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The Antarctic Muon and Neutrino Detector Array (AMANDA) began collecting data with ten strings in 1997. Results from the first year of operation are presented. Neutrinos coming through the Earth from the Northern Hemisphere are identified…

Astrophysics · Physics 2008-11-26 AMANDA Collaboration , J. Ahrens

We report the measurement of the differential cross section $d^{2}\sigma (E_{\nu})/ d\cos(\theta_{\mu}) dP_{\mu}$ for inclusive muon-neutrino charged-current scattering on argon. This measurement utilizes data from 6.4$\times10^{20}$…

High Energy Physics - Experiment · Physics 2025-11-27 MicroBooNE Collaboration , P. Abratenko , O. Alterkait , D. Andrade Aldana , L. Arellano , J. Asaadi , A. Ashkenazi , S. Balasubramanian , B. Baller , G. Barr , D. Barrow , J. Barrow , V. Basque , O. Benevides Rodrigues , S. Berkman , A. Bhanderi , A. Bhat , M. Bhattacharya , M. Bishai , A. Blake , B. Bogart , T. Bolton , J. Y. Book , L. Camilleri , Y. Cao , D. Caratelli , I. Caro Terrazas , F. Cavanna , G. Cerati , Y. Chen , J. M. Conrad , M. Convery , L. Cooper-Troendle , J. I. Crespo-Anadon , M. Del Tutto , S. R. Dennis , P. Detje , A. Devitt , R. Diurba , Z. Djurcic , R. Dorrill , K. Duffy , S. Dytman , B. Eberly , P. Englezos , A. Ereditato , J. J. Evans , R. Fine , O. G. Finnerud , B. T. Fleming , N. Foppiani , W. Foreman , D. Franco , A. P. Furmanski , D. Garcia-Gamez , S. Gardiner , G. Ge , S. Gollapinni , O. Goodwin , E. Gramellini , P. Green , H. Greenlee , W. Gu , R. Guenette , P. Guzowski , L. Hagaman , O. Hen , R. Hicks , C. Hilgenberg , G. A. Horton-Smith , Z. Imani , B. Irwin , R. Itay , C. James , X. Ji , L. Jiang , J. H. Jo , R. A. Johnson , Y. J. Jwa , D. Kalra , N. Kamp , G. Karagiorgi , W. Ketchum , M. Kirby , T. Kobilarcik , I. Kreslo , M. B. Leibovitch , I. Lepetic , J. -Y. Li , K. Li , Y. Li , K. Lin , B. R. Littlejohn , H. Liu , W. C. Louis , X. Luo , C. Mariani , D. Marsden , J. Marshall , N. Martinez , D. A. Martinez Caicedo , A. Mastbaum , N. McConkey , V. Meddage , J. Micallef , K. Miller , K. Mistry , T. Mohayai , A. Mogan , M. Mooney , A. F. Moor , C. D. Moore , L. Mora Lepin , M. Moudgalya , S. Mulleria Babu , D. Naples , A. Navrer-Agasson , N. Nayak , M. Nebot-Guinot , J. Nowak , N. Oza , O. Palamara , N. Pallat , V. Paolone , A. Papadopoulou , V. Papavassiliou , H. Parkinson , S. F. Pate , N. Patel , Z. Pavlovic , E. Piasetzky , I. Ponce-Pinto , I. Pophale , S. Prince , X. Qian , J. L. Raaf , V. Radeka , A. Rafique , M. Reggiani-Guzzo , L. Ren , L. Rochester , J. Rodriguez Rondon , M. Rosenberg , M. Ross-Lonergan , C. Rudolph von Rohr , I. Safa , G. Scanavini , D. W. Schmitz , A. Schukraft , W. Seligman , M. H. Shaevitz , R. Sharankova , J. Shi , E. L. Snider , M. Soderberg , S. Soldner-Rembold , J. Spitz , M. Stancari , J. St. John , T. Strauss , A. M. Szelc , W. Tang , N. Taniuchi , K. Terao , C. Thorpe , D. Torbunov , D. Totani , M. Toups , Y. -T. Tsai , J. Tyler , M. A. Uchida , T. Usher , B. Viren , M. Weber , H. Wei , A. J. White , Z. Williams , S. Wolbers , T. Wongjirad , M. Wospakrik , K. Wresilo , N. Wright , W. Wu , E. Yandel , T. Yang , L. E. Yates , H. W. Yu , G. P. Zeller , J. Zennamo , C. Zhang

We present the measurement of two event samples induced by atmospheric $\nu_\mu$ of average energy $ \bar {E}_\nu \sim 4 GeV$. In the first sample, the neutrino interacts inside the MACRO detector producing an upward-going muon leaving the…

High Energy Physics - Experiment · Physics 2012-08-27 The MACRO Collaboration

An estimate of the energy of neutrino-induced muons in MACRO is provided by a multiple Coulomb scattering measurement. The MACRO original upward-muon data sample has been subdivided according to the reconstructed muon energy. Data in each…

