Results 61 to 70 of about 46,693 (203)

The Evolution of Neutrino Astronomy

, 2000
How did neutrino astronomy evolve? Are there any useful lessons for astronomers and physicists embarking on new observational ventures today? We answer the first question; the reader can can decide if there are any useful parallels for other fields ...
Bahcall, John, Davis, Jr, Raymond
core   +1 more source

Flux of Atmospheric Neutrinos [PDF]

, 2002
Atmospheric neutrinos produced by cosmic-ray interactions in the atmosphere are of interest for several reasons. As a beam for studies of neutrino oscillations they cover a range of parameter space hitherto unexplored by accelerator neutrino beams.
Ahrens J, Engel R, Engel R, Gaisser TK, Gaisser TK, Goldschmidt A, Hebbeker T, Honda M, Ivanenko IP, Lipari P, Liu Y, M. Honda, Motoki M, Page DE, Papini P, Roesler S, Sanuki T, Stanev T, Störmer C, T. K. Gaisser, Tserkovnyak Y, Webber WR, Wentz J, Zatsepin GT, Zatsepin GT   +24 more
core   +4 more sources

Neutrino Astronomy with MACRO

Nuclear Physics B - Proceedings Supplements, 2002
High energy neutrinos from astrophysical sources can be detected as upward-going muons produced in charged-current interactions with the matter surrounding the detector. We present the results of a search for either a diffuse astrophysical neutrino flux or a point-like source of neutrinos in the sample of upward-going muons gathered by MACRO.
Ambrosio M, Antolini R, Assiro R, Auriemma G, Bakari D, Baldini A, Barbarino GC, Barbarito E, Barish BC, Battistoni G, Becherini Y, Bellotti R, Bemporad C, Bernardini P, Bilokon H, Bisi V, Bloise C, Bottazzi E, Bower C, Brigida M, BUSSINO, Severino Angelo Maria, Cafagna F, Calicchio M, Campana D, Candela A, Carboni M, Cecchini S, Cei F, Ceres A, Chiarella V, Choudhary BC, Coutu S, Cozzi M, Creti P, De Cataldo G, Degli Esposti L, Dekhissi H, De Marzo C, De Mitri I, Derkaoui J, De Vincenzi M, Di Credico A, Di Ferdinando D, Diotallevi R, Erriquez O, Favuzzi C, Forti C, Fusco P, Gebhard M, Giacomelli G, Giacomelli R, Giannini G, Giglietto N, Giorgini M, Giuliani R, Goretti M, Grassi M, Grau H, Gray L, Grillo A, Guarino F, Gustavino C, Habig A, Hanson J, Hanson K, Hawthorne A, Heinz R, Hong JT, Iarocci E, Katsavounidis E, Katsavounidis I, Kearns E, Kim H, Kyriazopoulou S, Lamanna E, Lane C, Leone A, Levin DS, Lipari P, Liu G, Liu R, Longley NP, Longo MJ, Loparco F, Maaroufi F, Mancarella G, Mandrioli G, Manzoor S, Marrelli V, Margiotta A, Marini A, Martello D, Marzari Chiesa A, Mazziotta MN, Michael DG, Mikheyev S, Miller L, Monacelli P, Mongelli M, Montaruli T, Monteno M, Mossbarger L, Mufson S, Musser J, Nicolo D, Nolty R, Okada C, Orsini M, Orth C, Osteria G, Ouchrif M, Palamara O, Parlati S, Patera V, Patrizii L, Pazzi R, Peck CW, Pellizzoni G, Perchiazzi M, Perrone L, Petrakis J, Petrera S, Pignatano N, Pinto C, Pistilli P, Popa V, Raino A, Reynoldson J, Ronga F, Rrhioua A, Sacchetti A, Saggese P, Satriano C, Satta L, Scapparone E, Scholberg K, Sciubba A, Serra P, Sioli M, Sirri G, Sitta M, Sondergaard S, Spinelli P, Spinetti M, Spurio M, Stalio S, Steinberg R, Stone JL, Sulak LR, Surdo A, Tarle G, Togo V, Vakili M, Valieri C, Walter CW, Webb R, Zaccheo N.   +156 more
openaire   +3 more sources

