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The experiments reveal the strong narrow band in the spectra of the emission from Au-film on the Cu substrate. The emission was excited by red He-Ne laser in standard geometry for Raman back-scattering experiments. Some additional…

Materials Science · Physics 2017-02-21 M. E. Kompan , B. A. -T. Melekh , S. E. Nikitin

Several cosmic ray experiments have measured excesses in electrons and positrons, relative to standard backgrounds, for energies from ~ 10 GeV - 1 TeV. These excesses could be due to new astrophysical sources, but an explanation in which…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Spencer Chang , Lisa Goodenough

We propose a {\em boomerang mechanism} for the explanation of the excess radio background detected by ARCADE. In an early stage, at a temperature $T \sim 100\,{\rm keV}$, a fraction of relic neutrinos is resonantly converted into dark…

High Energy Physics - Phenomenology · Physics 2025-10-14 Bhupal Dev , Pasquale Di Bari , Ivan Martinez-Soler , Rishav Roshan

Aluminum nitride (AlN) plays a key role in modern power electronics and deep-ultraviolet photonics, where an understanding of its thermal properties is essential. Here we measure the thermal conductivity of crystalline AlN by the…

Nuclear recoil measurements with high-purity Germanium detectors are very promising to directly detect dark matter candidates. The main background sources in such experiments are natural radioactivity and microphonic noise. Digital pulse…

High Energy Physics - Experiment · Physics 2009-10-31 L. Baudis , J. Hellmig , H. V. Klapdor-Kleingrothaus , Y. Ramachers , J. W. Hammer , A. Mayer

Solar neutrino detection is known to be a very challenging task, due to the minuscule absorption cross-section and mass of the neutrino. One research showed that relative large solar-flares affected the decay-rates of Mn-54 in December…

Solar and Stellar Astrophysics · Physics 2022-01-11 Jonathan Walg , Anatoly Rodnianski , Itzhak Orion

An X-ray detector based on the combination of an integrated Micromegas stage with a pixel chip has been built in order to be installed at the CERN Axion Solar Telescope. Due to its high granularity and spatial resolution this detector…

Instrumentation and Detectors · Physics 2014-10-02 Christoph Krieger , Klaus Desch , Jochen Kaminski , Michael Lupberger , Theodoros Vafeiadis

We report ALMA observations of molecular gas and continuum emission in the 90 and 350 GHz bands toward a nearby Seyfert galaxy NGC 613. Radio continuum emissions were detected at 95 and 350 GHz from both the circum-nuclear disk (CND)…

Astrophysics of Galaxies · Physics 2018-02-05 Yusuke Miyamoto , Naomasa Nakai , Masumichi Seta , Dragan Salak , Makoto Nagai , Hiroyuki Kaneko

The experiment "Neutrino-4" started in 2014 on a model, then it was continued on a full-scale detector, and now, has provided the measurement result on dependence of the flux and spectrum of reactor antineutrinos on the distance of 6 - 12…

The Standard Model of particle physics cannot explain the dominance of matter over anti-matter in our Universe. In many model extensions this is a very natural consequence of neutrinos being their own anti-particles (Majorana particles)…

