Reactor Neutrinos

Useful Links

References

Useful Links

The Reactor Antineutrino Anomaly

Reactor Neutrino Experiments @ The Neutrino Oscillation Industry

APS Neutrino Study: Reactor Working Group

Exploratory Information for Reactor Experiments

Towards a Future Reactor Neutrino Experiment to Measure

The Argonne Study on measuring with a reactor experiment

White Paper on Measuring with a reactor experiment

GLoBES: General Long Baseline Experiment Simulator

References

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Reactor Neutrino Experiments, Jun Cao, arXiv:0712.0897, 2007. XXIII International Symposium on Lepton and Photon Interactions at High Energy (LP07), 13-18 Aug 2007, Daegu, Korea.

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[5-1]

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Solar Neutrino Oscillation Parameters in Experiments with Reactor Anti-Neutrinos, Sandhya Choubey, arXiv:hep-ph/0402288, 2004. 2nd International Workshop on Neutrino oscillations in Venice (NOVE), December 3-5, 2003, Venice, Italy.

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[8-1]

Indication for the disappearance of reactor electron antineutrinos in the Double Chooz experiment, Y. Abe et al. (DOUBLE-CHOOZ), arXiv:1112.6353, 2011.

[8-2]

Enhanced Constraints on from A Three-Flavor Oscillation Analysis of Reactor Antineutrinos at KamLAND, A. Gando et al. (The KamLAND), Phys. Rev. D83 (2011) 052002, arXiv:1009.4771.

[8-3]

Measurement of Neutrino-Electron Scattering Cross-Section with a CsI(Tl) Scintillating Crystal Array at the Kuo-Sheng Nuclear Power Reactor, M. Deniz et al. (TEXONO), Phys. Rev. D81 (2010) 072001, arXiv:0911.1597.

[8-4]

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[8-5]

Precision Measurement of Neutrino Oscillation Parameters with KamLAND, Abe, S. et al. (KamLAND), Phys. Rev. Lett. 100 (2008) 221803, arXiv:0801.4589.
From the abstract: Combining with solar neutrino data, we obtain and .
From the article: The spectrum indicates almost two cycles of the periodic feature expected from neutrino oscillation.

[8-6]

Experimental Results from an Antineutrino Detector for Cooperative Monitoring of Nuclear Reactors, N. S. Bowden et al., arXiv:physics/0612152, 2006.

[8-7]

Production of Electron Neutrinos at Nuclear Power Reactors and the Prospects for Neutrino Physics, Xin, B. et al. (TEXONO), Phys. Rev. D72 (2005) 012006, arXiv:hep-ex/0502001.

[8-8]

Measurement of Neutrino Oscillation with KamLAND: Evidence of Spectral Distortion, T. Araki et al. (KamLAND), Phys. Rev. Lett. 94 (2005) 081801, arXiv:hep-ex/0406035.
From the article: See this summary.

[8-9]

Search for neutrino oscillations on a long base-line at the CHOOZ nuclear power station, Apollonio, M. et al. (CHOOZ), Eur. Phys. J. C27 (2003) 331, arXiv:hep-ex/0301017.
Comment: The (new) results obtained by using the prescription of Feldman and Cousins with the correct inclusion of systematics indicate that oscillations are excluded for mixing angles at high values. The limit obtained here is significantly higher than the one quoted in previous publication : ( at high values). (M.L.).

[8-10]

First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance, K. Eguchi et al. (KamLAND), Phys. Rev. Lett. 90 (2003) 021802, arXiv:hep-ex/0212021.
From the abstract: In an exposure of 162 tonyr (145.1 days) the ratio of the number of observed inverse -decay events to the expected number of events without disappearance is for energies 3.4 MeV. The deficit of events is inconsistent with the expected rate for standard propagation at the 99.95% confidence level. In the context of two-flavor neutrino oscillations with CPT invariance, these results exclude all oscillation solutions but the "Large Mixing Angle" solution to the solar neutrino problem using reactor sources.

[8-11]

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[9-1]

Latest News from Double Chooz Reactor Neutrino Experiment, Masahiro Kuze (Double Chooz), arXiv:1109.0074, 2011. 19th Particles and Nuclei International Conference, PANIC 2011, MIT, Cambridge, MA July 2011.

