Standard

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

в: Journal of Physics: Conference Series, Том 259, № 1, 012100, 01.01.2010.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Vergados, JD, Giomataris, Y & Novikov, YN 2010, 'Neutrino oscillometry', Journal of Physics: Conference Series, Том. 259, № 1, 012100. https://doi.org/10.1088/1742-6596/259/1/012100

APA

Vergados, J. D., Giomataris, Y., & Novikov, Y. N. (2010). Neutrino oscillometry. Journal of Physics: Conference Series, 259(1), [012100]. https://doi.org/10.1088/1742-6596/259/1/012100

Vancouver

Vergados JD, Giomataris Y, Novikov YN. Neutrino oscillometry. Journal of Physics: Conference Series. 2010 Янв. 1;259(1). 012100. https://doi.org/10.1088/1742-6596/259/1/012100

Author

Vergados, J. D. ; Giomataris, Y. ; Novikov, Yu.N. / Neutrino oscillometry. в: Journal of Physics: Conference Series. 2010 ; Том 259, № 1.

BibTeX

@article{22c56445b4974d929da91c9cc45dbe68,
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 L23 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 sin2 2θ13, one can measure or set a better limit on the unknown parameter θ13. 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",
author = "Vergados, {J. D.} and Y. Giomataris and Yu.N. Novikov",
year = "2010",
month = jan,
day = "1",
doi = "10.1088/1742-6596/259/1/012100",
language = "English",
volume = "259",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",

}

RIS

TY - JOUR

T1 - Neutrino oscillometry

AU - Vergados, J. D.

AU - Giomataris, Y.

AU - Novikov, Yu.N.

PY - 2010/1/1

Y1 - 2010/1/1

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 L23 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 sin2 2θ13, one can measure or set a better limit on the unknown parameter θ13. 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 L23 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 sin2 2θ13, one can measure or set a better limit on the unknown parameter θ13. 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

UR - http://www.scopus.com/inward/record.url?scp=79952366639&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/259/1/012100

DO - 10.1088/1742-6596/259/1/012100

M3 - Article

AN - SCOPUS:79952366639

VL - 259

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012100

ER -

ID: 46152320