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Cited by 176Neutrino Physics ResearchParticle physics theoretical and experimental studiesNuclear physics research studies

NEUTRINOLESS DOUBLE-BETA DECAY: A BRIEF REVIEW

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BILENKY, S. M., GIUNTI, C.·2012·Modern Physics Letters A
DOI 10.1142/s0217732312300157
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Abstract

In this brief review we discuss the generation of Majorana neutrino masses through the seesaw mechanism, the theory of neutrinoless double-beta decay, the implications of neutrino oscillation data for the effective Majorana mass, taking into account the recent Daya Bay measurement of ϑ 13, and the interpretation of the results of neutrinoless double-beta decay experiments.

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  • For a periodic Majorana neutrino, there are two solutions of V=0 for any value of mν,lightest allowed by experiment, mν,lightest ≳ 0.1 eV.

    “Figure 14 corresponds to Majorana neutrino, and there are two solutions of V = 0 for any value of m ν,lightest allowed by the experiment, m ν,lightest 0.1 eV [50,51].”

    From Weak gravity conjecture, multiple point principle and the standard model landscape (2017) · cites this paper as [51]

    Section 4 (p. 12) discusses effective Majorana mass as a function of the lightest neutrino mass, and the Conclusions (p. 19) note that cancellations can occur in the normal mass scheme. Searches for periodic Majorana neutrinos and two solutions of V = 0 found no passage addressing those claims or the stated mν,lightest ≳ 0.1 eV condition. (LLM, conf=0.76)

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Research works printed but not linked: 65

