Ultrahigh energy nu(tau) detection at Pierre Auger Observatory - INSPIRE

DataBETA

Ultrahigh energy nu(tau) detection at Pierre Auger Observatory

Gennaro Miele
(
- Naples U. and
- INFN, Naples
)
,
L. Perrone
(
- Wuppertal U.
)
,
O. Pisanti
(
- Naples U. and
- INFN, Naples
)

Dec, 2004

4 pages

Part of Proceedings, Neutrino Oscillation Workshop (NOW 2004), 347-350

Published in:

Nucl.Phys.B Proc.Suppl. 145 (2005) 347-350

Contribution to:

- NOW 2004
, 347-350

e-Print:

astro-ph/0412321 [astro-ph]

DOI:

10.1016/j.nuclphysbps.2005.04.037

Experiments:

AUGER

View in:

ADS Abstract Service

reference search4 citations

Citations per year

Abstract: (arXiv)

Earth--skimming UHE tau neutrinos have a chance to be detected by the Fluorescence Detector (FD) of Pierre Auger Observatory if their astrophysical flux is large enough. A detailed evaluation of the expected number of events is here performed for a wide class of neutrino flux models.

References(9)

Figures(0)

Cosmic rays at ultrahigh-energies (neutrino?)

V.S. Berezinsky
(
- Lebedev Inst.
)
,
G.T. Zatsepin
(
- Lebedev Inst.
)

- Phys.Lett.B 28 (1969) 423-424
•
DOI:
- 10.1016/0370-2693(69)90341-4

- Sov.J.Nucl.Phys. 11 111

Ultrahigh-energy neutrino fluxes and their constraints

Oleg E. Kalashev
(
- Moscow, INR
)
,
Vadim A. Kuzmin
(
- Moscow, INR
)
,
Dmitry V. Semikoz
(
- Moscow, INR and
- Munich, Max Planck Inst.
)
,
Gunter Sigl
(
- Paris, Inst. Astrophys.
)

- Phys.Rev.D 66 (2002) 063004
•
e-Print:
- hep-ph/0205050
•
DOI:
- 10.1103/PhysRevD.66.063004

Ultrahigh-energy neutrino fluxes: New constraints and implications

Dmitry V. Semikoz
(
- Munich, Max Planck Inst. and
- Moscow, INR
)
,
Gunter Sigl
(
- Paris, Inst. Astrophys.
)

- JCAP 04 (2004) 003
•
e-Print:
- hep-ph/0309328
•
DOI:
- 10.1088/1475-7516/2004/04/003

Earth-skimming UHE Tau neutrinos at the fluorescence detector of Pierre Auger observatory

C. Aramo
(
- Naples U. and
- INFN, Naples and
- Catania U. and
- INFN, Catania and
- Wuppertal U. and
- UCLA and
- Moscow, INR
)
,
A. Insolia
(
- Naples U. and
- INFN, Naples and
- Catania U. and
- INFN, Catania and
- Wuppertal U. and
- UCLA and
- Moscow, INR
)
,
A. Leonardi
(
- Naples U. and
- INFN, Naples and
- Catania U. and
- INFN, Catania and
- Wuppertal U. and
- UCLA and
- Moscow, INR
)
,
G. Miele
(
- Naples U. and
- INFN, Naples and
- Catania U. and
- INFN, Catania and
- Wuppertal U. and
- UCLA and
- Moscow, INR
)
,
L. Perrone
(
- Naples U. and
- INFN, Naples and
- Catania U. and
- INFN, Catania and
- Wuppertal U. and
- UCLA and
- Moscow, INR
)

et al.

- Astropart.Phys. 23 (2005) 65-77
•
e-Print:
- astro-ph/0407638
•
DOI:
- 10.1016/j.astropartphys.2004.11.008

Origin and propagation of extremely high-energy cosmic rays

- Phys.Rept. 327 (2000) 109-247
•
e-Print:
- astro-ph/9811011
•
DOI:
- 10.1016/S0370-1573(99)00101-5

Neutrino interactions at ultrahigh-energies

Raj Gandhi
(
- Harish-Chandra Res. Inst.
)
,
Chris Quigg
(
- Fermilab
)
,
Mary Hall Reno
(
- Iowa U.
)
,
Ina Sarcevic
(
- Arizona U.
)

- Phys.Rev.D 58 (1998) 093009
•
e-Print:
- hep-ph/9807264
•
DOI:
- 10.1103/PhysRevD.58.093009

Observability of earth skimming ultrahigh-energy neutrinos

- Phys.Rev.Lett. 88 (2002) 161102
•
e-Print:
- hep-ph/0105067
•
DOI:
- 10.1103/PhysRevLett.88.161102

Corsika+Herwig Monte Carlo Simulation of neutrino induced atmospheric air showers

M. Ambrosio
(
- INFN, Naples and
- Valencia U., IFIC
)
,
C. Aramo
(
- INFN, Naples and
- Valencia U., IFIC
)
,
A. Della Selva
(
- INFN, Naples and
- Valencia U., IFIC
)
,
G. Miele
(
- INFN, Naples and
- Valencia U., IFIC
)
,
S. Pastor
(
- INFN, Naples and
- Valencia U., IFIC
)

et al.

e-Print:
- astro-ph/0302602