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Geotomography with solar and supernova neutrinos

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Geotomography with solar and supernova neutrinos

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dc.contributor.author Akhmedov, Evgeny Kh.
dc.contributor.author Tórtola Baixauli, María Amparo
dc.contributor.author Furtado Valle, José Wagner
dc.date.accessioned 2015-09-30T11:44:08Z
dc.date.available 2015-09-30T11:44:08Z
dc.date.issued 2005
dc.identifier.citation Akhmedov, Evgeny Kh. Tórtola Baixauli, María Amparo Furtado Valle, José Wagner 2005 Geotomography with solar and supernova neutrinos Journal of High Energy Physics 2005 06 053
dc.identifier.uri http://hdl.handle.net/10550/47494
dc.description.abstract We show how by studying the Earth matter effect on oscillations of solar and supernova neutrinos inside the Earth one can in principle reconstruct the electron number density profile of the Earth. A direct inversion of the oscillation problem is possible due to the existence of a very simple analytic formula for the Earth matter effect on oscillations of solar and supernova neutrinos. From the point of view of the Earth tomography, these oscillations have a number of advantages over the oscillations of the accelerator or atmospheric neutrinos, which stem from the fact that solar and supernova neutrinos are coming to the Earth as mass eigenstates rather than flavour eigenstates. In particular, this allows reconstruction of density profiles even over relatively short neutrino path lengths in the Earth, and also of asymmetric profiles. We study the requirements that future experiments must meet to achieve a given accuracy of the tomography of the Earth.
dc.language.iso eng
dc.relation.ispartof Journal of High Energy Physics, 2005, vol. 2005, num. 06, p. 053
dc.subject Física
dc.title Geotomography with solar and supernova neutrinos
dc.type journal article es_ES
dc.date.updated 2015-09-30T11:44:08Z
dc.identifier.doi 10.1088/1126-6708/2005/06/053
dc.identifier.idgrec 026114
dc.rights.accessRights open access es_ES

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