[9-2]

Status of the Daya Bay Reactor Neutrino Oscillation Experiment, Cheng-Ju Lin (Daya Bay), PoS ICHEP2010 (2010) 305, arXiv:1101.0261. 35th International Conference of High Energy Physics, July 22-28, 2010, Paris, France.

[9-3]

A High Precision Reactor Neutrino Detector for the Double Chooz Experiment, Fumihiko Suekane (Double Chooz), Nucl. Instrum. Meth. A623 (2010) 440-441, arXiv:0906.1639. TIPP09.

[9-4]

Status of the Double Chooz Experiment, Dawson, J. V. (Double Chooz), arXiv:0905.4843, 2009. XIII International Workshop on Neutrino Telescopes (NEUTEL09), Venice, March 10-13, 2009.

[9-5]

Status Report on Double Chooz, A. Porta et al. (Double Chooz), arXiv:0905.2560, 2009. 44th Rencontres de Moriond, Electroweak interactions and unified theories, 7-14 March 2009, La Thuile.

[9-6]

Recent Results from KamLAND, Ichimura, Koichi, Collaboration, for the KamLAND (KamLAND), arXiv:0810.3448, 2008. ICHEP08.

[9-7]

Studies of Neutrino-Electron Scattering at the Kuo-Sheng Reactor Neutrino Laboratory, M. Deniz, H.T. Wong (TEXONO), arXiv:0810.0809, 2008. ICHEP08, Philadelphia, USA, July 2008.

[9-8]

High Sensitivity Anti-Neutrino Detection by KamLAND, S. Hatakeyama et al. (KamLAND), arXiv:hep-ex/0405001, 2004. Moriond EW04.

[9-9]

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[9-10]

KamLAND results, Inoue, K., arXiv:hep-ex/0307030, 2003. XXXVIII Rencontres de Moriond on Electroweak Interactions and Unified Theories Les Arcs, France, 15-22 March 2003.

[9-11]

Highlights of the TEXONO Research Program on Neutrino and Astroparticle Physics, H.T. Wong, J. Li, Z.Y. Zhou (TEXONO), arXiv:hep-ex/0307001, 2003. International Symposium on Neutrino and Dark Matter in Nuclear Physics (NDM03), Nara, Japan, June 9-14, 2003.

[9-12]

Status on the searches of neutrino magnetic moment at the Kuo-Sheng power reactor, Wong, H. T. (TEXONO), arXiv:hep-ex/0209003, 2002. International Conference on High Energy Physics, 2002.

[9-13]

An update on progress at KamLAND, Dazeley, S. A. (KamLAND), arXiv:hep-ex/0205041, 2002.

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KamLAND (Anti-Neutrino Status), I. Shimizu (KamLAND), 2007. TAUP 2007, 11-15 September 2007, Sendai, Japan. http://www.awa.tohoku.ac.jp/taup2007/slides/workshop14/roomA/02-KamLAND-AntiNeutrino-Status-Shimizu.pdf.

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[10-3]

Results from the KamLAND experiment, G. Gratta (KamLAND), 2004. Neutrino 2004, 13-19 June 2004, Paris, France. http://neutrino2004.in2p3.fr/slides/monday/gratta.pdf.
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[10-4]

KamLAND Results, Inoue, K. (KamLAND), 2003. The 4th Workshop on Neutrino Oscillations and their Origin (NOON2003), February 10-14, 2003, Ishikawa Kousei Nenkin Kaikan, Kanazawa, Japan. http://www-sk.icrr.u-tokyo.ac.jp/noon2003/transparencies/10/Inoue-KamLAND.pdf.

[10-5]

First Results from KamLAND: Evidence for disappearance, Gratta, G. (Kamland), 2002. SLAC Colloquium, December 2002. http://hep.stanford.edu/neutrino/KamLAND/TalksAndPublications/KamLAND_FirstResults_SLAC_Colloq.pdf.

