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Ultra-high energy neutrinos at the Pierre Auger Observatory
(Sociedade Brasileira de Fisica, 2016)
Neutrinos in the sub-EeV energy range and above can be detected with the Surface Detector (SD) of the Pierre Auger Observatory. They can be identified through the broad time structure of the signals induced in the SD ...
Through the looking-glass with ALICE into the quark-gluon plasma: A new test for hadronic interaction models used in air shower simulations
(Elsevier Science, 2020-11)
Recently, the ALICE Collaboration reported an enhancement of the yield ratio of strange and multi-strange hadrons to charged pions as a function of multiplicity at mid-rapidity in proton-proton, proton-lead, lead-lead, and ...
ATMOSPHERIC HADRONIC SHOWERS INDUCED BY ONE SINGLE NUCLEUS
(Editrice Compositori BolognaBolognaItália, 1992)
Detecção de neutrinos no observatório Pierre Auger
(Universidade Estadual Paulista (Unesp), 2003-03)
Faz-se aqui o estudo da detecção de neutrinos (v) de altas energias ('E IND.v' > '10 POT.9' GeV) no Observatório Pierre Auger usando os detectores de fluorescência. Introduzimos todo o conhecimento experimental dos raios ...
Detecção de neutrinos no observatório Pierre Auger
(Universidade Estadual Paulista (Unesp), 2003-03)
Faz-se aqui o estudo da detecção de neutrinos (v) de altas energias ('E IND.v' > '10 POT.9' GeV) no Observatório Pierre Auger usando os detectores de fluorescência. Introduzimos todo o conhecimento experimental dos raios ...
Possible Association of Two Stellar Bowshocks with Unidentified Fermi Sources
(IOP Publishing, 2018-07)
The bowshocks of runaway stars had been theoretically proposed as gamma-ray sources. However, this hypothesis has not been confirmed by observations to date. In this paper, we present two runaway stars (λ Cep and LS 2355) ...
Detecção de neutrinos no observatório Pierre Auger
(Universidade Estadual Paulista (UNESP), 2014)
Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications
(American Physical Society - APSCollege Park, 2014)
Using the data taken at the Pierre Auger Observatory between December 2004 and December 2012, we have examined the implications of the distributions of depths of atmospheric shower maximum (Xmax), using a hybrid technique, ...
Galactic Supernova Remnants: From radio frequencies to TeV
(Asociacion Argentina de Astronomia, 2007-09)
Supernova remnants are among the most valuable astrophysical laboratory to study numerous physical processes involved in their evolution and interaction with the surrounding interstellar medium. These objects are one of ...
On the energy of the protons producing the very high-energy astrophysical neutrinos
(IOP Publishing, 2021-03)
We study the distribution of the energy of the protons that can produce an astrophysical neutrino with a given observed energy, in the TeV-PeV range, both through pp or pγ interactions. Due to the increasing multiplicity ...