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In 2016, the NASA Juno spacecraft will initiate its one-year mission around Jupiter and become the first probe to explore the polar regions of Jupiter. The HST UV instruments (STIS and ACS) can greatly contribute to the success of the Juno…

Geo-neutrinos emitted by heat-producing elements (U, Th and K) represent a unique probe of the Earth interior. The characterization of their fluxes is subject, however, to rather large and highly correlated uncertainties. The geochemical…

地球物理 · 物理学 2009-11-13 G. L. Fogli , E. Lisi , A. Palazzo , A. M. Rotunno

The Jiangmen Underground Neutrino Observatory (JUNO) employs a 20 kt liquid scintillator (LS) detector located 700 m underground. To meet its physics objectives, the LS must achieve an ultra-low $^{238}$U/$^{232}$Th content of 10$^{-17}$…

仪器与探测器 · 物理学 2026-03-05 Jie Zhao , Chenyang Cui , Yongpeng Zhang , Gaosong Li , Nan Wang , Monica Sisti

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…

高能物理 - 唯象学 · 物理学 2021-10-19 Anil Kumar , Sanjib Kumar Agarwalla

In this paper we focus on the Earth matter effects for the solar parameter determination by a medium baseline reactor experiment such as JUNO. We derive perturbative expansions for the mixing angles $\theta_{12}$ and $\theta_{13}$ as well…

高能物理 - 唯象学 · 物理学 2020-03-12 Amir N. Khan , Hiroshi Nunokawa , Stephen J. Parke

The standard cosmological model predicts the existence of a Cosmic Neutrino Background, which has not yet been observed directly. Some experiments aiming at its detection are currently under development, despite the tiny kinetic energy of…

宇宙学与河外天体物理 · 物理学 2020-01-08 P. Mertsch , G. Parimbelli , P. F. de Salas , S. Gariazzo , J. Lesgourgues , S. Pastor

The Kamioka Liquid scintillator Anti-Neutrino Detector (KamLAND) is collecting antineutrino events generated by nuclear reactors and by Thorium and Uranium decay in the Earth interior. We comment on a systematic approach to the evaluation…

高能物理 - 唯象学 · 物理学 2007-05-23 G. L. Fogli , E. Lisi , A. Palazzo , A. M. Rotunno

The terrestrial distribution of U, Th, and K abundances governs the thermal evolution, traces the differentiation, and reflects the bulk composition of the earth. Comparing the bulk earth composition to chondritic meteorites estimates the…

地球物理 · 物理学 2015-05-19 Steve Dye

Reactor neutrinos have been an important tool for both discovery and precision measurement in the history of neutrino studies. Since the first generation of reactor neutrino experiments in the 1950s, the detector technology has been greatly…

高能物理 - 实验 · 物理学 2018-03-28 Liang-Jian Wen , Jun Cao , Yi-Fang Wang

We customized a laser calibration system and four radioactive $\gamma$-ray calibration sources for the Jiangmen Underground Neutrino Observatory (JUNO), a 20-kton liquid scintillator-based neutrino detector. The laser source system was…

The Jiangmen Underground Neutrino Observatory (JUNO) is a neutrino experiment to determine neutrino mass hierarchy. It has a central detector used for neutrino detection, which consists of a spherical acrylic vessel containing 20 kt LS and…

仪器与探测器 · 物理学 2019-08-13 Tao Lin , Jiaheng Zou , Weidong Li , Ziyan Deng , Guofu Cao , Xingtao Huang , Zhengyun You

A significant fraction of the 44TW of heat dissipation from the Earth's interior is believed to originate from the decays of terrestrial uranium and thorium. The only estimates of this radiogenic heat, which is the driving force for mantle…

Leptonic \textit{CP} violation search, neutrino mass hierarchy determination, and the precision measurement of oscillation parameters for a unitary test of the leptonic mixing matrix are among the major targets of the ongoing and future…

高能物理 - 唯象学 · 物理学 2021-07-07 S. Cao , A. Nath , T. V. Ngoc , P. T. Quyen , N. T. Hong Van , Ng. K. Francis

