dc.creatorKemp, E
dc.creatorMiguez, B
dc.creatorFulgione, W
dc.date2011
dc.dateDEC
dc.date2014-07-30T17:27:42Z
dc.date2015-11-26T17:29:00Z
dc.date2014-07-30T17:27:42Z
dc.date2015-11-26T17:29:00Z
dc.date.accessioned2018-03-29T00:16:04Z
dc.date.available2018-03-29T00:16:04Z
dc.identifierInternational Journal Of Modern Physics E-nuclear Physics. World Scientific Publ Co Pte Ltd, v. 20, n. 57, n. 60, 2011.
dc.identifier0218-3013
dc.identifierWOS:000299095100010
dc.identifier10.1142/S0218301311040591
dc.identifierhttp://www.repositorio.unicamp.br/jspui/handle/REPOSIP/65662
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/65662
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1285183
dc.descriptionThe neutrino telescopes of the present generation, depending on their specific features, can reconstruct the neutrino spectra from a galactic burst. Since the optical counterpart could be not available, it is desirable to have at hand alternative methods to estimate the distance of the supernova explosion using only the neutrino data. In this work we present preliminary results on the method we are proposing to estimate the distance from a galactic supernova based only on the spectral shape of the neutrino burst and assumptions on the gravitational binding energy released an a typical supernova explosion due to stellar collapses.
dc.description20
dc.description2
dc.description57
dc.description60
dc.languageen
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.publisherSingapore
dc.publisherSingapura
dc.relationInternational Journal Of Modern Physics E-nuclear Physics
dc.relationInt. J. Mod. Phys. E-Nucl. Phys.
dc.rightsfechado
dc.sourceWeb of Science
dc.subjectNeutrino spectra
dc.subjectgalactic burst
dc.subjectstellar colapse
dc.subjectSupernovae
dc.titleESTIMATIONS OF THE DISTANCES OF STELLAR COLLAPSES IN THE GALAXY BY ANALYZING THE ENERGY SPECTRUM OF NEUTRINO BURSTS
dc.typeArtículos de revistas


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