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One of the challenges that must be overcome in order to determine the neutrino mass hierarchy using reactor neutrinos is the theoretical uncertainty in the unoscillated reactor neutrino spectrum: this is one of the reasons why, recently, it…

High Energy Physics - Phenomenology · Physics 2020-01-08 Emilio Ciuffoli , Jarah Evslin , Hosam Mohammed

Constraints on the Earth's composition and on its radiogenic energy budget come from the detection of geoneutrinos. The KamLAND and Borexino experiments recently reported the geoneutrino flux, which reflects the amount and distribution of U…

Orbiting detectors will be able to observe showers initiated by neutrinos penetrating the Earth and interacting close to their exit point. There is a correlation between the impact parameter of the incident neutrino and its energy. We study…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Domokos , S. Kovesi-Domokos

Exotic explanations are considered for atmospheric neutrino observations. Our analysis includes matter effects and the mixing of all three neutrinos under the simplifying assumption of only one relevant mixing scale. Constraints from…

High Energy Physics - Phenomenology · Physics 2014-11-17 James Pantaleone , T. K. Kuo , Sadek Mansour

In preparation to the experimental results which will be available in the future, we consider geo-neutrino production in greater detail than in [F. Mantovani et al., arXiv:hep-ph/0309013], putting the basis for a more refined model. We…

High Energy Physics - Phenomenology · Physics 2007-05-23 Gianni Fiorentini , Marcello Lissia , Fabio Mantovani , Riccardo Vannucci

Neutrino-matter interactions play a key role in binary neutron star mergers. Thermodynamics conditions at the surfaces where neutrinos decouple from matter influence neutrino spectra, ultimately affecting the evolution of the remnant and…

The precise measurement of neutrino properties is among the highest priorities in fundamental particle physics, involving many experiments worldwide. Since the experiments rely on the interactions of neutrinos with bound nucleons inside…

Neutrino properties can be constrained by the detection of ultra-high energy cosmic neutrinos (UHECNs). By using the updated global fitting results of neutrino mixing parameters, we present predictions on the neutrino flavor ratios at the…

High Energy Physics - Phenomenology · Physics 2016-09-08 Yanqi Huang , Bo-Qiang Ma

Recent measurements of reactor-produced antineutrino fluxes and energy spectra are inconsistent with models based on measured thermal fission beta spectra. In this paper, we examine the dependence of antineutrino production on fission…

Nuclear Theory · Physics 2018-05-09 B. R. Littlejohn , A. Conant , D. A. Dwyer , A. Erickson , I. Gustafson , K. Hermanek

Reactor neutrinos play a substantial role in the study of the fundamental properties of neutrinos. With current and upcoming precision experiments, it is essential more than ever to understand the reactor neutrino flux and spectrum.…

Instrumentation and Detectors · Physics 2018-04-03 Bedrich Roskovec

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…

This article reports the optimized experimental requirements to determine neutrino mass hierarchy using electron antineutrinos ($\bar{\nu}_e$) generated in a nuclear reactor. The features of the neutrino mass hierarchy can be extracted from…

High Energy Physics - Experiment · Physics 2016-01-20 M. Y. Pac

We consider a model in which the neutrino is kinetically coupled to a scalar field and study its implications for environmentally dependent neutrino velocities. Following the usual effective field theory logic, this coupling is expected to…

High Energy Physics - Phenomenology · Physics 2013-01-22 Emilio Ciuffoli , Jarah Evslin , Jie Liu , Xinmin Zhang

Matter effects modify the mixing and the effective masses of neutrinos in a way which depends on the neutrino mass hierarchy. Consequently, for normal and inverted hierarchies the oscillations and flavor conversion results are different.…

High Energy Physics - Phenomenology · Physics 2013-12-30 Alexei Yu. Smirnov

In this review we present the main features of the current status of neutrino physics. After a review of the theory of neutrino mixing and oscillations, we discuss the current status of solar and atmospheric neutrino oscillation…

High Energy Physics - Phenomenology · Physics 2007-05-23 Carlo Giunti , Marco Laveder

Starting from a complete set of possible parametrisations of the quark-mass matrices that have the maximum number of texture zeros at the grand unification scale, and the Georgi-Jarlskog mass relations, we classify the neutrino spectra with…

High Energy Physics - Phenomenology · Physics 2015-06-25 E. Papageorgiu

Hints for the existence of a sterile neutrino at nuclear reactors are reexamined using two updated predictions for the fluxes of antineutrinos produced in fissions. These new predictions diverge in their preference for the rate deficit…

High Energy Physics - Phenomenology · Physics 2020-01-22 Jeffrey Berryman , Patrick Huber

Neutron-star mergers are interesting for several reasons: they are proposed as the progenitors of short gamma-ray bursts, they have been speculated to be a site for the synthesis of heavy elements, and they emit gravitational waves possibly…

Nuclear Theory · Physics 2016-08-03 O. L. Caballero

The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino mass hierarchy as a primary physics goal. It is also capable of…

