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The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful IceCube example, PINGU will provide a 6Mton…

High Energy Physics - Experiment · Physics 2017-04-10 Gen2 Collaboration

The Deep Underground Neutrino Experiment (DUNE) is a next-generation long-baseline neutrino oscillation experiment designed to make precision measurements in the world's most powerful neutrino beam. Neutrinos are measured at two detector…

High Energy Physics - Experiment · Physics 2025-01-28 Ciaran Hasnip

The CONUS+ experiment aims to detect coherent elastic neutrino-nucleus scattering (CEvNS) of reactor antineutrinos on germanium nuclei in the fully coherent regime, continuing on this way the CONUS physics program started at the Brokdorf…

We propose an EASY (Electroluminescent ApparatuS of high Yield) and SOFT (Separated Optimized FuncTion) time-projection chamber for the NEXT experiment, that will search for neutrinoless double beta decay (bb0nu) in Xe-136. Our experiment…

The lepton number violating process of neutrinoless double-beta decay could result from the physics beyond the Standard Model needed to generate the neutrino masses. Taking different approaches, the current generation of $^{76}$Ge…

Instrumentation and Detectors · Physics 2019-08-14 Jordan Myslik

We describe the upgrade and performance of the high-purity germanium counting facility Gator, which is dedicated to low-background $\gamma$-ray spectrometry. Gator is operated at the Gran Sasso Underground Laboratory in Italy, at an average…

Instrumentation and Detectors · Physics 2022-08-24 G. R. Araujo , L. Baudis , Y. Biondi , A. Bismark , M. Galloway

The Deep Underground Neutrino Experiment (DUNE) is a next-generation long-baseline neutrino oscillation experiment. Its primary goal is the determination of the neutrino mass hierarchy and the CP-violating phase. The DUNE physics program…

High Energy Physics - Experiment · Physics 2025-02-13 Francisco Martínez López

The investigation of the endpoint region of the tritium beta decay spectrum is still the most sensitive direct method to determine the neutrino mass scale. In the nineties and the beginning of this century the tritium beta decay experiments…

High Energy Physics - Experiment · Physics 2009-12-10 C. Weinheimer

Low-background experiments with stable ion beams are an important tool for putting the model of stellar hydrogen, helium, and carbon burning on a solid experimental foundation. The pioneering work in this regard has been done by the LUNA…

THESEUS is a space mission concept, currently under Phase A study by ESA as candidate M5 mission, aiming at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and…

Instrumentation and Methods for Astrophysics · Physics 2021-02-18 Lorenzo Amati , Paul T. O'Brien , Diego Götz , Enrico Bozzo , Andrea Santangelo

The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to measure a high-precision integral spectrum of the endpoint region of T2 beta decay, with the primary goal of probing the absolute mass scale of the neutrino. After a first…