High Energy Physics - Experiment · Physics 2019-08-14 M. Sioli

Cosmic-rays with energies up to $3\times10^{20}$ eV have been observed. The nuclear composition of these cosmic rays is unknown but if the incident nuclei are protons then the corresponding center of mass energy is $\sqrt{s_{nn}} = 700$…

Nuclear Experiment · Physics 2009-11-18 Spencer R. Klein

The final results of the MACRO experiment on the search for GUT supermassive magnetic monopoles in the penetrating cosmic radiation are presented and discussed. The 90% CL upper limits are at the level of 1.5 - 2 x 10^-16 cm^-2 s^-1 sr^-1…

High Energy Physics - Experiment · Physics 2019-08-14 G. Giacomelli

Neutrinos provide a unique probe of both particle physics and the high-energy universe, traversing astronomical distances with minimal interaction. Their charged-current scattering cross section encodes fundamental information about weak…

High Energy Physics - Experiment · Physics 2026-05-12 N. Bhuiyan , K. Abe , Y. Asaoka , M. Harada , Y. Hayato , K. Hiraide , T. H. Hung , K. Ieki , M. Ikeda , J. Kameda , Y. Kanemura , Y. Kataoka , S. Miki , S. Mine , M. Miura , S. Moriyama , K. Nakagiri , M. Nakahata , S. Nakayama , Y. Noguchi , G. Pronost , K. Sato , H. Sekiya , R. Shinoda , M. Shiozawa , Y. Suzuki , A. Takeda , Y. Takemoto , H. Tanaka , T. Yano , S. Chen , Y. Itow , T. Kajita , R. Nishijima , K. Okumura , T. Tashiro , T. Tomiya , X. Wang , P. Fernandez , F. J. de Garay Arcones , L. Labarga , D. Samudio , B. Zaldivar , C. Yanagisawa , B. Jargowsky , E. Kearns , J. Mirabito , L. Wan , T. Wester , B. W. Pointon , J. Bian , B. Cortez , N. J. Griskevich , Y. Jiang , M. B. Smy , H. W. Sobel , V. Takhistov , A. Yankelevich , J. Hill , D. H. Moon , R. G. Park , B. S. Yang , K. Scholberg , C. W. Walter , O. Drapier , A. Ershova , M. Ferey , E. Le Blévec , Th. A. Mueller , P. Paganini , C. Quach , R. Rogly , T. Nakamura , J. S. Jang , R. P. Litchfield , L. N. Machado , F. J. P. Soler , J. G. Learned , K. Choi , S. Cao , L. H. V. Anthony , N. W. Prouse , M. Scott , Y. Uchida , V. Berardi , N. F. Calabria , M. G. Catanesi , N. Ospina , E. Radicioni , A. Langella , G. De Rosa , G. Collazuol , M. Feltre , M. Mattiazzi , L. Ludovici , M. Gonin , L. Périssé , B. Quilain , M. Fukazawa , S. Horiuchi , A. Kawabata , M. Kobayashi , Y. M. Liu , Y. Maekawa , Y. Nishimura , A. Oka , R. Akutsu , M. Friend , T. Hasegawa , Y. Hino , T. Ishida , T. Kobayashi , T. Matsubara , T. Nakadaira , Y. Oyama , A. Portocarrero Yrey , K. Sakashita , T. Sekiguchi , G. T. Burton , F. Di Lodovico , T. Katori , R. Kralik , N. Latham , R. M. Ramsden , V. Siccardi , S. Aoyama , H. Banbara , Y. Inaba , H. Ito , M. Nishigami , T. Sone , A. T. Suzuki , Y. Takeuchi , S. Wada , H. Zhong , J. Feng , L. Feng , S. Han , J. Hikida , J. R. Hu , Z. Hu , M. Kawaue , T. Kikawa , T. Nakaya , T. V. Ngoc , R. A. Wendell , S. J. Jenkins , N. McCauley , A. Tarrant , M. Fanì , M. J. Wilking , Z. Xie , Y. Fukuda , H. Menjo , Y. Yoshioka , J. Lagoda , M. Mandal , J. Zalipska , M. Mori , J. Jiang , Y. Asano , K. Hamaguchi , H. Ishino , Y. Koshio , F. Nakanishi , S. Ohshita , T. Tada , T. Ishizuka , G. Barr , D. Barrow , L. Cook , S. Samani , D. Wark , A. Holin , F. Nova , M. Jo , S. Jung , J. Yoo , J. E. P. Fannon , L. Kneale , T. Peacock , P. Stowell , H. Okazawa , S. M. Lakshmi , S. Hong , E. Kwon , M. W. Lee , J. W. Seo , I. Yu , Y. Ashida , A. K. Ichikawa , K. D. Nakamura , S. Abe , S. Goto , S. Kodama , Y. Kong , H. Hayasaki , Y. Masaki , Y. Mizuno , T. Muro , K. Nakagiri , Y. Nakajima , M. Sekiyama , N. Taniuchi , T. Yamazumi , M. Yokoyama , P. de Perio , S. Fujita , C. Jesús-Valls , K. Martens , Ll. Marti , A. D. Santos , K. M. Tsui , M. R. Vagins , S. Izumiyama , M. Kuze , R. Matsumoto , R. Asaka , C. Ise , M. Ishitsuka , M. Sugo , M. Wako , K. Yamauchi , Y. Nakano , F. Cormier , R. Gaur , M. Hartz , A. Konaka , X. Li , B. R. Smithers , S. Chen , Y. Wu , B. D. Xu , A. Q. Zhang , B. Zhang , H. Adhikary , M. Girgus , P. Govindaraj , M. Posiadala-Zezula , Y. S. Prabhu , S. B. Boyd , R. Edwards , D. Hadley , M. O'Flaherty , B. Richards , A. Ali , B. Jamieson , C. Bronner , D. Horiguchi , A. Minamino , Y. Sasaki , R. Shibayama , R. Shimamura

