2005
DOI: 10.1143/jjap.44.3341
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Abstract: We estimate how well we will know the parameters of solar neutrino oscillations after KamLAND and Borexino. The expected error on ∆m 2 is few per-mille in the VO and QVO regions, few per-cent in the LMA region, and around 10% in the LOW region. The expected error on sin 2 2θ is around 5%. KamLAND and Borexino will tell unambiguously which specific new measurement, dedicated to pp solar neutrinos, is able to contribute to the determination of θ and perhaps of ∆m 2 . The present data suggest as more likely outco… Show more

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Cited by 5 publications
(1 citation statement)
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References 31 publications
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“…1,2 Especially, various innovative 3D nano-and microdevices with overhanging structures have been fabricated by free-space-nanowiring using FIB-CVD. 3,4 However, it is difficult to fabricate overhanging structures larger than several micrometers because the growth characteristics start to change. In the case of fabricating a horizontal free-space-nanowire by scanning the FIB laterally, the nanowire deviates from the initial growth angle and turns downward.…”
Section: Introductionmentioning
confidence: 99%