Related papers: First Constraint on the Diffuse Supernova Neutrino…

Constraints on Neutrino-Nucleon Interactions at energies of 1 EeV with the IceCube Neutrino Observatory

A search for extremely high energy cosmic neutrinos has been carried out with the IceCube Neutrino Observatory. The main signals in the search are neutrino-induced energetic charged leptons and their rate depends on the neutrino-nucleon…

High Energy Physics - Phenomenology · Physics 2010-12-23 Shigeru Yoshida

Measurement of the ambient neutron flux and spectral distribution at the Canfranc Underground Laboratory

We report on the measurement of the ambient neutron flux and its energy distribution over a broad range of neutron energies, conducted in Hall A of the Canfranc Underground Laboratory using the High Efficiency Neutron Spectrometry Array…

Nuclear Experiment · Physics 2025-12-24 S. E. A. Orrigo , J. L. Tain , N. Mont-Geli , A. Tarifeño-Saldivia , L. M. Fraile , M. Grieger , A. Quero-Ballesteros , J. Agramunt , A. Algora , D. Bemmerer , F. Calviño , G. Cortés , A. De Blas , I. Dillmann , R. García , E. Nacher

Measurement of the Cosmic Ray and Neutrino-Induced Muon Flux at the Sudbury Neutrino Observatory

Results are reported on the measurement of the atmospheric neutrino-induced muon flux at a depth of 2 kilometers below the Earth's surface from 1229 days of operation of the Sudbury Neutrino Observatory (SNO). By measuring the flux of…

High Energy Physics - Experiment · Physics 2012-08-27 SNO Collaboration

Diffuse Supernova Neutrino Background from extensive core-collapse simulations of $8$-$100 {\rm M}_\odot$ progenitors

We revisit the diffuse supernova neutrino background in light of recent systematic studies of stellar core collapse that reveal the quantitative impacts of the progenitor conditions on the collapse process. In general, the dependence of the…

High Energy Astrophysical Phenomena · Physics 2018-02-07 Shunsaku Horiuchi , Kohsuke Sumiyoshi , Ko Nakamura , Tobias Fischer , Alexander Summa , Tomoya Takiwaki , Hans-Thomas Janka , Kei Kotake

Supernova Neutrino Background Bound on the SFR History

The purpose of the present study is to compare the predictions of different models of star formation rate (SFR) history in the universe with the upper limit of Super Kamiokande for the neutrino background. To this aim we have calculated the…

High Energy Astrophysical Phenomena · Physics 2015-10-07 Jafar Khodagholizadeh , Sepehr Arbabi Bidgoli , Zamri Zainal Abidin

Supernova Neutrino Detection in the Deep Underground Neutrino Experiment

The Deep Underground Neutrino Experiment (DUNE) is a dual-site experiment for long-baseline neutrino oscillation studies and for neutrino astrophysics and nucleon decay searches. The Far Detector of DUNE will consist of four 10 kt liquid…

Instrumentation and Detectors · Physics 2019-10-25 A. Gallego-Ros

Dynamic Neutrino Mass Ordering and Its Imprint on the Diffuse Supernova Neutrino Background

Neutrino masses may have evolved dynamically throughout the history of the Universe, potentially leading to a mass spectrum distinct from the normal or inverted ordering observed today. While cosmological measurements constrain the total…

High Energy Physics - Phenomenology · Physics 2026-05-27 Yuber F. Perez-Gonzalez , Manibrata Sen

Measurement of the Gamma Ray Background in the Davis Cavern at the Sanford Underground Research Facility

Deep underground environments are ideal for low background searches due to the attenuation of cosmic rays by passage through the earth. However, they are affected by backgrounds from $\gamma$-rays emitted by $^{40}$K and the $^{238}$U and…