We have studied the muon decay energy spectrum from a sample of stopping muon events acquired during the test run of the ICARUS T600 prototype. This detector allows the spatial reconstruction of the events with fine granularity, hence the…

High Energy Physics - Experiment · Physics 2011-09-13 Javier Rico

This work is dedicated to the study of a technique for hadron identification in the TeV momentum range, based on the simultaneous measurement of the energies and of the emission angles of the Transition Radiation (TR) X-rays with respect to…

The Large Volume Detector (LVD), hosted in the INFN Laboratori Nazionali del Gran Sasso, is triggered by atmospheric muons at a rate of $\sim 0.1$~Hz. The data collected over almost a quarter of century are used to study the muon intensity…

We calculate event rate and demonstrate the observational feasibility of very high energy muons (1-1000 TeV) in a large mass underground detector operating as a pair-meter. This energy range corresponds to surface muon energies of $\sim$(5…

High Energy Physics - Phenomenology · Physics 2009-11-11 Raj Gandhi , Sukanta Panda

The front-end electronics of silicon detectors are typically designed to ensure optimal noise performance for the expected input charge. A combination of preamplifiers and shaper circuits result in a nontrivial response of the front-end to…

Instrumentation and Detectors · Physics 2024-07-02 M. J. Basso , E. Buchanan , B. J. Gallop , J. J. John , J. Kaplon , P. T. Keener , P. W. Phillips , L. Poley , C. A. Sawyer , D. Sperlich , M. Warren

After a brief presentation of the MACRO detector we discuss the updated data on atmospheric muon neutrinos, and the interpretation in terms of neutrino oscillations.

High Energy Physics - Experiment · Physics 2016-11-03 M. Spurio

ATLAS is a detector under construction to explore the physics at the Large Hadron Collider at CERN. It has a muon spectrometer with an excellent momentum resolution of 3-10%, provided by three layers of precision monitored-drift-tube…

Instrumentation and Detectors · Physics 2007-05-23 S. Horvat , O. Kortner , H. Kroha , A. Manz , S. Mohrdieck , V. Zhuravlov

IceCube detects neutrinos at energies orders of magnitude higher than any neutrinos produced at particle accelerators. Neutrinos are weakly interacting particles but at energies above 30 TeV the Earth becomes opaque to neutrinos. The…

High Energy Astrophysical Phenomena · Physics 2019-08-20 Sally Robertson

Upward throughgoing muons in underground detectors are induced by atmospheric $\nu_\mu$ with energies in the $1-10^4 GeV$ range. The oscillations of atmospheric muon neutrinos should affect mainly those with energy smaller than $E_\nu \sim…

High Energy Physics - Experiment · Physics 2007-05-23 D. Bakari , Y. Becherini , M. Spurio

Active Galactic Nuclei are considered as sources of neutrinos, with neutrino energies extending up to 10^{18} eV. It is expected that these highly energetic cosmic neutrinos will be detected by the neutrino telescopes, presently under…

High Energy Physics - Phenomenology · Physics 2010-11-30 N. Arteaga-Romero , C. Carimalo , A. Nicolaidis , O. Panella , G. Tsirigoti

Transport of fast electron in overdense plasmas is of key importance in high energy density physics. However, it is challenging to diagnose the fast electron transport in experiments. In this article, we study coherent transition radiation…

Measurements of the total cross section of e+e- -> hadrons are presented in two different ranges of centre-of-mass energy. The measurements are made using the CLEO III and CLEO-c detectors at the Cornell Electron Storage Ring. The absolute…

High Energy Physics - Experiment · Physics 2008-11-07 CLEO Collaboration , Jim Libby

Whether studying neutrinos for their own sake or as a messenger particle, neutrino cross sections are critically important for numerous analyses. On the low energy side, measurements from accelerator experiments reach up to a few 100s of…

High Energy Astrophysical Phenomena · Physics 2021-07-22 Sarah Nowicki
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