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相关论文: Precise predictions for the QCD axion contribution…

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Using the light front wave functions for the nucleons in a quark model in AdS/QCD, we calculate the nucleon electromagnetic form factors. The flavor decompositions of the nucleon form factors are calculated from the GPDs in this model. We…

高能物理 - 唯象学 · 物理学 2014-01-07 Dipankar Chakrabarti , Chandan Mondal

QCD axions can be a substantial part of dark matter if their mass $m_a\sim10^{-5}$eV. Since the axions were created by the misalignment mechanism, their local energy spectrum density is large. Consequently, the axion-induced atomic…

高能物理 - 唯象学 · 物理学 2023-06-21 Qiaoli Yang , Shiqin Dong

Non-relativistic QCD axions or axion-like particles are among the most popular candidates for cold Dark Matter (DM) in the universe. We proposed to detect axion-like DM, using linearly polarized pulsar light as a probe. Because of…

宇宙学与河外天体物理 · 物理学 2020-03-18 Tao Liu , George Smoot , Yue Zhao

Atomic dark matter is a simple but highly theoretically motivated possibility for an interacting dark sector that could constitute some or all of dark matter. We perform a comprehensive study of precision cosmological observables on minimal…

高能物理 - 唯象学 · 物理学 2023-07-31 Saurabh Bansal , Jared Barron , David Curtin , Yuhsin Tsai

We study for what specific values of the theoretical parameters the axion can form the totality of cold dark matter. We examine the allowed axion parameter region in the light of recent data collected by the WMAP5 mission plus baryon…

宇宙学与河外天体物理 · 物理学 2021-12-14 Luca Visinelli , Paolo Gondolo

We use the energy-momentum tensor (EMT) current to compute the EMT form factors of the nucleon in the framework of the light cone QCD sum rule formalism. In the calculations, we employ the most general form of the nucleon's interpolating…

高能物理 - 唯象学 · 物理学 2020-03-18 K. Azizi , U. Ozdem

The recent observations imply that there is an extra relativistic degree of freedom coined dark radiation. We argue that the QCD axion is a plausible candidate for the dark radiation, not only because of its extremely small mass, but also…

高能物理 - 唯象学 · 物理学 2015-06-03 Kwang Sik Jeong , Fuminobu Takahashi

The presence of a hot dark matter component has been hinted at 3 sigma by a combination of the results from different cosmological observations. We examine a possibility that pseudo Nambu-Goldstone bosons account for both hot and cold dark…

高能物理 - 唯象学 · 物理学 2014-03-03 Kwang Sik Jeong , Masahiro Kawasaki , Fuminobu Takahashi

Dark matter associated visible particle production at high energy colliders provides a unique way to determine the microscopic properties of the dark matter. We investigate a pair of fermionic dark matter particles associated with a b-jet…

高能物理 - 唯象学 · 物理学 2016-11-21 Li Gang , Yu Si-He , Song Mao , Zhang Yu , Zhou Ya-Jin , Guo Jian-You

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 properties of the QCD axion are strictly related to the dependence of strong interactions on the topological parameter theta. We present a determination of the topological properties of QCD for temperatures up to around 600 MeV,…

If QCD axions form a large fraction of the total mass of dark matter, then axion stars could be very abundant in galaxies. As a result, collisions with each other, and with other astrophysical bodies, can occur. We calculate the rate and…

宇宙学与河外天体物理 · 物理学 2017-05-24 Joshua Eby , Madelyn Leembruggen , Joseph Leeney , Peter Suranyi , L. C. R. Wijewardhana

The recent detection of B-modes by BICEP2 has non-trivial implications for axion dark matter implied by combining the tensor interpretation with isocurvature constraints from Planck. In this paper the measurement is taken as fact, and its…

宇宙学与河外天体物理 · 物理学 2014-07-09 David J. E. Marsh , Daniel Grin , Renee Hlozek , Pedro G. Ferreira

The QCD axion is a well-motivated hypothetical particle beyond the Standard Model (SM) and a compelling dark matter candidate. Its relic abundance is highly sensitive to the thermal history of the universe when the temperature is around the…

高能物理 - 唯象学 · 物理学 2025-06-26 Kun-Feng Lyu , Yue Zhao

We observe that photon cooling after big bang nucleosynthesis (BBN) but before recombination can remove the conflict between the observed and theoretically predicted value of the primordial abundance of $^7$Li. Such cooling is ordinarily…

宇宙学与河外天体物理 · 物理学 2015-05-27 O. Erken , P. Sikivie , H. Tam , Q. Yang

A new and simple statistical approach is performed to calculate the parton distribution functions (PDFs) of the nucleon in terms of light-front kinematic variables. Analytic expressions of x-dependent PDFs are obtained in the whole x…

高能物理 - 唯象学 · 物理学 2011-04-07 Lijing Shao , Yunhua Zhang , Bo-Qiang Ma

We study the cosmological evolution of the QCD axion coupled to hidden photons. For a moderately strong coupling, the motion of the axion field leads to an explosive production of hidden photons by tachyonic instability. We use lattice…

高能物理 - 唯象学 · 物理学 2018-05-23 Naoya Kitajima , Toyokazu Sekiguchi , Fuminobu Takahashi

We introduce a mechanism for multi-component dark matter (DM) that originates from axion mixing and present some of its defining properties. In this context, multi-component DM implies that the cold DM is composed of the QCD axion and many…

高能物理 - 唯象学 · 物理学 2025-12-30 Hai-Jun Li

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

We report on a search for ultra-low-mass axion-like dark matter by analysing the ratio of the spin-precession frequencies of stored ultracold neutrons and $^{199}$Hg atoms for an axion-induced oscillating electric dipole moment of the…

高能物理 - 实验 · 物理学 2018-05-28 N. J. Ayres