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Massive axions of the Kaluza-Klein type, created inside the solar core, can be gravitationally trapped by the Sun itself in orbits inside/outside the Sun, where they accumulate over cosmic times. Their radiative decay can give rise to…

天体物理学 · 物理学 2007-05-23 K. Zioutas

The origin of various celestial phenomena have remained mysterious for conventional astrophysics. Therefore, alternative solutions should be considered, taking into account the involvement of unstable dark-matter particle candidates, such…

天体物理学 · 物理学 2007-05-23 K. Zioutas , Y. Semertzidis , Th. Papaevangelou

There is reason to suspect that about half of the baryons are in pressure-supported plasma in the halos of normal galaxies, drawn in by gravity along with about half of the dark matter. To be consistent with the observations this baryonic…

天体物理学 · 物理学 2008-11-26 Masataka Fukugita , P. J. E. Peebles

A new physical phenomenon is identified: volumetric stellar emission into gravitationally bound orbits of weakly coupled particles such as axions, moduli, hidden photons, and neutrinos. While only a tiny fraction of the instantaneous…

高能物理 - 唯象学 · 物理学 2021-07-28 Ken Van Tilburg

Magnetic field dependent transient solar observations are suggestive for axion-photon oscillations with light axion(-like) particle involvement. Novel dark-moon measurements with the SMART X-ray detectors can be conclusive for radiatively…

Axions generated thermally in the solar core can convert nearly directly to X-rays as they pass through the solar atmosphere via interaction with the magnetic field. The result of this conversion process would be a diffuse…

太阳与恒星天体物理 · 物理学 2012-01-24 Hugh S. Hudson , L. W. Acton , E. DeLuca , I. G. Hannah , K. Reardon , K. Van Bibber

The X-ray emission from the Sun reveals a very dynamic hot atmosphere, the corona, which is characterized by a complex morphology and broad range of timescales of variability and spatial structuring. The solar magnetic fields play a…

太阳与恒星天体物理 · 物理学 2022-06-09 Paola Testa , Fabio Reale

A sudden increase in stellar luminosity may lead to the ejection of a large part of any optically thin gas orbiting the star. Test particles in circular orbits will become unbound, and will escape to infinity (if radiation drag is…

高能天体物理现象 · 物理学 2015-06-11 Włodek Kluźniak

Standard solar physics cannot account for the X-ray emission and other puzzles, the most striking example being the solar corona mystery. The corona temperature rise above the non-flaring magnetized sunspots, while the photosphere just…

An axion rotating in field space can produce dark photons in the early universe via tachyonic instability. This explosive particle production creates a background of stochastic gravitational waves that may be visible at pulsar timing arrays…

高能物理 - 唯象学 · 物理学 2022-01-05 Raymond T. Co , Keisuke Harigaya , Aaron Pierce

Context: According to theory, high-energy emission from the coronae of cool stars can severely erode the atmospheres of orbiting planets. No observational tests of the long term effects of erosion have yet been made. Aims: To analyze the…

太阳与恒星天体物理 · 物理学 2010-08-11 J. Sanz-Forcada , I. Ribas , G. Micela , A. M. T. Pollock , D. Garcia-Alvarez , E. Solano , C. Eiroa

We are investigating the possible origin of small-scale anomalies, like the annual stratospheric temperature anomalies. Unexpectedly within known physics, their observed planetary "dependency", does not match concurrent solar activity,…

The hot interiors of massive stars in the later stages of their evolution provide an ideal place for the production of heavy axion-like particles (ALPs) with mass up to O(100 keV) range. We show that a fraction of these ALPs could stream…

高能物理 - 唯象学 · 物理学 2024-12-31 James H. Buckley , P. S. Bhupal Dev , Francesc Ferrer , Takuya Okawa

As recently advocated in \cite{Fischer:2018niu}, there is a fundamentally new mechanism for the axion production in the Sun and Earth. However, the role of very slow axions in previous studies were neglected because of its negligible…

高能物理 - 唯象学 · 物理学 2019-01-30 Xunyu Liang , Ariel Zhitnitsky

Axions may be produced thermally inside the cores of neutron stars (NSs), escape the stars due to their feeble interactions with matter, and subsequently convert into X-rays in the magnetic fields surrounding the stars. We show that a…

高能物理 - 唯象学 · 物理学 2021-03-03 Malte Buschmann , Raymond T. Co , Christopher Dessert , Benjamin R. Safdi

Much of modern astrophysics is grounded on the observed chemical compositions of stars and the diffuse plasma that pervades the space between stars, galaxies and clusters of galaxies. X-ray and EUV spectra of the hot plasma in the outer…

天体物理学 · 物理学 2009-11-10 Jeremy J. Drake

Optically thin coronae around neutron stars suffering an X-ray burst can be ejected as a result of rapid increase in stellar luminosity. In general relativity (GR), radiation pressure from the central luminous star counteracts gravitational…

高能天体物理现象 · 物理学 2013-07-02 B. Mishra , W. Kluzniak

The anomalously large radii of strongly irradiated exoplanets have remained a major puzzle in astronomy. Based on a 2D steady state atmospheric circulation model, the validity of which is assessed by comparison to 3D calculations, we reveal…

地球与行星天体物理 · 物理学 2017-05-31 P. Tremblin , G. Chabrier , N. J. Mayne , D. S. Amundsen , I. Baraffe , F. Debras , B. Drummond , J. Manners , S. Fromang

The working principle of axion helioscopes can be behind unexpected solar X-ray emission, being associated with solar magnetic fields, which become the catalyst. Solar axion signals can be transient brightenings as well as continuous…

天体物理学 · 物理学 2016-11-09 K. Zioutas , M. Tsagri , Y. Semertzidis , Th. Papaevangelou , A. Nordt , V. Anastassopoulos

X-ray and UV line emission in X-ray binaries can be accounted for by a hot corona. Such a corona forms through irradiation of the outer disk by radiation produced in the inner accretion flow. The same irradiation can produce a strong…

高能天体物理现象 · 物理学 2015-07-15 Nick Higginbottom , Daniel Proga
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