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Related papers: The Gallium Anomaly

200 papers

PKS J2310-437 is an AGN with bright X-ray emission relative to its weak radio emission and optical continuum. It is believed that its jet lies far enough from the line of sight that it is not highly relativistically beamed. It thus provides…

High Energy Astrophysical Phenomena · Physics 2009-11-16 A. F. Bliss , D. M. Worrall , M. Birkinshaw , S. S. Murray , H. Tananbaum

The rapid neutron-capture ($r$-process) element europium (Eu) is a valuable tracer of neutron star mergers and other rare nucleosynthetic events. The stellar spectroscopic survey GALAH's unique wavelength range and setup include the Eu…

Astrophysics of Galaxies · Physics 2025-12-03 Sarah G. Kane , Zofia Kaczmarek , Andrew Garner , Sven Buder , Stephanie Monty , Elana Kane

We analyzed the electron neutrino data of the Gallium radioactive source experiments and the electron antineutrino data of the reactor Bugey and Chooz experiments in terms of neutrino oscillations. We found a hint of a CPT-violating…

High Energy Physics - Phenomenology · Physics 2015-05-20 Carlo Giunti , Marco Laveder

The bulk of X-ray spectroscopic studies of active galactic nuclei (AGN) are focused on local ($z < 0.1$) sources with low-to-moderate ($< 0.3$) Eddington ratio ($\lambda_\mathrm{Edd}$). It is then mandatory to overcome this limitation and…

Astrophysics of Galaxies · Physics 2023-04-03 M. Laurenti , F. Tombesi , F. Vagnetti , E. Piconcelli , M. Guainazzi , R. Middei

Numerous particle physics experiments utilize gadolinium (Gd), a rare earth element with the most significant neutron capture cross-section among all elements, to detect anti-neutrinos via inverse beta-decays or to remove neutron-induced…

Instrumentation and Detectors · Physics 2023-06-13 Y. Sakakieda , K. Hosokawa , F. Nakanishi , Y. Hino , Y. Inome , A. Sakaguchi , Y. Takaku , M. Ikeda , H. Sekiya

We collect data at all frequencies for the new sources classified as unknown active galactic nuclei (AGNs) in the latest Burst Alert Telescope (BAT) all-sky hard X-ray catalog. Focusing on the 36 sources with measured redshift, we compute…

High Energy Astrophysical Phenomena · Physics 2021-04-07 Luca Giuliani , Gabriele Ghisellini , Tullia Sbarrato

Possibilities of discriminating neutrons and gamma rays in the AGATA gamma-ray tracking spectrometer have been investigated with the aim of reducing the background due to inelastic scattering of neutrons in the high-purity germanium…

Nuclear Experiment · Physics 2009-09-09 A. Ataç , A. Kaşkaş , S. Akkoyun , M. Şenyiğit , T. Hüyük , S. O. Kara , J. Nyberg

The detection of new clusters of galaxies or the study of known clusters of galaxies in X-rays can be complicated by the presence of X-ray point sources, the majority of which will be active galactic nuclei (AGN). This can be addressed by…

High Energy Astrophysical Phenomena · Physics 2019-06-26 Ben J. Maughan , Thomas H. Reiprich

We present optical and X-ray data for a sample of serendipitous XMM-Newton sources that are selected to have 0.5-2 keV vs 2-4.5 keV X-ray hardness ratios which are harder than the X-ray background. The sources have 2-4.5 keV X-ray flux >=…

Time variability is a strong probe of energetic phenomena which occur at small spatial scales, like Active Galactic Nuclei (AGN). We use ALMA observations at 100 GHz executed over a period of 2.5 months to look for time variability in the…

A search for cosmic neutrino sources using six years of data collected by the ANTARES neutrino telescope has been performed. Clusters of muon neutrinos over the expected atmospheric background have been looked for. No clear signal has been…

