scholarly journals DEVELOPMENT OF ACOUSTIC SENSORS FOR THE ANTARES EXPERIMENT

2006 ◽  
Vol 21 (supp01) ◽  
pp. 92-96 ◽  
Author(s):  
C. NAUMANN ◽  
G. ANTON ◽  
K. GRAF ◽  
J. HÖSSL ◽  
A. KAPPES ◽  
...  

In order to study the possibility of acoustic detection of ultra-high energy neutrinos in water, our group is planning to deploy and operate an array of acoustic sensors using the ANTARES Neutrino telescope in the Mediterranean Sea. Therefore, acoustic sensor hardware has to be developed which is both capable of operation under the hostile conditions of the deep sea and at the same time provides the high sensitivity necessary to detect the weak pressure signals resulting from the neutrinos interaction in water. In this paper, two different approaches to building such sensors, as well as performance studies in the laboratory and in situ, are presented.

2019 ◽  
Vol 216 ◽  
pp. 04009
Author(s):  
Wladyslaw Henryk Trzaska ◽  
Kai Loo ◽  
Timo Enqvist ◽  
Jari Joutsenvaara ◽  
Pasi Kuusiniemi ◽  
...  

We propose to utilize bedrock as a medium for acoustic detection of particle showers following interactions of ultra-high energy neutrinos. With the density of rock three-times larger and the speed of sound four-times larger compared to water, the amplitude of the generated bipolar pressure pulse in rock should be larger by an order of magnitude. Our preliminary simulations confirm that prediction. Higher density of rock also guarantees higher interaction rate for neutrinos. A noticeably longer attenuation length in rock reduces signal dissipation. The Pyhäsalmi mine has a unique infrastructure and rock conditions to test this idea and, if successful, extend it to a full-size experiment.


2005 ◽  
Vol 20 (14) ◽  
pp. 3096-3098 ◽  
Author(s):  
◽  
ANDREA SILVESTRI

We present recent results from the Antarctic Muon And Neutrino Detector Array (AMANDA), located at the South Pole in Antarctica. AMANDA-II, commissioned in 2000, is a multipurpose high energy neutrino telescope with a broad physics and astrophysics scope. We summarize the results from searches for a variety of sources of ultra-high energy neutrinos: TeV-PeV diffuse sources by measuring either muon tracks or cascades, neutrinos in excess of PeV by searching for muons traveling in the down-going direction and point sources.


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