Instrumentation and Detectors · Physics 2016-02-02 Fengpeng An , Guangpeng An , Qi An , Vito Antonelli , Eric Baussan , John Beacom , Leonid Bezrukov , Simon Blyth , Riccardo Brugnera , Margherita Buizza Avanzini , Jose Busto , Anatael Cabrera , Hao Cai , Xiao Cai , Antonio Cammi , Guofu Cao , Jun Cao , Yun Chang , Shaomin Chen , Shenjian Chen , Yixue Chen , Davide Chiesa , Massimiliano Clemenza , Barbara Clerbaux , Janet Conrad , Davide D'Angelo , Herve De Kerret , Zhi Deng , Ziyan Deng , Yayun Ding , Zelimir Djurcic , Damien Dornic , Marcos Dracos , Olivier Drapier , Stefano Dusini , Stephen Dye , Timo Enqvist , Donghua Fan , Jian Fang , Laurent Favart , Richard Ford , Marianne Goger-Neff , Haonan Gan , Alberto Garfagnini , Marco Giammarchi , Maxim Gonchar , Guanghua Gong , Hui Gong , Michel Gonin , Marco Grassi , Christian Grewing , Mengyun Guan , Vic Guarino , Gang Guo , Wanlei Guo , Xin-Heng Guo , Caren Hagner , Ran Han , Miao He , Yuekun Heng , Yee Hsiung , Jun Hu , Shouyang Hu , Tao Hu , Hanxiong Huang , Xingtao Huang , Lei Huo , Ara Ioannisian , Manfred Jeitler , Xiangdong Ji , Xiaoshan Jiang , Cecile Jollet , Li Kang , Michael Karagounis , Narine Kazarian , Zinovy Krumshteyn , Andre Kruth , Pasi Kuusiniemi , Tobias Lachenmaier , Rupert Leitner , Chao Li , Jiaxing Li , Weidong Li , Weiguo Li , Xiaomei Li , Xiaonan Li , Yi Li , Yufeng Li , Zhi-Bing Li , Hao Liang , Guey-Lin Lin , Tao Lin , Yen-Hsun Lin , Jiajie Ling , Ivano Lippi , Dawei Liu , Hongbang Liu , Hu Liu , Jianglai Liu , Jianli Liu , Jinchang Liu , Qian Liu , Shubin Liu , Shulin Liu , Paolo Lombardi , Yongbing Long , Haoqi Lu , Jiashu Lu , Jingbin Lu , Junguang Lu , Bayarto Lubsandorzhiev , Livia Ludhova , Shu Luo , Vladimir Lyashuk , Randolph Mollenberg , Xubo Ma , Fabio Mantovani , Yajun Mao , Stefano M. Mari , William F. McDonough , Guang Meng , Anselmo Meregaglia , Emanuela Meroni , Mauro Mezzetto , Lino Miramonti , Thomas Mueller , Dmitry Naumov , Lothar Oberauer , Juan Pedro Ochoa-Ricoux , Alexander Olshevskiy , Fausto Ortica , Alessandro Paoloni , Haiping Peng , Jen-Chieh Peng , Ezio Previtali , Ming Qi , Sen Qian , Xin Qian , Yongzhong Qian , Zhonghua Qin , Georg Raffelt , Gioacchino Ranucci , Barbara Ricci , Markus Robens , Aldo Romani , Xiangdong Ruan , Xichao Ruan , Giuseppe Salamanna , Mike Shaevitz , Valery Sinev , Chiara Sirignano , Monica Sisti , Oleg Smirnov , Michael Soiron , Achim Stahl , Luca Stanco , Jochen Steinmann , Xilei Sun , Yongjie Sun , Dmitriy Taichenachev , Jian Tang , Igor Tkachev , Wladyslaw Trzaska , Stefan van Waasen , Cristina Volpe , Vit Vorobel , Lucia Votano , Chung-Hsiang Wang , Guoli Wang , Hao Wang , Meng Wang , Ruiguang Wang , Siguang Wang , Wei Wang , Yi Wang , Yi Wang , Yifang Wang , Zhe Wang , Zheng Wang , Zhigang Wang , Zhimin Wang , Wei Wei , Liangjian Wen , Christopher Wiebusch , Bjorn Wonsak , Qun Wu , Claudia-Elisabeth Wulz , Michael Wurm , Yufei Xi , Dongmei Xia , Yuguang Xie , Zhi-zhong Xing , Jilei Xu , Baojun Yan , Changgen Yang , Chaowen Yang , Guang Yang , Lei Yang , Yifan Yang , Yu Yao , Ugur Yegin , Frederic Yermia , Zhengyun You , Boxiang Yu , Chunxu Yu , Zeyuan Yu , Sandra Zavatarelli , Liang Zhan , Chao Zhang , Hong-Hao Zhang , Jiawen Zhang , Jingbo Zhang , Qingmin Zhang , Yu-Mei Zhang , Zhenyu Zhang , Zhenghua Zhao , Yangheng Zheng , Weili Zhong , Guorong Zhou , Jing Zhou , Li Zhou , Rong Zhou , Shun Zhou , Wenxiong Zhou , Xiang Zhou , Yeling Zhou , Yufeng Zhou , Jiaheng Zou

Knowledge of the amount and distribution of radiogenic heating in the mantle is crucial for understanding the dynamics of the Earth, including its thermal evolution, the style and planform of mantle convection, and the energetics of the…