High Energy Physics - Experiment · Physics 2018-06-13 ANTARES Collaboration , S. Adrián-Martínez , A. Albert , M. André , M. Anghinolfi , G. Anton , M. Ardid , J. -J. Aubert , B. Baret , J. Barrios-Martí , S. Basa , V. Bertin , S. Biagi , C. Bogazzi , R. Bormuth , M. Bou-Cabo , M. C. Bouwhuis , R. Bruijn , J. Brunner , J. Busto , A. Capone , L. Caramete , C. Cârloganu , J. Carr , T. Chiarusi , M. Circella , L. Core , H. Costantini , P. Coyle , A. Creusot , C. Curtil , G. De Rosa , I. Dekeyser , A. Deschamps , G. De Bonis , C. Distefano , C. Donzaud , D. Dornic , Q. Dorosti , D. Drouhin , A. Dumas , T. Eberl , D. Elsässer , A. Enzenhöfer , S. Escoffier , K. Fehn , I. Felis , P. Fermani , F. Folger , L. A. Fusco , S. Galatà , P. Gay , S. Geißelsöder , K. Geyer , V. Giordano , A. Gleixner , J. P. Gómez-González , K. Graf , G. Guillard , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , B. Herold , A. Herrero , J. Hößl , J. Hofestädt , C. W James , M. de Jong , M. Kadler , O. Kalekin , U. Katz , D. Kießling , P. Kooijman , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , E. Lambard , G. Lambard , D. Lattuada , D. Lefèvre , E. Leonora , H. Loehner , S. Loucatos , S. Mangano , M. Marcelin , A. Margiotta , J. A. Martínez-Mora , S. Martini , A. Mathieu , T. Michael , P. Migliozzi , C. Mueller , M. Neff , E. Nezri , D. Palioselitis , G. E. Păvălaş , C. Perrina , P. Piattelli , V. Popa , T. Pradier , C. Racca , G. Riccobene , R. Richter , K. Roensch , A. Rostovtsev , M. Saldaña , D. F. E. Samtleben , A. Sánchez-Losa , M. Sanguineti , P. Sapienza , J. Schmid , J. Schnabe , S. Schulte , F. Schüssler , T. Seitz , C. Sieger , A. Spies , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , M. Taiuti , C. Tamburini , Y. Tayalati , A. Trovato , B. Vallage , C. Vallée , V. Van Elewyck , E. Visser , D. Vivolo , S. Wagner , J. Wilms , E. de Wolf , K. Yatkin , H. Yepes , J. D. Zornoza , J. Zúñiga

Most heavy elements beyond the iron peak are synthesized via neutron capture processes. The nature of the astrophysical sites of neutron capture processes is still very unclear. In this work we explore the observational constraints of the…

Solar and Stellar Astrophysics · Physics 2023-09-25 Jianhui Lian , Nicholas Storm , Guillaume Guiglion , Aldo Serenelli , Benoit Cote , Amanda I. Karakas , Nick Boardman , Maria Bergemann

Since the GALLEX and GNO datasets were derived from closely related experiments, there is a natural tendency to merge them. This is perhaps appropriate for any analysis based on the hypothesis that the solar neutrino flux is constant, but…

High Energy Physics - Phenomenology · Physics 2008-11-26 P. A. Sturrock , D. O. Caldwell , J. D. Scargle

We propose a mechanism which provides an explanation of the Gallium and antineutrino reactor anomalies. Differently from original Pontecorvo's hypothesis, this mechanism is based on the phenomenological assumption in which the admixture of…

High Energy Physics - Phenomenology · Physics 2015-06-15 M. M. Guzzo , P. C. de Holanda , O. L. G. Peres , E. M. Zavanin

The $^8$B solar neutrino flux as measured by Super-Kamiokande is consistent with the $^{37}$Ar production rate in $^{37}$Cl at Homestake. GALLEX and SAGE, continue to observe $^{71}$Ge production rates in $^{71}$Ga that are consistent with…

Astrophysics · Physics 2011-04-15 Arnon Dar , Giora Shaviv

The GERmanium Detector Array, GERDA, searches for neutrinoless double beta decay in Ge-76 using bare high-purity germanium detectors submerged in liquid argon. For the calibration of these detectors gamma emitting sources have to be lowered…

Instrumentation and Detectors · Physics 2013-08-13 Laura Baudis , Alfredo D. Ferella , Francis Froborg , Michal Tarka

Background: Neutron-induced backgrounds are a significant concern for experiments that require extremely low levels of radioactive backgrounds such as direct dark matter searches and neutrinoless double-beta decay experiments. Unmeasured…

Coherent elastic neutrino-nucleus scattering (CE$\nu$NS) is a dominant low-energy neutrino interaction that remains experimentally challenging due to its weak-scale cross section and the small nuclear recoil energies involved. This thesis…

Instrumentation and Detectors · Physics 2026-03-18 Leire Larizgoitia
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