One-loop neutrino mass model without any additional symmetries

[1]  Talal Ahmed Chowdhury,et al.  Charged Lepton Flavor Violation in a class of Radiative Neutrino Mass Generation Models , 2018, Proceedings of The 39th International Conference on High Energy Physics — PoS(ICHEP2018).

[2]  K. Cheung,et al.  Generalized one-loop neutrino mass model with charged particles , 2018, 1801.00585.

[3]  K. Cheung,et al.  A testable radiative neutrino mass model with multi-charged particles , 2017, 1708.06111.

[4]  H. Okada,et al.  Neutrino mass with large S U (2 ) L multiplet fields , 2017, 1708.03204.

[5]  H. Okada,et al.  Loop suppressed light fermion masses with U(1)R gauge symmetry , 2017, 1704.03382.

[6]  E. Senaha,et al.  Dark matter, muon g -2 , electric dipole moments, and Z →ℓ i + ℓ j - in a one-loop induced neutrino model , 2017, 1703.09153.

[7]  M. Lindner,et al.  A Call for New Physics : The Muon Anomalous Magnetic Moment and Lepton Flavor Violation , 2016, 1610.06587.

[8]  H. Okada,et al.  Radiative neutrino model with SU(2)L triplet fields , 2016, 1610.04729.

[9]  K. Cheung,et al.  Testable radiative neutrino mass model without additional symmetries and explanation for the $b \to s \ell^+ \ell^-$ anomaly , 2016, 1610.02322.

[10]  H. Okada,et al.  Extended colored Zee-Babu model , 2016, 1607.04952.

[11]  H. Okada,et al.  An $SU(2)_L$ Septet Scalar Linking to Radiative Neutrino Model , 2016, 1605.02601.

[12]  H. Okada,et al.  An explanation of one-loop induced h → μτ decay , 2016, 1604.03738.

[13]  Yi-Fu Cai,et al.  Revisiting the RνMDM models , 2016, 1603.00255.

[14]  M. Chala,et al.  LHC bounds on lepton number violation mediated by doubly and singly-charged scalars , 2013, 1311.1510.

[15]  J. Wudka,et al.  Discriminating between lepton number violating scalars using events with four and three charged leptons at the LHC , 2013, 1305.3904.

[16]  K. Yagyu,et al.  Two-loop radiative seesaw model with inert triplet scalar field , 2013, 1303.3463.

[17]  Michael Gustafsson,et al.  Predictive model for radiatively induced neutrino masses and mixings with dark matter. , 2012, Physical review letters.

[18]  S. Kanemura,et al.  Neutrino mass, dark matter, and Baryon asymmetry via TeV-scale physics without fine-tuning. , 2008, Physical review letters.

[19]  A. Strumia,et al.  Cosmology and Astrophysics of Minimal Dark Matter , 2007, 0706.4071.

[20]  E. Ma Verifiable radiative seesaw mechanism of neutrino mass and dark matter , 2006, hep-ph/0601225.

[21]  A. Strumia,et al.  Minimal Dark Matter , 2005, hep-ph/0512090.

[22]  Astronomy,et al.  A Model for neutrino masses and dark matter , 2002, hep-ph/0210389.

[23]  J. Casas,et al.  Oscillating neutrinos and ? e, ? , 2001, hep-ph/0103065.

[24]  Takeuchi,et al.  Estimation of oblique electroweak corrections. , 1992, Physical review. D, Particles and fields.

[25]  Takeuchi,et al.  New constraint on a strongly interacting Higgs sector. , 1990, Physical review letters.

[26]  K. Babu,et al.  Model of 'Calculable' Majorana Neutrino Masses , 1988 .

[27]  Ta-Pei Cheng,et al.  Neutrino masses, mixings, and oscillations in SU(2)×U(1) models of electroweak interactions , 1980 .

[28]  A. Zee A theory of lepton number violation and neutrino Majorana masses [Phys. Lett. 93b(1980)389] , 1980 .

[29]  A. Zee,et al.  Quantum numbers of Majorana neutrino masses , 1986 .