Compressibility Function and Speed of Sound in the Non‐Commutative Quantum Hadrodynamics Type‐I Model for Neutron Stars

Astronomische Nachrichten, Volume 346, Issue 7-8, September 2025.
ABSTRACT We investigate the effects of a minimal measurable length on neutron stars, within the quantum hadrodynamics (QHD‐I) model modified by the Generalized Uncertainty Principle (GUP). Working in a deformed Poisson algebra framework, we incorporate GUP effects via a time‐invariant transformation of the phase space volume, effectively reducing the ...
João Gabriel Galli Gimenez, Dimiter Hadjimichef, César A. Zen Vasconcellos   +2 more
wiley   +1 more source

The Antares Neutrino Telescope and Multi-Messenger Astronomy [PDF]

, 2010
Antares is currently the largest neutrino telescope operating in the Northern Hemisphere, aiming at the detection of high-energy neutrinos from astrophysical sources.
Berezhko E G Völk H J, Bouwhuis M (for Antares), Chassande Mottin E, Dornic D (for Antares), Franckowiak A, Guillard G (for Antares), Halzen F, Holder J (Veritas Collaboration), Markov M A, Petrovic J, Thierry Pradier   +10 more
core   +3 more sources

Neutrino astronomy: An update [PDF]

Astroparticle Physics, 2012
AbstractDetecting neutrinos associated with the still enigmatic sources of cosmic rays has reached a new watershed with the completion of IceCube, the first detector with sensitivity to the anticipated fluxes. In this review, we will briefly revisit the rationale for constructing kilometer-scale neutrino detectors and summarize the status of the field.
openaire   +1 more source

Monitoring Fracture Hydromechanical Evolution in the Lab and Field Using Unsupervised Metric Learning

Journal of Geophysical Research: Machine Learning and Computation, Volume 2, Issue 3, September 2025.
Abstract Fractures evolve in time through thermal‐hydraulic‐mechanical‐chemical (THMC) processes that alter their long‐range hydraulic transport properties and modify subsurface behavior and activities. The location of subsurface fractures makes it necessary to use remote sensing techniques such as passive or active seismic monitoring for fracture ...
David D. Nolte, Laura J. Pyrak‐Nolte, Chet Hopp   +2 more
wiley   +1 more source

Neutrino physics and astrophysics with the MACRO detector [PDF]

, 2000
After a brief presentation of the MACRO detector we discuss the data on atmospheric neutrinos and neutrino oscillations, on high energy (E> 1 GeV) neutrino astronomy, on indirect searches for WIMPs and low energy (E >7 MeV) stellar collapse neutrinos ...
Giacomelli, G., Margiotta, A.
core   +1 more source

Revisiting the hot matter in the center of gamma-ray bursts and supernova [PDF]

, 2013
Hot matter with nucleons can be produced in the inner region of the neutrino-dominated accretion flow in gamma-ray bursts or during the proto-neutron star birth in successful supernova.
Li, A., Liu, T.
core   +1 more source

Magnetic Precursor to the Structural Phase Transition in V2O3

Advanced Electronic Materials, Volume 11, Issue 12, August 6, 2025.
V₂O₃, a model Mott insulator, undergoes a metal‐insulator transition linked to structural and magnetic transitions, though the underlying mechanism remains unclear. Through muon‐spin rotation and X‐ray diffraction on strain‐engineered thin films, a magnetic precursor to the structural transition is identified, emphasizing the key role of magnetism in ...
Chubin Huang, Abhishek Rakshit, Gianluca Janka, Zaher Salman, Andreas Suter, Thomas Prokscha, Benjamin A. Frandsen, Yoav Kalcheim   +7 more
wiley   +1 more source