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The Sun is believed to have been the recipient of a substantial amount of metal-rich material over the course of its evolution, particularly in the early stages of the Solar System. With a long diffusion timescale, the majority of this…

Astrophysics · Physics 2009-11-07 R. A. Winnick , Pierre Demarque , Sarbani Basu , D. B. Guenther

All presently known stellar-dynamical constraints on the size and mass of the supermassive compact dark object at the Galactic center are consistent with a ball of self-gravitating, nearly non-interacting, degenerate fermions with mass…

Astrophysics · Physics 2007-05-23 Neven Bilic , Gary B. Tupper , Raoul D. Viollier

The Sun operates like a giant plasma diffuser that sorts lighter isotopes and elements to the solar surface. Measurements indicate that the interior of the Sun consists mostly of the same seven, even-numbered elements as ordinary…

Astrophysics · Physics 2007-05-23 O. Manuel

X-ray flares and other solar brightenings have been discarded as potential axion signatures. An axion X-ray signal must appear exclusively near the disk centre, and its spectrum must peak at ~4.2keV, contrary to observation. We argue here…

Astrophysics · Physics 2008-10-20 K. Zioutas , M. Tsagri , Y. Semertzidis , T. Papaevangelou

The XENON1T collaboration reported an excess of the low-energy electron recoil events between 1 and 7 keV. We explore the possibility to explain such an anomaly by the MeV-scale dark matter (DM) heated by the interior of the Sun due to the…

High Energy Physics - Phenomenology · Physics 2021-05-05 Yifan Chen , Ming-Yang Cui , Jing Shu , Xiao Xue , Guanwen Yuan , Qiang Yuan

For a given solar magnetic field, the near-Sun (phase-space) density of cosmic ray electrons and positrons of energy above about 10GeV can be calculated from first principles, without any assumptions about the cosmic ray diffusion. This is…

High Energy Astrophysical Phenomena · Physics 2013-04-22 Andrei Gruzinov

Millicharged dark matter particles can be efficiently captured by the Sun, where they annihilate into tau leptons, leading to the production of high-energy neutrinos. In contrast to the Earth, the high temperature of the Sun suppresses the…

High Energy Physics - Phenomenology · Physics 2024-07-09 Asher Berlin , Dan Hooper

Small-scale eruptions could play an important role in coronal heating, generation of solar energetic particles (SEPs), and mass source of the solar wind. However, they are poorly observed, and their characteristics, distributions, and…

Solar and Stellar Astrophysics · Physics 2024-10-24 Rui Wang , Ying D. Liu , Xiaowei Zhao , Huidong Hu

Current problems with the solar model may be alleviated if a significant amount of dark matter from the galactic halo is captured in the Sun. We discuss the capture process in the case where the dark matter is a Dirac fermion and the…

High Energy Physics - Phenomenology · Physics 2015-08-20 Mattias Blennow , Stefan Clementz

Neutrino produced in a chain of nuclear reactions in the Sun starting from the fusion of two protons, for the first time has been detected in a real-time detector in spectrometric mode. The unique properties of the Borexino detector…

Recently, Jenkins, et al. have reported the detection of correlations between fluctuations in nuclear decay rates and Earth-Sun distance, which suggest that nuclear decay rates can be affected by solar activity. In this paper, we report the…

Astrophysics · Physics 2010-07-07 Jere H. Jenkins , Ephraim Fischbach

Dark matter may be charged under dark electromagnetism with a dark photon that kinetically mixes with the Standard Model photon. In this framework, dark matter will collect at the center of the Earth and annihilate into dark photons, which…

High Energy Physics - Phenomenology · Physics 2017-10-05 Jonathan L. Feng , Jordan Smolinsky , Philip Tanedo

Chameleon particles, which could explain dark energy, are in many ways similar to axions, suggesting that an axion helioscope can be used for chameleon detection. The distinguishing property of chameleon particles is that, unlike Standard…

Solar and Stellar Astrophysics · Physics 2012-01-04 Keith Baker , Axel Lindner , Amol Upadhye , Konstantin Zioutas

The trajectories of dust particles ejected from a comet are affected by solar radiation pressure as a function of their ratios of radiation pressure cross section to mass. Therefore, a study on the orbital evolution of the particles caused…

Earth and Planetary Astrophysics · Physics 2015-06-12 Hiroshi Kobayashi , Hiroshi Kimura , Satoru Yamamoto

Galactic Dark Matter (DM) annihilations can produce cosmic-ray anti-nuclei via the nuclear coalescence of the anti-protons and anti-neutrons originated directly from the annihilation process. Since anti-deuterons have been shown to offer a…

High Energy Physics - Phenomenology · Physics 2016-08-25 Marco Cirelli , Nicolao Fornengo , Marco Taoso , Andrea Vittino

We present a novel mechanism of using solar neutrinos to speed up dark matter, inspired by the fact that neutrinos are the most energetic particles from the Sun with a well-understood spectrum. In a neutrino portal dark sector model, we…

High Energy Physics - Phenomenology · Physics 2022-01-25 Yue Zhang

Detection of daemons in low-background conditions in September 2005 and March 2006 has provided evidence for the expected to occur at that times maxima in the flux of daemons with V ~ 10-15 km s-1, which hit the Earth from near-Earth,…

Astrophysics · Physics 2008-11-26 E. M. Drobyshevski , M. E. Drobyshevski

Dark matter (DM) particles captured by the Sun can produce high energy electrons outside the Sun through annihilating into meta-stable mediators. The corresponding cosmic-ray electron signals observed by the space-based experiments will be…

High Energy Physics - Phenomenology · Physics 2022-04-27 Mohammadreza Zakeri , Yu-Feng Zhou

The physics of the solar dark matter (DM) that are captured and thermalise through the DM-nucleon interaction has been extensively studied. In this work, we consider the leptophilic DM scenario where the DM particles interact exclusively…

High Energy Physics - Phenomenology · Physics 2018-10-31 Zheng-Liang Liang , Yi-Lei Tang , Zi-Qing Yang