Zobrazeno 1 - 10
of 305
pro vyhledávání: '"Kleinfelder S"'
Autor:
ARIANNA Collaboration, Anker, A., Baldi, P., Barwick, S. W., Beise, J., Besson, D. Z., Chen, P., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Liu, J., Nam, J., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Rice-Smith, R., Tatar, J., Terveer, K., Wang, S. -H, Zhao, L.
The ARIANNA experiment is an Askaryan radio detector designed to measure high-energy neutrino induced cascades within the Antarctic ice. Ultra-high-energy neutrinos above $10^{16}$ eV have an extremely low flux, so experimental data captured at trigg
Externí odkaz:
http://arxiv.org/abs/2307.07188
Autor:
ARIANNA Collaboration, Anker, A., Baldi, P., Barwick, S. W., Beise, J., Besson, D. Z., Bouma, S., Cataldo, M., Chen, P., Gaswint, G., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Liu, J., Magnuson, M., McAleer, S., Meyers, Z. M., Nam, J., Nelles, A., Novikov, A., Paul, M. P., Persichilli, C., Plaisier, I., Pyras, L., Rice-Smith, R., Tatar, J., Wang, S. -H, Welling, C., Zhao, L.
Publikováno v:
JINST 17 P03007 (2022)
The ARIANNA experiment is an Askaryan detector designed to record radio signals induced by neutrino interactions in the Antarctic ice. Because of the low neutrino flux at high energies ($E > 10^{16} $), the physics output is limited by statistics. He
Externí odkaz:
http://arxiv.org/abs/2112.01031
Autor:
ARIANNA Collaboration, Anker, A., Baldi, P., Barwick, S. W., Beise, J., Besson, D. Z., Bouma, S., Cataldo, M., Chen, P., Gaswint, G., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Liu, J., Magnuson, M., McAleer, S., Meyers, Z. S., Nam, J., Nelles, A., Novikov, A., Paul, M. P., Persichilli, C., Plaisier, I., Pyras, L., Rice-Smith, R., Tatar, J., Wang, S. -H, Welling, C., Zhao, L.
Publikováno v:
JCAP04(2022)022
The ARIANNA detector is designed to detect neutrinos with energies above $10^{17}$eV. Due to the similarities in generated radio signals, cosmic rays are often used as test beams for neutrino detectors. Some ARIANNA detector stations are equipped wit
Externí odkaz:
http://arxiv.org/abs/2112.01501
Autor:
Aguilar, J. A., Anker, A., Allison, P., Archambault, S., Baldi, P., Barwick, S. W., Beatty, J. J., Beise, J., Besson, D., Bishop, A., Bondarev, E., Botner, O., Bouma, S., Buitink, S., Cataldo, M., Chen, C. C., Chen, C. H., Chen, P., Chen, Y. C., Clark, B. A., Clay, W., Curtis-Ginsberg, Z., Connolly, A., Dasgupta, P., de Kockere, S., de Vries, K. D., Deaconu, C., DuVernois, M. A., Flaherty, J., Friedman, E., Gaior, R., Gaswint, G., Glaser, C., Hallgren, A., Hallmann, S., Hanson, J. C., Harty, N., Hendricks, B., Hoffman, K. D., Hornhuber, C., Hsu, S. Y., Hu, L., Huang, J. J., Huang, M. -H., Hughes, K., Ishihara, A., Karle, A., Kelley, J. L., Klein, S. R., Kleinfelder, S. A., Kim, K. -C., Kim, M. -C., Kravchenko, I., Krebs, R., Ku, Y., Kuo, C. Y., Kurusu, K., Lahmann, R., Landsman, H., Latif, U., Li, C. -J., Liu, J., Liu, T. -C., Lu, M. -Y., Madison, K., Mammo, J., Mase, K., McAleer, S., Meures, T., Meyers, Z. S., Michaels, K., Mikhailova, M., Mulrey, K., Nam, J., Nichol, R. J., Nelles, A., Novikov, A., Nozdrina, A., Oberla, E., Oeyen, B., Osborn, J., Pan, Y., Pandya, H., Paul, M. P., Persichilli, C., Plaisier, I., Punsuebsay, N., Pyras, L., Rice-Smith, R., Roth, J., Ryckbosch, D., Scholten, O., Seckel, D., Seikh, M. F. H., Shiao, Y. -S., Smith, D., Southall, D., Tatar, J., Torres, J., Toscano, S., Tosi, D., Touart, J., Broeck, D. J. Van Den, van Eijndhoven, N., Varner, G. S., Vieregg, A. G., Wang, M. -Z., Wang, S. -H, Wang, Y. H., Welling, C., Williams, D. R., Wissel, S., Xie, C., Yoshida, S., Young, R., Zhao, L., Zink, A.