This article presents the potential of a combined analysis of the JUNO and KM3NeT/ORCA experiments to determine the neutrino mass ordering. This combination is particularly interesting as it significantly boosts the potential of either…

高能物理 - 实验 · 物理学 2023-10-05 KM3NeT Collaboration , S. Aiello , A. Albert , M. Alshamsi , S. Alves Garre , Z. Aly , A. Ambrosone , F. Ameli , M. Andre , G. Androulakis , M. Anghinolfi , M. Anguita , M. Ardid , S. Ardid , J. Aublin , C. Bagatelas , B. Baret , S. Basegmez du Pree , M. Bendahman , F. Benfenati , E. Berbee , A. M. van den Berg , V. Bertin , S. Biagi , M. Boettcher , M. Bou Cabo , J. Boumaaza , M. Bouta , M. Bouwhuis , C. Bozza , H. Brânzaş , R. Bruijn , J. Brunner , R. Bruno , E. Buis , R. Buompane , J. Busto , B. Caiffi , D. Calvo , S. Campion , A. Capone , V. Carretero , P. Castaldi , S. Celli , M. Chabab , N. Chau , A. Chen , S. Cherubini , V. Chiarella , T. Chiarusi , M. Circella , R. Cocimano , J. A. B. Coelho , A. Coleiro , M. Colomer Molla , R. Coniglione , P. Coyle , A. Creusot , A. Cruz , G. Cuttone , R. Dallier , B. De Martino , I. Di Palma , A. F. Díaz , D. Diego-Tortosa , C. Distefano , A. Domi , C. Donzaud , D. Dornic , M. Dörr , D. Drouhin , T. Eberl , A. Eddyamoui , T. van Eeden , D. van Eijk , I. El Bojaddaini , A. Enzenhöfer , V. Espinosa , P. Fermani , G. Ferrara , M. D. Filipovic , F. Filippini , L. A. Fusco , T. Gal , J. García Méndez , A. Garcia Soto , F. Garufi , Y. Gatelet , C. Gatius , N. Geisselbrecht , L. Gialanella , E. Giorgio , S. R. Gozzini , R. Gracia , K. Graf , G. Grella , D. Guderian , C. Guidi , B. Guillon , M. Gutiérrez , J. Haefner , S. Hallmann , H. Hamdaoui , H. van Haren , A. Heijboer , A. Hekalo , L. Hennig , J. J. Hernández-Rey , J. Hofestädt , F. Huang , W. Idrissi Ibnsalih , G. Illuminati , C. W. James , M. de Jong , P. de Jong , B. J. Jung , P. Kalaczynski , O. Kalekin , U. F. Katz , N. R. Khan Chowdhury , G. Kistauri , F. van der Knaap , P. Kooijman , A. Kouchner , V. Kulikovskiy , M. Labalme , R. Lahmann , M. Lamoureux , G. Larosa , C. Lastoria , A. Lazo , R. Le Breton , S. Le Stum , G. Lehaut , O. Leonardi , F. Leone , E. Leonora , N. Lessing , G. Levi , M. Lincetto , M. Lindsey Clark , T. Lipreau , C. Llorens Alvarez , F. Longhitano , D. Lopez-Coto , A. Lygda , L. Maderer , J. Majumdar , J. Mańczak , A. Margiotta , A. Marinelli , C. Markou , L. Martin , J. A. Martínez-Mora , A. Martini , F. Marzaioli , S. Mastroianni , K. W. Melis , G. Miele , P. Migliozzi , E. Migneco , P. Mijakowski , L. S. Miranda , C. M. Mollo , M. Moser , A. Moussa , R. Muller , M. Musumeci , L. Nauta , S. Navas , C. A. Nicolau , B. Nkosi , B. Ó Fearraigh , M. O'Sullivan , M. Organokov , A. Orlando , J. Palacios González , G. Papalashvili , R. Papaleo , A. M. Păun , G. E. Păvălaş , C. Pellegrino , M. Perrin-Terrin , V. Pestel , P. Piattelli , C. Pieterse , O. Pisanti , C. Poirè , V. Popa , T. Pradier , I. Probst , S. Pulvirenti , G. Quéméner , N. Randazzo , S. Razzaque , D. Real , S. Reck , G. Riccobene , A. Romanov , A. Rovelli , F. Salesa Greus , D. F. E. Samtleben , A. Sánchez Losa , M. Sanguineti , D. Santonocito , P. Sapienza , J. Schnabel , M. F. Schneider , J. Schumann , H. M. Schutte , J. Seneca , I. Sgura , R. Shanidze , A. Sharma , A. Sinopoulou , B. Spisso , M. Spurio , D. Stavropoulos , S. M. Stellacci , M. Taiuti , Y. Tayalati , H. Thiersen , S. Tingay , S. Tsagkli , V. Tsourapis , E. Tzamariudaki , D. Tzanetatos , V. Van Elewyck , G. Vasileiadis , F. Versari , D. Vivolo , G. de Wasseige , J. Wilms , R. Wojaczyński , E. de Wolf , T. Yousfi , S. Zavatarelli , A. Zegarelli , D. Zito , J. D. Zornoza , J. Zúñiga , N. Zywucka , JUNO Collaboration members , : , S. Ahmad , J. P. A. M. de André , E. Baussan , C. Bordereau , A. Cabrera , C. Cerna , G. Donchenko , E. A. Doroshkevich , M. Dracos , F. Druillole , C. Jollet , L. N. Kalousis , P. Kampmann , K. Kouzakov , A. Lokhov , B. K. Lubsandorzhiev , S. B. Lubsandorzhiev , A. Meregaglia , L. Miramonti , F. Perrot , L. F. Piñeres Rico , A. Popov , R. Rasheed , M. Settimo , K. Stankevich , H. Steiger , M. R. Stock , A. Studenikin , A. Triossi , W. Trzaska , M. Vialkov , B. Wonsak , J. Wurtz , F. Yermia

