Semantic Scholar Open Access 2015 1189 sitasi

Neutrino Physics with JUNO

F. An G. An Q. An V. Antonelli E. Baussan +222 lainnya

Lihat Sumber DOI

Abstrak

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 (MH) as a primary physics goal. The excellent energy resolution and the large fiducial volume anticipated for the JUNO detector offer exciting opportunities for addressing many important topics in neutrino and astro-particle physics. In this document, we present the physics motivations and the anticipated performance of the JUNO detector for various proposed measurements. Following an introduction summarizing the current status and open issues in neutrino physics, we discuss how the detection of antineutrinos generated by a cluster of nuclear power plants allows the determination of the neutrino MH at a 3–4σ significance with six years of running of JUNO. The measurement of antineutrino spectrum with excellent energy resolution will also lead to the precise determination of the neutrino oscillation parameters ${\mathrm{sin}}^{2}{\theta }_{12}$, ${\rm{\Delta }}{m}_{21}^{2}$, and $| {\rm{\Delta }}{m}_{{ee}}^{2}| $ to an accuracy of better than 1%, which will play a crucial role in the future unitarity test of the MNSP matrix. The JUNO detector is capable of observing not only antineutrinos from the power plants, but also neutrinos/antineutrinos from terrestrial and extra-terrestrial sources, including supernova burst neutrinos, diffuse supernova neutrino background, geoneutrinos, atmospheric neutrinos, and solar neutrinos. As a result of JUNO's large size, excellent energy resolution, and vertex reconstruction capability, interesting new data on these topics can be collected. For example, a neutrino burst from a typical core-collapse supernova at a distance of 10 kpc would lead to ∼5000 inverse-beta-decay events and ∼2000 all-flavor neutrino–proton ES events in JUNO, which are of crucial importance for understanding the mechanism of supernova explosion and for exploring novel phenomena such as collective neutrino oscillations. Detection of neutrinos from all past core-collapse supernova explosions in the visible universe with JUNO would further provide valuable information on the cosmic star-formation rate and the average core-collapse neutrino energy spectrum. Antineutrinos originating from the radioactive decay of uranium and thorium in the Earth can be detected in JUNO with a rate of ∼400 events per year, significantly improving the statistics of existing geoneutrino event samples. Atmospheric neutrino events collected in JUNO can provide independent inputs for determining the MH and the octant of the ${\theta }_{23}$ mixing angle. Detection of the (7)Be and (8)B solar neutrino events at JUNO would shed new light on the solar metallicity problem and examine the transition region between the vacuum and matter dominated neutrino oscillations. Regarding light sterile neutrino topics, sterile neutrinos with ${10}^{-5}\,{{\rm{eV}}}^{2}\lt {\rm{\Delta }}{m}_{41}^{2}\lt {10}^{-2}\,{{\rm{eV}}}^{2}$ and a sufficiently large mixing angle ${\theta }_{14}$ could be identified through a precise measurement of the reactor antineutrino energy spectrum. Meanwhile, JUNO can also provide us excellent opportunities to test the eV-scale sterile neutrino hypothesis, using either the radioactive neutrino sources or a cyclotron-produced neutrino beam. The JUNO detector is also sensitive to several other beyondthe-standard-model physics. Examples include the search for proton decay via the $p\to {K}^{+}+\bar{\nu }$ decay channel, search for neutrinos resulting from dark-matter annihilation in the Sun, search for violation of Lorentz invariance via the sidereal modulation of the reactor neutrino event rate, and search for the effects of non-standard interactions. The proposed construction of the JUNO detector will provide a unique facility to address many outstanding crucial questions in particle and astrophysics in a timely and cost-effective fashion. It holds the great potential for further advancing our quest to understanding the fundamental properties of neutrinos, one of the building blocks of our Universe.

Topik & Kata Kunci

Physics

Penulis (227)

