Results 91 to 100 of about 698 (138)

The NEXT-100 Detector. [PDF]

Eur Phys J C Part Fields
NEXT Collaboration.
europepmc   +1 more source

An axisymmetric shock breakout indicated by prompt polarized emission from the type II supernova 2024ggi. [PDF]

Sci Adv
Yang Y, Wen X, Wang L, Baade D, Wheeler JC, Filippenko AV, Gal-Yam A, Maund J, Schulze S, Wang X, Ashall C, Bulla M, Cikota A, Gao H, Hoeflich P, Li G, Mishra D, Patat F, Patra KC, Vasylyev SS, Yan S.   +20 more
europepmc   +1 more source

Invisible Labor and the "Ghost Particle": Underground Physics at the Kolar Gold Fields. [PDF]

Ber Wiss
Rao N.
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First demonstration of a TES based cryogenic Li 2 MoO 4 detector for neutrinoless double beta decay search. [PDF]

Eur Phys J C Part Fields
Bratrud G, Chang CL, Chen R, Cudmore E, Figueroa-Feliciano E, Hong Z, Kennard KT, Lewis S, Lisovenko M, Mateo LO, Novati V, Novosad V, Oliveri E, Ren R, Scarpaci JA, Schmidt B, Wang G, Winslow L, Yefremenko VG, Zhang J, Baxter D, Hollister M, James C, Lukens P, Temples DJ.   +24 more
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Probing the Higgs portal to a strongly-interacting dark sector at the FCC-ee. [PDF]

Eur Phys J C Part Fields
Cazzaniga C, de Cosa A, Kahlhoefer F, Maria AS, Seidita R, Sitti E.   +5 more
europepmc   +1 more source

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A new solar neutrino detector

Nuclear Physics B - Proceedings Supplements, 1993
Abstract This paper describes the main features of the proposed low energy solar neutrino detector Borexino, planned to be installed at the Gran Sasso Laboratory. This real time detector is based on a massive, calorimetric, liquid scintillation spectroscopy technique, whose high luminosity is the base for the attempt to achieve a low signal detection
G. Alimonti, B. Alpat, C. Arpesella, G. Bellini, P. Benetti, S. Bonetti, F. Calaprice, M. Campanella, G. Cecchet, A. Debari, M. Deutsch, A. Donati, F. Elisei, F. Vonfeilitzsch, D. Franciotti, M. Giammarchi, D. Giugni, A. Golubchikov, G. Husser, T. Kovacs, I. Manno, G. Mantovani, G. Manuzio, F. Masetti, U. Mazzucato, E. Meroni, J. Mitchell, L. Oberauer, S. Pakvasa, A. Perotti, A. Preda, P. Raghavan, R. Raghavan, F. Ragusa, G. Ranucci, R. Scardaoni, S. Schonert, O. Smirnov, R. Tartaglia, G. Testera, P. Ullucci, S. Vitale, O. Zaimidoroga   +42 more
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Dumand: The Ocean as a Neutrino Detector

1977
We consider the possibility of using the ocean as a neutrino detector; neutrino-produced interactions result in charged particles that generate Cerenkov radiation in the water, which can be detected by light-gathering equipment and photomultipliers. The properties of the ocean as seen from this standpoint are critically examined, and the advantages and
A. Roberts, H. Blood, J. Learned, F. Reines   +3 more
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Solar flares and neutrino detectors

Physical Review Letters, 1988
Solar flares have been suggested as the cause of occasional high counting rates in the $^{37}\mathrm{Cl}$ solar-neutrino experiment. The sensitivity of neutrino detectors to flares is evaluated. Several neutrino detectors will show large signals when prominent flares are observed electromagnetically, if flares are detected in the chlorine experiment.
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The AMANDA Neutrino Detector

Nuclear Physics B - Proceedings Supplements, 1999
The first stage of the AMANDA High Energy Neutrino Detectorat the South Pole, the 302 PMT array AMANDA-B with an expected effectivearea for TeV neutrinos of similar to 10(4) m(2), has been taking datasince 1997. Progress with calibration, investigation of ice properties,as well as muon and neutrino data analysis are described.
R. Wischnewski, E. Andrés, P. Askebjer, S. Barwick, R. Bay, L. Bergström, A. Biron, J. Booth, O. Botner, A. Bouchta, S. Carius, M. Carlson, W. Chinowsky, D. Chirkin, D. Cowen, C. Costa, E. Dalberg, T. Deyoung, J. Edsjo, P. Ekström, A. Goobar, L. Gray, A. Hallgren, F. Halzen, R. Hardtke, Y. He, G. Hill, P. Hulth, S. Hundertmark, J. Jacobsen, V. Kandhadai, A. Karle, J. Kim, H. Leich, M. Leuthold, P. Lindahl, T. Liss, I. Liubarsky, P. Loaiza, D. Lowder, P. Marciniewski, T. Miller, P. Miocinovic, P. Mock, R. Morse, M. Newcomer, P. Niessen, D. Nygren, C. Pérez de los Heros, R. Porrata, P. Price, G. Przybylski, W. Rhode, S. Richter, J. Rodriguez, P. Romenesko, D. Ross, H. Rubinstein, T. Schmidt, E. Schneider, R. Schwarz, U. Schwendicke, G. Smoot, M. Solarz, V. Sorin, C. Spiering, P. Steffen, R. Stokstad, O. Streicher, L. Thollander, T. Thon, S. Tilav, C. Walck, C. Wiebusch, K. Woschnagg, W. Wu, G. Yodh, S. Young   +77 more
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Salt neutrino detector for ultrahigh-energy neutrinos

Physics of Atomic Nuclei, 2004
Rock salt and limestone are studied to determine their suitability for use as a radio-wave transmission medium in an ultrahigh energy (UHE) cosmic neutrino detector. A sensible radio wave would be emitted by the coherent Cherenkov radiation from negative excess charges inside an electromagnetic shower upon interaction of a UHE neutrino in a high ...
M. Chiba, T. Kamijo, O. Yasuda, Y. Chikashige, T. Kon, Y. Takeoka, R. Yoshida   +6 more
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