A search for nearly vertical up-going muon-neutrinos from neutralino annihilations in the center of the Earth has been performed with the AMANDA-B10 neutrino detector. The data sample collected in 130.1 days of live-time in 1997, ~10^9 events, has been analyzed for this search. No excess over the expected atmospheric neutrino background is oberved. An upper limit at 90% confidence level on the annihilation rate of neutralinos in the center of the Earth is obtained as a function of the neutralino mass in the range 100 GeV-5000 GeV, as well as the corresponding muon flux limit
The Antarctic Muon And Neutrino Detector Array, AMANDA, is a Cherenkov detector deployed deep in the...
The design and operation of the MACRO (Monopole, Astrophysics, and Cosmic Ray Observatory) detector ...
A relic density of Weakly Interacting Massive Particles (WIMPs) remaining from the Big Bang constitu...
A search for nearly vertical up-going muon-neutrinos from neutralino annihilations in the center of ...
A search has been performed for nearly vertically upgoing neutrino-induced muons with the Antarctic ...
We report on the search for nearly vertical up-going muon neutrinos from WIMP annihilations in the c...
If dark matter in the Universe is constituted by super-symmetric particles in the form of neutralino...
The nature of the dark matter in the Universe is one of the greatest mysteries in modern astronomy. ...
The young field of high energy neutrino astronomy can be motivated by the search for the origin of t...
A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the Ice...
High-energy neutrinos are capable of carrying information over vast distances, and neutrino telescop...
A search for an excess of muon neutrinos from dark matter annihilations in the Sun has been performe...
A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the Ice...
Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of ...
Interactions of cosmic rays with the galactic interstellar medium produce high-energy neutrinos thro...
The Antarctic Muon And Neutrino Detector Array, AMANDA, is a Cherenkov detector deployed deep in the...
The design and operation of the MACRO (Monopole, Astrophysics, and Cosmic Ray Observatory) detector ...
A relic density of Weakly Interacting Massive Particles (WIMPs) remaining from the Big Bang constitu...
A search for nearly vertical up-going muon-neutrinos from neutralino annihilations in the center of ...
A search has been performed for nearly vertically upgoing neutrino-induced muons with the Antarctic ...
We report on the search for nearly vertical up-going muon neutrinos from WIMP annihilations in the c...
If dark matter in the Universe is constituted by super-symmetric particles in the form of neutralino...
The nature of the dark matter in the Universe is one of the greatest mysteries in modern astronomy. ...
The young field of high energy neutrino astronomy can be motivated by the search for the origin of t...
A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the Ice...
High-energy neutrinos are capable of carrying information over vast distances, and neutrino telescop...
A search for an excess of muon neutrinos from dark matter annihilations in the Sun has been performe...
A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the Ice...
Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of ...
Interactions of cosmic rays with the galactic interstellar medium produce high-energy neutrinos thro...
The Antarctic Muon And Neutrino Detector Array, AMANDA, is a Cherenkov detector deployed deep in the...
The design and operation of the MACRO (Monopole, Astrophysics, and Cosmic Ray Observatory) detector ...
A relic density of Weakly Interacting Massive Particles (WIMPs) remaining from the Big Bang constitu...