Nuclear Experiment · Physics 2023-06-21 M. Aker , M. Balzer , D. Batzler , A. Beglarian , J. Behrens , A. Berlev , U. Besserer , M. Biassoni , B. Bieringer , F. Block , S. Bobien , L. Bombelli , D. Bormann , B. Bornschein , L. Bornschein , M. Böttcher , C. Brofferio , C. Bruch , T. Brunst , T. S. Caldwell , M. Carminati , R. M. D. Carney , S. Chilingaryan , W. Choi , O. Cremonesi , K. Debowski , M. Descher , D. Díaz Barrero , P. J. Doe , O. Dragoun , G. Drexlin , F. Edzards , K. Eitel , E. Ellinger , R. Engel , S. Enomoto , A. Felden , D. Fink , C. Fiorini , J. A. Formaggio , C. Forstner , F. M. Fränkle , G. B. Franklin , F. Friedel , A. Fulst , K. Gauda , A. S. Gavin , W. Gil , F. Glück , A. Grande , R. Grössle , M. Gugiatti , R. Gumbsheimer , V. Hannen , J. Hartmann , N. Haußmann , K. Helbing , S. Hickford , R. Hiller , D. Hillesheimer , D. Hinz , T. Höhn , T. Houdy , A. Huber , A. Jansen , C. Karl , J. Kellerer , P. King , M. Kleifges , M. Klein , C. Köhler , L. Köllenberger , A. Kopmann , M. Korzeczek , A. Kovalík , B. Krasch , H. Krause , T. Lasserre , L. La Cascio , O. Lebeda , P. Lechner , B. Lehnert , T. L. Le , A. Lokhov , M. Machatschek , E. Malcherek , D. Manfrin , M. Mark , A. Marsteller , E. L. Martin , E. Mazzola , C. Melzer , S. Mertens , J. Mostafa , K. Müller , A. Nava , H. Neumann , S. Niemes , P. Oelpmann , A. Onillon , D. S. Parno , M. Pavan , A. Pigliafreddo , A. W. P. Poon , J. M. L. Poyato , S. Pozzi , F. Priester , M. Puritscher , D. C. Radford , J. Ráliš , S. Ramachandran , R. G. H. Robertson , W. Rodejohann , C. Rodenbeck , M. Röllig , C. Röttele , M. Ryšavý , R. Sack , A. Saenz , R. W. J. Salomon , P. Schäfer , L. Schimpf , K. Schlösser , M. Schlösser , L. Schlüter , S. Schneidewind , M. Schrank , A. K. Schütz , A. Schwemmer , A. Sedlak , M. Šefčík , V. Sibille , D. Siegmann , M. Slezák , F. Spanier , D. Spreng , M. Steidl , M. Sturm , H. H. Telle , L. A. Thorne , T. Thümmler , N. Titov , I. Tkachev , P. Trigilio , K. Urban , K. Valerius , D. Vénos , A. P. Vizcaya Hernández , P. Voigt , C. Weinheimer , E. Weiss , S. Welte , J. Wendel , C. Wiesinger , J. F. Wilkerson , J. Wolf , L. Wunderl , S. Wüstling , J. Wydra , W. Xu , S. Zadoroghny , G. Zeller

We explore the possibility to use advanced germanium (Ge) detectors as a low-energy solar neutrino observatory by means of neutrino-nucleus elastic scattering. A Ge detector utilizing internal charge amplification for the charge carriers…

Instrumentation and Detectors · Physics 2021-09-03 S. Bhattarai , D. -M. Mei , M. -S. Raut

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 GERDA experiment aims to search for the neutrinoless double beta-decay of 76Ge and possibly for other rare processes. The sensitivity of the first phase is envisioned to be more than one order of magnitude better than in previous…

The upcoming European Spallation Source (ESS) will soon provide the most intense neutrino source in the world. We propose the Search for Hidden Neutrinos at the ESS (SHiNESS) experiment, highlighting its unique opportunities to search for…

High Energy Physics - Experiment · Physics 2025-05-28 Stefano Roberto Soleti , Pilar Coloma , Juan Jose Gómez Cadenas , Anatael Cabrera

The \underline{KA}rlsruhe \underline{TRI}tium \underline{N}eutrino Mass Experiment is a next generation tritium beta decay experiment designed to reach a sensitivity of $0.2~ \mathrm{eV}/\mathrm{c}^2$. KATRIN will allow to investigate the…

High Energy Physics - Experiment · Physics 2019-08-14 Lutz Bornschein

The Large Enriched Germanium Experiment for Neutrinoless $\beta\beta$ Decay (LEGEND) is a future ton-scale experimental program that will search for neutrinoless double beta decay ($0\nu\beta\beta$) in the isotope $^{76}$Ge with an…

Instrumentation and Detectors · Physics 2020-05-20 Frank Edzards , Susanne Mertens , Michael Willers

The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the $\nu_\mu \to \nu_\tau$ channel, via the detection of the $\tau$-leptons created in charged current…