[10-6]

KamLAND: Examination of the LMA solution with reactor neutrinos, Suzuki, A. (Kamland), 2002. XVI International Conference on Particles and Nuclei, Osaka, Japan, September 30 - October 4, 2002. http://www.rcnp.osaka-u.ac.jp/Divisions/np2/PaNic02/Suzuki.pdf.

[11-1]

On-site underground background measurements for the KASKA reactor-neutrino experiment, H. Furuta et al., Nucl. Instrum. Meth. A568 (2006) 710-715, arXiv:hep-ex/0607015.

[12-1]

Simulation of Reactors for Antineutrino Experiments Using DRAGON, L. Winslow, arXiv:1109.6632, 2011.

[12-2]

Reactor Simulation for Antineutrino Experiments using DRAGON and MURE, C.L. Jones et al., arXiv:1109.5379, 2011.

[12-3]

On the determination of anti-neutrino spectra from nuclear reactors, Patrick Huber, Phys. Rev. C84 (2011) 024617, arXiv:1106.0687.

[12-4]

Radiative Correction to the anti-nu_e (nu_e) Spectrum in beta-Decay, A. Sirlin, Phys. Rev. D84 (2011) 014021, arXiv:1105.2842.

[12-5]

Simulation of the SONGS Reactor Antineutrino Flux Using DRAGON, C. L. Jones, arXiv:1103.3307, 2011.

[12-6]

Improved Predictions of Reactor Antineutrino Spectra, Th. A. Mueller et al., Phys. Rev. C83 (2011) 054615, arXiv:1101.2663.

[12-7]

Measuring of fissile isotopes partial antineutrino spectra in direct experiment at nuclear reactor, Sinev, V. V., arXiv:0902.3781, 2009.

[12-8]

Uncertainties in the Anti-neutrino Production at Nuclear Reactors, Z. Djurcic et al., J. Phys. G36 (2009) 045002, arXiv:0808.0747.

[12-9]

Conversion of electron spectrum associated with fission into the antineutrino spectrum, Petr Vogel, Phys. Rev. C76 (2007) 025504, arXiv:0708.0556.

[12-10]

A simple model of reactor cores for reactor neutrino flux calculations for the KamLAND experiment, K. Nakajima et al., arXiv:physics/0607126, 2006.

[12-11]

Reactor as a Source of Antineutrinos: Thermal Fission Energy, V. Kopeikin, L. Mikaelyan, V. Sinev, Phys. Atom. Nucl. 67 (2004) 1892, arXiv:hep-ph/0410100.

[12-12]

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Components of Antineutrino Emission in Nuclear Reactor, V. Kopeikin, L. Mikaelyan, V. Sinev, Phys. Atom. Nucl. 67 (2004) 1963, arXiv:hep-ph/0308186. 4th International Conference on Nonaccelerator New Physics (NANP 03), Dubna, Russia, 23-28 June 2003.

[14-1]

New Reactor Antineutrino Spectra, Lhuillier, M., 2011. Workshop on Sterile Neutrinos and on the Reactor (anti)-Neutrino Anomaly, TUM, Garching, February 8th 2011. http://www.e15.physik.tu-muenchen.de/fileadmin/downloads/seminars/1011/SterileNeutrinosWorkshop/lhuillier_Munich08Feb2011.pdf.

[15-1]

Large scale Gd-beta-diketonate based organic liquid scintillator production for antineutrino detection, C. Aberle et al., arXiv:1112.5941, 2011.

[15-2]

Self-Calibration of Neutrino Detectors using characteristic Backgrounds, Joachim Kopp, Manfred Lindner, Alexander Merle, Nucl. Instrum. Meth. A582 (2007) 456-461, arXiv:hep-ph/0703055.

[15-3]

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Comment: Another junk paper in which it is claimed that solar, atmospheric and LSND data can be fitted in a three-neutrino model.
Important data (energy spectra) are omitted and the analysis is very approximate.
The claimed best-fit values of the largest are either or .
The smaller value give in LSND. Therefore, this case is equivalent to neglect LSND.
The larger values obviously cannot fit the energy spectra of atmospheric neutrinos, which have been omitted in the analysis.
[C.G.].

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Neutrino Unbound

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