O. G. Miranda
University of Valencia
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Publication
Featured researches published by O. G. Miranda.
Journal of High Energy Physics | 2005
Juan Barranco; O. G. Miranda; Timur I. Rashba
The possibility off measuring for the first time neutrino-nuclei coherent scattering has been recently discussed by several experimental collaborations. It is shown that such a measurement may be very sensitive to non-standard interactions of neutrinos with quarks and might set better constraints than those coming from future neutrino factory experiments. We also comment on other types of new physics tests, such as extra heavy neutral gauge bosons, where the sensitivity to some models is slightly better than the Tevatron constraint and, therefore, could give complementary bounds.
Physical Review D | 2009
Azucena Bolaños; O. G. Miranda; A. Palazzo; M. Tórtola; J.W.F. Valle
18 pages, 3 figures.-- ISI article identifier:000267701300027 .-- ArXiv pre-print avaible at:http://arxiv.org/abs/0812.4417
Physical Review D | 2007
Juan Barranco; O. G. Miranda; Timur Rashba
We study the sensitivity of future low energy neutrino experiments to extra neutral gauge bosons, leptoquarks, and R-parity breaking interactions. We focus on future proposals to measure coherent neutrino-nuclei scattering and neutrino-electron elastic scattering. We introduce a new comparative analysis between these experiments and show that in different types of new physics it is possible to obtain competitive bounds to those of present and future collider experiments. For the cases of leptoquarks and R-parity breaking interactions we found that the expected sensitivity for most of the future low energy experimental setups is better than the current constraints.
Physical Review D | 2002
Juan Barranco; O. G. Miranda; Timur I. Rashba; Victor B. Semikoz; J.W.F. Valle
A global analysis of spin flavor precession (SFP) solutions to the solar neutrino problem is given, taking into account the impact of the full set of latest solar neutrino data, including the recent SNO data and the 1496-day Super-Kamiokande data. These are characterized by three effective parameters:
Physical Review D | 2015
F. J. Escrihuela; D.V. Forero; O. G. Miranda; Mariam Tórtola; J.W.F. Valle
\ensuremath{\Delta}{m}_{\mathrm{SOL}}^{2}\ensuremath{\equiv}\ensuremath{\Delta}{m}^{2},
Physical Review D | 2011
F. J. Escrihuela; Mariam Tórtola; J.W.F. Valle; O. G. Miranda
the neutrino mixing angle
Physical Review D | 2009
F. J. Escrihuela; O. G. Miranda; Mariam Tórtola; J.W.F. Valle
{\ensuremath{\theta}}_{\mathrm{SOL}}\ensuremath{\equiv}\ensuremath{\theta},
Physical Review Letters | 2004
O. G. Miranda; Timur Rashba; A. I. Rez; J.W.F. Valle
and the magnetic field parameter
Physics Letters B | 2001
O. G. Miranda; Carlos Pena-Garay; T.I Rashba; V.B Semikoz; J.W.F. Valle
\ensuremath{\mu}{B}_{\ensuremath{\perp}}.
New Journal of Physics | 2017
F. J. Escrihuela; D. V. Forero; O. G. Miranda; M. Tórtola; J.W.F. Valle
For the last we adopt a self-consistent magnetohydrodynamics field profile in the convective zone and identify an optimum