Instrumentation and Detectors · Physics 2019-11-18 D. S. Akerib , C. W. Akerlof , S. K. Alsum , N. Angelides , H. M. Araújo , J. E. Armstrong , M. Arthurs , X. Bai , J. Balajthy , S. Balashov , A. Baxter , E. P. Bernard , A. Biekert , T. P. Biesiadzinski , K. E. Boast , B. Boxer , P. Brás , J. H. Buckley , V. V. Bugaev , S. Burdin , J. K. Busenitz , C. Carels , D. L. Carlsmith , M. C. Carmona-Benitez , M. Cascella , C. Chan , A. Cole , A. Cottle , J. E. Cutter , C. E. Dahl , L. de Viveiros , J. E. Y. Dobson , E. Druszkiewicz , T. K. Edberg , A. Fan , S. Fiorucci , H. Flaecher , T. Fruth , R. J. Gaitskell , J. Genovesi , C. Ghag , M. G. D. Gilchriese , S. Gokhale , M. G. D. van der Grinten , C. R. Hall , S. Hans , J. Harrison , S. J. Haselschwardt , S. A. Hertel , J. Y-K. Hor , M. Horn , D. Q. Huang , C. M. Ignarra , O. Jahangir , W. Ji , J. Johnson , A. C. Kaboth , K. Kamdin , D. Khaitan , A. Khazov , W. T. Kim , C. D. Kocher , L. Korley , E. V. Korolkova , J. Kras , H. Kraus , S. W. Kravitz , L. Kreczko , B. Krikler , V. A. Kudryavtsev , E. A. Leason , J. Lee , D. S. Leonard , K. T. Lesko , C. Levy , J. Li , J. Liao , F. -T. Liao , J. Lin , A. Lindote , R. Linehan , W. H. Lippincott , R. Liu , X. Liu , C. Loniewski , M. I. Lopes , B. López Paredes , W. Lorenzon , S. Luitz , J. M. Lyle , P. A. Majewski , A. Manalaysay , L. Manenti , R. L. Mannino , N. Marangou , M. F. Marzioni , D. N. McKinsey , J. McLaughlin , Y. Meng , E. H. Miller , M. E. Monzani , J. A. Morad , E. Morrison , B. J. Mount , A. St. J. Murphy , D. Naim , A. Naylor , C. Nedlik , C. Nehrkorn , H. N. Nelson , F. Neves , J. Nikoleyczik , A. Nilima , I. Olcina , K. C. Oliver-Mallory , S. Pal , K. J. Palladino , E. K. Pease , B. P. Penning , G. Pereira , A. Piepke , K. Pushkin , J. Reichenbacher , C. A. Rhyne , Q. Riffard , G. R. C. Rischbieter , J. P. Rodrigues , R. Rosero , P. Rossiter , G. Rutherford , A. B. M. R. Sazzad , R. W. Schnee , M. Schubnell , P. R. Scovell , D. Seymour , S. Shaw , T. A. Shutt , J. J. Silk , C. Silva , M. Solmaz , V. N. Solovov , P. Sorensen , I. Stancu , A. Stevens , T. M. Stiegler , K. Stifter , M. Szydagis , W. C. Taylor , R. Taylor , D. Temples , P. A. Terman , D. R. Tiedt , M. Timalsina , A Tomás , M. Tripathi , L. Tvrznikova , U. Utku , S. Uvarov , A. Vacheret , J. J. Wang , J. R. Watson , R. C. Webb , R. G. White , T. J. Whitis , F. L. H. Wolfs , D. Woodward , J. Yin

Limits on spin-dependent WIMP-nucleon cross section obtained from the complete LUX exposure

We present experimental constraints on the spin-dependent WIMP-nucleon elastic cross sections from the total 129.5 kg-year exposure acquired by the Large Underground Xenon experiment (LUX), operating at the Sanford Underground Research…

