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Neutrino oscillometry. / Vergados, J.D.; Giomataris, Y.; Novikov, Yu.N.

In: Nuclear Physics B - Proceedings Supplements, Vol. 229-232, 01.08.2012, p. 381-385.

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Harvard

Vergados, JD, Giomataris, Y & Novikov, YN 2012, 'Neutrino oscillometry', Nuclear Physics B - Proceedings Supplements, vol. 229-232, pp. 381-385. https://doi.org/10.1016/j.nuclphysbps.2012.09.060

APA

Vergados, J. D., Giomataris, Y., & Novikov, Y. N. (2012). Neutrino oscillometry. Nuclear Physics B - Proceedings Supplements, 229-232, 381-385. https://doi.org/10.1016/j.nuclphysbps.2012.09.060

Vancouver

Vergados JD, Giomataris Y, Novikov YN. Neutrino oscillometry. Nuclear Physics B - Proceedings Supplements. 2012 Aug 1;229-232:381-385. https://doi.org/10.1016/j.nuclphysbps.2012.09.060

Author

Vergados, J.D. ; Giomataris, Y. ; Novikov, Yu.N. / Neutrino oscillometry. In: Nuclear Physics B - Proceedings Supplements. 2012 ; Vol. 229-232. pp. 381-385.

BibTeX

@article{952aa7dc472c43e59c9b0ce7f75136b1,
title = "Neutrino oscillometry",
abstract = "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.",
keywords = "Gaseous Spherical TPC, LENA Detector, Monochromatic Neutrino Sources, Neutrino Oscillation",
author = "J.D. Vergados and Y. Giomataris and Yu.N. Novikov",
year = "2012",
month = aug,
day = "1",
doi = "10.1016/j.nuclphysbps.2012.09.060",
language = "English",
volume = "229-232",
pages = "381--385",
journal = "Nuclear and Particle Physics Proceedings",
issn = "2405-6014",
publisher = "Elsevier",

}

RIS

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