  1. [1]1. Super-Kamiokande, R. Wendell et al., Phys. Rev. D81 (2010) 092004, arXiv:1002.3471. · arXiv
  2. [2]2. SNO, B. Aharmim et al., (2011), arXiv:1109.0763. · arXiv
  3. [3]3. KamLAND, A. Gando et al., Phys. Rev. D83 (2011) 052002, arXiv:1009.4771. · arXiv
  4. [4]4. K2K, M.H. Ahn et al., Phys. Rev. Lett. 90 (2003) 041801, hep-ex/0212007. · arXiv
  5. [5]5. MINOS, P. Adamson et al., Phys. Rev. Lett. 106 (2011) 181801, arXiv:1103.0340. · arXiv
  6. [9]9. S.M. Bilenky, C. Giunti and W. Grimus, Prog. Part. Nucl. Phys. 43 (1999) 1, hep-ph/9812360. · arXiv
  7. [13]13. C. Giunti, Phys. Lett. B686 (2010) 41, arXiv:1001.0760. · arXiv
  8. [14]14. DAYA-BAY, F.P. An et al., Phys. Rev. Lett. 108 (2012) 171803, arXiv:1203.1669. · arXiv
  9. [15]15. T2K, K. Abe et al., Phys. Rev. Lett. 107 (2011) 041801, arXiv:1106.2822. · arXiv
  10. [16]16. MINOS, P. Adamson et al., Phys. Rev. Lett. 107 (2011) 181802, arXiv:1108.0015. · arXiv
  11. [17]17. DOUBLE-CHOOZ, Y. Abe et al., Phys. Rev. Lett. 108 (2012) 131801, arXiv:1112.6353. · arXiv
  12. [18]18. G.L. Fogli et al., (2008), arXiv:0809.2936, NO-VE 2008, IV International Workshop on 'Neutrino Oscillations in Venice' (Venice, Italy, April 15-18, 2008). · arXiv
  13. [19]19. A.B. Balantekin and D. Yilmaz, J. Phys. G35 (2008) 075007, arXiv:0804.3345. · arXiv
  14. [20]20. G. Fogli et al., Phys. Rev. Lett. 101 (2008) 141801, arXiv:0806.2649. · arXiv
  15. [21]21. H. Ge, C. Giunti and Q. Liu, Phys. Rev. D80 (2009) 053009, arXiv:0810.5443. · arXiv
  16. [22]22. M. Gonzalez-Garcia, M. Maltoni and J. Salvado, JHEP 04 (2010) 056, arXiv:1001.4524. · arXiv
  17. [23]23. Z. zhong Xing, Chin. Phys. C36 (2012) 281, arXiv:1203.1672. · arXiv
  18. [24]24. M. Mezzetto and T. Schwetz, J. Phys. G37 (2010) 103001, arXiv:1003.5800. · arXiv
  19. [25]25. LSND, A. Aguilar et al., Phys. Rev. D64 (2001) 112007, hep-ex/0104049. · arXiv
  20. [26]26. MiniBooNE, A.A. Aguilar-Arevalo et al., Phys. Rev. Lett. 105 (2010) 181801, arXiv:1007.1150. · arXiv
  21. [27]27. G. Mention et al., Phys. Rev. D83 (2011) 073006, arXiv:1101.2755. · arXiv
  22. [28]28. T.A. Mueller et al., Phys. Rev. C83 (2011) 054615, arXiv:1101.2663. · arXiv
  23. [29]29. P. Huber, Phys. Rev. C84 (2011) 024617, arXiv:1106.0687. · arXiv
  24. [30]30. C. Giunti and M. Laveder, Nucl. Phys. Proc. Suppl. 217 (2011) 193, arXiv:1012.4356, NOW 2010, 4-11 September 2010, Conca Specchiulla (Otranto, Lecce, Italy). · arXiv
  25. [31]31. C. Kraus et al., Eur. Phys. J. C40 (2005) 447, hep-ex/0412056. · arXiv
  26. [32]32. Troitsk, V. Aseev et al., Phys. Rev. D84 (2011) 112003, arXiv:1108.5034. · arXiv
  27. [33]33. C. Giunti and C.W. Kim, Fundamentals of Neutrino Physics and Astrophysics (Oxford University Press, Oxford, UK, 2007), ISBN 978-0-19-850871-7.
  28. [36]36. T. Yanagida, (1979), Workshop on the Baryon Number of the Universe and Unified Theories, Tsukuba, Japan, 13-14 Feb 1979.
  29. [38]38. S.M. Bilenky et al., Phys. Rep. 379 (2003) 69, hep-ph/0211462. · arXiv
  30. [39]39. S.R. Elliott and P. Vogel, Ann. Rev. Nucl. Part. Sci. 52 (2002) 115, hep-ph/0202264. · arXiv
  31. [40]40. S.R. Elliott and J. Engel, J. Phys. G30 (2004) R183, hep-ph/0405078. · arXiv
  32. [41]41. I. Avignone, Frank T., S.R. Elliott and J. Engel, Rev. Mod. Phys. 80 (2008) 481, arXiv:0708.1033. · arXiv
  33. [42]42. S.M. Bilenky, Lect. Notes Phys. 817 (2010) 139, arXiv:1001.1946. · arXiv
  34. [43]43. W. Rodejohann, Int. J. Mod. Phys. E20 (2011) 1833, arXiv:1106.1334. · arXiv
  35. [44]44. J. Gomez-Cadenas et al., Riv. Nuovo Cim. 35 (2012) 29, arXiv:1109.5515. · arXiv
  36. [45]45. B. Schwingenheuer, (2012), arXiv:1201.4916, TAUP 2011. · arXiv
  37. [47]47. E. Ma, Phys.Rev.Lett. 81 (1998) 1171, hep-ph/9805219. · arXiv
