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Detailed timetable
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3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
Support
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HE 2.3
Place
Location: Merida, Mexico
Room: Yucatan II+III+IV (Fiesta Americana)
Date:
from 5 Jul 08:29 to 7 Jul 11:57
Timetable | Contribution List
Current status and results of the experiment on recording
neutrino bursts are presented.
The observation livetime (since 1980) is 22.6 years.
The upper bound of collapse frequency in our Galaxy
is 0.10 $y^{-1}$ (90% CL).
Presented by Dr. Yuriy NOVOSELTSEV
on
5/7/2007
at
17:46
The ANtarctic Impulsive Transient Antenna (ANITA) searches for
ultra high energy neutrinos interacting in the antarctic ice cap.
It is a long duration balloon experiment composed of an array of
broadband dual-polarized horn antennas that had its first science
flight over Antarctica in December 2006 through January 2007. ANITA
relies upon the Askaryan effect, in which a particle shower
in a d
... More
Presented by Kimberly J. PALLADINO
on
7/7/2007
at
16:45
Air-fluorescence detectors such as the High Resolution Fly's Eye (HiRes) instrument
are very sensitive to upward-going, Earth-skimming ultrahigh energy
electron-neutrino-induced showers.
This is due to the relatively large interaction cross sections of these high-energy
neutrinos and the Landau-Pomeranchuk-Migdal (LPM) effect, which is responsible for a
significant decrease in the cross secti
... More
Presented by Dr. Lauren SCOTT
on
5/7/2007
at
17:24
Many astrophysical models predict a diffuse flux of high-energy neutrinos from active
galactic nuclei and other extra-galactic sources. At muon energies above 1 TeV, the
upward-going muon flux induced by neutrinos from active galactic nuclei is expected
to exceed the flux due to atmospheric neutrinos. We have performed a search for this
astrophysical neutrino flux by looking for upward-going m
... More
Presented by Molly SWANSON
on
5/7/2007
at
17:35
The AMANDA-II data collected during the period 2000-03 have been analysed in a search
for a diffuse flux of high-energy extra-terrestrial neutrinos from the sum of all sources in
the universe. With no excess of events seen, an upper limit on an E-2 flux of E2 Phi < 8.8
x 10-8 GeV cm-2 s-1 sr-1 was obtained. The astrophysical implications of this bound and
of others obtained for specific mo
... More
Presented by Gary HILL, Jessica HODGES, Kotoyo HOSHINA
on
5/7/2007
at
14:35
The ANTARES telescope is being built in the Mediterranean Sea. The detector
consists of a 3D array of photomultipliers (PMTs) that detects the Cherenkov
light induced by the muons produced in neutrino interactions. Since the
neutrino fluxes from point-like sources are expected to be small, it is of
the utmost importance to take advantage of the ANTARES accurate pointing
power (angular resolut
... More
Presented by Mr. Juan Antonio AGUILAR SÁNCHEZ
on
5/7/2007
at
13:53
A method is presented for the identification of high-energy neutrinos from
gamma ray bursts by means of a large-scale neutrino telescope.
The procedure makes use of a time profile stacking technique of observed
neutrino induced signals in correlation with satellite observations.
By selecting a rather wide time window, a possible difference between the
arrival times of the gamma and neutrino
... More
Presented by Dr. Nick VAN EIJNDHOVEN
on
5/7/2007
at
18:08
The Pierre Auger Observatory has the capability of detecting
ultra-high energy neutrinos by searching for very inclined showers
with a significant electromagnetic component. In this work we discuss
the discrimination power of the instrument for ultra-high energy
neutrinos. Based on the data collected since January 2004 an upper
limit to the diffuse flux of neutrinos at EeV energies is presen
... More
Presented by Dr. Oscar BLANCH-BIGAS
on
5/7/2007
at
17:13
We perform a study of the ultra high energy neutrino detection performances of
a km^3 Neutrino Telescope sitting at the three proposed sites for ANTARES,
NEMO and NESTOR in the Mediterranean sea. We focus on the effect of the
underwater surface profile on the total amount of yearly expected tau and mu
crossing the fiducial volume in the limit of full detection efficiency and energy
resol
... More
Presented by Dr. Ofelia PISANTI
on
5/7/2007
at
15:30
AMANDA is a high volume neutrino telescope designed to search in the down-going direction for muons from
astrophysical muon-neutrinos. It is possible to extend the range of AMANDA to search for neutrinos with
extremely high energies. The atmospheric neutrino flux becomes negligible above 10^15 eV, so this value serves
as rough energy threshold for this search. Above 10^16 eV the Earth is ess
... More
Presented by Lisa GERHARDT
on
5/7/2007
at
16:30
The construction of the IceCube Neutrino Observatory began during the austral summer
of 2004-05, and is expected to continue through 2011. During 2006, nine of the
projected 80 strings were already deployed and taking data, making IceCube an
operational neutrino observatory while still at about 10% of its final size. We
present the first results of a point-source search based on the analysis o
... More
Presented by Dr. Chad FINLEY
on
5/7/2007
at
14:47
Current point source searches mostly apply only the direction of the reconstructed
event; furthermore, they reduce available information by grouping events into sky
bins. In this analysis we use a search based on maximum likelihood techniques,
utilizing both event direction and energy, to enhance our ability to detect point
sources. Especially, use of energy information allows us to fit the sp
... More
Presented by Mr. James BRAUN
on
5/7/2007
at
16:42
The Antarctic Muon And Neutrino Detector Array (AMANDA) is a Cherenkov
detector deployed in the Antarctic ice cap at the South Pole.
