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Prospects for improved understanding of isotopic reactor antineutrino fluxes
Phys. Rev. D 97, 013003 – Published 23 January, 2018
DOI: https://doi.org/10.1103/PhysRevD.97.013003
Abstract
Predictions of antineutrino fluxes produced by fission isotopes in a nuclear reactor have recently received increased scrutiny due to observed differences in predicted and measured inverse beta decay (IBD) yields, referred to as the “reactor antineutrino flux anomaly.” In this paper, global fits are applied to existing IBD yield measurements to produce constraints on antineutrino production by individual plutonium and uranium fission isotopes. We find that fits including measurements from highly -enriched cores and fits including Daya Bay’s new fuel evolution result produce discrepant best-fit IBD yields for and . This discrepancy can be alleviated in a global analysis of all data sets through simultaneous fitting of , , and yields. The measured IBD yield of in this analysis is , nearly two standard deviations below existing predictions. Future hypothetical IBD yield measurements by short-baseline reactor experiments are examined to determine their possible impact on the global understanding of isotopic IBD yields. It is found that future improved short-baseline IBD yield measurements at both high-enriched and low-enriched cores can significantly improve constraints for , , and , providing comparable or superior precision to existing conversion- and summation-based antineutrino flux predictions. Systematic and experimental requirements for these future measurements are also investigated.
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References (70)
- F. Reines and C. Cowan, Phys. Rev. 113, 273 (1959).
- Y. Declais et al., Phys. Lett. B 338, 383 (1994).
- A. Afonin, S. Ketov, V. Kopeikin, L. Mikaelyan, and M. Skorokhvatov, Sov. Phys. JETP 67, 213 (1988).
- E. Pasierb, H. Gurr, J. Lathrop, F. Reines, and H. Sobel, Phys. Rev. Lett. 43, 96 (1979).
- Yu. V. Kozlov, S. V. Khaltourtcev, I. N. Machulin, A. V. Martemyanov, V. P. Martemyanov, S. V. Sukhotin, V. G. Tarasenkov, E. V. Turbin, and V. N. Vyrodov, Phys. At. Nucl. 63, 1016 (2000).
- M. Deniz et al. (TEXONO Collaboration), Phys. Rev. D 81, 072001 (2010).
- K. Eguchi et al. (KamLAND Collaboration), Phys. Rev. Lett. 90, 021802 (2003).
- F. P. An et al. (Daya Bay Collaboration), Phys. Rev. Lett. 108, 171803 (2012).
- J. Ahn et al. (RENO Collaboration), Phys. Rev. Lett. 108, 191802 (2012).
- Y. Abe et al. (Double Chooz Collaboration), J. High Energy Phys. 10 (2014) 086; 02 (2015) 74.
- F. P. An et al. (Daya Bay Collaboration), Phys. Rev. D 95, 072006 (2017).
- K. Way and E. Wigner, Phys. Rev. 73, 1318 (1948).
- F. T. Avignone and Z. D. Greenwood, Phys. Rev. C 22, 594 (1980).
- H. Klapdor and J. Metzinger, Phys. Lett. B 112, 22 (1982).
- K. Schreckenbach, G. Colvin, W. Gelletly, and F. Von Feilitzsch, Phys. Lett. 160B, 325 (1985).
- F. Von Feilitzsch, A. A. Hahn, and K. Schreckenbach, Phys. Lett. 118B, 162 (1982).
- A. A. Hahn, K. Schreckenbach, W. Gelletly, F. von Feilitzsch, G. Colvin, and B. Krusche, Phys. Lett. B 218, 365 (1989).
- P. Vogel, Phys. Rev. C 76, 025504 (2007).
- B. Achkar et al., Phys. Lett. B 374, 243 (1996).
- T. A. Mueller et al., Phys. Rev. C 83, 054615 (2011).
- P. Huber, Phys. Rev. C 84, 024617 (2011).
- G. Mention, M. Fechner, Th. Lasserre, Th. A. Mueller, D. Lhuillier, M. Cribier, and A. Letourneau, Phys. Rev. D 83, 073006 (2011).
- F. P. An et al. (Daya Bay Collaboration), Phys. Rev. Lett. 116, 061801 (2016).
- S.-H. Seo (RENO Collaboration)AIP Conf. Proc. 1666, 080002 (2015).
- J. Kopp, P. A. N. Machado, M. Maltoni, and T. Schwetz, J. High Energy Phys. 05 (2013) 050.
- C. Giunti, M. Laveder, Y. F. Li, and H. W. Long, Phys. Rev. D 88, 073008 (2013).
- D. A. Dwyer and T. J. Langford, Phys. Rev. Lett. 114, 012502 (2015).
- A. C. Hayes, J. L. Friar, G. T. Garvey, D. Ibeling, G. Jungman, T. Kawano, and R. W. Mills, Phys. Rev. D 92, 033015 (2015).
- A. C. Hayes, J. L. Friar, G. T. Garvey, G. Jungman, and G. Jonkmans, Phys. Rev. Lett. 112, 202501 (2014).
