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Related papers: The Sun in Hidden Photons

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Dark photon as an ultralight dark matter candidate can interact with the Standard Model particles via kinetic mixing. We propose to search for the ultralight dark photon dark matter using radio telescopes with solar observations. The dark…

High Energy Physics - Phenomenology · Physics 2021-05-07 Haipeng An , Fa Peng Huang , Jia Liu , Wei Xue

The Sun emits copious amounts of photons and neutrinos in an approximately spatially isotropic distribution. Diffuse $\gamma$-rays and ultra-high energy (UHE) neutrinos from extragalactic sources may subsequently interact and annihilate…

High Energy Astrophysical Phenomena · Physics 2024-07-22 Shyam Balaji

Light extra U(1) gauge bosons, so called hidden photons, which reside in a hidden sector have attracted much attention since they are a well motivated feature of many scenarios beyond the Standard Model and furthermore could mediate the…

High Energy Physics - Phenomenology · Physics 2013-11-22 Sarah Andreas , Mark D. Goodsell , Andreas Ringwald

Common extensions of the Standard Model of particle physics predict the existence of a "hidden" sector that comprises particles with a vanishing or very weak coupling to particles of the Standard Model (visible sector). For very light (m <…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 A. P. Lobanov , H. -S. Zechlin , D. Horns

If Dark Matter is composed of hidden-sector photons that kinetically mix with photons of the visible sector, then Dark Matter has a tiny oscillating electric field component. Its presence would lead to a small amount of visible radiation…

Instrumentation and Detectors · Physics 2014-10-02 Babette Döbrich , Kai Daumiller , Ralph Engel , Marek Kowalski , Axel Lindner , Javier Redondo , Markus Roth

The possibility of estimating the mass composition of primary cosmic rays above the knee of its energy spectrum through the study of high energy gamma rays, muons and neutrinos produced in the interactions of cosmic rays with the solar…

High Energy Astrophysical Phenomena · Physics 2017-04-05 Prabir Banik , Biplab Bijay , Samir K. Sarkar , Arunava Bhadra

We present some bottom-up motivations of axions and other weakly interacting sub-eV particles (WISPs) coupling to photons. Typically, these light particles are strongly constrained by their production or interaction in astrophysical and…

High Energy Physics - Phenomenology · Physics 2009-10-13 Markus Ahlers

The hope is that in the near future neutrino astronomy, born with the identification of thermonuclear fusion in the sun and the particle processes controlling the fate of a nearby supernova, will reach throughout and beyond our Galaxy and…

Astrophysics · Physics 2009-10-28 S. Barwick , F. Halzen , P. B. Price

High energy neutrinos are produced by the annihilation of dark matter particles in our galaxy. These are presently searched for with large area, deep underground neutrino telescopes. Cold dark matter particles, trapped inside the sun, are…

High Energy Physics - Phenomenology · Physics 2009-09-25 F. Halzen , J. E. Jacobsen

In this Letter we report on the results of our search for photons from a U(1) gauge factor in the hidden sector of the full theory. With our experimental setup we observe the single spectrum in a HPGe detector arising as a result of the…

High Energy Physics - Experiment · Physics 2013-04-16 R. Horvat , D. Kekez , M. Krcmar , Z. Krecak , A. Ljubicic

We present prospects of two experiments using the Tokyo Axion Helioscope. One is a search for solar axions. In the past measurements, axion mass from 0 to 0.27 eV and from 0.84 to 1.00 eV have been scanned and no positive evidence was seen.…

Instrumentation and Methods for Astrophysics · Physics 2010-02-04 R. Ohta , M. Minowa , Y. Inoue , Y. Akimoto , T. Mizumoto , A. Yamamoto

Astrophysical neutrinos can be produced in proton interactions of charged cosmic rays with ambient photon or baryonic fields. Cosmic rays are observed in balloon, satellite and air shower experiments every day, from below 1e9 eV up to…

Astrophysics · Physics 2008-12-18 Julia K. Becker

The magnetic fields that emerge from beneath the solar surface and permeate the solar atmosphere are the key drivers of space weather and, thus, understanding them is important to human society. Direct observations, used to measure magnetic…

Solar and Stellar Astrophysics · Physics 2024-05-29 Kenny C. Y. Ng , Andrew Hillier , Shin'ichiro Ando

Top-down models of cosmic rays produce more neutrinos than photons and more photons than protons. In these models, we reevaluate the fluxes of neutrinos associated with the highest energy cosmic rays in light of mounting evidence that they…

High Energy Physics - Phenomenology · Physics 2014-11-17 C. Barbot , M. Drees , F. Halzen , D. Hooper

Neutrino astrophysics offers new perspectives on the Universe investigation: high energy neutrinos, produced by the most energetic phenomena in our Galaxy and in the Universe, carry complementary (if not exclusive) information about the…

High Energy Astrophysical Phenomena · Physics 2010-02-11 T. Chiarusi , M. Spurio

Solar nuclear reactions can occasionally produce sub-MeV elusive beyond the Standard Model particles that escape the solar interior without further interactions. This study focuses on massive spin-one particles. We construct the general…

High Energy Physics - Phenomenology · Physics 2023-12-29 Francesco D'Eramo , Giuseppe Lucente , Newton Nath , Seokhoon Yun

Hidden sectors in connection with GeV-scale dark forces and dark matter are not only a common feature of physics beyond the Standard Model such as string theory and SUSY but are also phenomenologically of great interest regarding recent…

High Energy Physics - Phenomenology · Physics 2012-11-22 Sarah Andreas

I discuss the recent exciting results of discovery of TeV photons from several galactic and extragalactic sources, and highlight some objectives of VHE gamma ray astronomy that can be achieved in the near future by means of new generation…

Astrophysics · Physics 2007-05-23 F. A. Aharonian

ANTARES is the first neutrino telescope in the sea. It consists of a three-dimensional array of 885 photomultipliers to collect the Cherenkov light induced by relativistic muons produced in CC interactions of high energy neutrinos. One of…

High Energy Astrophysical Phenomena · Physics 2015-06-04 J. D. Zornoza

High-energy photons with $\mathcal{O}$(MeV) energies from radioactive contaminants can scatter in a solid-state target material and constitute an important low-energy background for sub-GeV dark matter direct-detection searches. This…

High Energy Physics - Phenomenology · Physics 2022-08-17 Kim V. Berghaus , Rouven Essig , Yonit Hochberg , Yutaro Shoji , Mukul Sholapurkar