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Related papers: CUORE: A Cryogenic Underground Observatory for Rar…

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The Mu2e experiment at Fermilab searches for the charged-lepton flavour violating (CLFV) conversion of a negative muon into an electron in the field of an aluminum nucleus, with a distinctive signature of a mono-energetic electron of energy…

The next generation neutrino telescope, IceCube-Gen2, will be sensitive to the astrophysical and cosmogenic flux of neutrinos across a broad energy range, from the TeV to the EeV scale. The planned design includes 8 cubic kilometers of ice…

High Energy Astrophysical Phenomena · Physics 2025-07-11 Christian Glaser

The LUMINEU is designed to investigate the possibility to search for neutrinoless double beta decay in $^{100}$Mo by means of a large array of scintillating bolometers based on ZnMoO$_4$ crystals enriched in $^{100}$Mo. High energy…

A scintillating bolometer technology based on $^{100}$Mo-enriched lithium molybdate (Li$_2$$^{100}$MoO$_4$) crystals has been developed by LUMINEU to search for neutrinoless double-beta ($0\nu 2\beta$) decay of $^{100}$Mo. The results of…

Instrumentation and Detectors · Physics 2017-11-06 D. V. Poda

IceCube-Gen2, the extension of the IceCube Neutrino Observatory, will feature three main components: an optical array in the deep ice, a large-scale radio array in the shallow ice and firn, and a surface detector above the optical array.…

High Energy Astrophysical Phenomena · Physics 2022-09-21 Frank G. Schroeder

WIMP-nucleon cross sections below 10^(-9) pb may be probed by ton-scale experiments with low thresholds and background rates ~20 events per year. An array of cryogenic detectors ("CryoArray") could perform well enough to reach this goal.…

Astrophysics · Physics 2009-11-07 R. W. Schnee , D. S. Akerib , R. J. Gaitskell

We present the characterization of cosmogenic muon backgrounds for the Colorado Underground Research Institute (CURIE), located in the Edgar Experimental Mine (EEM) in Idaho Springs, Colorado. The CURIE facility at the EEM offers a…

Instrumentation and Detectors · Physics 2025-01-23 Dakota K. Keblbeck , Eric Mayotte , Uwe Greife , Kyle G. Leach , Wouter Van De Pontseele

Applications for ultra-stable lasers outside controlled laboratory environments require compact and robust optical resonators with reduced sensitivity to temperature fluctuations. The low thermal expansion coefficient (CTE) and the high…

Optics · Physics 2026-05-07 Nico Wagner , Thomas Legero , Stefanie Kroker

In preparation to the CROSS $2\beta$ decay experiment, we installed a new detector suspension with magnetic dumping inside a pulse-tube cryostat of a dedicated low-background facility at the LSC (Spain). The suspension was tested with two…

The search for neutrinoless double beta decay is a very active field in which the number of proposals for next-generation experiments has proliferated. In this paper we attempt to address both the sense and the sensitivity of such…

High Energy Physics - Experiment · Physics 2011-06-09 J. J. Gomez-Cadenas , J. Martin-Albo , M. Sorel , P. Ferrario , F. Monrabal , J. Munoz-Vidal , P. Novella , A. Poves

DUNE is an international experiment dedicated to addressing some of the questions at the forefront of particle physics and astrophysics, including the mystifying preponderance of matter over antimatter in the early universe. The dual-site…

Instrumentation and Detectors · Physics 2023-12-15 LBNF/DUNE , : , M. Adamowski , J. Bremer , M. Delaney , R. Doubnik , D. Mladenov , D. Montanari , T. Nichols , A. Parchet , F. Resnati , I. Young

The B-mode Foreground Experiment (BFORE) is a proposed NASA balloon project designed to make optimal use of the sub-orbital platform by concentrating on three dust foreground bands (270, 350, and 600 GHz) that complement ground-based cosmic…

The proposed 50 kt Iron Calorimeter (ICAL) detector at the India-based Neutrino Observatory (INO) aims to detect atmospheric muon neutrinos and antineutrinos separately in the multi-GeV range of energies and over a wide range of path…

High Energy Physics - Phenomenology · Physics 2021-10-19 Anil Kumar , Sanjib Kumar Agarwalla

CLOVER is an experiment which aims to detect the signature of gravitational waves from inflation by measuring the B-mode polarization of the cosmic microwave background. CLOVER consists of three telescopes operating at 97, 150, and 220 GHz.…

(Abridged) Context. Core condensation is a critical step in the star-formation process, but is still poorly characterized observationally. Aims. We have studied the 10 pc-long L1495/B213 complex in Taurus to investigate how dense cores have…

Astrophysics of Galaxies · Physics 2015-06-15 A. Hacar , M. Tafalla , J. Kauffmann , A. Kovacs

IceCube-Gen2 is a proposed extension to the existing IceCube Neutrino Observatory at the South Pole. It will consist of three components: an in-ice optical array, a surface array on top of the optical array, and a radio array for detecting…

High Energy Astrophysical Phenomena · Physics 2025-03-18 Manisha Lohan

The NEMO prototype detector, called "NEMO Phase-1", has been successfully operated at 2000 m depth from December 2006 to May 2007. The apparatus comprises a \emph{Junction Box} and a \emph{Mini-Tower} hosting 16 optical sensors. Preliminary…

Astrophysics · Physics 2019-08-13 Isabella Amore

Borexino is a large unsegmented calorimeter featuring 300 tons of liquid scintillator, contained in a 8.5 meter nylon vessel, viewed by 2200 PMTs. The main goal of Borexino is the study, in real time, of low energy solar neutrinos, and in…

High Energy Physics - Experiment · Physics 2017-08-23 Lino Miramonti

Ultra-high-energy cosmic rays (UHECR), of energy >10 EeV, arrive at the Earth regularly, but their sources, acceleration mechanisms, details of propagation through the universe, and particle composition remain mysteries. In addition, their…

Instrumentation and Methods for Astrophysics · Physics 2020-12-10 Sijbrand de Jong

ALTO is a wide field-of-view air shower detector array for very-high-energy (VHE) gamma-ray astronomy, proposed to be installed in the Southern Hemisphere at an altitude of about 5.1 km above sea level. The array will use water Cherenkov…

Instrumentation and Methods for Astrophysics · Physics 2017-08-04 Satyendra Thoudam , Yvonne Becherini , Michael Punch
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