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We propose a solar production mechanism of MeV dark matter to overcome the energy threshold in direct detection experiments. In particular, the proton and deuteron fussion to ${}^3 \mathrm{He}$ of the $pp$ chain that produces energetic…

高能物理 - 唯象学 · 物理学 2025-12-09 Shao-Feng Ge , Jie Sheng , Chen Xia , Chuan-Yang Xing

Despite significant efforts over the past decade, the origin of the cosmic ray positron excess has still not been unambiguously established. A popular class of candidate sources are pulsars or pulsar wind nebulae but these cannot also…

高能天体物理现象 · 物理学 2021-12-13 Philipp Mertsch , Andrea Vittino , Subir Sarkar

We investigate the consequences of models where dark sector quarks could be produced at the LHC, which subsequently undergo a dark parton shower, generating jets of dark hadrons that ultimately decay back to Standard Model hadrons. This…

高能物理 - 唯象学 · 物理学 2023-08-16 Timothy Cohen , Jennifer Roloff , Christiane Scherb

A precise understanding of the radio emission from extensive air showers is of fundamental importance for the design of cosmic ray radio detectors as well as the analysis and interpretation of their data. In recent years, tremendous…

高能天体物理现象 · 物理学 2015-06-12 T. Huege

Radio detection of cosmic-ray-induced air showers has come to a flight the last decade. Along with the experimental efforts, several theoretical models were developed. The main radio-emission mechanisms are established to be the geomagnetic…

高能天体物理现象 · 物理学 2013-04-05 Krijn D. de Vries , Olaf Scholten , Klaus Werner

Dark matter is poorly constrained by direct detection experiments at masses below 1 MeV. This is an important target for the next generation of experiments, and several methods have been proposed to probe this mass range. One class of such…

高能物理 - 唯象学 · 物理学 2020-07-31 Benjamin V. Lehmann , Stefano Profumo

A Monte-Carlo study is presented using ground based measurements of the electromagnetic part of showers initiated in the atmosphere by high energetic cosmic rays to reconstruct energy and mass of primary particles with energies above 300…

天体物理学 · 物理学 2011-04-15 A. Lindner

The effect of a magnetized plasma on the resonant photoproduction of axions on the electromagnetic multipole components of the medium, $i \to f+a$, has been considered. It has been shown that the axion resonant emissivity, due to various…

高能物理 - 唯象学 · 物理学 2010-09-30 N. V. Mikheev , D. A. Rumyantsev , Yu. E. Shkol'nikova

Long-lived particles are predicted in extensions of the Standard Model that involve relatively light but very weakly interacting sectors. In this paper we consider the possibility that some of these particles are produced in atmospheric…

高能物理 - 唯象学 · 物理学 2020-03-18 Carlos Argüelles , Pilar Coloma , Pilar Hernández , Víctor Muñoz

We discuss the possibility of solving the inverse problem of the cosmic-ray electron/positron from decaying/annihilating dark matter, and show simple analytic formulae to reconstruct the source spectrum of the electron/positron from the…

高能物理 - 唯象学 · 物理学 2009-10-02 Koichi Hamaguchi , Kouhei Nakaji , Eita Nakamura

The zenith angle distributions of atmospheric neutrinos are determined by the possible presence of neutrino oscillations and the combination of three most important contributions: (1) geomagnetic effects on the primary cosmic rays, that…

高能物理 - 唯象学 · 物理学 2011-05-23 Paolo Lipari

The detection of atmospheric fluorescence light from extensive air showers has become a powerful tool for accurate measurements of the energy and mass of ultra-high energy cosmic ray particles. Employing large area imaging telescopes with…

天体物理仪器与方法 · 物理学 2009-07-22 Daniel Kruppke-Hansen , Karl-Heinz Kampert

The existence of a large primordial neutrino asymmetry is an intriguing possibility, both observationally and theoretically. Such an asymmetry can lead to the resonant production of $\mathrm{keV}$-scale sterile neutrinos, which are a…

高能物理 - 唯象学 · 物理学 2025-10-08 Kentaro Kasai , Masahiro Kawasaki , Kai Murai

Ultra-high energy cosmic rays can be measured through the detection of radio-frequency radiation from air showers. The radio-frequency emission originates from deflections of the air-shower particles in the geomagnetic field and from a…

高能天体物理现象 · 物理学 2018-10-01 Christian Glaser , Sijbrand de Jong , Martin Erdmann , Jörg R. Hörandel

Sub-MeV cold dark-matter particles are unable to produce electronic recoil in conventional dark-matter direct detection experiments such as XENONnT and LUX-ZEPLIN above the detector threshold. The mechanism of boosted dark matter comes into…

高能物理 - 唯象学 · 物理学 2024-08-08 Atanu Guha , Jong-Chul Park

I describe a dark matter candidate based in qcd physics in which the dark matter is composed of macroscopically large "nuggets" of quark and anti-quark matter. These objects may have a sufficiently massive low number density to avoid…

高能天体物理现象 · 物理学 2010-12-01 Kyle Lawson

We show that the existence of low scale gravity at TeV scale could lead to a direct production of photons with energies above 10^22 eV due to annihilation of ultra high energy neutrinos on relic massive neutrinos of the galactic halo. Air…

天体物理学 · 物理学 2009-10-31 R. V. Konoplich , S. G. Rubin

We have investigated exclusive photoproduction of light vector mesons ($\omega$, $\rho$ and $\phi$) on the nucleon at low energies. In order to explore the questions concerning the so-called missing nucleon resonances, we first establish…

核理论 · 物理学 2007-05-23 Yongseok Oh , Alexander I. Titov , T. -S. Harry Lee

We revisit and extend the analysis supporting a 60 year-old suggestion that cosmic rays air showers resulting from primary particles with energies above 10^{18} eV should be straightforward to detect with radar ranging techniques, where the…

高能物理 - 实验 · 物理学 2011-05-23 Peter. W. Gorham

We show that all features of the ultrahigh energy cosmic ray spectrum from 10^{17} eV to 10^{21} eV can be described with a simple power-like injection spectrum of protons under the assumption that the neutrino-nucleon cross-section is…

高能物理 - 唯象学 · 物理学 2007-05-23 Z. Fodor , S. D. Katz , A. Ringwald , H. Tu