The charged-current interaction of high-energy electron or tau neutrinos,
as well as neutral-current interactions of neutrinos of any flavor, can
produce isolated electromagnetic or hadronic cascades.
There are several advantages associated with the cascade chan
... More
Presented by Oxana TARASOVA
on
5/7/2007
at
16:18
A search for supernova neutrino bursts was conducted using data from the
Super-Kamiokande (SK) detector. SK detector is an imaging water Cherenkov
detector containing 50,000 tons of pure water with 22,500 tons of fiducial
volume, and it is sensitive to core-collapse supernova explosions
via observation of their neutrino emissions. The expected number of events
comprising such a burst is
... More
Presented by Mr. Motoyasu IKEDA
on
5/7/2007
at
15:54
Supernova relic neutrinos (SRN) is diffuse supernova neutrino background from
all past supernova. No experiments have succeeded in detecting SRN yet.
Measurement of SRN enable us investigate history of past supernova. For
example, the flux of SRN shows star formation rate and supernova rate in
galaxies.
A search for SRN was conducted using Super-Kamiokande (SK) data. SK is a
large water
... More
Presented by Takashi IIDA
on
5/7/2007
at
16:06
The Large Volume Detector LVD (Gran Sasso National Laboratory, Italy) is a neutrino scintillator observatory
monitoring the Galaxy since 1992, searching for low energy neutrino bursts from gravitational stellar
collapses. We present the status of the detector that reached its final active mass of 1000 t in 2001. No
candidates have been detected over all the fifteen years of observation: the
... More
Presented by - THE LVD COLLABORATION
on
5/7/2007
at
18:19
We use CORSIKA+Herwig simulation code to produce ultra-high energy neutrino
interactions in the atmosphere. Our aim is to reproduce extensive air showers
originated by extragalactic tau-neutrinos. As we have no code available which can
simulate the tau-neutrino as primary particle in the atmosphere, we use muon-neutrino
as primaries. For charged current tau-neutrino interactions in the atmosph
... More
Presented by Dr. Celio ADREGA DE MOURA
on
5/7/2007
at
17:57
ANTARES is a large volume, deep-sea, neutrino telescope currently under construction off La Seyne-sur-mer,
France.
Neutrino telescopes aims at detecting neutrinos as a new probe for a sky study at energies greater than 1 TeV.
The detection principle relies on the observation, using photomultipliers, of the Cherenkov light emitted by
charged leptons induced by neutrino interactions in the s
... More
Presented by Dr. Antoine KOUCHNER
on
5/7/2007
at
13:29
The ANTARES Collaboration is deploying a large neutrino detector at a depth of 2500 m
in the Mediterranean Sea, 40 km off shore from La Seyne-sur-Mer in South France. The
construction of this 12-line detector with 75 phototubes per line will be completed
by the end of 2007. Data taking has begun since April 2005 with an instrumentation
line also equipped with optical modules. The first 5 detec
... More
Presented by Dr. Stephanie ESCOFFIER
on
5/7/2007
at
13:41
The NEMO (NEutrino Mediterranean Observatory) Project aims at the construction of a
km3-scale neutrino telescope in the Mediterranean Sea.
After extensive deep-sea surveys performed in several sites in the Mediterranean, an
optimal installation site for the apparatus has been identified at a depth of 3500 m,
about 80 km off Capo Passero, at the SE corner of Sicily, Italy.
In this talk, we wil
... More
Presented by Prof. MAURO TAIUTI
on
5/7/2007
at
15:42
Extremely high energy (EHE) cosmic neutrinos (E>10^8GeV) are considered to carry
important information about particle acceleration mechanisms in the universe and the
origin of EHE cosmic-ray. The IceCube experiment is uniquely designed to detect
highly energetic astrophysical neutrino events using Antarctic ice as a natural
Cherenkov radiator to overcome difficulties associated in the search
... More
Presented by Dr. Aya ISHIHARA
on
5/7/2007
at
17:02
