001094076 001__ 1094076
001094076 003__ SzGeCERN
001094076 005__ 20230315201115.0
001094076 0247_ $$2DOI$$a10.1016/j.physletb.2008.07.092
001094076 0248_ $$aoai:cds.cern.ch:1094076$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
001094076 035__ $$9arXiv$$aoai:arXiv.org:0803.1790
001094076 035__ $$9SPIRES$$a7687290
001094076 035__ $$9Inspire$$a781243
001094076 037__ $$9arXiv$$aarXiv:0803.1790$$chep-ph
001094076 037__ $$aIFIC-08-17
001094076 037__ $$aVPI-IPNAS-08-06
001094076 037__ $$aCERN-PH-TH-2008-049
001094076 041__ $$aeng
001094076 084__ $$2CERN Library$$aTH-2008-049
001094076 088__ $$aCERN-PH-TH-2008-049
001094076 088__ $$aIFIC-2008-17
001094076 088__ $$aVPI-IPNAS-2008-06
001094076 100__ $$aEsteban-Pretel, Andreu$$uValencia U.
001094076 245__ $$aCan OPERA help in constraining neutrino non-standard interactions?
001094076 260__ $$c2008
001094076 269__ $$aGeneva$$bCERN$$c13 Mar 2008
001094076 300__ $$a8 p
001094076 520__ $$aWe study how much the unique ability of the OPERA experiment to directly detect \nu_\tau can help in probing new, non-standard contact interactions of the third family of neutrinos. We perform a combined analysis of future, high-statistics MINOS and OPERA data. For the case of non-standard interactions in \nu_\mu to \nu_e transitions we also include the impact of possible DoubleCHOOZ data. In all cases we find that the \nu_\tau sample of OPERA is too small to be statistically significant, even if one doubles the nominal exposure of OPERA to 4.5E20 pot. OPERA's real benefit for this measurement lies in its very high neutrino energy and hence very different L/E compared to MINOS.
001094076 520__ $$9Elsevier$$aWe study how much the unique ability of the OPERA experiment to directly detect ντ can help in probing new, non-standard contact interactions of the third family of neutrinos. We perform a combined analysis of future, high-statistics MINOS and OPERA data. For the case of non-standard interactions in νμ to νe transitions we also include the impact of possible Double Chooz data. In all cases we find that the ντ sample of OPERA is too small to be statistically significant, even if one doubles the nominal exposure of OPERA to 9×1019 pot. OPERA's real benefit for this measurement lies in its very high neutrino energy and hence very different L/E compared to MINOS.
001094076 520__ $$9arXiv$$aWe study how much the unique ability of the OPERA experiment to directly detect \nu_\tau can help in probing new, non-standard contact interactions of the third family of neutrinos. We perform a combined analysis of future, high-statistics MINOS and OPERA data. For the case of non-standard interactions in \nu_\mu to \nu_e transitions we also include the impact of possible DoubleCHOOZ data. In all cases we find that the \nu_\tau sample of OPERA is too small to be statistically significant, even if one doubles the nominal exposure of OPERA to 4.5E20 pot. OPERA's real benefit for this measurement lies in its very high neutrino energy and hence very different L/E compared to MINOS.
001094076 542__ $$fCopyright © unknown. Published by Elsevier B.V.
001094076 595__ $$aCERN-TH
001094076 595__ $$aLANL EDS
001094076 595__ $$aOA
001094076 65017 $$2SzGeCERN$$aParticle Physics - Phenomenology
001094076 690C_ $$aCERN
001094076 690C_ $$aARTICLE
001094076 693__ $$aNot applicable$$eNot applicable
001094076 695__ $$9LANL EDS$$ahep-ph
001094076 700__ $$aValle, Jose W.F.$$iINSPIRE-00133260$$uValencia U.
001094076 700__ $$aHuber, Patrick$$uCERN$$uVirginia Tech.
001094076 710__ $$5PH-TH
001094076 773__ $$c197-201$$pPhys. Lett. B$$v668$$y2008
001094076 8564_ $$uhttp://weblib.cern.ch/abstract?CERN-PH-TH-2008-049$$yPreprint
001094076 8564_ $$82439837$$s150559$$uhttp://cds.cern.ch/record/1094076/files/arXiv:0803.1790.pdf
001094076 8564_ $$82439835$$s22306$$uhttp://cds.cern.ch/record/1094076/files/M2+O_ett_c95_25e20.png$$y00000 Shown is the allowed region in the $\sin^22\theta_{23}$-$\Delta m^2_{31}$-plane at 95\% CL (2 dof). In this fit $\theta_{13}$, $\varepsilon_{e\tau}$ and $\varepsilon_{\tau\tau}$ are left free. The different lines correspond to different valuesfor $\varepsilon_{\tau\tau}$ as explained in the legend.
001094076 8564_ $$82439836$$s25966$$uhttp://cds.cern.ch/record/1094076/files/M2+DC_M2+O+DC_t13_0-0.01-0.05-0.1_c95_25e20.png$$y00001 Shown are the allowed regions in the $\sin2\theta_{23}$-$\varepsilon_{e\tau}$-plane at 95\% CL (2 dof). $\Delta m^2_{31}$, $\theta_{23}$ and $\varepsilon_{\tau\tau}$ are left free in this fit. The solid lines correspond to the combination of MINOS$_2$ and DoubleCHOOZ while the dashed lines also include OPERA in the analysis. Each set of lines correspond to different true values for $\sin^22\theta_{13}$, from left to right: 0, 0.01, 0.05and 0.1.
001094076 916__ $$sn$$w200810$$ya2008
001094076 960__ $$a13
001094076 961__ $$c20100409$$h2244$$lCER01$$x20080313
001094076 963__ $$aPUBLIC
001094076 970__ $$a002748362CER
001094076 980__ $$aARTICLE