LOGIN TO YOUR ACCOUNT

Username
Password
Remember Me
Or use your Academic/Social account:

CREATE AN ACCOUNT

Or use your Academic/Social account:

Congratulations!

You have just completed your registration at OpenAire.

Before you can login to the site, you will need to activate your account. An e-mail will be sent to you with the proper instructions.

Important!

Please note that this site is currently undergoing Beta testing.
Any new content you create is not guaranteed to be present to the final version of the site upon release.

Thank you for your patience,
OpenAire Dev Team.

Close This Message

CREATE AN ACCOUNT

Name:
Username:
Password:
Verify Password:
E-mail:
Verify E-mail:
*All Fields Are Required.
Please Verify You Are Human:
fbtwitterlinkedinvimeoflicker grey 14rssslideshare1
Peeters, S J M; The SNO Collaboration, (2015)
Publisher: Elsevier
Languages: English
Types: Article
Subjects: Astrophysics - Solar and Stellar Astrophysics, QC, Nuclear Experiment

Classified by OpenAIRE into

arxiv: High Energy Physics::Experiment, Astrophysics::High Energy Astrophysical Phenomena, High Energy Physics::Phenomenology, Physics::Instrumentation and Detectors, Astrophysics::Solar and Stellar Astrophysics
The Sudbury Neutrino Observatory (SNO) has confirmed the standard solar model and neutrino oscillations through the observation of neutrinos from the solar core. In this paper we present a search for neutrinos associated with sources other than the solar core, such as gamma-ray bursters and solar flares. We present a new method for looking for temporal coincidences between neutrino events and astrophysical bursts of widely varying intensity. No correlations were found between neutrinos detected in SNO and such astrophysical sources.
  • The results below are discovered through our pilot algorithms. Let us know how we are doing!

    • Aglietta, M., Badino, G., Bologna, G., et al. 1991, Astrophys.J., 382, 344
    • Aharmim, B., et al. 2005, Phys.Rev., D72, 052010
    • Davis, R. 1994, Prog.Part.Nucl.Phys., 32, 13
    • -. 1996, Nucl.Phys.Proc.Suppl., 48, 284
    • Feldman, G. J., & Cousins, R. D. 1998, Phys.Rev., D57, 3873
    • Fukuda, S., et al. 2002, Astrophys.J., 578, 317
    • Hirata, K., Kajita, T., Kifune, T., et al. 1988, Phys.Rev.Lett., 61, 2653
    • Hirata, K. S., et al. 1990, Astrophys.J., 359, 574
    • Lorimer, D. R., Bailes, M., McLaughlin, M. A., Narkevic, D. J., & Crawford, F. 2007, Science, 318, 777
    • Mission, N. G. R. 2009, Electronic Catalogue, http://hesperia.gsfc.nasa.gov/hessi/
    • NASA. 2006, Swift, Electronic Catalogue, URL: http://heasarc.gsfc.nasa.gov/docs/swift/swiftsc.html
    • Odrzywolek, A., & Plewa, T. 2011, Astron.Astrophys, 529, A156
    • Palmer, D. M., Barthelmy, S., Gehrels, N., et al. 2005, Nature, 434, 1107
    • Piran, T. 2004, Rev.Mod.Phys., 76, 1143
    • Thrane, E., et al. 2009, Astrophys.J., 697, 730
  • No related research data.
  • No similar publications.

Share - Bookmark

Published in

Related to

  • egi

Cite this article