Nuclear Experiment · Physics 2017-04-07 M. Agostini , M. Allardt , A. M. Bakalyarov , M. Balata , I. Barabanov , L. Baudis , C. Bauer , E. Bellotti , S. Belogurov , S. T. Belyaev , G. Benato , A. Bettini , L. Bezrukov , T. Bode , D. Borowicz , V. Brudanin , R. Brugnera , A. Caldwell , C. Cattadori , A. Chernogorov , V. D'Andrea , E. V. Demidova , N. DiMarco , A. diVacri , A. Domula , E. Doroshkevich , V. Egorov , R. Falkenstein , O. Fedorova , K. Freund , N. Frodyma , A. Gangapshev , A. Garfagnini , C. Gooch , P. Grabmayr , V. Gurentsov , K. Gusev , J. Hakenmüller , A. Hegai , M. Heisel , S. Hemmer , W. Hofmann , M. Hult , L. V. Inzhechik , J. Janicskó Csáthy , J. Jochum , M. Junker , V. Kazalov , T. Kihm , I. V. Kirpichnikov , A. Kirsch , A. Kish , A. Klimenko , R. Kneißl , K. T. Knöpfle , O. Kochetov , V. N. Kornoukhov , V. V. Kuzminov , M. Laubenstein , A. Lazzaro , V. I. Lebedev , B. Lehnert , H. Y. Liao , M. Lindner , I. Lippi , A. Lubashevskiy , B. Lubsandorzhiev , G. Lutter , C. Macolino , B. Majorovits , W. Maneschg , E. Medinaceli , M. Miloradovic , R. Mingazheva , M. Misiaszek , P. Moseev , I. Nemchenok , D. Palioselitis , K. Panas , L. Pandola , K. Pelczar , A. Pullia , S. Riboldi , N. Rumyantseva , C. Sada , F. Salamida , M. Salathe , C. Schmitt , B. Schneider , S. Schönert , J. Schreiner , O. Schulz , A. -K. Schütz , B. Schwingenheuer , O. Selivanenko , E. Shevchik , M. Shirchenko , H. Simgen , A. Smolnikov , L. Stanco , L. Vanhoefer , A. A. Vasenko , A. Veresnikova , K. von Sturm , V. Wagner , M. Walter , A. Wegmann , T. Wester , C. Wiesinger , M. Wojcik , E. Yanovich , I. Zhitnikov , S. V. Zhukov , D. Zinatulina , K. Zuber , G. Zuzel

The GERmanium Detector Array (GERDA) experiment at the Gran Sasso underground laboratory (LNGS) of INFN is searching for neutrinoless double-beta ($0\nu\beta\beta$) decay of $^{76}$Ge. The technological challenge of GERDA is to operate in a…

Nuclear Experiment · Physics 2020-04-02 GERDA collaboration , Matteo Agostini , Alexander M. Bakalyarov , Marco Balata , Igor Barabanov , Laura Baudis , Christian Bauer , Enrico Bellotti , Sergej Belogurov , Alessandro Bettini , Leonid Bezrukov , Dariusz Borowicz , Elisabetta Bossio , Vikas Bothe , Victor Brudanin , Riccardo Brugnera , Allen Caldwell , Carla Cattadori , Andrey Chernogorov , Tommaso Comellato , Valerio D'Andrea , Elena V. Demidova , Natalia Di Marco , Alexander Domula , Evgenyi Doroshkevich , Viacheslav Egorov , Felix Fischer , Maria Fomina , Albert Gangapshev , Alberto Garfagnini , Chris Gooch , Peter Grabmayr , Valery Gurentsov , Konstantin Gusev , Janina Hakenmüller , Sabine Hemmer , Roman Hiller , Werner Hofmann , Mikael Hult , Lev V. Inzhechik , Jozsef Janicskó Csáthy , Josef Jochum , Matthias Junker , Vladimir Kazalov , Yoann Kermaïdic , Thomas Kihm , Igor V. Kirpichnikov , Alexander Klimenko , Raphael Kneißl , Karl T. Knöpfle , Oleg Kochetov , Vasily N. Kornoukhov , Patrick Krause , Valery V. Kuzminov , Matthias Laubenstein , Andrea Lazzaro , Manfred Lindner , Ivano Lippi , Alexey Lubashevskiy , Bayarto Lubsandorzhiev , Guillaume Lutter , Carla Macolino , Bela Majorovits , Werner Maneschg , Michael Miloradovic , Rizalina Mingazheva , Marcin Misiaszek , Pavel Moseev , Igor Nemchenok , Krysztof Panas , Luciano Pandola , Krysztof Pelczar , Luigi Pertoldi , Paolo Piseri , Alberto Pullia , Chloe Ransom , Stefano Riboldi , Nadezda Rumyantseva , Cinzia Sada , Francesco Salamida , Stefan Schönert , Jochen Schreiner , Mario Schütt , Ann-Katrin Schütz , Oliver Schulz , Mario Schwarz , Bernhard Schwingenheuer , Oleg Selivanenko , Egor Shevchik , Mark Shirchenko , Hardy Simgen , Anatoly Smolnikov , Danila Stukov , Laura Vanhoefer , Andrey A. Vasenko , Anna Veresnikova , Chiara Vignoli , Katharina von Sturm , Thomas Wester , Christoph Wiesinger , Marcin Wojcik , Evgeny Yanovich , Birgit Zatschler , Igor Zhitnikov , Sergey V. Zhukov , Daniya Zinatulina , Andreas Zschocke , Anna J. Zsigmond , Kai Zuber , Grzegorz Zuzel