- A. Sonzogni, E. McCutchan, and A. C. Hayes, Phys. Rev. Lett. 119, 112501 (2017).
- M. Fallot et al., Phys. Rev. Lett. 109, 202504 (2012).
- A. A. Sonzogni, T. D. Johnson, and E. A. McCutchan, Phys. Rev. C 91, 011301 (2015).
- A. A. Sonzogni, E. A. McCutchan, T. D. Johnson, and P. Dimitriou, Phys. Rev. Lett. 116, 132502 (2016).
- C. Buck, A. P. Collin, J. Haser, and M. Lindner, Phys. Lett. B 765, 159 (2017).
- J. Ashenfelter et al. (PROSPECT Collaboration), J. Phys. G 43, 113001 (2016).
- D. LhuillierAIP Conf. Proc. 1666, 180003 (2015).
- Y. Abreyu et al., J. Instrum. 12, P04024 (2017).
- F. P. An et al. (Daya Bay Collaboration), Phys. Rev. Lett. 118, 251801 (2017).
- P. Huber, Phys. Rev. Lett. 118, 042502 (2017).
- C. Giunti, Phys. Lett. B 764, 145 (2017).
- C. Giunti, Phys. Rev. D 96, 033005 (2017).
- C. Giunti, X. Ji, M. Laveder, Y. Li, and B. Littlejohn, J. High Energy Phys. 10 (2017) 143.
- G. S. Vidyakin et al., Sov. Phys. JETP 66, 243 (1987).
- G. S. Vidyakin et al., Sov. Phys. JETP 71, 424 (1990).
- H. Kwon, F. Boehm, A. A. Hahn, H. E. Henrikson, J.-L. Vuilleumier, J.-F. Cavaignac, D. H. Koang, B. Vignon, F. v. Feilitzsch, and R. L. Mössbauer, Phys. Rev. D 24, 1097 (1981).
- G. Boireau et al. (NUCIFER Collaboration), Phys. Rev. D 93, 112006 (2016).
- Z. Greenwood et al., Phys. Rev. D 53, 6054 (1996).
- G. Zacek et al. (CalTech-SIN-TUM Collaboration), Phys. Rev. D 34, 2621 (1986).
- A. Kuvshinnikov et al., JETP Lett. 54, 253 (1991).
- M. Apollonio et al., Phys. Lett. B 466, 415 (1999).
- N. Haag, A. Gütlein, M. Hofmann, L. Oberauer, W. Potzel, K. Schreckenbach, and F. M. Wagner, Phys. Rev. Lett. 112, 122501 (2014).
- G. D’Agostini, Nucl. Instrum. Methods Phys. Res., Sect. A 362, 487 (1995).
- S. Gariazzo, C. Giunti, M. Laveder, and Y. Li, J. High Energy Phys. 06 (2017) 135.
- W. Mampe, K. Schreckenbach, P. Jeuch, B. Maier, F. Braumandl, J. Larysz, and T. von Egidy, Nucl. Instrum. Methods Phys. Res., Sect. A 154, 127 (1978).
- M. Danilov, Neutrino 2016: XXVII International Conference on Neutrino Physics and Astrophysics, LOCATION, 2016 (unpublished).
- Y. J. Ko et al., Phys. Rev. Lett. 118, 121802 (2017).
- A. Serebrov et al., arXiv:1708.00421.
- Y. Klimov, V. Kopeikin, L. Mikaelyan, K. Ozerov, and V. Sinev, At. Energ. 76, 123 (1994).
- F. P. An et al. (Daya Bay Collaboration), Chin. Phys. C 41, 013002 (2017).
- X. B. Ma, W. L. Zhong, L. Z. Wang, Y. X. Chen, and J. Cao, Phys. Rev. C 88, 014605 (2013).
- A. Cabrera, CERN EP Seminar, 2016 (unpublished).
- K. Olive et al. (Particle Data Group), Chin. Phys. C 40, 100001 (2016).
- A. Bernstein, N. Bowden, and A. Erickson, arXiv:1612.00540.
- P. Jaffke and P. Huber, Phys. Rev. Applied 8, 034005 (2017).
- K. Heeger, B. Littlejohn, P. Mumm, and M. Tobin, Phys. Rev. D 87, 073008 (2013).
- C. Zhang, X. Qian, and P. Vogel, Phys. Rev. D 87, 073018 (2013).
- X. Qian, C. Zhang, M. Diwan, and P. Vogel, arXiv:1308.5700.
- F. An et al. (JUNO Collaboration), J. Phys. G 43, 030401 (2016).
- A. Aguilar-Arevalo et al. (CONNIE Collaboration), J. Instrum. 11, P07024 (2016).
- A. G. Beda, V. B. Brudanin, V. G. Egorov, D. V. Medvedev, V. S. Pogosov, E. A. Shevchik, M. V. Shirchenko, A. S. Starostin, and I. V. Zhitnikov, Phys. Part. Nucl. Lett. 10, 139 (2013).