F. An

G. An

Q. An

V. Antonelli

E. Baussan

J. Beacom

L. Bezrukov

S. Blyth

R. Brugnera

M. Avanzini

J. Busto

A. Cabrera

H. Cai

Xiao Cai

A. Cammi

G. Cao

Jun Cao

Yung-Hsi Chang

Shaomin Chen

Shenjian Chen

Yixue Chen

D. Chiesa

M. Clemenza

B. Clerbaux

J. Conrad

D. D’Angelo

H. Kerret

Z. Deng

Yayun Ding

Z. Djurcic

D. Dornic

M. Dracos

O. Drapier

S. Dusini

S. Dye

T. Enqvist

D. Fan

Jian Fang

L. Favart

R. Ford

M. Goger-Neff

H. Gan

A. Garfagnini

M. Giammarchi

M. Gonchar

G. Gong

H. Gong

M. Gonin

M. Grassi

C. Grewing

M. Guan

V. Guarino

G. Guo

Wanlei Guo

Xinheng Guo

C. Hagner

R. Han

M. He

Y. Heng

Y. Hsiung

Jun Hu

Shouyang Hu

T. Hu

Hanxiong Huang

X. Huang

L. Huo

A. Ioannisian

M. Jeitler

X. Ji

Xiaoshan Jiang

C. Jollet

L. Kang

M. Karagounis

N. Kazarian

Z. Krumshteyn

A. Kruth

P. Kuusiniemi

T. Lachenmaier

R. Leitner

Chao Li

Jiaxing Li

Weidong Li

Wei-guo Li

Xiaomei Li

Xiao-nan Li

Yi Li

Yufeng Li

Zhibing Li

Haojun Liang

G. Lin

Tao Lin

Yen-Hsun Lin

J. Ling

I. Lippi

Dawei W. Liu

Hongbang Liu

Hu Liu

Jianglai Liu

Jianli Liu

Jinchang Liu

Qian Liu

Shubin Liu

Shulin Liu

P. Lombardi

Yongbing Long

Haoqi Lu

Jia-Shu Lu

Jing-qiao Lu

Junguang Lu

B. Lubsandorzhiev

L. Ludhova

S. Luo

V. Lyashuk

R. Mollenberg

Xubo Ma

F. Mantovani

Y. Mao

S. Mari

W. McDonough

Guangyuan Meng

A. Meregaglia

E. Meroni

M. Mezzetto

L. Miramonti

T. Mueller

D. Naumov

L. Oberauer

J. Ochoa-Ricoux

A. Olshevskiy

F. Ortica

A. Paoloni

H. Peng

J. Peng

E. Previtali

M. Qi

S. Qian

X. Qian

Y. Qian

Z. Qin

G. Raffelt

G. Ranucci

B. Ricci

M. Robens

A. Romani

X. Ruan

G. Salamanna

M. Shaevitz

V. Sinev

C. Sirignano

M. Sisti

O. Smirnov

M. Soiron

A. Stahl

L. Stanco

J. Steinmann

Xilei Sun

Y. Sun

D. Taichenachev

Jian Tang

I. Tkachev

W. Trzaska

S. Waasen

C. Volpe

V. Vorobel

L. Votano

Chung-Hsiang Wang

Guoli Wang

Hao Wang

Meng Wang

Ruiguang Wang

Siguang Wang

Wei Wang

Yi Wang

Yifang Wang

Zhe Wang

Zheng Wang

Zhi-gang Wang

Zhimin Wang

Wei Wei

L. Wen

C. Wiebusch

B. Wonsak

Qun Wu

C. Wulz

M. Wurm

Y. Xi

D. Xia

Yu-guang Xie

Z. Xing

Jilei Xu

B. Yan

Chang-gen Yang

Chaowen Yang

Guang Yang

Lei Yang

Yifan Yang

Yuyao Yao

U. Yegin

F. Yermia

Z. You

Boxiang Yu

Chun-xu Yu

Zeyuan Yu

S. Zavatarelli

L. Zhan

Chao Zhang

Honghao Zhang

Jiawen Zhang

Jingbo Zhang

Qingmin Zhang

Yu-Mei Zhang

Zhenyu Zhang

Zhenghua Zhao

Yangheng Zheng

W. Zhong

Guorong Zhou

Jing Zhou

Li Zhou

R. Zhou

Shun Zhou

Wenxiong Zhou

Xiang Zhou

Ye Zhou

Yu-Feng Zhou

Jiaheng Zou

Format Sitasi

APA MLA BibTeX

An, F., An, G., An, Q., Antonelli, V., Baussan, E., Beacom, J. et al. (2015). Neutrino Physics with JUNO. https://doi.org/10.1088/0954-3899/43/3/030401