Cosmology and Nongalactic Astrophysics · Physics 2017-06-27 LUX Collaboration , D. S. Akerib , S. Alsum , H. M. Araújo , X. Bai , A. J. Bailey , J. Balajthy , P. Beltrame , E. P. Bernard , A. Bernstein , T. P. Biesiadzinski , E. M. Boulton , P. Brás , D. Byram , S. B. Cahn , M. C. Carmona-Benitez , C. Chan , A. A. Chiller , C. Chiller , A. Currie , J. E. Cutter , T. J. R. Davison , A. Dobi , J. E. Y. Dobson , E. Druszkiewicz , B. N. Edwards , C. H. Faham , S. R. Fallon , S. Fiorucci , R. J. Gaitskell , V. M. Gehman , C. Ghag , M. G. D. Gilchriese , C. R. Hall , M. Hanhardt , S. J. Haselschwardt , S. A. Hertel , D. P. Hogan , M. Horn , D. Q. Huang , C. M. Ignarra , R. G. Jacobsen , W. Ji , K. Kamdin , K. Kazkaz , D. Khaitan , R. Knoche , N. A. Larsen , C. Lee , B. G. Lenardo , K. T. Lesko , A. Lindote , M. I. Lopes , A. Manalaysay , R. L. Mannino , M. F. Marzioni , D. N. McKinsey , D. M. Mei , J. Mock , M. Moongweluwan , J. A. Morad , A. St. J. Murphy , C. Nehrkorn , H. N. Nelson , F. Neves , K. O'Sullivan , K. C. Oliver-Mallory , K. J. Palladino , E. K. Pease , L. Reichhart , C. Rhyne , S. Shaw , T. A. Shutt , C. Silva , M. Solmaz , V. N. Solovov , P. Sorensen , S. Stephenson , T. J. Sumner , M. Szydagis , D. J. Taylor , W. C. Taylor , B. P. Tennyson , P. A. Terman , D. R. Tiedt , W. H. To , M. Tripathi , L. Tvrznikova , S. Uvarov , V. Velan , J. R. Verbus , R. C. Webb , J. T. White , T. J. Whitis , M. S. Witherell , F. L. H. Wolfs , J. Xu , K. Yazdani , S. K. Young , C. Zhang

Measurement of the muon flux at the SND@LHC experiment

The Scattering and Neutrino Detector at the LHC (\SND) started taking data at the beginning of Run 3 of the LHC. The experiment is designed to perform measurements with neutrinos produced in proton-proton collisions at the LHC in an energy…

High Energy Physics - Experiment · Physics 2023-11-17 LHC Collaboration

Impact of the Dresden-II and COHERENT neutrino scattering data on neutrino electromagnetic properties and electroweak physics

Coherent elastic neutrino-nucleus scattering (CE$\nu$NS) represents a powerful tool to investigate key electroweak physics parameters and neutrino properties since its first observation in 2017 by the COHERENT experiment exploiting the…

High Energy Physics - Phenomenology · Physics 2023-03-15 M. Atzori Corona , M. Cadeddu , N. Cargioli , F. Dordei , C. Giunti , Y. F. Li , C. A. Ternes , Y. Y. Zhang

First Demonstration of a Scintillating Xenon Bubble Chamber for Detecting Dark Matter and Coherent Elastic Neutrino-Nucleus Scattering

A 30-g xenon bubble chamber, operated at Northwestern University in June and November 2016, has for the first time observed simultaneous bubble nucleation and scintillation by nuclear recoils in a superheated liquid. This chamber is…

Instrumentation and Detectors · Physics 2017-06-12 D. Baxter , C. J. Chen , M. Crisler , T. Cwiok , C. E. Dahl , A. Grimsted , J. Gupta , M. Jin , R. Puig , D. Temples , J. Zhang

Diffuse neutrinos from extragalactic supernova remnants: Dominating the 100 TeV IceCube flux

IceCube has measured a diffuse astrophysical flux of TeV-PeV neutrinos. The most plausible sources are unique high energy cosmic ray accelerators like hypernova remnants (HNRs) and remnants from gamma ray bursts in star-burst galaxies,…

High Energy Physics - Phenomenology · Physics 2015-05-19 Sovan Chakraborty , Ignacio Izaguirre

Implication of the non-detection of neutrinos above 2PeV

The IceCube telescope has detected diffuse neutrino emission, 20 events of which were reported to be above 60~TeV. In this paper, we fit the diffuse neutrino spectrum using Poisson statistics, which are the most appropriate for the low…

High Energy Astrophysical Phenomena · Physics 2016-06-01 Lee Yacobi , Dafne Guetta , Ehud Behar

A deuterated liquid scintillator for supernova neutrino detection

For the next galactic supernova, operational neutrino telescopes will measure the neutrino flux several hours before their optical counterparts. Existing detectors, relying mostly on charged current interactions, are mostly sensitive to…

High Energy Physics - Phenomenology · Physics 2022-12-06 Bhavesh Chauhan , Basudeb Dasgupta , Vivek Datar

