中文
相关论文

相关论文: Magnetic axion vortex and very light QCD axions

200 篇论文

In supersymmetric theories, the presence of axions usually implies the existence of a non-compact, (pseudo)moduli space. In gauge mediated models, the axion would seem a particularly promising dark matter candidate. The cosmology of the…

高能物理 - 理论 · 物理学 2013-05-29 Linda M. Carpenter , Michael Dine , Guido Festuccia , Lorenzo Ubaldi

We study the possibility of the vortices formation in axion condensate on the galactic scale. Such vortices can occur as a result of global rotation of the early universe. We study analytical models of vortices and calculate exemplary…

天体物理学 · 物理学 2010-09-28 Jakub Mielczarek , Tomasz Stachowiak , Marek Szydlowski

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

If the dark matter is composed of axions, then axion stars are expected to be abundant in the Universe. We demonstrate in fully non-linear (3+1) numerical relativity the instability of compact axion stars due to the electromagnetic…

高能物理 - 唯象学 · 物理学 2024-11-26 Liina M. Chung-Jukko , Eugene A. Lim , David J. E. Marsh , Josu C. Aurrekoetxea , Eloy de Jong , Bo-Xuan Ge

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

It has been pointed out in the literature that in the presence of an external magnetic field the axion mass receives an electromagnetic contribution. We show that if a magnetic field with energy density larger than ~10^{-8} times the energy…

天体物理学 · 物理学 2009-11-13 L. Campanelli , M. Giannotti

We study an axion soliton, which weakly interacts with background matter and magnetic fields. A mirror-symmetric soliton, for which the magnetic flow is due to secondary magnetic helicity invariant, is described by the Iroshnikov-Kreichnan…

高能物理 - 理论 · 物理学 2025-11-14 P. M. Akhmetiev , M. S. Dvornikov

Axion particles can form macroscopic condensates, whose size can be galactic in scale for models with very small axion masses $m\sim10^{-22}$ eV, and which are sometimes referred to under the name of Fuzzy Dark Matter. Many analyses of…

高能物理 - 唯象学 · 物理学 2018-02-21 Joshua Eby , Michael Ma , Peter Suranyi , L. C. R. Wijewardhana

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

The axion is a hypothetical elementary particle and a cold dark matter candidate. It could dominate potential wells of most astrophysical objects. Axions spontaneously decay into nearly monochromatic microwave photons. We present results…

天体物理学 · 物理学 2009-10-31 B. D. Blout , E. J. Daw , M. P. Decowski , Paul T. P. Ho , L. J Rosenberg , D. B. Yu

We analyze the behavior of axion dark matter before it falls into a galactic gravitational potential well. The axions thermalize sufficiently fast by gravitational self-interactions that almost all go to their lowest energy state consistent…

星系天体物理 · 物理学 2015-06-16 N. Banik , P. Sikivie

The particle that makes up the dark matter of the universe could be an axion or axion-like particle. A collection of axions can condense into a bound Bose-Einstein condensate called an axion star. It is possible that a significant fraction…

高能物理 - 唯象学 · 物理学 2018-10-30 Eric Braaten , Hong Zhang

Axions are possible candidates of dark matter in the present Universe. They have been argued to form axionic boson stars with small masses $\sim 10^{-12}M_{\odot}$. Since they possess oscillating electric fields in a magnetic field, they…

高能物理 - 唯象学 · 物理学 2014-11-17 Aiichi Iwazaki

The investigation on the production of particles in slowly varying but extremely intense magnetic field in extended to the case of axions. The motivation is, as for some previously considered cases, the possibility that such kind of…

高能物理 - 唯象学 · 物理学 2008-11-26 Giorgio Calucci

If there are a plethora of axions in nature, they may have a complicated potential and create an axion landscape. We study a possibility that one of the axions is so light that it is cosmologically stable, explaining the observed dark…

高能物理 - 唯象学 · 物理学 2017-03-03 Ryuji Daido , Takeshi Kobayashi , Fuminobu Takahashi

Axions are possible candidates of dark matter in the present Universe. They have been argued to form axionic boson stars with small masses $10^{-14}M_{\odot}\sim 10^{-11}M_{\odot}$. Since they possess oscillating electric fields in a…

高能物理 - 唯象学 · 物理学 2009-10-31 Aiichi Iwazaki

In axion electrodynamics, magnetic fields enable axion-photon mixing. Recent proposals suggest that rotating, conductive plasmas in neutron star magnetospheres could trigger axion superradiant instabilities -- an intriguing idea, given that…

高能物理 - 唯象学 · 物理学 2025-06-19 Thomas F. M. Spieksma , Enrico Cannizzaro

Magnetic fields mix axions with photons, allowing for the cyclotron process e -> e + a by virtue of an intermediate plasmon even if axions do not couple to electrons at tree level. The axion and longitudinal-plasmon dispersion relations…

高能物理 - 唯象学 · 物理学 2009-10-31 N. V. Mikheev , G. Raffelt , L. A. Vassilevskaya

Low mass axion-like particles could be produced in abundance within the cores of hot, compact magnetic white dwarf (MWD) stars from electron bremsstrahlung and converted to detectable X-rays in the strong magnetic fields surrounding these…

高能天体物理现象 · 物理学 2024-11-11 Orion Ning , Christopher Dessert , Vi Hong , Benjamin R. Safdi

Scalar field dark matter likely is able to solve all small-scale cosmology problems facing the cold dark matter (CDM), and has become an emerging contender to challenge the CDM. It however requires a particle mass $\sim 1 - 2…

宇宙学与河外天体物理 · 物理学 2014-09-26 Tzihong Chiueh
‹ 上一页 1 2 3 10 下一页 ›