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相关论文: Axion Stars and Fast Radio Bursts

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As a new kind of radio transient sources detected at $\sim 1.4$ GHz, fast radio bursts are specially characterized by their short durations and high intensities. Although only ten events are detected so far, fast radio bursts may actually…

高能天体物理现象 · 物理学 2015-12-22 Y. F. Huang , J. J. Geng

Axions are one of the most promising candidates of dark matter. The axions have been shown to form miniclusters with masses $\sim 10^{-12}M_{\odot}$ and to become dominant component of dark matter. Some of the axion miniclusters condense to…

高能物理 - 唯象学 · 物理学 2015-11-18 Aiichi Iwazaki

Fast radio bursts can be caused by some phenomena related to 'new physics'.One of the most prominent candidates of the kind are axion Bose stars which can engender bursts when undergoing conversion into photons in magnetospheres of neutron…

高能天体物理现象 · 物理学 2020-05-07 Maxim S. Pshirkov

We study the radio signals generated when an axion star enters the magnetosphere of a neutron star. As the axion star moves through the resonant region where the plasma-induced photon mass becomes equal to the axion mass, the axions can…

高能天体物理现象 · 物理学 2021-02-25 James H. Buckley , P. S. Bhupal Dev , Francesc Ferrer , Fa Peng Huang

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

Axion is a promising candidate of dark matter in the universe. A fraction of dark matter axion may forms axion star with radius $\sim 10^2$km. We show that the axion star emits radiation burst by the collision with K and M types main…

高能物理 - 唯象学 · 物理学 2022-04-20 Aiichi Iwazaki

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

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

If primordial black holes with masses of $10^{25}\,\mbox{g}\gtrsim m \gtrsim 10^{17}\,\mbox{g}$ constitute a non-negligible fraction of the galactic dark-matter haloes, their existence should have observable consequences: they necessarily…

高能天体物理现象 · 物理学 2018-11-28 Marek A. Abramowicz , Michał Bejger , Maciek Wielgus

Fast radio bursts (FRBs) are newly discovered radio transient sources. Their high dispersion measures indicate an extragalactic origin. But due to the lack of observational data in other wavelengths, their progenitors still remain unclear.…

高能天体物理现象 · 物理学 2017-05-11 J. J. Geng , Y. F. Huang

We point out that the bursts of photons with the energy of the axion mass may appear coincidentally with gamma ray bursts if the gamma ray bursts are caused by collisions between neutron stars and axionic boson stars. In this mechanism,…

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

We propose a model in which ultra high energy cosmic rays and gamma ray bursts are produced by collisions between neutron stars and axion stars. The acceleration of such a cosmic ray is made by the electric field, $\sim 10^{15} (B/10^{12}…

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

Non-linear effects in the evolution of the axion field in the early Universe may lead to the formation of gravitationally bound clumps of axions, known as "miniclusters". Minicluster masses should be in the range $M_{\rm mc}\sim10^{-12}…

高能天体物理现象 · 物理学 2015-06-23 Igor I. Tkachev

Popular models of repeating Fast Radio Bursts (and perhaps of all Fast Radio Bursts) involve neutron stars because of their high rotational or magnetostatic energy densities. These models take one of two forms: giant but rare pulsar-like…

高能天体物理现象 · 物理学 2020-03-04 J. I. Katz

We have proposed a model of non repeating fast radio bursts ( FRBs ); the collisions between axion stars and neutron stars generate the bursts. In this paper, we propose a model of repeating FRBs which shows that they arise from the several…

高能天体物理现象 · 物理学 2018-04-04 Aiichi Iwazaki

We propose the model describing the observed multiple fast radio bursts due to the close encounters and collisions of neutron stars in the central clusters of the evolved galactic nuclei. The subsystem of neutron star cluster may originate…

高能天体物理现象 · 物理学 2017-12-07 V. I. Dokuchaev , Yu. N. Eroshenko

Fast radio bursts appear to exhibit large dispersion measures, typically exceeding any expected galactic interstellar contribution, especially along the moderate to high-galactic-latitude directions in which such events have been most often…

高能天体物理现象 · 物理学 2015-06-19 Brian Dennison

We propose that the periodic fast radio bursts of FRB 180916.J0158+65 are sourced by axion emission (mass $m_{a} \sim 10^{-14}$ eV) from cosmic superstrings. Some of the emitted axions are converted to photons by magnetic fields as they…

宇宙学与河外天体物理 · 物理学 2020-03-17 David F. Chernoff , Shing Yan Li , S. -H. Henry Tye

We propose a model in which ultra high energy cosmic rays are produced by collisions between neutron stars and axion stars. The acceleration of such a cosmic ray is made by the electric field, $\sim 10^{15} (B/10^{12} {G}) {eV} {cm}^{-1}$,…

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

The model that fast radio bursts are caused by plunges of asteroids onto neutron stars can explain both repetitive and non-repetitive bursts. If a neutron star passes through an asteroid belt around another star, there would be a series of…

高能天体物理现象 · 物理学 2017-04-04 Manjari Bagchi
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