@article{an2015, author = {F. An and G. An and Q. An and V. Antonelli and E. Baussan and J. Beacom and L. Bezrukov and S. Blyth and R. Brugnera and M. Avanzini and J. Busto and A. Cabrera and H. Cai and Xiao Cai and A. Cammi and G. Cao and Jun Cao and Yung-Hsi Chang and Shaomin Chen and Shenjian Chen and Yixue Chen and D. Chiesa and M. Clemenza and B. Clerbaux and J. Conrad and D. D’Angelo and H. Kerret and Z. Deng and Z. Deng and Yayun Ding and Z. Djurcic and D. Dornic and M. Dracos and O. Drapier and S. Dusini and S. Dye and T. Enqvist and D. Fan and Jian Fang and L. Favart and R. Ford and M. Goger-Neff and H. Gan and A. Garfagnini and M. Giammarchi and M. Gonchar and G. Gong and H. Gong and M. Gonin and M. Grassi and C. Grewing and M. Guan and V. Guarino and G. Guo and Wanlei Guo and Xinheng Guo and C. Hagner and R. Han and M. He and Y. Heng and Y. Hsiung and Jun Hu and Shouyang Hu and T. Hu and Hanxiong Huang and X. Huang and L. Huo and A. Ioannisian and M. Jeitler and X. Ji and Xiaoshan Jiang and C. Jollet and L. Kang and M. Karagounis and N. Kazarian and Z. Krumshteyn and A. Kruth and P. Kuusiniemi and T. Lachenmaier and R. Leitner and Chao Li and Jiaxing Li and Weidong Li and Wei-guo Li and Xiaomei Li and Xiao-nan Li and Yi Li and Yufeng Li and Zhibing Li and Haojun Liang and G. Lin and Tao Lin and Yen-Hsun Lin and J. Ling and I. Lippi and Dawei W. Liu and Hongbang Liu and Hu Liu and Jianglai Liu and Jianli Liu and Jinchang Liu and Qian Liu and Shubin Liu and Shulin Liu and P. Lombardi and Yongbing Long and Haoqi Lu and Jia-Shu Lu and Jing-qiao Lu and Junguang Lu and B. Lubsandorzhiev and L. Ludhova and S. Luo and V. Lyashuk and R. Mollenberg and Xubo Ma and F. Mantovani and Y. Mao and S. Mari and W. McDonough and Guangyuan Meng and A. Meregaglia and E. Meroni and M. Mezzetto and L. Miramonti and T. Mueller and D. Naumov and L. Oberauer and J. Ochoa-Ricoux and A. Olshevskiy and F. Ortica and A. Paoloni and H. Peng and J. Peng and E. Previtali and M. Qi and S. Qian and X. Qian and Y. Qian and Z. Qin and G. Raffelt and G. Ranucci and B. Ricci and M. Robens and A. Romani and X. Ruan and X. Ruan and G. Salamanna and M. Shaevitz and V. Sinev and C. Sirignano and M. Sisti and O. Smirnov and M. Soiron and A. Stahl and L. Stanco and J. Steinmann and Xilei Sun and Y. Sun and D. Taichenachev and Jian Tang and I. Tkachev and W. Trzaska and S. Waasen and C. Volpe and V. Vorobel and L. Votano and Chung-Hsiang Wang and Guoli Wang and Hao Wang and Meng Wang and Ruiguang Wang and Siguang Wang and Wei Wang and Yi Wang and Yifang Wang and Zhe Wang and Zheng Wang and Zhi-gang Wang and Zhimin Wang and Wei Wei and L. Wen and C. Wiebusch and B. Wonsak and Qun Wu and C. Wulz and M. Wurm and Y. Xi and D. Xia and Yu-guang Xie and Z. Xing and Jilei Xu and B. Yan and Chang-gen Yang and Chaowen Yang and Guang Yang and Lei Yang and Yifan Yang and Yuyao Yao and U. Yegin and F. Yermia and Z. You and Boxiang Yu and Chun-xu Yu and Zeyuan Yu and S. Zavatarelli and L. Zhan and Chao Zhang and Honghao Zhang and Jiawen Zhang and Jingbo Zhang and Qingmin Zhang and Yu-Mei Zhang and Zhenyu Zhang and Zhenghua Zhao and Yangheng Zheng and W. Zhong and Guorong Zhou and Jing Zhou and Li Zhou and R. Zhou and Shun Zhou and Wenxiong Zhou and Xiang Zhou and Ye Zhou and Yu-Feng Zhou and Jiaheng Zou}, title = {Neutrino Physics with JUNO}, year = {2015}, journal = {Semantic Scholar}, doi = {10.1088/0954-3899/43/3/030401}, url = {https://www.semanticscholar.org/paper/492d4b11579429cda2a6bb1b0e7ef8fbaa014869}, }

Akses Cepat

Lihat di Sumber doi.org/10.1088/0954-3899/43/3/030401

Informasi Jurnal

Tahun Terbit: 2015
Bahasa: en
Total Sitasi: 1189×
Sumber Database: Semantic Scholar
DOI: 10.1088/0954-3899/43/3/030401
Akses: Open Access ✓