First Indication of Solar $^8$B Neutrino Flux through Coherent Elastic Neutrino-Nucleus Scattering in PandaX-4T

The PandaX-4T liquid xenon detector at the China Jinping Underground Laboratory is used to measure the solar $^8$B neutrino flux by detecting neutrinos through coherent scattering with xenon nuclei. Data samples requiring the coincidence of…

High Energy Physics - Experiment · Physics 2024-09-16 PandaX Collaboration , Zihao Bo , Wei Chen , Xun Chen , Yunhua Chen , Zhaokan Cheng , Xiangyi Cui , Yingjie Fan , Deqing Fang , Zhixing Gao , Lisheng Geng , Karl Giboni , Xunan Guo , Xuyuan Guo , Zichao Guo , Chencheng Han , Ke Han , Changda He , Jinrong He , Di Huang , Houqi Huang , Junting Huang , Ruquan Hou , Yu Hou , Xiangdong Ji , Xiangpan Ji , Yonglin Ju , Chenxiang Li , Jiafu Li , Mingchuan Li , Shuaijie Li , Tao Li , Zhiyuan Li , Qing Lin , Jianglai Liu , Congcong Lu , Xiaoying Lu , Lingyin Luo , Yunyang Luo , Wenbo Ma , Yugang Ma , Yajun Mao , Yue Meng , Xuyang Ning , Binyu Pang , Ningchun Qi , Zhicheng Qian , Xiangxiang Ren , Dong Shan , Xiaofeng Shang , Xiyuan Shao , Guofang Shen , Manbin Shen , Wenliang Sun , Yi Tao , Anqing Wang , Guanbo Wang , Hao Wang , Jiamin Wang , Lei Wang , Meng Wang , Qiuhong Wang , Shaobo Wang , Siguang Wang , Wei Wang , Xiuli Wang , Xu Wang , Zhou Wang , Yuehuan Wei , Weihao Wu , Yuan Wu , Mengjiao Xiao , Xiang Xiao , Kaizhi Xiong , Yifan Xu , Shunyu Yao , Binbin Yan , Xiyu Yan , Yong Yang , Peihua Ye , Chunxu Yu , Ying Yuan , Zhe Yuan , Youhui Yun , Xinning Zeng , Minzhen Zhang , Peng Zhang , Shibo Zhang , Shu Zhang , Tao Zhang , Wei Zhang , Yang Zhang , Yingxin Zhang , Yuanyuan Zhang , Li Zhao , Jifang Zhou , Jiaxu Zhou , Jiayi Zhou , Ning Zhou , Xiaopeng Zhou , Yubo Zhou , Zhizhen Zhou

Disentangling Sub-GeV Dark Matter from the Diffuse Supernova Neutrino Background using Hyper-Kamiokande

The upcoming Hyper-Kamiokande (HyperK) experiment is expected to detect the Diffuse Supernova Neutrino Background (DSNB). This requires to ponder all possible sources of background. Sub-GeV dark matter (DM) which annihilates into neutrinos…

High Energy Physics - Phenomenology · Physics 2023-07-07 Sandra Robles

The DAE{\delta}ALUS Project: Rationale and Beam Requirements

Neutrino physics focuses on huge detectors deep underground. The Sanford Lab in South Dakota will build a 300 kiloton water-Cherenkov detector 1500 meters deep for muon neutrino oscillation studies of the mass hierarchy and CP violation.…

High Energy Physics - Experiment · Physics 2019-08-14 Jose R. Alonso

First search for extraterrestrial neutrino-induced cascades with IceCube

We report on the first search for extra-terrestrial neutrino-induced cascades in IceCube. The analyzed data were collected in the year 2007 when 22 detector strings were installed and operated. We will discuss the analysis methods used to…

High Energy Astrophysical Phenomena · Physics 2019-08-13 J. Kiryluk

ESSnuSB status

ESSnuSB (the European Spallation neutrino Super Beam) is a design study for a long-baseline neutrino experiment to precisely measure the CP violation in the leptonic sector, at the second neutrino oscillation maximum, using a beam driven by…

High Energy Physics - Experiment · Physics 2025-01-22 George Fanourakis , ESSnuSB Collaboration