Constraints on light sterile neutrinos and scalar non-standard neutrino interactions are obtained from the first reactor antineutrino results reported by JUNO. The analysis is based on a spectral $\chi^2$ fit to the prompt-energy…

高能物理 - 唯象学 · 物理学 2026-05-19 L. J. Flores , R. Pacheco-Aké , Eduardo Peinado , G. Sanchez Garcia , E. Vázquez-Jáuregui

Neutrino radiography may provide an alternative tool to study the very deep structures of the Earth. Though these measurements are unable to resolve the fine density layer features, nevertheless the information which can be obtained are…

地球与行星天体物理 · 物理学 2009-07-09 E. Borriello , G. Mangano , A. Marotta , G. Miele , P. Migliozzi , C. A. Moura , S. Pastor , O. Pisanti , P. Strolin

The Jiangmen Underground Neutrino Observatory (JUNO), a 20ktons multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino mass hierarchy as a primary physics goal. Due to low background…

仪器与探测器 · 物理学 2018-07-02 C. Guo , Y. P. Zhang , J. C. Liu , C. G. Yang , P. Zhang

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…

高能物理 - 唯象学 · 物理学 2025-09-29 Riya Gaba , Maitreyee Mukherjee , Vipin Bhatnagar

The energy spectrum of geo-neutrinos plays a vital role in the experimental measurement of geo-neutrinos that have profound implications for both particle physics and earth sciences. In this letter, we present a state-of-the-art calculation…

高能物理 - 唯象学 · 物理学 2024-12-12 Yu-Feng Li , Zhao Xin

An observation of Jupiter's tidal response is anticipated for the on-going Juno spacecraft mission. We combine self-consistent, numerical models of Jupiter's equilibrium tidal response with observed Doppler shifts from the Juno gravity…

地球与行星天体物理 · 物理学 2020-03-11 Sean M Wahl , Marzia Parisi , William M Folkner , William B Hubbard , Burkhard Militzer
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