High Energy Physics - Experiment · Physics 2013-08-13 OPERA Collaboration , N. Agafonova , A. Aleksandrov , A. Anokhina , S. Aoki , A. Ariga , T. Ariga , T. Asada , D. Autiero , A. Badertscher , A. Ben Dhahbi , D. Bender , A. Bertolin , C. Bozza , R. Brugnera , G. Brunetti , B. Buettner , S. Buontempo , L. Chaussard , M. Chernyavskiy , V. Chiarella , A. Chukanov , L. Consiglio , N. D'Ambrosio , P. Del Amo Sanchez , G. De Lellis , M. De Serio , A. Di Crescenzo , D. Di Ferdinando , N. Di Marco , S. Dmitrievski , M. Dracos , D. Duchesneau , S. Dusini , J. Ebert , A. Ereditato , J. Favier , T. Ferber , R. A. Fini , T. Fukuda , A. Garfagnini , G. Giacomelli , C. Goellnitz , J. Goldberg , Y. Gornushkin , G. Grella , F. Grianti , A. M. Guler , C. Gustavino , C. Hagner , K. Hakamata , T. Hara , T. Hayakawa , M. Hierholzer , A. Hollnagel , B. Hosseini , H. Ishida , K. Ishiguro , M. Ishikawa , K. Jakovcic , C. Jollet , C. Kamiscioglu , M. Kamiscioglu , T. Katsuragawa , H. Kawahara , J. Kawada , J. H. Kim , S. H. Kim , M. Kimura , N. Kitagawa , B. Klicek , K. Kodama , M. Komatsu , U. Kose , I. Kreslo , A. Lauria , J. Lenkeit , A. Ljubicic , A. Longhin , P. Loverre , A. Malgin , G. Mandrioli , J. Marteau , T. Matsuo , V. Matveev , N. Mauri , E. Medinaceli , A. Meregaglia , P. Migliozzi , S. Mikado , A. Minotti , M. Miyanishi , E. Miyashita , P. Monacelli , M. C. Montesi , K. Morishima , M. T. Muciaccia , N. Naganawa , T. Naka , M. Nakamura , T. Nakano , Y. Nakatsuka , K. Niwa , S. Ogawa , N. Okateva , A. Olshevsky , T. Omura , K. Ozaki , A. Paoloni , B. D. Park , I. G. Park , A. Pastore , L. Patrizii , E. Pennacchio , H. Pessard , C. Pistillo , D. Podgrudkov , N. Polukhina , M. Pozzato , K. Pretzl , F. Pupilli , R. Rescigno , M. Roda , T. Roganova , H. Rokujo , G. Rosa , I. Rostovtseva , A. Rubbia , A. Russo , O. Ryazhskaya , O. Sato , Y. Sato , A. Schembri , W. Schmidt-Parzefall , I. Shakiryanova , T. Schcedrina , A. Sheshukov , H. Shibuya , T. Shiraishi , G. Shoziyoev , S. Simone , M. Sioli , C. Sirignano , G. Sirri , M. Spinetti , L. Stanco , N. Starkov , S. M. Stellacci , M. Stipcevic , T. Strauss , P. Strolin , K. Suzuki , S. Takahashi , M. Tenti , F. Terranova , V. Tioukov , P. Tolun , S. Tufanli , P. Vilain , M. Vladimirov , L. Votano , J. L. Vuilleumier , G. Wilquet , B. Wonsak , C. S. Yoon , J. Yoshida , M. Yoshimoto , Y. Zaitsev , S. Zemskova , A. Zghiche

Supernovae represent some of the most energetically explosive events in the universe, with a substantial fraction of their released gravitational energy carried away by neutrinos. This study evaluates the sensitivity of three…

High Energy Physics - Phenomenology · Physics 2025-09-29 Riya Gaba , Maitreyee Mukherjee , Vipin Bhatnagar