  38. [48]48. S. Davidson, E. Nardi and Y. Nir, Phys. Rept. 466 (2008) 105, arXiv:0802.2962. · arXiv
  39. [53]53. F. Simkovic et al., Phys. Rev. C60 (1999) 055502, hep-ph/9905509. · arXiv
  40. [54]54. F. Simkovic et al., Phys. Rev. C77 (2008) 045503, arXiv:0710.2055. · arXiv
  41. [55]55. S. Hannestad, Prog. Part. Nucl. Phys. 65 2010 (2010) 185, arXiv:1007.0658. · arXiv
  42. [56]56. F. Vissani, JHEP 06 (1999) 022, hep-ph/9906525. · arXiv
  43. [57]57. S.M. Bilenky, S. Pascoli and S.T. Petcov, Phys. Rev. D64 (2001) 053010, hep-ph/0102265. · arXiv
  44. [58]58. T. Schwetz, M. Tortola and J.W.F. Valle, New J. Phys. 13 (2011) 109401, arXiv:1108.1376. · arXiv
  45. [59]59. S. Bilenky, Introduction to the physics of massive and mixed neutrinos (Springer, 2010), Lecture Notes in Physics, Volume 817; ISBN 978-3-642-14042-6.
  46. [60]60. KATRIN, A. Osipowicz et al., (2001), hep-ex/0109033. · arXiv
  47. [62]62. K.N. Abazajian et al., Astropart. Phys. 35 (2011) 177, arXiv:1103.5083. · arXiv
  48. [63]63. V.A. Rodin et al., Phys. Rev. C68 (2003) 044302, nucl-th/0305005. · arXiv
  49. [64]64. V.A. Rodin et al., Nucl. Phys. A766 (2006) 107, arXiv:0706.4304. · arXiv
  50. [65]65. A. Bobyk, W.A. Kaminski and F. Simkovic, Phys. Rev. C63 (2001) 051301, nucl-th/0012010. · arXiv
  51. [67]67. T.R. Rodriguez and G. Martinez-Pinedo, Prog.Part.Nucl.Phys. 66 (2011) 436, arXiv:1012.1783. · arXiv
  52. [68]68. T.R. Rodriguez and G. Martinez-Pinedo, Phys.Rev.Lett. 105 (2010) 252503, arXiv:1008.5260. · arXiv
  53. [70]70. P. Rath, J.Phys.Conf.Ser. 322 (2011) 012019.
  54. [72]72. F. Iachello and J. Barea, Nucl.Phys.Proc.Suppl. 217 (2011) 5.
  55. [73]73. F. Iachello and J. Barea, AIP Conf.Proc. 1355 (2011) 7.
  56. [74]74. J. Menendez et al., J.Phys.Conf.Ser. 312 (2011) 072005.
  57. [75]75. J. Menendez et al., Nucl.Phys. A818 (2009) 139, arXiv:0801.3760. · arXiv
  58. [78]78. CUORICINO, E. Andreotti et al., Astropart. Phys. 34 (2011) 822, arXiv:1012.3266. · arXiv
  59. [79]79. NEMO, R. Arnold et al., Nucl. Phys. A765 (2006) 483, hep-ex/0601021. · arXiv
  60. [80]80. NEMO, A. Barabash et al., Phys.Atom.Nucl. 74 (2011) 312, arXiv:1002.2862, Fundamental Interactions Physics (ITEP, Moscow, November 23-27, 2009). · arXiv
  61. [82]82. GERDA Collaboration, C. Ur, Nucl.Phys.Proc.Suppl. 217 (2011) 38.
  62. [83]83. F. Bellini et al., Astropart. Phys. 33 (2010) 169, arXiv:0912.0452. · arXiv
  63. [84]84. KamLAND-Zen, Phys. Rev. C85 (2012) 045504, arXiv:1201.4664. · arXiv
  64. [85]85. EXO Collaboration, R. Gornea, J.Phys.Conf.Ser. 309 (2011) 012003.
  65. [86]86. A. Ibarra, E. Molinaro and S.T. Petcov, Phys. Rev. D84 (2011) 013005, arXiv:1103.6217. · arXiv

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Authors
BILENKY, S. M., & GIUNTI, C.
Affiliations
  • Joint Institute for Nuclear Research (RU)
  • INFN, Sezione di Torino, Via P. Giuria 1, I–10125 Torino, Italy
ORCID
BILENKY, S. M.
Venue
Modern Physics Letters A
Publisher
World Scientific Pub Co Pte Lt
Published
2012-04-30
Volume
27
Issue
13
Pages
1230015
ISSN
  • 0217-7323 (ISSN-L)
  • 1793-6632
DOI
10.1142/s0217732312300157
OpenAlex
W2075000414
Cited by
176
References
0
Citations by year
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FWCI
10.02
Type
journal article
Language
en
Open access
Locations
  • Modern Physics Letters A (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Neutrino Physics Research
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Particle physics theoretical and experimental studies
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Nuclear physics research studies
Keywords
neutrinoless double beta decay, Majorana neutrino masses, seesaw mechanism, neutrino oscillations, effective Majorana mass, theta13, Daya Bay, neutrino mass

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