Casas-Ibarra parametrization and leptogenesis

XING Zhi-Zhong

doi:10.1088/1674-1137/34/1/001

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2024年10月30日

Chinese Physics C> 2010, Vol. 34> Issue(1) : 1-6 DOI: 10.1088/1674-1137/34/1/001

Casas-Ibarra parametrization and leptogenesis

XING Zhi-Zhong ^,

Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

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Abstract：
The Casas-Ibarra parametrization is a description of the Dirac neutrino mass matrix M_D in terms of the neutrino mixing matrix V, an orthogonal matrix O and the diagonal mass matrices of light and heavy Majorana neutrinos in the type-I seesaw mechanism. Because M_DM_D is apparently independent of V but dependent on O in this parametrization, a number of authors have claimed that unflavored leptogenesis has nothing to do with CP violation at low energies. Here we question this logic by clarifying the physical meaning of O. We establish a clear relationship between O and the observable quantities, and find that O does depend on V. We show that both unflavored leptogenesis and flavored leptogenesis have no direct connection with low-energy CP violation.

References

[1]

. Minkowski P. Phys. Lett. B, 1977, 67: 4212. Casas J A, Ibarra A. Nucl. Phys. B, 2001, 618: 1713. Fukugita M, Yanagida T. Phys. Lett. B, 1986, 174: 454. Kuzmin V A, Rubakov V A, Shaposhnikov ME. Phys. Lett.B, 1985, 155: 365. Luty M A, Phys. Rev. D. 1992, 45: 455; Flanz M, PaschosE A, Sarkar U. Phys. Lett. B, 1995, 345: 248; CoviL, Roulet E, Vissani F. Phys. Lett. B, 1996 384: 169;Plumacher M. Z. Phys. C, 1997, 74: 549; Pilaftsis A. Phys.Rev. D, 1997, 56: 5431; Buchmuller W, Plumacher M.Phys. Lett. B, 1998, 431: 3546. Masina I. hep-ph/0210125; Lavignac S, Masina I, Savoy CA. Nucl. Phys. B, 2002, 633: 139; Branco G C et al. Phys.Rev. D, 2003, 67: 0730257. Rebelo M N. Phys. Rev. D, 2003, 67: 0130088. Pascoli S, Petcov S T, Rodejohann W. Phys. Rev. D, 2003,68: 093007; Pascoli S, Petcov S T, Riotto A. Phys. Rev.D, 2007, 75: 083511; Nucl. Phys. B, 2007, 774: 19. Branco G C, Rebelo M N, Silva-Marcos J I. Phys. Lett. B,2006, 633: 345; Branco G C, Buras A J, Jager S, Uhlig S,Weiler A. JHEP, 2007, 0709: 00410. Molinaro E, Petcov S T. Phys. Lett. B, 2009, 671: 60;arXiv:0803.412011. Branco G C, Rebelo M N. arXiv:0902.016212. XING Z Z, ZHOU S. High Energy Phys. Nucl. Phys., 2006,30: 82813. XING Z Z. Phys. Lett. B, 2008, 660: 51514. Amsler C et al (Particle Data Group). Phys. Lett. B, 2008,667: 115. Antusch S, Biggio C, Fernandez-Martinez E, Gavela M B,Lopez-Pavon J. JHEP, 2006, 0610: 084; Abada A, BiggioC, Bonnet F, Gavela M B, Hambye T. JHEP, 2007, 0712:06116. Fritzsch H, XING Z Z. Prog. Part. Nucl. Phys., 2000, 45: 1;Altarelli G, Feruglio F. New J. Phys., 2004, 6: 106; XINGZ Z. Int. J. Mod. Phys. A, 2004, 19: 1; Mohapatra R N,Smirnov A Yu. Ann. Rev. Nucl. Part. Sci., 2006, 56: 569;Strumia A, Vissani F. hep-ph/060605417. Barbieri R, Creminelli P, Strumia A, Tetradis N. Nucl.Phys. B, 2000, 575: 6118. Davidson S, Nardi E, Nir Y. Phys. Rept., 2008, 466: 10519. Endoh T, Morozumi T, XIONG Z H. Prog. Theor. Phys.,2004, 111: 12320. Davidson S, Garayoa J, Palorini F, Rius N. Phys. Rev.Lett., 2007, 99: 161801; JHEP, 2008, 0809: 05321. XING Z Z. Int. J. Mod. Phys. A, 2008, 23: 4255;arXiv:0901.0209

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XING Zhi-Zhong. Casas-Ibarra parametrization and leptogenesis[J]. Chinese Physics C, 2010, 34(1): 1-6. doi: 10.1088/1674-1137/34/1/001

XING Zhi-Zhong. Casas-Ibarra parametrization and leptogenesis[J]. Chinese Physics C, 2010, 34(1): 1-6. doi: 10.1088/1674-1137/34/1/001 shu

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Received: 2009-05-07
Revised: 2009-06-01

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沈阳化工大学材料科学与工程学院沈阳 110142

Casas-Ibarra parametrization and leptogenesis

XING Zhi-Zhong ^,

Corresponding author: XING Zhi-Zhong,

Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

Received Date: 2009-05-07
Accepted Date: 2009-06-01
Available Online: 2010-01-05

Abstract:

The Casas-Ibarra parametrization is a description of the Dirac neutrino mass matrix M_D in terms of the neutrino mixing matrix V, an orthogonal matrix O and the diagonal mass matrices of light and heavy Majorana neutrinos in the type-I seesaw mechanism. Because M_DM_D is apparently independent of V but dependent on O in this parametrization, a number of authors have claimed that unflavored leptogenesis has nothing to do with CP violation at low energies. Here we question this logic by clarifying the physical meaning of O. We establish a clear relationship between O and the observable quantities, and find that O does depend on V. We show that both unflavored leptogenesis and flavored leptogenesis have no direct connection with low-energy CP violation.