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相关论文: Dark matter from an even lighter QCD axion: trappe…

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We discuss production of QCD axion dark matter in a novel scenario, which assumes time-varying scale of Peccei-Quinn symmetry breaking. The latter decreases as the Universe's temperature at early times and eventually stabilises at a large…

高能物理 - 唯象学 · 物理学 2023-05-30 Sabir Ramazanov , Rome Samanta

The Peccei Quinn (PQ) solution of the strong CP problem requires the existence of axions, which are a viable candidate for Dark Matter. Here we show that, if the Nambu Goldstone potential of the PQ model is replaced by a potential V(|\Phi|)…

天体物理学 · 物理学 2009-11-10 Roberto Mainini , Silvio A. Bonometto

The Peccei-Quinn anomalous global U(1)_{PQ} symmetry is important not only for solving the strong CP problem with a cosmologically relevant axion, but it may also be the origin of a residual Z_2 symmetry. This new symmetry may be…

高能物理 - 唯象学 · 物理学 2014-03-12 Basudeb Dasgupta , Ernest Ma , Koji Tsumura

As a simple model for dark matter, we propose a QCD-like theory based on $\rm{SU}(2)$ gauge theory with one flavor of dark quark. The model is confining at low energy and we use lattice simulations to investigate the properties of the…

高能物理 - 唯象学 · 物理学 2019-01-30 Anthony Francis , Renwick J. Hudspith , Randy Lewis , Sean Tulin

A number of nuclear decay anomalies have been reported in the literature, which purport to show periodic variations in the decay rates of certain radioisotopes. If these reports reflect reality, they would necessitate a seismic shift in our…

高能物理 - 唯象学 · 物理学 2023-11-23 Xin Zhang , Nick Houston , Tianjun Li

A leading direction in the hunt for axion dark matter is to search for its influence on nuclear spins. The detection scheme involves polarizing a sample of nuclei within a strong static magnetic field and then looking for a spin precession…

高能物理 - 唯象学 · 物理学 2023-05-15 Jeff A. Dror , Stefania Gori , Jacob M. Leedom , Nicholas L. Rodd

We propose simple scenarios where lepton flavor-violating couplings generate the observed dark matter abundance through freeze-in of an axion-like particle with mass in the few keV range. Compared to flavor-diagonal freeze-in, this…

高能物理 - 唯象学 · 物理学 2023-05-03 Paolo Panci , Diego Redigolo , Thomas Schwetz , Robert Ziegler

Asymmetric dark matter is a well-motivated approach to explain the apparent coincidence between the relic densities of visible and dark matter, $\Omega_D \simeq 5.4\Omega_b$. A complete explanation requires two components, a relation…

高能物理 - 唯象学 · 物理学 2026-03-04 Peter Cox , Rafael E. Pérez , Raymond R. Volkas

We study an axion-like particle (ALP) that experiences the first-order phase transition with respect to its mass or potential minimum. This can be realized if the ALP obtains a potential from non-perturbative effects of SU($N$) gauge theory…

高能物理 - 唯象学 · 物理学 2023-04-05 Shota Nakagawa , Fuminobu Takahashi , Masaki Yamada , Wen Yin

In all supersymmetric theories, gravitinos, with mass suppressed by the Planck scale, are an obvious candidate for dark matter; but if gravitinos ever reached thermal equilibrium, such dark matter is apparently either too abundant or too…

高能物理 - 唯象学 · 物理学 2017-08-03 Raymond T. Co , Francesco D'Eramo , Lawrence J. Hall , Keisuke Harigaya

The QCD axion is one of the most appealing candidates for the dark matter in the Universe. In this article, we discuss the possibility to predict the axion mass in the context of a simple renormalizable grand unified theory where the…

高能物理 - 唯象学 · 物理学 2019-11-21 Pavel Fileviez Perez , Clara Murgui , Alexis D. Plascencia

Thermal misalignment provides an alternative to the standard misalignment mechanism for the cosmological production of scalar dark matter. In this framework, feeble couplings to particles in the thermal bath generate a finite-temperature…

高能物理 - 唯象学 · 物理学 2026-03-20 Brian Batell , Akshay Ghalsasi , Subhajit Ghosh , Mudit Rai

The misalignment mechanism for axion production depends on the temperature-dependent axion mass. The latter has recently been determined within the interacting instanton liquid model (IILM), and provides for the first time a well-motivated…

宇宙学与河外天体物理 · 物理学 2011-02-15 Olivier Wantz , E. P. S. Shellard

We show that the strong CP problem can, in principle, be solved dynamically by adding extra-dimensions with compact topology. To this aim we consider a toy model for QCD, which contains a vacuum angle and a strong CP like problem. We…

高能物理 - 理论 · 物理学 2011-08-04 F. L. Bezrukov , Y. Burnier

The comparable abundances of dark matter and baryons imply a deep connection between the dark sector and the QCD sector. In models of asymmetric dark matter, the number densities of both sectors are ensured to be similar. However, a…

高能物理 - 唯象学 · 物理学 2025-12-09 Yi Chung

The axion mass receives a large correction from small instantons if the QCD gets strongly coupled at high energies. We discuss the size of the new CP violating phases caused by the fact that the small instantons are sensitive to the UV…

高能物理 - 唯象学 · 物理学 2021-07-28 Ryuichiro Kitano , Wen Yin

Abelian quiver gauge theories provide candidates for the conformality approach to physics beyond the standard model which possess novel cancellation mechanisms for quadratic divergences. A $Z_2$ symmetry (R parity) can be imposed and leads…

天体物理学 · 物理学 2008-11-26 P. H. Frampton

We consider a model in which dark matter is a composite baryon of a dark sector governed by $SU(3)$ gauge theory, with vector-like quarks also charged under $U(1)_Y$. The model provides simple answer to the dark matter stability problem: it…

高能物理 - 唯象学 · 物理学 2016-10-21 Ran Huo , Shigeki Matsumoto , Yue-Lin Sming Tsai , Tsutomu T. Yanagida

The axion is one of the best motivated candidates for particle dark matter. We study and update the constraints imposed by the recent CMB and LSS experiments on the mass of axions produced by the misalignment mechanism, as a function of…

高能物理 - 唯象学 · 物理学 2008-11-26 Maria Beltran , Juan Garcia-Bellido , Julien Lesgourgues

One of the most puzzling problems of modern physics is the identification of the nature a non-relativistic matter component present in the universe, contributing to more than 25$\%$ of the total energy budget, known as Dark Matter. Weakly…

高能物理 - 唯象学 · 物理学 2019-01-18 Mathias Pierre