Charge and magnetic moment of the neutrino in the background field method and in the linear 
                $R_{\xi}^L$
               gauge

Cabral-Rosetti, Luis G.; Bernabéu, J.; Vidal, J. Ruiz; Zepeda, A.

doi:10.1007/s100520000304

Cited by 32 publications

(33 citation statements)

References 20 publications

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“…Thus Eq. (57) gives for the neutrino magnetic moment the value of 3.2 × 10 −19 ( mν eV )µ B and agrees with the previous analyses given in the Standard Model [76,77]. We note that the underlying assumptions of [76,77] regarding a small Dirac mass is identical to ours except that our analysis is more general in that it includes both supersymmetry and mirror contributions.…”

Section: Neutrino Magnetic Momentsupporting

confidence: 89%

MSSM extension with a mirror fourth generation, neutrino magnetic moments, and CERN LHC signatures

Ibrahim

Nath

2008

Phys. Rev. D

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Recent analyses have shown that a sequential fourth generation can be consistent with precision electroweak data. We consider the possibility that the new generation could be a mirror generation with V + A rather than V − A interactions. Specifically we consider an extension of the minimal supersymmetric standard model with a light mirror generation (mirMSSM) . Implications of this extension are explored. One consequence is an enhancement of the tau neutrino magnetic moment by several orders of magnitude consistent with the current limits on the magnetic moment of the tau. The masses of the mirror generation arise due to electroweak symmetry breaking, and if a mirror generation exists its mass spectrum must lye below a TeV, and thus should be discovered at the LHC. Mirror particles and mirror sparticles produce many characteristic signatures which should be detectable at the LHC. Heavy higgs boson decays into mirror particles and an analysis of the forward-backward asymmetries can distinguish a mirror generation from a sequential fourth generation. The validity of the model can thus be tested at the LHC. A model of the type discussed here could arise from a more unified structure such as grand unification or strings where a mirror generation escapes the survival hypothesis, i.e., a generation and a mirror generation do not tie up to acquire a mass of size M GU T or M string due to a symmetry, and thus remain massless down to the electroweak scale.

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Section: Neutrino Magnetic Momentsupporting

confidence: 89%

MSSM extension with a mirror fourth generation, neutrino magnetic moments, and CERN LHC signatures

Ibrahim

Nath

2008

Phys. Rev. D

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“…Therefore, charge is quantized and from Eq. (7.1) neutrinos are exactly neutral (see also the explicit calculations in Bardeen et al (1972); Beg et al (1978); Marciano and Sirlin (1980); Sakakibara (1981); Lucio et al (1984Lucio et al ( , 1985; Cabral-Rosetti et al (2000)). This beautiful proof of charge quantization is spoiled by the introduction of a right-handed SU(2) L singlet neutrino ν R in order to have a Dirac neutrino mass.…”

Section: A Neutrino Electric Chargementioning

confidence: 95%

Neutrino electromagnetic interactions: A window to new physics

2015

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We review the theory and phenomenology of neutrino electromagnetic interactions, which give us powerful tools to probe the physics beyond the Standard Model. After a derivation of the general structure of the electromagnetic interactions of Dirac and Majorana neutrinos in the one-photon approximation, we discuss the effects of neutrino electromagnetic interactions in terrestrial experiments and in astrophysical environments. We present the experimental bounds on neutrino electromagnetic properties and we confront them with the predictions of theories beyond the Standard Model.

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“…The dependence of the diagonal magnetic moment of a massive Dirac neutrino on the neutrino b i = m 2 i /m 2 W and charged lepton a l = m 2 l /m 2 W mass parameters in the one-loop approximation in the minimally-extended Standard Model with right-handed neutrinos was studied in [12][13][14]. The calculations of the neutrino magnetic moment which take into account exactly the dependence on the masses of all particles [13,14] can be useful in the case of a heavy neutrino with a mass comparable or even exceeding the values of the masses of other known particles.…”

Section: Magnetic and Electric Dipole Moments In Gauge Modelsmentioning

confidence: 99%

Electromagnetic neutrino: a short review

Studenikin

2016

Nuclear and Particle Physics Proceedings

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A short review on selected issues related to the problem of neutrino electromagnetic properties is given. After a flash look at the theoretical basis of neutrino electromagnetic form factors, constraints on neutrino magnetic moments and electric millicharge from terrestrial experiments and astrophysical observations are discussed. We also focus on some recent studies of the problem and on perspectives.The passed two years, since the previous ICHEP conference held in Melbourne in 2012, have been celebrated by a spectacular step further in high energy physics. The prediction of the now-termed BEH symmetry breaking mechanism, attributed to Robert Brout, Francois Englert and Peter Higgs, recently supported by an excellent job done by two CERN collaborations for discovering of the Higgs boson provides the final glorious triumph of the Standard Model.Within the initial formulation of the Standard Model neutrinos are massless particles. However, already now it is known that the Standard Model should be extended to some more general theory in particular because of neutrinos which are the only particles exhibiting experimentally well-confirmed properties beyond the Standard Model. This is because of neutrino mixing and oscillations supported by the discovery of flavour conversion of neutrinos from different sources, the effect that is not possible for massless neutrinos.

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Charge and magnetic moment of the neutrino in the background field method and in the linear $R_{\xi}^L$ gauge

Cited by 32 publications

References 20 publications

MSSM extension with a mirror fourth generation, neutrino magnetic moments, and CERN LHC signatures

MSSM extension with a mirror fourth generation, neutrino magnetic moments, and CERN LHC signatures

Neutrino electromagnetic interactions: A window to new physics

Electromagnetic neutrino: a short review

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