hypothetical objects with nuclear density that would have formed during the quark-hadron transition and could make up most of the dark matter today. These objects have a mass greater than a few grams and are…

宇宙学与河外天体物理 · 物理学 2025-11-26 Michael Sekatchev , Xunyu Liang , Fereshteh Majidi , Ben Scully , Ludovic Van Waerbeke , Ariel Zhitnitsky

We consider the formation and evolution of Axion Quark Nugget dark matter particles in the early universe. The goal of this work is to estimate the mass distribution of these objects and assess their ability to form and survive to the…

高能物理 - 唯象学 · 物理学 2019-07-03 Shuailiang Ge , Kyle Lawson , Ariel Zhitnitsky

It has been known for quite sometime that the Neutron Stars (NS) can play a role of the Dark Matter (DM) detectors due to many uniques features of NS. We apply these (previously developed) ideas to a specific form of the DM when it is…

高能物理 - 唯象学 · 物理学 2024-03-18 Ariel Zhitnitsky

It has been recently argued [1-3] that there is a strong component of the diffuse far-ultraviolet (FUV) background which is hard to explain by conventional physics in terms of the dust-scattered starlight. We propose that this excess in FUV…

高能物理 - 唯象学 · 物理学 2022-03-17 Ariel Zhitnitsky

We study a testable dark matter (DM) model outside of the standard WIMP paradigm in which the observed ratio $\Omega_{\rm dark} \simeq \Omega_{\rm visible}$ for visible and dark matter densities finds its natural explanation as a result of…

高能物理 - 唯象学 · 物理学 2016-10-12 Xunyu Liang , Ariel Zhitnitsky

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

Axion quark nuggets (AQNs) are macroscopic dark-matter candidates, with masses of the order of a few grams to a kilogram and sub-micron radius, thought to form at the Quantum Chromo Dynamic era through axion-induced charge separation. This…

宇宙学与河外天体物理 · 物理学 2025-12-08 Fereshteh Majidi , Xunyu Liang , Michael Sekatchev , Ludovic Van Waerbeke , Ariel Zhitnitsky

We study the new mechanism of the axion production suggested recently in [1,2]. This mechanism is based on the so-called Axion Quark Nugget (AQN) dark matter model, which was originally invented to explain the similarity of the dark and…

宇宙学与河外天体物理 · 物理学 2020-02-19 Xunyu Liang , Alexander Mead , Md Shahriar Rahim Siddiqui , Ludovic Van Waerbeke , Ariel Zhitnitsky

The axion anti-quark nugget (A$\bar{\mathrm{Q}}$N) model was developed to explain in a natural way the asymmetry between matter and antimatter in Universe. In this hypothesis, a similitude between the dark and the visible components exists.…

高能物理 - 唯象学 · 物理学 2024-07-10 Ionel Lazanu , Mihaela Parvu

We review a testable dark matter (DM) model outside of the standard WIMP paradigm. The model is unique in a sense that the observed ratio $\Omega_{\rm dark} \simeq \Omega_{\rm visible}$ for visible and dark matter densities finds its…

高能物理 - 唯象学 · 物理学 2017-04-05 Ariel Zhitnitsky

Anti-quark nuggets (AQNs) have been suggested to solve the dark matter (DM) and the missing antimatter problem in the universe and have been proposed as an explanation of various observations. Their size is in the {\mu}m range and their…

The Quark Nugget (QN) model of dark matter suggests that the dark matter may consist of compact composite objects of quark matter. Although such composite particles can strongly interact with visible matter, they may remain undetected…

宇宙学与河外天体物理 · 物理学 2024-11-18 V. V. Flambaum , I. B. Samsonov

Ball lighting (BL) has been observed for centuries. There are large number of books, review articles, and original scientific papers devoted to different aspects of BL phenomenon. Yet, the basic features of this phenomenon have never been…

高能物理 - 唯象学 · 物理学 2025-08-26 Ariel Zhitnitsky

We advocate an idea that the presence of the daily and annual modulations of the axion flux on the Earth surface may dramatically change the strategy of the axion searches. Our computations are based on the so-called Axion Quark Nugget…

高能物理 - 唯象学 · 物理学 2020-02-19 Dmitry Budker , Victor V. Flambaum , Xunyu Liang , Ariel Zhitnitsky

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

"Dark quark nuggets", a lump of dark quark matter, can be produced in the early universe for a wide range of confining gauge theories and serve as a macroscopic dark matter candidate. The two necessary conditions, a nonzero dark baryon…

高能物理 - 唯象学 · 物理学 2019-11-26 Yang Bai , Andrew J. Long , Sida Lu

We advocate the idea that there is a fundamentally new mechanism for the axion production in the Sun, which has never been discussed previously in the literature. This novel mechanism of the axion production is based on the so-called Axion…

高能物理 - 唯象学 · 物理学 2018-08-22 H. Fischer , X. Liang , Y. Semertzidis , A. Zhitnitsky , K. Zioutas
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