High-energy neutrino astronomy with the super-kamiokande detector

Alec T Habig

High-energy neutrino astronomy with the super-kamiokande detector

Alec T Habig

Physics & Astronomy (Duluth)

Research output: Contribution to conference › Paper › peer-review

Abstract

The Super-Kamiokande experiment has collected a large sample of high-energy neutrino events. These are primarily atmospheric neutrinos, but a bright enough astrophysical source could also be visible. The data have been examined for possible point and bursting neutrino sources, as well as possible WIMP annihilation signatures. No significant evidence for such sources have been found, and the resulting flux limits have been calculated.

Original language	English (US)
Pages	267-270
Number of pages	4
State	Published - Jan 1 2005
Event	29th International Cosmic Ray Conference, ICRC 2005 - Pune, India Duration: Aug 3 2005 → Aug 10 2005

Other

Other	29th International Cosmic Ray Conference, ICRC 2005
Country/Territory	India
City	Pune
Period	8/3/05 → 8/10/05

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@conference{43f089d0b42f46a19ed23dc5906b017f,

title = "High-energy neutrino astronomy with the super-kamiokande detector",

abstract = "The Super-Kamiokande experiment has collected a large sample of high-energy neutrino events. These are primarily atmospheric neutrinos, but a bright enough astrophysical source could also be visible. The data have been examined for possible point and bursting neutrino sources, as well as possible WIMP annihilation signatures. No significant evidence for such sources have been found, and the resulting flux limits have been calculated.",

author = "Habig, \{Alec T\}",

year = "2005",

month = jan,

day = "1",

language = "English (US)",

pages = "267--270",

note = "29th International Cosmic Ray Conference, ICRC 2005 ; Conference date: 03-08-2005 Through 10-08-2005",

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TY - CONF

T1 - High-energy neutrino astronomy with the super-kamiokande detector

AU - Habig, Alec T

PY - 2005/1/1

Y1 - 2005/1/1

N2 - The Super-Kamiokande experiment has collected a large sample of high-energy neutrino events. These are primarily atmospheric neutrinos, but a bright enough astrophysical source could also be visible. The data have been examined for possible point and bursting neutrino sources, as well as possible WIMP annihilation signatures. No significant evidence for such sources have been found, and the resulting flux limits have been calculated.

AB - The Super-Kamiokande experiment has collected a large sample of high-energy neutrino events. These are primarily atmospheric neutrinos, but a bright enough astrophysical source could also be visible. The data have been examined for possible point and bursting neutrino sources, as well as possible WIMP annihilation signatures. No significant evidence for such sources have been found, and the resulting flux limits have been calculated.

UR - https://www.scopus.com/pages/publications/84898987601

UR - https://www.scopus.com/pages/publications/84898987601#tab=citedBy

M3 - Paper

AN - SCOPUS:84898987601

SP - 267

EP - 270

T2 - 29th International Cosmic Ray Conference, ICRC 2005

Y2 - 3 August 2005 through 10 August 2005

ER -

High-energy neutrino astronomy with the super-kamiokande detector

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