A comprehensive GEANT4 simulation framework was developed to model the background of the TEXONO experiment, including contributions from radioactive isotopes in detector components and the surrounding environment. The HPGe detector…

High Energy Physics - Experiment · Physics 2026-05-19 Subhasis Parhi , Lakhwinder Singh , Manoj Kumar Singh , Henry Tsz-King Wong , Venktesh Singh

We report the detection of an Al II line at 2669.155 Angstroms in 11 metal-poor stars, using ultraviolet spectra obtained with the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope. We derive Al abundances from this…

Solar and Stellar Astrophysics · Physics 2021-05-19 Ian U. Roederer , James E. Lawler

The $\nu$BDX-DRIFT collaboration seeks to detect low-energy nuclear recoils from CE$\nu$NS or BSM interactions at FNAL. Backgrounds due to rock neutrons are an important concern. We present a~\texttt{GENIE} and~\texttt{GEANT4} based model…

High Energy Physics - Experiment · Physics 2023-01-25 D. Aristizabal Sierra , J. L. Barrow , B. Dutta , D. Kim , D. Snowden-Ifft , L. Strigari , M. H. Wood

The GERDA experiment searches for neutrinoless double beta ($0\nu\beta\beta$) decay in $^{76}$Ge using an array of high purity germanium (HPGe) detectors immersed in liquid argon (LAr). Phase II of the experiment uses 30 new broad energy…

Instrumentation and Detectors · Physics 2016-08-06 Björn Lehnert

A significant decay branch of 8B to the ground state of 8Be would extend the solar neutrino spectrum to higher energies than anticipated in the standard solar models. These high-energy neutrinos would affect current neutrino oscillation…

Nuclear Experiment · Physics 2008-11-26 M. K. Bacrania , N. M. Boyd , R. G. H. Robertson , D. W. Storm

Development of ultra low background gas proportional counters has made the contribution from naturally occurring radioactive isotopes -- primarily $\alpha$ and $\beta$ activity in the uranium and thorium decay chains -- inconsequential to…

Instrumentation and Detectors · Physics 2015-12-24 Craig E. Aalseth , Paul H. Humble , Emily K. Mace , John L. Orrell , Allen Seifert , Richard M. Williams

Efficient solid-state photon emitters with longer operating lifetimes in the ultraviolet (UV) wavelength range are crucial for optoelectronic devices. However, finding suitable material candidates has been a significant challenge. Here, we…

Mesoscale and Nanoscale Physics · Physics 2024-09-04 Pushpendra Yadav , Amit Agarwal , Sitangshu Bhattacharya

We propose the idea of "Earth Shielding" to reject cosmic-ray backgrounds, in the search for boosted dark matter at surface neutrino detectors, resulting in the enhancement of the signal-to-background ratio. The identification of…

High Energy Physics - Phenomenology · Physics 2018-09-26 Doojin Kim , Kyoungchul Kong , Jong-Chul Park , Seodong Shin

To understand the origin of nuclear ($\lesssim$ 100 pc) millimeter-wave (mm-wave) continuum emission in active galactic nuclei (AGNs), we systematically analyzed sub-arcsec resolution Band-6 (211-275 GHz) ALMA data of 98 nearby AGNs ($z <$…