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We calculate the solar neutrino and antineutrino flux in the keV energy range. The dominant thermal source processes are photoproduction ($\gamma e\to e \nu\bar\nu$), bremsstrahlung ($e+Ze\to Ze+e+\nu\bar\nu$), plasmon decay…

High Energy Physics - Phenomenology · Physics 2017-12-14 Edoardo Vitagliano , Javier Redondo , Georg Raffelt

Limiting ourselves to two flavor approximation the motion of the neutrino flux in the solar matter and twisting magnetic field is considered. For the neutrino system described by the 4-component wave function $\Psi^T = (\nu_{eL}, \nu_{XL},…

High Energy Physics - Phenomenology · Physics 2016-10-26 O. M. Boyarkin , G. G. Boyarkina

The 48Ti on 40Ca reactions have been studied at 300 and 600 MeV focusing on the fusion-evaporation (FE) and fusion-fission (FF) exit channels. Energy spectra and multiplicities of the emitted light charged particles have been compared to…

Observations by the Fermi-LAT have uncovered a bright, spherically symmetric excess surrounding the center of the Milky Way galaxy. The spectrum of the gamma-ray excess peaks sharply at an energy ~2 GeV, exhibiting a hard spectrum at lower…

High Energy Astrophysical Phenomena · Physics 2017-02-28 Tim Linden , Nicholas L. Rodd , Benjamin R. Safdi , Tracy R. Slatyer

Conventional lore from Tremaine and Gunn excludes fermionic dark matter lighter than a few hundred eV, based on the Pauli exclusion principle. We highlight a simple way of evading this bound with a large number of species that leads to…

High Energy Physics - Phenomenology · Physics 2021-03-22 Hooman Davoudiasl , Peter B. Denton , David A. McGady

Neutrinos are produced in several neutrino nuclear reactions of the proton-proton chain and carbon-nitrogen-oxygen cycle that take place at different radius of the Sun's core. Hence, measurements of solar neutrino fluxes provide a precise…

Solar and Stellar Astrophysics · Physics 2013-10-01 Ilidio Lopes , Joseph Silk

The all-flavor solar neutrino flux measured by the Sudbury Neutrino Observatory (SNO) constrains nonstandard energy losses to less than about 10% of the Sun's photon luminosity, superseding a helioseismological argument and providing new…

Astrophysics · Physics 2010-04-30 Paolo Gondolo , Georg Raffelt

Motivated by recent data on comets in the low corona, we discuss destruction of sun impacting comets in the dense lower solar atmosphere. Perihelion distances q less than the solar radius and incident masses Mo much greater than 1E12 g are…

Solar and Stellar Astrophysics · Physics 2015-07-22 John C. Brown , Robert W. Carlson , Mark P. Toner

We revisit the flux of chameleons (light scalar particles which could play a role in the dark energy phenomenon) produced in the interior of the Sun. Our novel analysis incorporates various important details and new processes that have…

High Energy Physics - Phenomenology · Physics 2024-09-16 Tomás O'Shea , Anne-Christine Davis , Maurizio Giannotti , Sunny Vagnozzi , Luca Visinelli , Julia K. Vogel

Isospin e ffects on multifragmentation properties were studied thanks to nuclear collisions between di fferent isotopes of xenon beams and tin targets. It is shown that, in central collisions leading to multifragmentation, the mean number…

Heat and charge transport were used to probe the magnetic field-tuned quantum critical point in the heavy-fermion metal CeCoIn$_5$. A comparison of electrical and thermal resistivities reveals three characteristic energy scales. A…

Strongly Correlated Electrons · Physics 2007-05-23 Johnpierre Paglione , M. A. Tanatar , D. G. Hawthorn , F. Ronning , R. W. Hill , M. Sutherland , Louis Taillefer , C. Petrovic

We present a new method for probing the thermal electron content of the Galaxy by spectral analysis of background point sources in the absorption-only limit to the radiative transfer equation. In this limit, calculating the spectral index,…

High Energy Astrophysical Phenomena · Physics 2016-05-25 D. I. Jones , A. P. Igoshev , M. Haverkorn

We search for an excess of electrons and positrons in the interplanetary space from the decays of heavy neutrinos produced in nuclear reactions in the Sun. Using measurements of the electron spectra in the MeV range from the Ulysses and…

High Energy Astrophysical Phenomena · Physics 2025-05-14 Marco Drewes , Jan Heisig , Valentin Weber

Recent radio observations support a picture for star formation where there is accretion of matter onto a central protostar with the ejection of molecular outflows that can affect the surrounding medium. The impact of a supersonic outflow on…

Astrophysics · Physics 2011-03-10 A. T. Araudo , G. E. Romero , V. Bosch-Ramon , J. M. Paredes

We explore the effects of electromagnetic (EM) fluctuations in plasmas on solar neutrino fluxes exploiting the fluctuation-dissipation theorem. We find that the EM spectrum in the solar core is enhanced by the EM fluctuations due to the…

Using the bimetric formalism, we compute the production and emission rates of light spin-2 particles in non-degenerate stellar interiors through photoproduction and bremsstrahlung processes, including the effects of plasma screening. By…

High Energy Physics - Phenomenology · Physics 2025-11-06 Camilo García-Cely , Andreas Ringwald

We present the results of 720 hours of observations of transient solar events at ground level, during the summer season 2005 (Souther Hemisphere). Data were taken with the TUPI muon telescope, working at a high counting rate (up to 100 KHz)…

Astrophysics · Physics 2016-08-30 C. E. Navia , C. R. A. Augusto , M. B. Robba

Some models of inelastic dark matter posit the existence of bound states under some new $U(1)'$ gauge symmetry. If this new dark photon kinetically mixes with the standard model photon, then the constituent particles in these bound states…

High Energy Physics - Phenomenology · Physics 2014-12-03 Audrey K. Kvam , David C. Latimer

Recent results from the PAMELA, ATIC, PPB BETS and Fermi collaborations extend the energy range in the electron flux measurement up to unexplored energies in the hundred GeVs range confirming the bump starting at about 10GeV already…

High Energy Astrophysical Phenomena · Physics 2014-11-18 Ignacio Cernuda