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Related papers: Constraints on millicharged particles from nuclear…

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It has been recently suggested that the vacuum magnetic dichroism observed by the PVLAS experiment could be explained by the pair production of a new light, m ~0.1 eV, millicharged, q ~ 3 10^{-6} e, fermions. In addition, it has been…

High Energy Physics - Phenomenology · Physics 2008-11-26 S. N. Gninenko , N. V. Krasnikov , A. Rubbia

It is postulated that heavy dark matter $\phi$ with a mass on the order of TeV, once captured by the Earth, can decay into relativistic milli-charged particles (MCPs). These MCPs are potentially detectable at the IceCube neutrino telescope.…

High Energy Astrophysical Phenomena · Physics 2025-12-01 Ye Xu

Particles with millicharge q and sub-eV mass can be produced in photon-photon collisions, distorting the energy spectrum of the Cosmic Microwave Background. We derive the conservative bound q < 10^-7 e (as well as model-dependent bounds two…

High Energy Physics - Phenomenology · Physics 2008-11-26 Alessandro Melchiorri , Antonello Polosa , Alessandro Strumia

The Gamma Factory (GF) is an ambitious proposal, currently explored within the CERN Physics Beyond Colliders program, for a source of photons with energies up to $\approx 400\,$MeV and photon fluxes (up to $\approx 10^{17}$ photons per…

Ultra-high energy cosmic rays interacting with the radiation fields in the universe cause electromagnetic cascades resulting in a flux of extragalactic gamma rays, detectable to some 100 GeV. Recent precise measurements of the extragalactic…

High Energy Astrophysical Phenomena · Physics 2015-06-19 A. D. Erlykin , A. W. Wolfendale

Light millicharged particles can be copiously produced from meson decays in cosmic ray collisions with the atmosphere, leading to detectable signals in large underground neutrino detectors. In this paper we study a new channel for…

High Energy Physics - Phenomenology · Physics 2025-07-24 Mingxuan Du , Rundong Fang , Zuowei Liu

High flux of electron neutrinos($\nue$) is produced at nuclear power reactors through the decays of nuclei activated by neutron capture. Realistic simulation studies on the neutron transport and capture at the reactor core were performed.…

High Energy Physics - Experiment · Physics 2009-09-29 B. Xin , TEXONO Collaboration

The location of the (gamma,p)/(gamma,n) and (gamma,alpha)/(gamma,n) line at gamma-process temperatures is discussed, using updated reaction rates based on global Hauser-Feshbach calculations. The results can directly be compared to classic…

Astrophysics · Physics 2007-05-23 T. Rauscher

Particles with electric charge q < 10^(-3)e and masses in the range 1--100 MeV/c^2 are not excluded by present experiments. An experiment uniquely suited to the production and detection of such "millicharged" particles has been carried out…

The IceCube Neutrino Observatory at the South Pole has measured astrophysical neutrinos using through-going and starting events in the TeV to PeV energy range. The origin of these astrophysical neutrinos is still largely unresolved, and…

High Energy Astrophysical Phenomena · Physics 2023-02-01 Barbara Skrzypek , Marco Chianese , Carlos Argüelles Delgado

With the high resolution of microcalorimeter detectors, previously unresolvable gamma-ray lines are now clearly resolvable. A careful measurement of Am-241 decay with a large array of gamma-ray microcalorimeters has revealed never before…

The relic abundance of light millicharged particles (MCPs) with the electric charge $e' = 5\cdot 10^{-5} e$ and with the mass slightly below or above the electron mass is calculated. The abundance depends on the mass ratio $\eta=m_X/m_e$…

High Energy Physics - Phenomenology · Physics 2017-05-18 A. D. Dolgov , A. S. Rudenko

Dark matter annihilation and other processes may precipitate a flux of diffuse ultra-high energy $\gamma$-rays. These $\gamma$-rays may be observable in present day experiments which observe diffuse fluxes at the GeV scale. Yet the universe…

Astrophysics · Physics 2007-05-23 John A. Cairns

It is assumed that heavy dark matter $\phi$ with O(TeV) mass captured by the Earth may decay to relativistic light milli-charged particles (MCPs). These MCPs could be measured by the IceCube neutrino telescope. The massless hidden photon…

High Energy Astrophysical Phenomena · Physics 2024-05-02 Ye Xu

Diffuse ultrahigh energy gamma-radiation can arise from a variety of astrophysical sources, including the interaction of extremely high energy cosmic rays with the 3K microwave background radiation or the collapse of topological defects…

Astrophysics · Physics 2011-08-17 MIA Collaboration

Superheavy (SH) quasistable particles generated in the Early Universe could be responsable for Ultra High Energy Cosmic Rays (UHECR) and be a component of Cold Dark Matter (CDM) in the universe. These particles are likely to cluster in the…

Astrophysics · Physics 2009-10-31 Pasquale Blasi

We conduct a dedicated study of searches for millicharged particles (mCPs) utilizing scintillator-based detectors at high-intensity fixed-target experiments, with particular focus on the SpinQuest and forthcoming Search for Hidden Particles…

High Energy Physics - Phenomenology · Physics 2025-12-15 Leo Bailloeul , Matthew Citron , Yanou Cui , Saeid Foroughi-Abari , Insung Hwang , Fengyi Li , Yu-Dai Tsai , Ming Xiong Liu , Kranti Gunthoti , Jae Hyeok Yoo

We propose a high statistics experiment to search for invisible decay modes in nuclear gamma cascades. A radioactive source (such as $^{60}$Co or $^{24}$Na) that triggers gamma cascades is placed in the middle of a large, hermetically…

High Energy Physics - Phenomenology · Physics 2019-02-27 Giovanni Benato , Alexey Drobizhev , Surjeet Rajendran , Harikrishnan Ramani

We explore the possibility that the astrophysical neutrinos are produced in $pp$-interactions with a gas cloud near the source acting as a beam dump, which is sufficiently dense to significantly attenuate the associated gamma-ray flux…

High Energy Astrophysical Phenomena · Physics 2020-04-08 Matthias Vereecken , Krijn D. de Vries

The Gamma Factory is a proposal to back-scatter laser photons off a beam of partially-stripped ions at the LHC, producing a beam of $\sim 10$ MeV to $1$ GeV photons with intensities of $10^{16}$ to $10^{18}~\text{s}^{-1}$. This implies…

High Energy Physics - Phenomenology · Physics 2021-09-23 Sreemanti Chakraborti , Jonathan L. Feng , James K. Koga , Mauro Valli