中文
相关论文

相关论文: Energy Dissipation of Axionic Boson Stars in Magne…

200 篇论文

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

Axions have been argued to form coherent axionic boson stars as well as incoherent axion gas. These are ones of most plausible candidates of dark matters. Since the axionic boson stars generate oscillating electric fields in an external…

高能物理 - 唯象学 · 物理学 2007-05-23 Aiichi Iwazaki

We considered recently as a new axion production mechanism the process $e^- \to e^- +a$ in a strong magnetic field $B$. Requiring that for a strongly magnetized neutron star the axion luminosity is smaller than the neutrino luminosity we…

天体物理学 · 物理学 2007-05-23 M. Kachelriess

White dwarf (WD) stars may radiate keV-energy axions produced in their stellar cores. This has been extensively studied as an extra channel by which WDs may cool, with some analyses even suggesting that axions can help explain the observed…

高能物理 - 唯象学 · 物理学 2021-03-03 Christopher Dessert , Andrew J. Long , Benjamin R. Safdi

When axion stars fly through an astrophysical magnetic background, the axion-to-photon conversion may generate a large electromagnetic radiation power. After including the interference effects of the spacially-extended axion-star source and…

高能天体物理现象 · 物理学 2018-04-11 Yang Bai , Yuta Hamada

The energy loss rate of a magnetized electron gas emitting axions a due to the process $e^- \to e^- +a$ is derived for arbitrary magnetic field strength B. Requiring that for a strongly magnetized neutron star the axion luminosity is…

天体物理学 · 物理学 2008-11-26 M. Kachelriess , C. Wilke , G. Wunner

Axion as one of the promising dark matter candidates can be detected through narrow radio lines emitted from the magnetic white dwarf stars. Due to the existence of the strong magnetic field, the axion may resonantly convert into the radio…

高能物理 - 唯象学 · 物理学 2021-06-23 Jin-Wei Wang , Xiao-Jun Bi , Run-Min Yao , Peng-Fei Yin

We explore consequences of the idea that the cooling speed of white dwarfs can be interpreted in terms of axion emission. In this case the Yukawa coupling to electrons has to be g_{ae} 10^-13, corresponding to an axion mass of a few meV.…

高能物理 - 唯象学 · 物理学 2015-02-02 Georg G. Raffelt , Javier Redondo , Nicolás Viaux

We show that axionic boson stars collide with isolated old neutron stars with strong magnetic field ($>10^8$ Gauss) and causes the neutron stars to radiate X ray by heating them. Surface temperatures of such neutron stars becomes$10^5 K…

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

Axions may make a significant contribution to the dark matter of the universe. It has been suggested that these dark matter axions may condense into localized clumps, called "axion stars." In this paper we argue that collisions of dilute…

高能物理 - 唯象学 · 物理学 2016-12-09 Stuart Raby

We explore the dynamics of boson stars in the presence of axionic couplings through nonlinear evolutions of Einstein's field equations. We show that, for large axionic couplings, isolated boson stars become unstable, and decay via a large…

广义相对论与量子宇宙学 · 物理学 2022-10-05 Nicolas Sanchis-Gual , Miguel Zilhão , Vitor Cardoso

Axion dark matter or any ultralight bosonic dark matter can go through Bose-Einstein condensation due to the large phase density, leading to the formation of axion stars or solitons in dark matter halo centers. The formation rate is…

高能物理 - 唯象学 · 物理学 2025-08-13 Patrick J. Fox , Neal Weiner , Huangyu Xiao

We indicate a possible mechanism of generating gamma ray bursts. They are generated by a collision between an axionic boson star and a neutron star. The axionic boson star can dissipates its whole energy $10^{50}$ erg in the magnetized…

天体物理学 · 物理学 2009-10-31 Aiichi Iwazaki

If the dark matter particles are axions, gravity can cause them to coalesce into axion stars, which are stable gravitationally bound systems of axions. In the previously known solutions for axion stars, gravity and the attractive force…

高能物理 - 唯象学 · 物理学 2016-09-20 Eric Braaten , Abhishek Mohapatra , Hong Zhang

We solve numerically a field equation of axions coupled with gravity and show solutions representing oscillating axionic boson stars with small mass $\sim 10^{-12}M_{\odot}$ and large radius $\sim 10^{8}$ cm. We present explicitly a…

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

It was shown in ref. [1] that cold dark matter axions reach thermal contact with baryons, and therefore cool them, shortly after the axions thermalize among themselves and form a Bose-Einstein condensate. The recent observation by the EDGES…

宇宙学与河外天体物理 · 物理学 2018-08-02 Pierre Sikivie

If dark matter is mainly composed of axions, the density distribution can be nonuniformly distributed, being clumpy instead. By solving the Einstein-Klein-Gordon system of a scalar field with the potential energy density of an axionlike…

宇宙学与河外天体物理 · 物理学 2013-06-17 J. Barranco , A. Carrillo Monteverde , D. Delepine

Axions and axion-like particles are ubiquitous in extensions of the Standard Model and offer a unifying framework for addressing open problems in cosmology. Depending on their mass and interactions, axions can act as dark matter, drive…

高能物理 - 唯象学 · 物理学 2026-05-01 Luca Visinelli

We show that a stable vortex soliton, carrying a constant magnetic flux, exists in the homogeneous medium of axions with a constant time-derivative. Axions can be bound in the vortex, having energy less than the axion mass. If the observed…

高能物理 - 唯象学 · 物理学 2024-04-02 Deog Ki Hong , Stephen J. Lonsdale

Recently it has been suggested that dark radiation in the form of axions produced during the decay of string theory moduli fields could be responsible for the soft x-ray excess in galaxy clusters. These soft X-ray photons come about due to…

宇宙学与河外天体物理 · 物理学 2014-03-19 Malcolm Fairbairn
‹ 上一页 1 2 3 10 下一页 ›