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相关论文: Solar Chameleons

200 篇论文

The issue of predicting solar flares is one of the most fundamental in physics, addressing issues of plasma physics, high-energy physics, and modelling of complex systems. It also poses societal consequences, with our ever-increasing need…

太阳与恒星天体物理 · 物理学 2014-11-20 R. T. James McAteer , Peter T. Gallagher , Paul A. Conlon

The flux of hypothetical "hidden photons" from the Sun is computed under the assumption that they interact with normal matter only through kinetic mixing with the ordinary standard model photon. Requiring that the exotic luminosity is…

高能物理 - 唯象学 · 物理学 2008-11-26 Javier Redondo

Cosmic Microwave Background (CMB) photons can undergo resonant conversion into axions in the presence of magnetized plasma distributed inside non-linear large-scale structure (LSS). This process leads to axion-induced patchy screening:…

高能物理 - 唯象学 · 物理学 2024-11-12 Cristina Mondino , Dalila Pîrvu , Junwu Huang , Matthew C. Johnson

Axions seem ubiquitous in string theories and some of them may be produced non-thermally by heavy scalar decays, contributing to dark radiation. We study various cosmological effects of photons produced from the axionic dark radiation…

高能物理 - 唯象学 · 物理学 2015-06-16 Tetsutaro Higaki , Kazunori Nakayama , Fuminobu Takahashi

Observational evidence implying the accelerated expansion of the universe has been the motivation to develop various classes of modified gravity theories. One of them uses the so-called "screening mechanism", which is successful in…

广义相对论与量子宇宙学 · 物理学 2019-11-18 Noshad Khosravi Largani , Mohammad Taghi Mirtorabi

X-rays and gamma-rays from astronomical sources such as solar flares are mostly absorbed by the Earth's atmosphere. Resulting electron-ion production rate as a function of height depends on the intensity and wavelength of the injected…

地球与行星天体物理 · 物理学 2016-04-27 Sourav Palit , Suman Ray , Sandip K. Chakrabarti

The QCD axion, originally proposed to solve the strong CP problem in QCD, is a prominent candidate for dark matter (DM). In the presence of strong magnetic fields, such as those around neutron stars, axions can theoretically convert into…

宇宙学与河外天体物理 · 物理学 2025-02-19 Luca Visinelli , Bradley Johnson , Bradley J. Kavanagh , David J. E. Marsh , Jordan E. Shroyer , Liam Walters

We reexamine the axion-photon couplings in various invisible axion models motivated by the recent proposal of using optical interferometry at the ASST facility in the SSCL to search for axion. We illustrate that the assignment of…

高能物理 - 唯象学 · 物理学 2009-10-28 S. L. Cheng , C. Q. Geng , W. -T. Ni

Experimental searches for axions or axion-like particles rely on semiclassical phenomena resulting from the postulated coupling of the axion to two photons. Sensitive probes of the extremely small coupling constant can be made by exploiting…

高能物理 - 实验 · 物理学 2010-09-28 Aaron S. Chou

We present a new mechanism to produce the dark photon ($\gamma'$) in the early universe with a help of the axion ($a$) using a recently proposed dark axion portal. The dark photon, a light gauge boson in the dark sector, can be a relic dark…

高能物理 - 唯象学 · 物理学 2017-07-05 Kunio Kaneta , Hye-Sung Lee , Seokhoon Yun

Evidence of magnetic interaction between late-type stars and close-in giant planets is provided by the observations of stellar hot spots rotating synchronously with the planets and showing an enhancement of chromospheric and X-ray fluxes.…

太阳与恒星天体物理 · 物理学 2015-05-13 A. F. Lanza

In the presence of a magnetic field, axions can convert into photons and vice versa. The phenomenology of the conversion is captured by a system of two coupled Klein-Gordon equations, which, assuming that the axion is relativistic, is…

高能物理 - 唯象学 · 物理学 2025-03-24 Clemente Smarra , Pierluca Carenza

The purpose of this paper is to assess the feasibility of axion detection by X-ray spectroscopy of the sun. We review the theory of axion-photon mode conversion with special attention to axions emitted in the 14.4 keV M1 decay of 57Fe at…

太阳与恒星天体物理 · 物理学 2015-06-15 J. Martin Laming

In this paper, we propose that the accelerated electrons in the quiet Sun could collide with the solar atmosphere to emit Hard X-rays (HXRs) via non-thermal bremsstrahlung, while some of these electrons would move upwards and escape into…

太阳与恒星天体物理 · 物理学 2016-05-31 Wen Wang , Linghua Wang , Sam Krucker , Iain Hannah

Chameleons are a well motivated scalar field that might explain the observed late time accelerated expansion of the universe. Chameleons possess the interesting property that their mass, and hence interaction range, is dependent on the…

宇宙学与河外天体物理 · 物理学 2013-09-27 Robert Poltis

The axion, as a leading dark matter candidate, is the target of many ongoing and proposed experimental searches based on its coupling to photons. Ultralight axions that couple to photons can also cause polarization rotation of light, which…

高能物理 - 唯象学 · 物理学 2024-10-08 Xucheng Gan , Lian-Tao Wang , Huangyu Xiao

Interstellar antiproton fluxes can arise from dark matter annihilating or decaying into quarks or gluons that subsequently fragment into antiprotons. Evaporation of primordial black holes also can produce a significant antiproton cosmic-ray…

高能物理 - 唯象学 · 物理学 2009-10-31 James D. Wells , Alexander Moiseev , Jonathan F. Ormes

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

We compute the X-ray spectra produced by non-static coronae atop accretion discs around black holes and neutron stars. The hot corona is radiatively coupled to the underlying disc (the reflector) and generates an X-ray spectrum which is…

天体物理学 · 物理学 2008-11-26 Julien Malzac , Andrei M. Beloborodov , Juri Poutanen