Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Neutrino oscillometry. / Vergados, J.D.; Giomataris, Y.; Novikov, Yu.N.
в: Nuclear Physics B - Proceedings Supplements, Том 229-232, 01.08.2012, стр. 381-385.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Neutrino oscillometry
AU - Vergados, J.D.
AU - Giomataris, Y.
AU - Novikov, Yu.N.
PY - 2012/8/1
Y1 - 2012/8/1
N2 - Neutrino oscillations are studied employing sources of low energy monoenergetic neutrinos following electron capture by the nucleus and measuring electron recoils. Since the neutrino energy is very low the oscillation length L 23 appearing in this electronic neutrino disappearance experiment can be so small that the full oscillation can take place inside the detector so that one may determine very accurately the neutrino oscillation parameters. In particular, since the oscillation probability is proportional to sin 22θ 13, one can measure or set a better limit on the unknown parameter θ 13. One, however, has to pay the price that the expected counting rates are very small. Thus one needs a very intensive neutrino source and a large detector with as low as possible energy threshold and high energy and position resolution. Both spherical gaseous and cylindrical liquid detectors are studied. Different source candidates are considered.
AB - Neutrino oscillations are studied employing sources of low energy monoenergetic neutrinos following electron capture by the nucleus and measuring electron recoils. Since the neutrino energy is very low the oscillation length L 23 appearing in this electronic neutrino disappearance experiment can be so small that the full oscillation can take place inside the detector so that one may determine very accurately the neutrino oscillation parameters. In particular, since the oscillation probability is proportional to sin 22θ 13, one can measure or set a better limit on the unknown parameter θ 13. One, however, has to pay the price that the expected counting rates are very small. Thus one needs a very intensive neutrino source and a large detector with as low as possible energy threshold and high energy and position resolution. Both spherical gaseous and cylindrical liquid detectors are studied. Different source candidates are considered.
KW - Gaseous Spherical TPC
KW - LENA Detector
KW - Monochromatic Neutrino Sources
KW - Neutrino Oscillation
UR - http://www.scopus.com/inward/record.url?scp=84870190699&partnerID=8YFLogxK
U2 - 10.1016/j.nuclphysbps.2012.09.060
DO - 10.1016/j.nuclphysbps.2012.09.060
M3 - Article
AN - SCOPUS:84870190699
VL - 229-232
SP - 381
EP - 385
JO - Nuclear and Particle Physics Proceedings
JF - Nuclear and Particle Physics Proceedings
SN - 2405-6014
ER -
ID: 46101181