Results 11 to 20 of about 44,470 (237)

Supernova Neutrino Neutrino Astronomy [PDF]

Journal of Cosmology and Astroparticle Physics, 2018
Modern neutrino facilities will be able to detect a large number of neutrinos from the next Galactic supernova. We investigate the viability of the triangulation method to locate a core-collapse supernova by employing the neutrino arrival time ...
Brdar, Vedran, Lindner, Manfred, Xu, Xun-Jie   +2 more
core   +7 more sources

Multimessenger Astronomy with Neutrinos [PDF]

Universe, 2021
Multimessenger astronomy is arguably the branch of the astroparticle physics field that has seen the most significant developments in recent years. In this manuscript, we will review the state-of-the-art, the recent observations, and the prospects and ...
Francisco Salesa Greus, Agustín Sánchez Losa   +1 more
doaj   +4 more sources

The Evolution of Neutrino Astronomy [PDF]

Publications of the Astronomical Society of the Pacific, 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   +3 more sources

Neutrino astronomy with MACRO [PDF]

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.
L Perrone
openalex   +5 more sources

Neutrino Astronomy in the Ice [PDF]

Nuclear Physics B - Proceedings Supplements, 2009
The South Pole is an optimal location for hosting astrophysical observatories. The status of the construction of the IceCube Observatory and some selected physics results will be discussed. Moreover prospects for detection of Ultra-High Energy cosmogenic neutrinos and techniques that can address this energy region will be considered.
T. Montaruli
openalex   +5 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.
F. Halzen
openalex   +6 more sources

High-energy neutrino astronomy [PDF]

Astrophysics and Space Sciences Transactions, 2011
Neutrinos constitute a unique probe since they escape from their sources, travel undisturbed on cosmological distances and are produced in high-energy (HE) hadronic processes. In particular they would allow a direct detection and unambiguous identification of the acceleration sites of HE baryonic cosmic rays (CR), which remain unknown.
A. Kouchner
openalex   +4 more sources

Progress in neutrino astronomy [PDF]

Journal of the Korean Physical Society, 2021
AbstractThe dream of observing our universe through neutrinos is rapidly becoming a reality. More than three decades after the first observation of neutrinos from beyond our solar system associated with Supernova SN1987A, neutrino astronomy is in the midst of a revolution.
C. Rott
openalex   +2 more sources

UHE neutrino astronomy and neutrino oscillations

, 2009
UHE neutrinos with $E>10^{17}$ eV can be produced by ultra-high energy cosmic rays (UHECR) interacting with CMB photons (cosmogenic neutrinos) and by top-down sources, such as topological defects (TD), superheavy dark matter (SHDM) and mirror matter.
V. Berezinsky
openalex   +4 more sources

Neutrino Astronomy with the MACRO Detector [PDF]

The Astrophysical Journal, 2001
High energy gamma ray astronomy is now a well established field and several sources have been discovered in the region from a few GeV up to several TeV. If sources involving hadronic processes exist, the production of photons would be accompanied by neutrinos too.
A. Sciubba, C. De Marzo, Alec Habig, A. Rainò, V. Bisi, Mario Sitta, Donato Nicolo, Donato Nicolo, L. R. Sulak, M. Vakili, N. Giglietto, G. Mandrioli, M. De Vincenzi, E. Vilela, O. Palamara, D. Bakari, L. Perrone, M. Spinetti, J. Derkaoui, Eugenio Scapparone, F. Maaroufi, Halina Bilokon, C. Bemporad, G. Giannini, G. Giannini, A. A. Grillo, D. Levin, R. Pazzi, E. Lamanna, E. Lamanna, M. Grassi, S. L. Mufson, Kael Hanson, Annarita Margiotta, C. Satriano, M. Brigida, P. Bernardini, P. Spinelli, R. Antolini, G. Battistoni, F. Cafagna, S. Petrera, J. Reynoldson, Maurizio Spurio, P. Monacelli, M. Carboni, C. Forti, C. Favuzzi, E. Iarocci, L. Miller, L. Miller, Severino Angelo Maria Bussino, H. Dekhissi, M. Ouchrif, C. Bloise, C. Okada, R. Steinberg, S. Kyriazopoulou, R.M. Heinz, P. Serra, A. Marzari-Chiesa, L. Patrizii, Michael J. Longo, Frederic Jean Ronga, J. A. Musser, A. Baldini, Erik Katsavounidis, A. Di Credico, Roberto Bellotti, Paolo Lipari, D. Campana, Vincenzo Patera, Shahid Manzoor, Shahid Manzoor, Marco Monteno, Andrea Carlo Marini, S. Cecchini, J. L. Stone, C. W. Peck, C. W. Walter, C. W. Walter, M. Calicchio, C. Gustavino, F. Loparco, V. Chiarella, C. Orth, Gregory Tarle, Ioannis Katsavounidis, Kate Scholberg, C. R. Bower, G. Auriemma, D. G. Michael, V. Popa, E. Kearns, G. Mancarella, Np Longley, Np Longley, Lindsey Gray, R. Nolty, G. Giacomelli, O. Enriquez, G. de Cataldo, L. Satta, Hyun-Chul Kim, F. Guarino, Maximiliano Sioli, Teresa Montaruli, V. Togo, A. Surdo, G. C. Barbarino, R. C. Webb, M. N. Mazziotta, M. Ambrosio, P. Pistilli, S P Mikheyev, S P Mikheyev, M. Giorgini, S. Coutu, S. Coutu, I. De Mitri, Barry C. Barish, Fabrizio Cei, D. Martello, C. E. Lane, P. Fusco, G. Osteria, B. C. Choudhary   +126 more
openaire   +11 more sources