The proposed IceCube-Gen2 (ICG2) seeks to instrument ~500 sq. km of Antarctic ice near the geographic South Pole with radio antennas, in order to observe the highest energy (E>1 EeV) neutrinos in the Universe. To this end, ICG2 will use the impulsive
Externí odkaz:
http://arxiv.org/abs/2103.06079
Autor:
ARIANNA Collaboration, Anker, A., Barwick, S. W., Bernhoff, H., Besson, D. Z., Bingefors, N., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Latif, U., Meyers, Z. S., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Tatar, J., Wang, S. H., Welling, C.
Publikováno v:
Journal of Instrumentation JINST 15 (2020) P09039
The sources of ultra-high energy (UHE) cosmic rays, which can have energies up to 10^20 eV, remain a mystery. UHE neutrinos may provide important clues to understanding the nature of cosmic-ray sources. ARIANNA aims to detect UHE neutrinos via radio
Externí odkaz:
http://arxiv.org/abs/2006.03027
Autor:
Anker, A., Baldi, P., Barwick, S. W., Bergman, D., Bernhoff, H., Besson, D. Z., Bingefors, N., Botner, O., Chen, P., Chen, Y., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Huang, J. J., Klein, S. R., Kleinfelder, S. A., Kuo, C. -Y., Lahmann, R., Latif, U., Liu, T., Lyu, Y., McAleer, S., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Shiao, J. Y., Tatar, J., van Vliet, A., Wang, S. -H., Wang, Y. -H., Welling, C.
The proposed ARIANNA-200 neutrino detector, located at sea-level on the Ross Ice Shelf, Antarctica, consists of 200 autonomous and independent detector stations separated by 1 kilometer in a uniform triangular mesh, and serves as a pathfinder mission
Externí odkaz:
http://arxiv.org/abs/2004.09841
Autor:
Anker, A., Barwick, S. W., Bernhoff, H., Besson, D. Z., Bingefors, N., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Latif, U., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Prakash, T., Shively, S. R., Tatar, J., Unger, E., Wang, S. H., Welling, C., Zierke, S.
Publikováno v:
Journal of Cosmology and Astroparticle Physics 11(2019)030
Ultra high energy neutrinos ($E_\nu > 10^{16.5}$eV$)$ are efficiently measured via radio signals following a neutrino interaction in ice. An antenna placed $\mathcal{O}$(15 m) below the ice surface will measure two signals for the vast majority of ev
Externí odkaz:
http://arxiv.org/abs/1909.02677
Autor:
Anker, A., Barwick, S. W., Bernhoff, H., Besson, D. Z., Bingefors, N., García-Fernández, D., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S. A., Lahmann, R., Latif, U., Nam, J., Novikov, A., Nelles, A., Paul, M. P., Persichilli, C., Plaisier, I., Prakash, T., Shively, S. R., Tatar, J., Unger, E., Wang, S. -H., Welling, C.
Publikováno v:
JCAP03(2020)053
The primary mission of the ARIANNA ultra-high energy neutrino telescope is to uncover astrophysical sources of neutrinos with energies greater than $10^{16}\mathrm{eV}$. A pilot array, consisting of seven ARIANNA stations located on the surface of th
Externí odkaz:
http://arxiv.org/abs/1909.00840
Autor:
Anker, A., Barwick, S. W., Bernhoff, H., Besson, D. Z., Bingefors, Nils, Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Lahmann, R., Latif, U., Nam, J., Novikov, A., Klein, S. R., Kleinfelder, S. A., Nelles, A., Paul, M. P., Persichilli, C., Shively, S. R., Tatar, J., Unger, E., Wang, S. -H., Yodh, G.
Publikováno v:
Advances in Space Research 64 (2019) 2595-2609
The measurement of ultra-high energy (UHE) neutrinos (E $>$ \SI{e16}{eV}) opens a new field of astronomy with the potential to reveal the sources of ultra-high energy cosmic rays especially if combined with observations in the electromagnetic spectru
Externí odkaz:
http://arxiv.org/abs/1903.01609
Autor:
Barwick, S. W., Berg, E. C., Besson, D. Z., Gaswint, G., Glaser, C., Hallgren, A., Hanson, J. C., Klein, S. R., Kleinfelder, S., Köpke, L., Kravchenko, I., Lahmann, R., Latif, U., Nam, J., Nelles, A., Persichilli, C., Sandstrom, P., Tatar, J., Unger, E.
Publikováno v:
JCAP07(2018)055
Ongoing experimental efforts in Antarctica seek to detect ultra-high energy neutrinos by measurement of radio-frequency (RF) Askaryan radiation generated by the collision of a neutrino with an ice molecule. An array of RF antennas, deployed either in
Externí odkaz:
http://arxiv.org/abs/1804.10430