Revisiting the Triangulation Method for Pointing to Supernova and Failed Supernova with Neutrinos

Article, Preprint English OPEN
Mühlbeier, T.; Nunokawa, H.; Funchal, R. Zukanovich; (2013)
  • Publisher: AMER PHYSICAL SOC
  • Journal: PHYSICAL REVIEW D (issn: 1550-7998)
  • Related identifiers: doi: 10.1103/PhysRevD.88.085010
  • Subject: High Energy Physics - Phenomenology | High Energy Physics - Experiment | Astrophysics - High Energy Astrophysical Phenomena
    arxiv: Physics::Instrumentation and Detectors | Astrophysics::High Energy Astrophysical Phenomena | High Energy Physics::Experiment

In view of the advent of large-scale neutrino detectors such as IceCube, the future Hyper-Kamiokande and the ones proposed for the Laguna project in Europe, we re-examine the determination of the directional position of a Galactic supernova by means of its neutrinos usi... View more
  • References (29)
    29 references, page 1 of 3

    So, if we have two detectors, say, one at site 1 and

    the other at site 2, we can, explicitly, write the observed

    arrival time di erence as [1] H. A. Bethe, Rev. Mod. Phys. 62, 801 (1990). [2] H. -T. Janka, Ann. Rev. Nucl. Part. Sci. 62, 407 (2012)

    [arXiv:1206.2503 [astro-ph.SR]]. [3] A. S. Dighe and A. Y. .Smirnov, Phys. Rev. D 62, 033007

    (2000) [hep-ph/9907423]. [4] P. D. Serpico, S. Chakraborty, T. Fischer, L. Hudepohl,

    H. -T. Janka and A. Mirizzi, Phys. Rev. D 85, 085031

    (2012) [arXiv:1111.4483 [astro-ph.SR]]. [5] G. Pagliaroli, F. Vissani, E. Coccia and W. Fulgione,

    Phys. Rev. Lett. 103, 031102 (2009) [arXiv:0903.1191

    [hep-ph]]. [6] A. Burrows, D. Klein and R. Gandhi, Phys. Rev. D 45,

    3361 (1992). [7] A. Habig, K. Scholberg, and M. Vargin, poster pre-

  • Metrics
    No metrics available
Share - Bookmark